We propose new visible-light observations of a well-selected sample of circumstellar (CS) debris disks, all with HST pedigree, using STIS PSF-subtracted multi-roll coronagraphic imaging. Our new observations will probe the interior CS regions of these debris systems (with inner working distances of < approximately 8 AU for half the stars in this sample), corresponding to the giant planet and Kuiper belt regions within our own solar system. These new images will enable us to directly inter-compare the architectures of these exoplanetary debris systems in the context of our own Solar System. These observations will also permit us, for the first time, to characterize the material in these regions at high spatial resolution and to look for sub-structures within the disks that are the sign posts of planetary formation and evolution; in particular, asymmetries and non-uniform debris structures signal the presence of co-orbiting perturbing planets. Additionally, all of our objects have been observed previously at longer wavelengths (but much lower spatial resolution and imaging efficacy) with NICMOS, but with an inner working angle comparable to STIS multi-roll coronagraphy. The combination of new optical and existing near-IR imaging will strongly constrain the dust properties, thus enabling an assessment of grain processing and planetesimal populations. These results will directly inform upon the posited planet formation mechanisms that occur after the ~ 10 My epoch of gas depletion, at a time in our solar system when giant planets were migrating and the terrestrial planets were forming, and directly test theoretical models of these processes. The outer reaches (only) of most of these systems were previously observed with a much larger (~ 6x on average), spatially limiting, effective inner working angle of the ACS coronagraph. The previous ACS images are therefore completely inadequate to address our science goals of imaging the inner structures of these CS disks. Our proposed investigation, enabled ONLY with HST STIS visible-light coronagraphy, will uniquely probe into the interior regions of these systems for the first time with spatial resolution comparable to ACS and with augmenting NICMOS near-IR disk photometry in hand. VISITS AND EXPOSURE DETAILS =========================== Guide Star Acquisitions: We require pointing and roll control with 2-FGS guiding. Single-FGS guiding does not offer sufficient target position stability for coronagraphy. Each visit (after its Guide Star acquisition) begins with a mode-2 target acquisition, is followed by a sequence of repetitive "short" exposures (by CR-SPLIT or exposure replication) at the WedgeA0.6 position followed by a sequence of repetitive "long" exposures (also by CR-SPLIT or exposure replication) at the Wedge A1.0 position. Exceptions to this are Visits 83 and 87 (Alpha Pic as PSF template. Due to Alpha Pic's brightness we use short, medium,and long imaging sequences (ordered to mitigate non-parallel buffer dumps), and also Visits A1-A8 where we use only a single imaging sequence at Wedge A0.6 due to the relative faintness of the target. 1) Target Acquisitions. We expose our TA images to a SNR > appx 100 using the STIS ETC. While robust target acquisition is enabled with SNR 40, we also use the TA images as a pre mode-2 astrometric anchor to assess the "behind the wedge" target position to high precision (separate from "diffraction spike" analysis, for which higher SNR for precision centroiding is required. We also use these F25ND3 filtered imagesto photometrically obtain target:PSF template brightness ratios in the broad STIS passband. The STIS Target Acquisition ETC was used to determine the eposure times for all acquisition images. In the case of Alpha Pic we use F25ND5 for the ACQ imaging due to its brightness. 2) The "short" exposure times are designed to reach 90% of full-well depth, with the target coronagraphically occulted, at the edge of the wedge 0.3" from the star. We scale, using the ETC, this from observations predicated upon an A0 star with V = 3.55 reach 90% full well from the PSF halo in 1 second based upon preious STIS coronagraphic observations allowing for up to as much of 1/2 pixel of possible target decentering in acquisition performance. We generally repeat these exposures to fill appx 35% of the target visibility interval (except for Visits A1-A8) after subtracting the time required for the preceding guide star and target acquisitions. In the case of Visits A1-A4 these exposures are quite long (comparitively) due to the relative faintness of this target and we fill the visibility period with these images (labelled as "FAINT"). 3) Following the short exposures we execute a Type-2 slew (by a change in instrument aperture to Wedge1.0) for the "long" exposure imaging (except Visits A1-A8). 4) The "long" exposures when possible are 20 x longer than the "short" exposures - but truncated to >= 10x if required to not overfill a visibility period with a minimum of 3 repeats (by CR Splitting). These, usually, are repeated to fill the visibility period. Note: In some cases, with a cannonical F30 target visibility period filled, the observations will not find schedulability in the APT Visit Planner at some relative orientations (Orient From V##). In those cases we shorten the pre-CR Split exposure time on the "long" exposures, leaving typically a few tens of seconds (but sometimes more or less) so the visit can find a Cy 18 scheduling opportunity (so do NOT use "auto-fill"). Sub-Array Readouts. For most coronagraphic exposures we use subarray readouts (SIZEAXIS2) symmetrically centered on the target to fully read-out the region along the wedge (Axis2, image Y axis) to the edge of the FOV at the small end of the wedge taper, and symmetrically on the diametrically opposing side. For WedgeA1.0 the max SIZEAXIS2 (without displacing with an “unsupported” CENTERAXIS2) is 427 pixels. This implies that the A1.0 position is 10.82” from the edge of the FOV (whole sub-array centered on target symmetrically 21.65” along the wedge). For WedgeA0.6 is (without displacing with an “unsupported” CENTERAXIS2) is 137 pixels. This implies that the A0.6 position is 3.47” from the edge of the FOV (whole sub-array centered on target symmetrically 6.95” along the wedge). VISIT LINKAGES (RELATIVE ORIENTATION CONSTRAINTS AND INTERLEAVED PSF OBSERVATIONS) ============================================================ We use 6 orbits to observe each science target. Along with every science target we observe a PSF template/calibration star using two orbits. Thus each science target and its unique PSF template consumes 8 orbits. We have 11 science targets, and 11 PSF template stars, for which a total of 88 orbits will be used. Each science target and its matched PSF star is observed in two "sets" of four single-orbit visits (X1-X4 and X5-X8). Within each set, three visits are used to observe the science target (X1, X2, X4 [for the second set X5, X6, X8], and one (each) the PSF star [X3 and X7]. These four visits within each set must be executed in sequential, contiguous orbits (i.e., back to back with no interruptions except Earth occultation). The three science target visits in each set are at different RELATIVE orientation of *NOMINALLY* -30, 0, and +30 degrees from nominal roll, with the second science target observation at nominal roll. The 3rd orbit (visit) in each 4-visit set is of the PSF template star paired with the science target. In general, the PSF template stars are generally very close in the sky to the science targets (within a few degrees). As a result we, anticipate that with scheduling of the second science orbit at nominal roll, the PSF calibration star will also be at or close to its nominal roll and usually these two orbits will have nearly the same celestial orientation angle. We do not levy that as a requirement (is a natural consequence of the "nearness" criteria and time linkage), but that is important for the stability of the PSF. In a few cases because of a lack of suitable PSF template stars (predicated on B-V color match, sufficient brightness, lack of duplicity or IR-excess indicative of dust) we had to look for trmplate stars further away (e.g. Alpha Pic for HD 53143; Visits 81-88; in this case Alpha Pic is a CVZ target that aids in finding schedualbility despite its greater distance from the target). The second identical second set of four visits (X5-X8; but may be SLIGHTLY different due to variable lengths of target visibility periods as found by the Visit Planner) is executed, but at different relative orientations for each visit. Nominally, the first later "repeated" orbit (X05) should be scheduled at either a +90 deg or -90 deg relative orientation from the first (X01). We sometimes relax this with an allowable range to assist in scheduling. Note that APT 18.2 does not have the capability to specify allowable multiple (in this case two) relative orientations. So, here we advise our PC that although the parity of the first orbit in the second set's (X5) relative orientation was found schedulable by APT, if for some reason it turns out not to be, our PC may freely change the sign of this relative offset range from positive to negative (or vice versa). In doing so the signs on the relative orientations (and ranges if any) on the Visit X6 and X8 Orient Froms must also be changed in concert. Either positive or negative Orients From of appx |90| are acceptable on Visit X5, with corresponding sign changes on Visits X6 and X8. In many cases we could not find schedulbility for all visits in the 8-visit link-sets with the ideal Orient From and required sequential orbit (visit) timing linkages (X01-X04 and X05-X08). In those cases we (laboriously) "relaxed" the Orient Froms within acceptable limits (for science reasons) to find schedualbilities (iteratively with multiple trials to find one permutation at least that would both "work" (schedule) and is acceptable for our science goals). This varies on a target by target and visit by visit basis. If guide stars (or other issues) preclude scheduling these visits as specified (as informed by our PC) we could look to modifying these Orient From requirements or, in some cases, suggest an alternate PSF star. Generic Single-Orbit per visit link-set structure with Nominal "Orient Froms" is as below: X1: Target Star. Orient from X2 by -30 to -30 deg X2: Target Star. Roll unconstrained. After X1 by 0.5 to 1.5 Orbits X3: Neaby PSF-Star. Roll Unconstrained. After X2 by 0.5 to 1.5 Orbits X4: Target Star: Orient from X2 by +30 to +30 deg. After X3 by 0.5 to 1.5 Orbits X5: Target Star. Orient from X1 by +90 to +90 deg (or -90 deg to -90 deg). No time constraint. X6: Target Star. Orient from X5 by +30 deg to +30 deg*. After X5 by 0.5 to 1.5 Orbits X7: Neaby PSF-Star. Roll Unconstrained. After X6 by 0.5 to 1.5 Orbits X8: Target Star: Orient from X2 by +60 to +60 deg*. After X7 by 0.5 to 1.5 Orbits * If sign change on X5 Orient From , signs must change on X7 and X8 Orient Froms as well. As noted in some cases these ideal angles are not schedulable, hence some deviations from these will be seen on a target by target and Visit by Visit basis. PSF TEMPLATE STARS (Targets 11 - 22) =================================== Each science target has a carefully selected "matched" PSF template star to be observed interleaved in each of the linked-visit sets as the third and seventh visit in each link-set. PSF star selection was the result of a careful vetting and down-selection process, leaving in many cases a vanishingly small set of "best" stars for any particular target WITH schedualibity as required. In the event of scheduling difficulties (e.g., guide star selections) if any visit (and thus the link-set) becomes unschedulable due to the PSF star,in SOME cases we can suggest an alternate - but in general we would look to further "relaxing" Orient From or other requirements that may be constraining that. We name our PSF stars somewhat unconventionally as: PSF##-targetname-psfname. This readily helps identify immediately which PSF star is paired with which science target. In all cases we select PSF stars that are matched in color, B-V within 0.1 of its corresponsing science target and, with only one exception, (by +0.5 mag) at least as bright as its science target. PSF stars, to the extent possible, have been vetted against binarity, field-crowding, and/or nebulosity (including known light-scattering CS dust of their own). PSF stars are usually constrained to be ~ < 5 deg from their science targets to minimize differences in contemporaneous observations in Sun and Beta angles that can drive OTA breathing mode (phase) changes. We have been forced to relax this in some targets due to lack of sufficient candidates and/or unschedualbility. Summary selection notes are provided for each PSF star in the APT file. COMMENTS ADDED MARCH 2, 2011 ========================== We are replacing the PSF template star originally programmed for Visit 87 with HD 59780. This star is 4.82 deg away from our original template (+3.26 deg in declination @ -58.07 deg and so still falls within the limits of the CZV though we do not ask for CVZ scheduling but we expect should "schedule in place" of the original template, or nearly so). With this target substitution, at the Visit level, we have retained all relative orient linkages between visits (81,82,84 [already executed]) and (85, 86, 88) to be executed along with the visit 81-88 temopral linkages to assure "back-to-back" sequential scheduling of the single-orbit visits 85-88. We impose NO relative orientation constraints on Visit 87 (replacement PSF template observation), though we change the exposure sequence details within the visit. We also alter the exposure definition for Visit 85, as the previously defined "back end" exposures needed for the science target with the previous (Visit 87) PSF template are no longer needed. We also take the opportunity to correct a few typos in exposure level descriptive commentary (only) in Visits 86 and 88. N.B. The B-V listed in the Fixded target definition for HD53143 as +0.20 is *incorrect* and should instead be +0.80; however, this is uneditable in APT as visits 81,82 and 84 have already executed. The corect value of +0.80 was used in selecting a replacement PSF calibration star (HD53143) used in Visit 87 (and was the basis for the need for a change in PSF template star. We have no real-time requirments. We ask for no SPECIAL calibrations for this proposal (and called none out in Phase 1). We did not because we ASSUME that STScI will acquire GAIN=4 (supported mode) bias, DARK, and flat-field frames (and derived hot/bad pixel maps) as part of their Cycle 18 calibration plan in support of approved Cycle 18 science programs. If this is NOT the case then we must obtain GAIN=4 calibration reference bias/dark data as part of our program using NON-POINTED (internal) orbits only. Our CS has advised us that the Cycle 18 calibration plan will not be built until AFTER the Phase 2 submission deadline. If that plan does not include acquiring for broader purposes the reference data we need, then we will need to add those internal calibrations to this program AFTER the Phase 2 deadline. Our thanks to Karla Peterson for her suggestions vis-a-vis APT 18.2 multi-roll constrained scheduling. EXTRA-SOLAR PLANETS 12 false 0.0 0.0 false false false false SUPPORTED STAR A0-A3 V-IV This object was generated by the targetselector and retrieved from the SIMBAD database. Spec: A0V HIP23451 GSC00110-0042 J2000 J2000 B-V = + 0.02 STAR F3-F9 This object was generated by the targetselector and retrieved from the SIMBAD database. Spec: F6V HIP95270 GSC08765-00638 J2000 J2000 B-V = + 0.48 STAR G V-IV This object was generated by the targetselector and retrieved from the SIMBAD database. Spec: G2V LTT13439 GSC01445-02267 J2000 J2000 B-V = + 0.62 STAR M V-IV This object was generated by the targetselector and retrieved from the SIMBAD database. Spec. M1V HD197481 HIP102409 J2000 J2000 B-V = +1.45 STAR F0-F2 This object was generated by the targetselector and retrieved from the SIMBAD database. Spec: F2 HIP11360 GSC00045-00990 J2000 J2000 B-V = +0.35 STAR G V-IV This object was generated by the targetselector and retrieved from the SIMBAD database. Spec. G8V HIP36948 GSC07109-02638 J2000 J2000 B-V = +0.71 STAR K V-IV This object was generated by the targetselector and retrieved from the SIMBAD database. Spec. K1V HIP52462 GSC06645-00338 J2000 J2000 B-V = +0.89 STAR F0-F2 This object was generated by the targetselector and retrieved from the SIMBAD database. Spec. F2V HIP11847 GSC02335-01209 J2000 J2000 B-V = +0.32 STAR G V-IV This object was generated by the targetselector and retrieved from the SIMBAD database. G9V HIP33690 SAO249700 J2000 J2000 B-V = +0.20 STAR F3-F9 This object was generated by the targetselector and retrieved from the SIMBAD database. Spec. F5V HIP76829 SAO226064 J2000 J2000 B-V = +0.40 STAR K V-IV This object was generated by the targetselector and retrieved from the SIMBAD database. Spec. K1V MP-MUS GSC09246-00971 J2000 J2000 B-V = +1.01 STAR B6-B9.5 V-IV Spec. B9V USNO-2: R=14 @ r = 0.74'; 6 stars R=14.0-19.5 @ 0.53' < r < 0.76' No HST Pedigree. No ref. as binary. Hipparcos photometery not available, HIP24048 GSC00103-00634 J2000 J2000 B-V = +0.01 STAR F3-F9 Spec. F7V. USNO-2: R=12.7 @ r = 0.95'; 6 stars R=12.7-18.0 @ 0.78' < r < 0.99' *** SPITZER EVIDENCE OF *COLD* DUST *** -- Smith et al. 2006 ApJL 644 125 Dean Hines Second Author - under re-eavaluation No HST Pedigree. HIP94858 GSC08760-02151 J2000 J2000 B-V = + 0.45 STAR G V-IV Spec. G0.5 IV-V USNO-2: R=13.4 @ r = 0.80'; 5 stars R=12.6-18.6 @ 0.64' < r < 0.86' HST/ACS-coron Pedigree (Ardila et al 2004) HIP67246 LHS2798 J2000 J2000 B-V = +0.66 STAR F0-F2 Spec. F2 USNO-: R=17.4 @ r = 0.55'; 7 stars R=17.4-19.1 @ 0.5' < r < 0.86' No HST Pedigree. No reference as binary SAO110616 GSC00639-00227 J2000 J2000 B-V = +0.35 STAR M V-IV Spec. M0V USNO-2: R=15.1 @ r = 0.39'; 6 stars R=15.1-17.9 @ 0.39' < r < 0.92' HST/ACS-coron perigree: Graham et al 2007 HST/NICMOS 7240 Verified Suitable from HST Images GJ784 HIP99701 J2000 J2000 B-V = +1.46 STAR F3-F9 Spec: F3V USNO-2: R=16.8 @ r = 0.67'; 3 stars R=15.6-18.0 @ 0.66' < r < 0.95' HST/NICMOS-Coron Pedigree Debes et al 2008 Verified Suitable from HST Iamges HR783 GSC00053-00623 J2000 J2000 B-V = +0.37 STAR G V-IV Spec. G5IV USNO-2: R=14.0 @ r = 0.61'; 19 stars R=12.7-17.9 @ 0.6' < r < 1.0' No HST Pedigree. Possible astrometric binary (Frankowski et al 2007). Possible Variale. HIP35017 SAO197738 J2000 J2000 B - V = +0.747 STAR G V-IV Spec. G5III USNO-2: R=15.6 @ r = 0.77'; 12 stars R=15.6-18.0 @ 0.6' < r < 0.96' No HST Pedigree. No reference as binary. Hipparchis photometry not variable. HIP50559 GSC07183-01474 J2000 J2000 B-V = +0.88 STAR A4-A9 III-I A4-A9 V-IV Spec. A8V APLHA-PICTORIS HD50241 J2000 J2000 B-V = +0.28 STAR F3-F9 Spec. F7V This is not an ideal PSF star for HD139664, but pickings are slim. It is 0.53 Vmag magnitude fainter,and +0.10 B-V reder tahn HD135344. It also is further away than prefeable (for Sun/Beta angle considertions), but at dec= -64 deg passess through the CVZ so aids in scheduling. On the positive side it has been observed previously with STIS and is known single. HIP76371 HR4413 J2000 J2000 B-V = +0.50 STAR M V-IV Spec. ? Color implies likely M star No obvious 3rd light contamination of POSS, DSS, or GSC2 survey plates GSC09246-00862 TYC9246-862-1 J2000 J2000 B-V - +1.08 STAR G III-I Spec type G8III Replacement PSF template for HD59780 Viits 85-88 SAO235221 HIP36287 J2000 J2000 B=7.441, B-V = +0.919 STAR F0-F2 Replacement PSF template star for HD 15745 to use in Visit B7 HIP15356 GSC02848-01101 J2000 STIS/CCD Imaging Yes No WEDGEA0.6 STIS/CCD Imaging Yes No WEDGEA1.0 STIS/CCD Imaging Yes No WEDGEA0.6 STIS/CCD Imaging Yes No WEDGEA1.0 STIS/CCD Imaging Yes No WEDGEA0.6 STIS/CCD Imaging Yes No WEDGEA1.0 STIS/CCD Imaging Yes No WEDGEA0.6 STIS/CCD Imaging Yes No WEDGEA1.0 STIS/CCD Imaging Yes No WEDGEA0.6 STIS/CCD Imaging Yes No WEDGEA1.0 STIS/CCD Imaging Yes No WEDGEA0.6 STIS/CCD Imaging Yes No WEDGEA1.0 STIS/CCD Imaging Yes No WEDGEA0.6 STIS/CCD Imaging Yes No WEDGEA1.0 STIS/CCD Imaging Yes No WEDGEA0.6 STIS/CCD Imaging Yes No WEDGEA1.0 STIS/CCD Imaging Yes No WEDGEA0.6 STIS/CCD Imaging Yes No WEDGEA1.0 STIS/CCD Imaging Yes No WEDGEA0.6 STIS/CCD Imaging Yes No WEDGEA1.0 STIS/CCD Imaging Yes No WEDGEA0.6 STIS/CCD Imaging Yes No WEDGEA1.0 STIS/CCD Imaging Yes No WEDGEA0.6 STIS/CCD Imaging Yes No WEDGEA1.0 STIS/CCD Imaging Yes No WEDGEA0.6 STIS/CCD Imaging Yes No WEDGEA1.0 STIS/CCD Imaging Yes No WEDGEA0.6 STIS/CCD Imaging Yes No WEDGEA1.0 STIS/CCD Imaging Yes No WEDGEA0.6 STIS/CCD Imaging Yes No WEDGEA1.0 STIS/CCD Imaging Yes No WEDGEA0.6 STIS/CCD Imaging Yes No WEDGEA1.0 STIS/CCD Imaging Yes No WEDGEA0.6 STIS/CCD Imaging Yes No WEDGEA1.0 STIS/CCD Imaging Yes No WEDGEA0.6 STIS/CCD Imaging Yes No WEDGEA1.0 STIS/CCD Imaging Yes No WEDGEA0.6 STIS/CCD Imaging Yes No WEDGEA1.0 STIS/CCD Imaging Yes No WEDGEA0.6 STIS/CCD Imaging Yes No WEDGEA1.0 STIS/CCD Imaging Yes No WEDGEA0.6 STIS/CCD Imaging Yes No WEDGEA1.0 STIS/CCD Imaging Yes No WEDGEA0.6 STIS/CCD Imaging Yes No WEDGEA1.0 Timing link suitability includes constraints ([02 After 01 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. HD32297 (V=8.13, B-V = +0.02). First of two sets of visits, each containing three visits of HD32297 at different relative orientations with one PSF calibration observation interleaved. This is the first HD32297 visit in the first set. The four visits within each set must be executed sequentally in contiguous orbits interrupted only for Earth occultation. Orientation: We wish to schedule this visit (01) at -30 deg from Visit 02, with the absolute orientation of Visit 02 unconstrained. To aid in scheduling we allow an Orient from Roll Range of -30 to -20 deg from Visit 02, but if possible we would prefer as close to -30 degrees as possible. Relative Timing: This visit (01) should immediately preceed visit (02). I.e., They should be executed sequentially in "back-to-back" orbits. 1320588508000 267.0 (Tic-Visit :proposal-id 12228 :visit-id "01" :proposal-version -1 :trans-version "20100505" :date "28-Jun-2010 16:49:21.0" :trans-errors '(:WARNINGS 7 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 44928 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "01" :obset-id "01" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "01" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2909 :al-overhead-at-end 0 :internal-dur-at-end 351 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3242 :pcs-gap 0 ) false 1 0 SNR = 100, V = 8.13, sp = A0V, Exptimne rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD 32297 is V = 8.13 so saturation in 68s. So 90% full well in appx 61.2s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD 32297 is V = 8.13 so saturation in 68s. So 90% full well in appx 61.2s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD 32297 is V = 8.13 so saturation in 68s. So 90% full well in appx 60s. For long exposures at WedgeA1.0 go < = 20x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. Timing link suitability includes constraints ([02 After 01 by 0.0 to 0.1 days] [03 After 02 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. HD32297 (V=8.13, B-V = +0.02). First of two sets of visits, each containing three visits of HD32297 at different relative orientations with one PSF calibration observation interleaved. This is the second HD32297 visit in the first set. The four visits within each set must be executed sequentally in contiguous orbits interrupted only for Earth occultation. Orientation: There are no orientation constraints on this visit (02). TVisits 01, 03, 04, 05, and 08 carry relative orientation constraints w.r.t. this visit. Relative Timing: This visit (02) should immediately follow Visit 01 and immediately preceed Visit 03 in back-to-back orbits. 1320594258000 287.0 (Tic-Visit :proposal-id 12228 :visit-id "02" :proposal-version -1 :trans-version "20100505" :date "28-Jun-2010 16:49:23.0" :trans-errors '(:WARNINGS 7 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 44928 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "02" :obset-id "02" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "02" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2909 :al-overhead-at-end 0 :internal-dur-at-end 351 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3242 :pcs-gap 0 ) false 1 0 SNR = 100, V = 8.13, sp = A0V, Exptimne rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD 32297 is V = 8.13 so saturation in 68s. So 90% full well in appx 61.2s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD 32297 is V = 8.13 so saturation in 68s. So 90% full well in appx 61.2s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD 32297 is V = 8.13 so saturation in 68s. So 90% full well in appx 60s. For long exposures at WedgeA1.0 go <= 20x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. Timing link suitability includes constraints ([03 After 02 by 0.0 to 0.1 days] [04 After 03 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. PSF01A (HD33403). PSF calibration target for HD32297. V = 8.31. B-V = +0.01. This is the PSF star calibrator for the flanking visits (01-04). We levy no orientation constraints on this visit (03). However, we choose this target very close in the sky to its paired science target. So as Visits 02 and 03 must be scheduled in sequential contiguous orbits, if scheduled at nominal roll (as we expect also Visit 02 will be) the we expect absolute orientations of Visits 02 and 03 to be very similar (within a few degrees). This is important so we maintain similar Sun and Beta angles for the science target and its PSF calibrator Relative Timing: This visit (03) should immediately follow visit 02 and immediately precede visit 04. I.e., They should be executed sequentially in "back-to-back" orbits. 1320600062000 292.5692809188158 (Tic-Visit :proposal-id 12228 :visit-id "03" :proposal-version -1 :trans-version "20100505" :date "28-Jun-2010 16:49:25.0" :trans-errors '(:WARNINGS 3 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 42496 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "03" :obset-id "03" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "03" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2901 :al-overhead-at-end 0 :internal-dur-at-end 348 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3234 :pcs-gap 0 ) false 1 0 SNR = 100, V = 8.31, sp = B9V, Exptime rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. V = 8.31 so saturation in 80.2s. So 90% full well in appx 72s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD 32297 is V = 8.13 so saturation in 68s. So 90% full well in appx 61.2s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD 32297 is V = 8.13 so saturation in 68s. So 90% full well in appx 60s. For long exposures at WedgeA1.0 go <=20x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. Timing link suitability includes constraints ([04 After 03 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. HD32297 (V=8.13, B-V = +0.02). First of two sets of visits, each containing three visits of HD32297 at different relative orientations with one PSF calibration observation interleaved. This is the third HD32297 visit in the first set. The four visits within each set must be executed sequentally in contiguous orbits interrupted only for Earth occultation. Orientation: We wish to schedule this visit (04) at +30 deg from Visit 02, with the absolute orientation of Visit 02 unconstrained. To aid in scheduling we allow an Orient from Roll Range of +20 to+30 deg from Visit 02 If possible we would prefer as close to +30 degrees as can be scheduled. Relative Timing: This visit (04) should immediately follow Visit 03. I.e., They should be executed sequentially in "back-to-back" orbits. 1320605759000 307.0 (Tic-Visit :proposal-id 12228 :visit-id "04" :proposal-version -1 :trans-version "20100505" :date "28-Jun-2010 16:49:27.0" :trans-errors '(:WARNINGS 7 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 44928 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "04" :obset-id "04" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "04" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2909 :al-overhead-at-end 0 :internal-dur-at-end 351 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3242 :pcs-gap 0 ) false 1 0 SNR = 100, V = 8.13, sp = A0V, Exptimne rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD 32297 is V = 8.13 so saturation in 68s. So 90% full well in appx 61.2s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD 32297 is V = 8.13 so saturation in 68s. So 90% full well in appx 61.2s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD 32297 is V = 8.13 so saturation in 68s. So 90% full well in appx 60s. For long exposures at WedgeA1.0 go <= 20x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. Timing link suitability includes constraints ([06 After 05 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. HD32297 (V=8.13, B-V = +0.02). Second of two sets of visits, each containing three visits of HD32297 at different relative orientations with one PSF calibration observation interleaved. This is the first HD32297 visit in the second set. The four visits within each set must be executed sequentally in contiguous orbits interrupted only for Earth occultation. Relative Orientation: We wish to schedule this visit (05) at EITHER -90 deg OR +90 deg from Visit 01. Either is equally acceptable, but there is no way to specifich this via APT 18.2, so we arbitraily specify an acceptable Orinet From in the positive range (becasuse it worked) of +70 to +110 deg (to aid in schedulability and acceptable to our needs). If guide stars or other scheduling issues arise which APT is not cognizant of that makes these linked visits unschedualable she may freely change the parity of the relative orientation to -110 deg to -70 deg from Visit 01 Schedule in orbit immediately before Visit 06. 1293003981000 10.0 (Tic-Visit :proposal-id 12228 :visit-id "05" :proposal-version -1 :trans-version "20100505" :date "28-Jun-2010 16:49:28.0" :trans-errors '(:WARNINGS 7 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 44928 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "05" :obset-id "05" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "05" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2909 :al-overhead-at-end 0 :internal-dur-at-end 351 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3242 :pcs-gap 0 ) false 1 0 SNR = 100, V = 8.13, sp = A0V, Exptimne rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD 32297 is V = 8.13 so saturation in 68s. So 90% full well in appx 61.2s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD 32297 is V = 8.13 so saturation in 68s. So 90% full well in appx 61.2s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD 32297 is V = 8.13 so saturation in 68s. So 90% full well in appx 60s. For long exposures at WedgeA1.0 go <= 20x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. Timing link suitability includes constraints ([06 After 05 by 0.0 to 0.1 days] [07 After 06 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. HD32297 (V=8.13, B-V = +0.02). Second of two sets of visits, each containing three visits of HD32297 at different relative orientations with one PSF calibration observation interleaved. This is the second HD32297 visit in the second set. The four visits within each set must be executed sequentally in contiguous orbits interrupted only for Earth occultation. Orientation: We wish to schedule this visit (06) at +30 deg from Visit 05. We specify this exactly, and would relax this relative orientation requirment only if a suitable guide stars cannot be found. Relative Timing: This visit (06) should immediately follow visit 05 and immediately precede visit 07. I.e., They should be executed sequentially in "back-to-back" orbits. 1293009731000 40.0 (Tic-Visit :proposal-id 12228 :visit-id "06" :proposal-version -1 :trans-version "20100505" :date "28-Jun-2010 16:49:30.0" :trans-errors '(:WARNINGS 7 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 44928 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "06" :obset-id "06" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "06" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2909 :al-overhead-at-end 0 :internal-dur-at-end 351 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3242 :pcs-gap 0 ) false 1 0 SNR = 100, V = 8.13, sp = A0V, Exptimne rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD 32297 is V = 8.13 so saturation in 68s. So 90% full well in appx 61.2s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD 32297 is V = 8.13 so saturation in 68s. So 90% full well in appx 61.2s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD 32297 is V = 8.13 so saturation in 68s. So 90% full well in appx 60s. For long exposures at WedgeA1.0 go <= 20x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. Timing link suitability includes constraints ([07 After 06 by 0.0 to 0.1 days] [08 After 07 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. PSF01A (HD33403). PSF calibration target for HD32297. V = 8.31. B-V = +0.01. This is the PSF star calibrator for the flanking visits (05-08). We levy no orientation constraints on this visit (07). However, we choose this target very close in the sky to its paired science target. So as Visits 06 and 07 must be scheduled in sequential contiguous orbits, if scheduled at nominal roll (as we expect also Visit 06 will be) the we expect absolute orientations of Visits 06 and 07 to be very similar (within a few degrees). This is important so we maintain similar Sun and Beta angles for the science target and its PSF calibrator Relative Timing: This visit (07) should immediately follow visit 06 and immediately precede visit 08. I.e., They should be executed sequentially in "back-to-back" orbits. 1293015477000 30.2480483181387 (Tic-Visit :proposal-id 12228 :visit-id "07" :proposal-version -1 :trans-version "20100505" :date "28-Jun-2010 16:49:31.0" :trans-errors '(:WARNINGS 3 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 42496 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "07" :obset-id "07" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "07" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2901 :al-overhead-at-end 0 :internal-dur-at-end 348 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3234 :pcs-gap 0 ) false 1 0 SNR = 100, V = 8.31, sp = B9V, Exptime rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. V = 8.31 so saturation in 80.2s. So 90% full well in appx 72s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD 32297 is V = 8.13 so saturation in 68s. So 90% full well in appx 61.2s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD 32297 is V = 8.13 so saturation in 68s. So 90% full well in appx 60s. For long exposures at WedgeA1.0 go <= 20x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. Timing link suitability includes constraints ([08 After 07 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. HD32297 (V=8.13, B-V = +0.02). Second of two sets of visits, each containing three visits of HD32297 at different relative orientations with one PSF calibration observation interleaved. This is the third HD32297 visit in the second set. The four visits within each set must be executed sequentally in contiguous orbits interrupted only for Earth occultation. Orientation: We wish to schedule this visit (08) at +60 deg from Visit 05. We specify this exactly, and would relax this relative orientation requirment only if a suitable guide stars cannot be found. Relative Timing: This visit (08) should immediately follow Visit 07. I.e., They should be executed sequentially in "back-to-back" orbits. 1293021233000 70.0 (Tic-Visit :proposal-id 12228 :visit-id "08" :proposal-version -1 :trans-version "20100505" :date "28-Jun-2010 16:49:33.0" :trans-errors '(:WARNINGS 7 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 44928 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "08" :obset-id "08" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "08" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2909 :al-overhead-at-end 0 :internal-dur-at-end 351 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3242 :pcs-gap 0 ) false 1 0 SNR = 100, V = 8.13, sp = A0V, Exptimne rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD 32297 is V = 8.13 so saturation in 68s. So 90% full well in appx 61.2s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD 32297 is V = 8.13 so saturation in 68s. So 90% full well in appx 61.2s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD 32297 is V = 8.13 so saturation in 68s. So 90% full well in appx 60s. For long exposures at WedgeA1.0 go <= 20x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. Timing link suitability includes constraints ([12 After 11 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. HD181327 (V=7.03, B-V = +0.48). First of two sets of visits, each containing three visits of HD181327 at different relative orientations with one PSF calibration observation interleaved. This is the first HD181327 visit in the first set. The four visits within each set must be executed sequentally in contiguous orbits interrupted only for Earth occultation. Orientation: We wish to schedule this visit (11) at -30 deg from Visit 12, with the absolute orientation of Visit 12 unconstrained. To aid in scheduling we allow an Orient from Roll Range of -30 to -20 deg from Visit 12, but if possible we would prefer as close to -30 degrees as can be scheduled. Relative Timing: This visit (11) should immediately preceed visit (12). I.e., They should be executed sequentially in "back-to-back" orbits. 1305851161000 268.0 (Tic-Visit :proposal-id 12228 :visit-id "11" :proposal-version -1 :trans-version "20100505" :date "28-Jun-2010 16:49:36.0" :trans-errors '(:WARNINGS 4 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 79216 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "11" :obset-id "11" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "11" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3112 :al-overhead-at-end 0 :internal-dur-at-end 387 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3445 :pcs-gap 0 ) false 1 0 SNR = 100, V = 7.03, sp = F6V, Exptime rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD181327 (F6V) is V = 7.03 so saturation in 24.4s. So 90% full well in appx 21.9s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD181327 (F6V) is V = 7.03 so saturation in 24.4s. So 90% full well in appx 21.9s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD181327 (F6V) is V = 7.03 so saturation in 24.4s. So 90% full well in appx 21.9s. Use this for the "short" exposures, repeated (2x) with CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD181327 (F6V) is V = 7.03 so saturation in 24.4s. For long exposures at WedgeA1.0 go <=20x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. Timing link suitability includes constraints ([12 After 11 by 0.0 to 0.1 days] [13 After 12 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. HD181327 (V=7.03, B-V = +0.48). First of two sets of visits, each containing three visits of HD181327 at different relative orientations with one PSF calibration observation interleaved. This is the second HD181327 visit in the first set. The four visits within each set must be executed sequentally in contiguous orbits interrupted only for Earth occultation. Orientation: There are no orientation constraints on this visit (12). Visits 11, 13, 14, 15, and 18 carry relative orientation constraints w.r.t. this visit. Relative Timing: This visit (12) should immediately follow Visit 11 and immediately preceed Visit 13 in back-to-back orbits. 1305859654000 288.0 (Tic-Visit :proposal-id 12228 :visit-id "12" :proposal-version -1 :trans-version "20100505" :date "28-Jun-2010 16:49:38.0" :trans-errors '(:WARNINGS 4 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 79216 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "12" :obset-id "12" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "12" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3112 :al-overhead-at-end 0 :internal-dur-at-end 387 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3445 :pcs-gap 0 ) false 1 0 SNR = 100, V = 7.03, sp = F6V, Exptime rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD181327 (F6V) is V = 7.03 so saturation in 24.4s. So 90% full well in appx 21.9s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD181327 (F6V) is V = 7.03 so saturation in 24.4s. So 90% full well in appx 21.9s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD181327 (F6V) is V = 7.03 so saturation in 24.4s. So 90% full well in appx 21.9s. Use this for the "short" exposures, repeated (2x) with CR Split. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD181327 (F6V) is V = 7.03 so saturation in 24.4s. For long exposures at WedgeA1.0 go <= 20x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. Timing link suitability includes constraints ([13 After 12 by 0.0 to 0.1 days] [14 After 13 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. PSF02A (HD180134). PSF calibration target for HD180134. V = 6.372. B-V = +0.45. This is the PSF star calibrator for the flanking visits (11-14). We levy no orientation constraints on this visit (13). However, we choose this target very close in the sky to its paired science target. So as Visits 12 and 13 must be scheduled in sequential contiguous orbits, if scheduled at nominal roll (as we expect also Visit 12 will be) the we expect absolute orientations of Visits 12 and 13 to be very similar (within a few degrees). This is important so we maintain similar Sun and Beta angles for the science target and its PSF calibrator Relative Timing: This visit (13) should immediately follow visit 12 and immediately precede visit 14. I.e., They should be executed sequentially in "back-to-back" orbits. 1305865410000 288.480722653315 (Tic-Visit :proposal-id 12228 :visit-id "13" :proposal-version -1 :trans-version "20100505" :date "28-Jun-2010 16:49:41.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 119088 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "13" :obset-id "13" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "13" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3112 :al-overhead-at-end 0 :internal-dur-at-end 430 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3445 :pcs-gap 0 ) false 1 0 SNR = 100, V = 6.372, sp = F7V, Exptime rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. V = 6.372 so saturation in 13.2s. So 90% full well in appx 11.9s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. V = 6.372 so saturation in 13.2s. So 90% full well in appx 11.9s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. V = 6.372 so saturation in 13.2s. So 90% full well in appx 11.9s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD 32297 is V = 8.13 so saturation in 68s. So 90% full well in appx 60s. For long exposures at WedgeA1.0 go <= 20x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. Timing link suitability includes constraints ([14 After 13 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. HD181327 (V=7.03, B-V = +0.48). First of two sets of visits, each containing three visits of HD181327 at different relative orientations with one PSF calibration observation interleaved. This is the third Hhd181327 visit in the first set. The four visits within each set must be executed sequentally in contiguous orbits interrupted only for Earth occultation. Orientation: We wish to schedule this visit (14) at +30 deg from Visit 12, with the absolute orientation of Visit 12 unconstrained. To aid in scheduling we allow an Orient from Roll Range of +20 to+30 deg from Visit 1, but if possible we would prefer as close to +30 degrees as can be scheduled. Relative Timing: This visit (14) should immediately follow Visit 13. I.e., They should be executed sequentially in "back-to-back" orbits 1305871953000 308.0 (Tic-Visit :proposal-id 12228 :visit-id "14" :proposal-version -1 :trans-version "20100505" :date "28-Jun-2010 16:49:43.0" :trans-errors '(:WARNINGS 4 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 79216 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "14" :obset-id "14" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "14" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3112 :al-overhead-at-end 0 :internal-dur-at-end 387 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3445 :pcs-gap 0 ) false 1 0 SNR = 100, V = 7.03, sp = F6V, Exptime rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD181327 (F6V) is V = 7.03 so saturation in 24.4s. So 90% full well in appx 21.9s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD181327 (F6V) is V = 7.03 so saturation in 24.4s. So 90% full well in appx 21.9s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD181327 (F6V) is V = 7.03 so saturation in 24.4s. So 90% full well in appx 21.9s. Use this for the "short" exposures, repeated (2x) with CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD181327 (F6V) is V = 7.03 so saturation in 24.4s. For long exposures at WedgeA1.0 go <=20x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. Timing link suitability includes constraints ([16 After 15 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. HD181327 (V=7.03, B-V = +0.48). Second of two sets of visits, each containing three visits of HD181327 at different relative orientations with one PSF calibration observation interleaved. This is the first HD181327 visit in the second set. The four visits within each set must be executed sequentally in contiguous orbits interrupted only for Earth occultation. Relative Orientation: We wish to schedule this visit (15) at EITHER -90 deg OR +90 deg from Visit 11. Either is equally acceptable, but there is no way to specifich this via APT 18.2, so we arbitraily specify an acceptable Orient From in the positive range (because it worked) of +70 to +110 deg (to aid in schedulability and acceptable to our needs). If guide stars or other scheduling issues arise which APT is not cognizant of that makes these linked visits unschedualable she may freely change the parity of the relative orientation to -110 deg to -70 deg from Visit 11 Relative Timing: Schedule in orbit immediately before Visit 16. 1310270108000 338.0 (Tic-Visit :proposal-id 12228 :visit-id "15" :proposal-version -1 :trans-version "20100505" :date "28-Jun-2010 16:49:46.0" :trans-errors '(:WARNINGS 4 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 79216 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "15" :obset-id "15" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "15" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3112 :al-overhead-at-end 0 :internal-dur-at-end 387 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3445 :pcs-gap 0 ) false 1 0 SNR = 100, V = 7.03, sp = F6V, Exptime rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD181327 (F6V) is V = 7.03 so saturation in 24.4s. So 90% full well in appx 21.9s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD181327 (F6V) is V = 7.03 so saturation in 24.4s. So 90% full well in appx 21.9s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD181327 (F6V) is V = 7.03 so saturation in 24.4s. So 90% full well in appx 21.9s. Use this for the "short" exposures, repeated (2x) with CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD181327 (F6V) is V = 7.03 so saturation in 24.4s. For long exposures at WedgeA1.0 go <=20x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. Timing link suitability includes constraints ([16 After 15 by 0.0 to 0.1 days] [17 After 16 by 0.5 to 1.5 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. HD181327 (V=7.03, B-V = +0.48). Second of two sets of visits, each containing three visits of HD181327 at different relative orientations with one PSF calibration observation interleaved. This is the second HD181327 visit in the first set. The four visits within each set must be executed sequentally in contiguous orbits interrupted only for Earth occultation. Orientation: We wish to schedule this visit (16) at +30 deg from Visit 15. We specify this exactly, and would relax this relative orientation requirment only if a suitable guide stars cannot be found. Relative Timing: This visit (16) should immediately follow visit 15 and immediately precede visit 17. I.e., They should be executed sequentially in "back-to-back" orbits. 1310275859000 358.5 (Tic-Visit :proposal-id 12228 :visit-id "16" :proposal-version -1 :trans-version "20100505" :date "28-Jun-2010 16:49:48.0" :trans-errors '(:WARNINGS 4 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 79216 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "16" :obset-id "16" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "16" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3112 :al-overhead-at-end 0 :internal-dur-at-end 387 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3445 :pcs-gap 0 ) false 1 0 SNR = 100, V = 7.03, sp = F6V, Exptime rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD181327 (F6V) is V = 7.03 so saturation in 24.4s. So 90% full well in appx 21.9s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD181327 (F6V) is V = 7.03 so saturation in 24.4s. So 90% full well in appx 21.9s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD181327 (F6V) is V = 7.03 so saturation in 24.4s. So 90% full well in appx 21.9s. Use this for the "short" exposures, repeated (2x) with CR Split. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD181327 (F6V) is V = 7.03 so saturation in 24.4s. For long exposures at WedgeA1.0 go <= 20x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. Timing link suitability includes constraints ([17 After 16 by 0.5 to 1.5 days] [18 After 17 by 0.5 to 1.5 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. PSF02A (HD180134). PSF calibration target for HD180134. V = 6.372. B-V = +0.45. This is the PSF star calibrator for the flanking visits (15-18). We levy no orientation constraints on this visit (17). However, we choose this target very close in the sky to its paired science target. So as Visits 16 and 17 must be scheduled in sequential contiguous orbits, if scheduled at nominal roll (as we expect also Visit 16 will be) then we expect absolute orientations of Visits 16 and 17 to be very similar (within a few degrees). This is important so we maintain similar Sun and Beta angles for the science target and its PSF calibrator Relative Timing: This visit (17) should immediately follow visit 16 and immediately precede visit 18. I.e., They should be executed sequentially in "back-to-back" orbits. 1310281652000 359.1755324182102 (Tic-Visit :proposal-id 12228 :visit-id "17" :proposal-version -1 :trans-version "20100505" :date "28-Jun-2010 16:49:51.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 119088 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "17" :obset-id "17" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "17" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3112 :al-overhead-at-end 0 :internal-dur-at-end 430 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3445 :pcs-gap 0 ) false 1 0 SNR = 100, V = 6.372, sp = F7V, Exptime rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. V = 6.372 so saturation in 13.2s. So 90% full well in appx 11.9s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. V = 6.372 so saturation in 13.2s. So 90% full well in appx 11.9s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. V = 6.372 so saturation in 13.2s. So 90% full well in appx 11.9s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD 32297 is V = 8.13 so saturation in 68s. So 90% full well in appx 60s. For long exposures at WedgeA1.0 go <= 20x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. Timing link suitability includes constraints ([18 After 17 by 0.5 to 1.5 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. HD181327 (V=7.03, B-V = +0.48). Second of two sets of visits, each containing three visits of HD181327 at different relative orientations with one PSF calibration observation interleaved. This is the third HD181327 visit in the first set. The four visits within each set must be executed sequentally in contiguous orbits interrupted only for Earth occultation. Orientation: We wish to schedule this visit (18) at +60 deg from Visit 15, with the absolute orientation of Visit 15 linked to visit 11. To aid in scheduling we allow an Orient from Roll Range of +45 to+60 deg from Visit 1, but if possible we would prefer as close to +60 degrees as can be scheduled. Relative Timing: This visit (17) should immediately follow Visit 16. I.e., They should be executed sequentially in "back-to-back" orbits. 1310287359000 19.0 (Tic-Visit :proposal-id 12228 :visit-id "18" :proposal-version -1 :trans-version "20100505" :date "28-Jun-2010 16:49:54.0" :trans-errors '(:WARNINGS 4 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 79216 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "18" :obset-id "18" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "18" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3112 :al-overhead-at-end 0 :internal-dur-at-end 387 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3445 :pcs-gap 0 ) false 1 0 SNR = 100, V = 7.03, sp = F6V, Exptime rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD181327 (F6V) is V = 7.03 so saturation in 24.4s. So 90% full well in appx 21.9s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD181327 (F6V) is V = 7.03 so saturation in 24.4s. So 90% full well in appx 21.9s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD181327 (F6V) is V = 7.03 so saturation in 24.4s. So 90% full well in appx 21.9s. Use this for the "short" exposures, repeated (2x) with CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD181327 (F6V) is V = 7.03 so saturation in 24.4s. For long exposures at WedgeA1.0 go <=20x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. Timing link suitability includes constraints ([22 After 21 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. HD 107146 (V=7.07, B-V = +0.62). First of two sets of visits, each containing three visits of HD107146 at different relative orientations with one PSF calibration observation interleaved. This is the first HD107146 visit in the first set. The four visits within each set must be executed sequentally in contiguous orbits interrupted only for Earth occultation. Orientation: We wish to schedule this visit (21) at -30 deg from Visit 22, with the absolute orientation of Visit 22 unconstrained. To aid in scheduling we allow an Orient from Roll Range of -30 to -15 deg from Visit 22, but if possible we would prefer as close to -30 degrees as possible. Relative Timing: This visit (21) should immediately preceed visit (22). I.e., They should be executed sequentially in "back-to-back" orbits. 1304415516000 112.0 (Tic-Visit :proposal-id 12228 :visit-id "21" :proposal-version -1 :trans-version "20100505" :date "28-Jun-2010 16:49:56.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 69488 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "21" :obset-id "21" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "21" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2916 :al-overhead-at-end 0 :internal-dur-at-end 377 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3249 :pcs-gap 0 ) false 1 0 SNR = 100, V = 7.07, sp = G2V, Exptime rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD 107146 (F2V) is V = 7.07 so saturation in 24.7s. So 90% full well in appx 22.2s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD 107146 (F2V) is V = 7.07 so saturation in 24.7s. So 90% full well in appx 22.2s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD 107146 (F2V) is V = 7.07 so saturation in 24.7s. For long exposures at WedgeA1.0 go <=20x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. Timing link suitability includes constraints ([22 After 21 by 0.0 to 0.1 days] [23 After 22 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. HD 107146 (V=7.07, B-V = +0.62). First of two sets of visits, each containing three visits of HD107146 at different relative orientations with one PSF calibration observation interleaved. This is the second HD107146 visit in the first set. The four visits within each set must be executed sequentally in contiguous orbits interrupted only for Earth occultation. Orientation: There are no orientation constraints on this visit (22). Visits 21, 23, 24, 25, and 28 carry relative orientation constraints w.r.t. this visit. Relative Timing: This visit (22) should immediately follow Visit 21 and immediately preceed Visit 23 in back-to-back orbits. 1304421267000 127.0 (Tic-Visit :proposal-id 12228 :visit-id "22" :proposal-version -1 :trans-version "20100505" :date "28-Jun-2010 16:49:58.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 69488 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "22" :obset-id "22" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "22" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2916 :al-overhead-at-end 0 :internal-dur-at-end 377 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3249 :pcs-gap 0 ) false 1 0 SNR = 100, V = 7.07, sp = G2V, Exptime rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD181327 (F6V) is V = 7.03 so saturation in 24.4s. So 90% full well in appx 21.9s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD181327 (F6V) is V = 7.03 so saturation in 24.4s. So 90% full well in appx 21.9s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD181327 (F6V) is V = 7.03 so saturation in 24.4s. For long exposures at WedgeA1.0 go <= 20x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. Timing link suitability includes constraints ([23 After 22 by 0.0 to 0.1 days] [24 After 23 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. PSF03A (HD115617). PSF calibration target for HD107146. V = 4.74. B-V = +0.71. This is the PSF star calibrator for the flanking visits (21-24). We levy no orientation constraints on this visit (23). However, we choose this target very close in the sky to its paired science target. So as Visits 22 and 23 must be scheduled in sequential contiguous orbits, if scheduled at nominal roll (as we expect also Visit 22 will be) the we expect absolute orientations of Visits 22 and 23 to be somewhat similar. This is important so we maintain similar Sun and Beta angles for the science target and its PSF calibrator Relative Timing: This visit (23) should immediately follow visit 22 and immediately precede visit 24. I.e., They should be executed sequentially in "back-to-back" orbits. 1304427497000 130.922000651296 (Tic-Visit :proposal-id 12228 :visit-id "23" :proposal-version -1 :trans-version "20100505" :date "28-Jun-2010 16:50:02.0" :trans-errors '(:WARNINGS 7 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 111552 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "23" :obset-id "23" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "23" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2894 :al-overhead-at-end 0 :internal-dur-at-end 422 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3242 :pcs-gap 0 ) false 1 0 SNR = 100, V = 6.30, sp = G0V, Exptime rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. V = 6.30 so saturation in 12.2s. So 90% full well in appx 11.0s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. V = 6.30 so saturation in 12.2s. So 90% full well in appx 11.0s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. V = 6.30 so saturation in 12.2s. So 90% full well in appx 11.0s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. V = 6.30 so saturation in 12.2s. So 90% full well in appx 11.0s. For long exposures at WedgeA1.0 go <= 20x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. Timing link suitability includes constraints ([24 After 23 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. HD 107146 (V=7.07, B-V = +0.62). First of two sets of visits, each containing three visits of HD107146 at different relative orientations with one PSF calibration observation interleaved. This is the third HD107146 visit in the first set. The four visits within each set must be executed sequentally in contiguous orbits interrupted only for Earth occultation. Orientation: We wish to schedule this visit (24) at +30 deg from Visit 22, with the absolute orientation of Visit 22 unconstrained. To aid in scheduling we allow an Orient from Roll Range of +15 to +30 deg from Visit 22, but if possible we would prefer as close to +30 degrees as can be scheduled. Relative Timing: This visit (24) should immediately follow Visit 23. I.e., They should be executed sequentially in "back-to-back" orbits 1304434798000 142.0 (Tic-Visit :proposal-id 12228 :visit-id "24" :proposal-version -1 :trans-version "20100505" :date "28-Jun-2010 16:50:04.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 69488 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "24" :obset-id "24" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "24" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2900 :al-overhead-at-end 0 :internal-dur-at-end 377 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3249 :pcs-gap 0 ) false 1 0 SNR = 100, V = 7.07, sp = G2V, Exptime rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD181327 (F6V) is V = 7.03 so saturation in 24.4s. So 90% full well in appx 21.9s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD181327 (F6V) is V = 7.03 so saturation in 24.4s. So 90% full well in appx 21.9s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD181327 (F6V) is V = 7.03 so saturation in 24.4s. For long exposures at WedgeA1.0 go <=20x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. Timing link suitability includes constraints ([26 After 25 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. HD 107146 (V=7.07, B-V = +0.62). Second of two sets of visits, each containing three visits of HD181327 at different relative orientations with one PSF calibration observation interleaved. This is the first HD107146 visit in the second set. The four visits within each set must be executed sequentally in contiguous orbits interrupted only for Earth occultation. Relative Orientation: We wish to schedule this visit (25) at EITHER -90 deg OR +90 deg from Visit 21. Either is equally acceptable, but there is no way to specifich this via APT 18.2, so we arbitraily specify an acceptable Orient From in the positive range. Here we cannot get the optimum (|90| deg) differentail and we specify +125 to +130 to force scheddualibility. If guide stars or other scheduling issues arise which APT is not cognizant of that makes these linked visits unschedualable the parity of the relative orientation to -120 deg to -130 deg from Visit 22 (or more optimum negative offsets) may be used as an alternate. Relative Timing: Schedule in orbit immediately before Visit 26. 1298394394000 237.0 (Tic-Visit :proposal-id 12228 :visit-id "25" :proposal-version -1 :trans-version "20100505" :date "28-Jun-2010 16:50:06.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 69488 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "25" :obset-id "25" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "25" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2916 :al-overhead-at-end 0 :internal-dur-at-end 377 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3249 :pcs-gap 0 ) false 1 0 SNR = 100, V = 7.07, sp =G2V, Exptime rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD181327 (F6V) is V = 7.03 so saturation in 24.4s. So 90% full well in appx 21.9s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD181327 (F6V) is V = 7.03 so saturation in 24.4s. So 90% full well in appx 21.9s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD181327 (F6V) is V = 7.03 so saturation in 24.4s. For long exposures at WedgeA1.0 go <=20x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. Timing link suitability includes constraints ([26 After 25 by 0.0 to 0.1 days] [27 After 26 by 0.5 to 1.5 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. HD 107146 (V=7.07, B-V = +0.62). Second of two sets of visits, each containing three visits of HD107146 at different relative orientations with one PSF calibration observation interleaved. This is the second HD107146 visit in the first set. The four visits within each set must be executed sequentally in contiguous orbits interrupted only for Earth occultation. Orientation: We wish to schedule this visit (26) at +30 deg from Visit 25, but the schedualable roll range is apparenly more limited. Here we specify exactly +17.t to +17.5 deg for enable schedualbility for all linked viits still within an accepatbel minimum orienentation offset for this visit. Relative Timing: This visit (26) should immediately follow visit 25 and immediately precede visit 27. I.e., They should be executed sequentially in "back-to-back" orbits. 1298400145000 254.5 (Tic-Visit :proposal-id 12228 :visit-id "26" :proposal-version -1 :trans-version "20100505" :date "28-Jun-2010 16:50:08.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 69488 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "26" :obset-id "26" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "26" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2916 :al-overhead-at-end 0 :internal-dur-at-end 377 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3249 :pcs-gap 0 ) false 1 0 SNR = 100, V = 7.07, sp = G2V, Exptime rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD181327 (F6V) is V = 7.03 so saturation in 24.4s. So 90% full well in appx 21.9s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD181327 (F6V) is V = 7.03 so saturation in 24.4s. So 90% full well in appx 21.9s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD181327 (F6V) is V = 7.03 so saturation in 24.4s. For long exposures at WedgeA1.0 go <= 20x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. Timing link suitability includes constraints ([27 After 26 by 0.5 to 1.5 days] [28 After 27 by 0.5 to 1.5 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. PSF02A (HD180134). PSF calibration target for HD107146. V = 6.372. B-V = +0.45. This is the PSF star calibrator for the flanking visits (25-28). We levy no orientation constraints on this visit (27). However, we choose this target very close in the sky to its paired science target. So as Visits 26 and 27 must be scheduled in sequential contiguous orbits, if scheduled at nominal roll (as we expect also Visit 26 will be) then we expect absolute orientations of Visits 26 and 27 to be very similar (within a few degrees). This is important so we maintain similar Sun and Beta angles for the science target and its PSF calibrator Relative Timing: This visit (27) should immediately follow visit 26 and immediately precede visit 28. I.e., They should be executed sequentially in "back-to-back" orbits. 1298406275000 277.9817253453034 (Tic-Visit :proposal-id 12228 :visit-id "27" :proposal-version -1 :trans-version "20100505" :date "28-Jun-2010 16:50:11.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 111552 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "27" :obset-id "27" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "27" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2866 :al-overhead-at-end 0 :internal-dur-at-end 422 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3242 :pcs-gap 0 ) false 1 0 SNR = 100, V = 6.30, sp = G0V, Exptime rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. V = 6.30 so saturation in 12.2s. So 90% full well in appx 11.0s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. V = 6.30 so saturation in 12.2s. So 90% full well in appx 11.0s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. V = 6.30 so saturation in 12.2s. So 90% full well in appx 11.0s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. V = 6.30 so saturation in 12.2s. So 90% full well in appx 11.0s. For long exposures at WedgeA1.0 go <= 20x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. Timing link suitability includes constraints ([28 After 27 by 0.5 to 1.5 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. HD 107146 (V=7.07, B-V = +0.62). Second of two sets of visits, each containing three visits of HD107146 at different relative orientations with one PSF calibration observation interleaved. This is the third HD107146 visit in the first set. The four visits within each set must be executed sequentally in contiguous orbits interrupted only for Earth occultation. Orientation: We wish to schedule this visit (28) at +60 deg from Visit 25, with the absolute orientation of Visit 25 linked to visit 21. To aid in scheduling we allow an Orient from Roll Range of +17.t to +17.5 deg for enable schedualbility for all linked viits still within an accepatbel minimum orienentation offset for this visit. Relative Timing: This visit (27) should immediately follow Visit 26. I.e., They should be executed sequentially in "back-to-back" orbits. 1298411645000 272.0 (Tic-Visit :proposal-id 12228 :visit-id "28" :proposal-version -1 :trans-version "20100505" :date "28-Jun-2010 16:50:13.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 69488 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "28" :obset-id "28" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "28" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2916 :al-overhead-at-end 0 :internal-dur-at-end 377 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3249 :pcs-gap 0 ) false 1 0 SNR = 100, V = 7.07, sp = G2V, Exptime rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD181327 (F6V) is V = 7.03 so saturation in 24.4s. So 90% full well in appx 21.9s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD181327 (F6V) is V = 7.03 so saturation in 24.4s. So 90% full well in appx 21.9s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD181327 (F6V) is V = 7.03 so saturation in 24.4s. For long exposures at WedgeA1.0 go <=20x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. Timing link suitability includes constraints ([32 After 31 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. AU MIC (V=8.61, B-V = + 1.45). First of two sets of visits, each containing three visits of AU MIC at different relative orientations with one PSF calibration observation interleaved. This is the first AU MIC visit in the first set. The four visits within each set must be executed sequentally in contiguous orbits interrupted only for Earth occultation. Orientation: We wish to schedule this visit (31) at -30 deg from Visit 32, with the absolute orientation of Visit 32 unconstrained. Relative Timing: This visit (31) should immediately preceed visit (32). I.e., They should be executed sequentially in "back-to-back" orbits. 1310852457000 273.0 (Tic-Visit :proposal-id 12228 :visit-id "31" :proposal-version -1 :trans-version "20100505" :date "28-Jun-2010 16:50:15.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 52224 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "31" :obset-id "31" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "31" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2940 :al-overhead-at-end 0 :internal-dur-at-end 358 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3275 :pcs-gap 0 ) false 1 0 SNR = 100, V = 8.61, sp = M1Ve, Exptime rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. AU MIC is V = 8.61 so saturation in 50.6s. So 90% full well in appx 45.5s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. AU MIC is V = 8.61 so saturation in 50.6s. So 90% full well in appx 45.5s. Use this for the "short" exposures, repeated with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. AU MIC is V = 8.61 so saturation in 50.6s. So 90% full well in appx 45.5s. For long exposures at WedgeA1.0 go > 10x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. Timing link suitability includes constraints ([32 After 31 by 0.0 to 0.1 days] [33 After 32 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. AU MIC (V=8.61, B-V = + 1.45). First of two sets of visits, each containing three visits of AU MIC at different relative orientations with one PSF calibration observation interleaved. This is the second AU MIC visit in the first set. The four visits within each set must be executed sequentally in contiguous orbits interrupted only for Earth occultation. Orientation: There are no orientation constraints on this visit (32). Visits 31, 33, 34, 35, and 38 carry relative orientation constraints w.r.t. this visit. Relative Timing: This visit (32) should immediately follow Visit 31 and immediately preceed Visit 33 in back-to-back orbits. 1310858210000 302.0 (Tic-Visit :proposal-id 12228 :visit-id "32" :proposal-version -1 :trans-version "20100505" :date "28-Jun-2010 16:50:17.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 52224 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "32" :obset-id "32" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "32" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2940 :al-overhead-at-end 0 :internal-dur-at-end 358 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3275 :pcs-gap 0 ) false 1 0 SNR = 100, V = 8.61, sp = M1Ve, Exptime rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. AU MIC is V = 8.61 so saturation in 50.6s. So 90% full well in appx 45.5s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. AU MIC is V = 8.61 so saturation in 50.6s. So 90% full well in appx 45.5s. Use this for the "short" exposures, repeated with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. AU MIC is V = 8.61 so saturation in 50.6s. So 90% full well in appx 45.5s. For long exposures at WedgeA1.0 go > 10x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. Timing link suitability includes constraints ([33 After 32 by 0.0 to 0.1 days] [34 After 33 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. PSF04A (HD191849). PSF calibration target for AU MIC. V = 7.97. B-V = +1.46. This is the PSF star calibrator for the flanking visits (31-34). We levy no orientation constraints on this visit (43). However, we choose this target very close in the sky to its paired science target. So as Visits 32 and 33 must be scheduled in sequential contiguous orbits, if scheduled at nominal roll (as we expect also Visit 32 will be) the we expect absolute orientations of Visits 32 and 33 to be very similar (within a few degrees). This is important so we maintain similar Sun and Beta angles for the science target and its PSF calibrator Relative Timing: This visit (33) should immediately follow visit 32 and immediately precede visit 34. I.e., They should be executed sequentially in "back-to-back" orbits. 1310864042000 342.9365350660603 (Tic-Visit :proposal-id 12228 :visit-id "33" :proposal-version -1 :trans-version "20100505" :date "28-Jun-2010 16:50:19.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 61952 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "33" :obset-id "33" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "33" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3056 :al-overhead-at-end 0 :internal-dur-at-end 369 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3391 :pcs-gap 0 ) false 1 0 SNR = 100, V = 7.97, sp = M0Ve, Exptime rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. V = 7.97 so saturation in 34.0s. So 90% full well in appx 30.6s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. V = 7.97 so saturation in 34.0s. So 90% full well in appx 30.6s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. V = 6.26 so saturation in 12.1s. So 90% full well in appx 10.9s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. For long exposures at WedgeA1.0 go <=20x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. Timing link suitability includes constraints ([34 After 33 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. AU MIC (V=8.61, B-V = + 1.45). First of two sets of visits, each containing three visits of AU MIC at different relative orientations with one PSF calibration observation interleaved. This is the third AU MIC visit in the first set. The four visits within each set must be executed sequentally in contiguous orbits interrupted only for Earth occultation. Orientation: We wish to schedule this visit (34) at +30 deg from Visit 32, with the absolute orientation of Visit 32 unconstrained. Relative Timing: This visit (34) should immediately follow Visit 33. I.e., They should be executed sequentially in "back-to-back" orbits. 1310869716000 332.0 (Tic-Visit :proposal-id 12228 :visit-id "34" :proposal-version -1 :trans-version "20100505" :date "28-Jun-2010 16:50:21.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 52224 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "34" :obset-id "34" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "34" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2940 :al-overhead-at-end 0 :internal-dur-at-end 358 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3275 :pcs-gap 0 ) false 1 0 SNR = 100, V = 8.61, sp = M1Ve, Exptime rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. AU MIC is V = 8.61 so saturation in 50.6s. So 90% full well in appx 45.5s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. AU MIC is V = 8.61 so saturation in 50.6s. So 90% full well in appx 45.5s. Use this for the "short" exposures, repeated with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. AU MIC is V = 8.61 so saturation in 50.6s. So 90% full well in appx 45.5s. For long exposures at WedgeA1.0 go > 10x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. Timing link suitability includes constraints ([36 After 35 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. AU MIC (V=8.61, B-V = + 1.45). Second of two sets of visits, each containing three visits of HD15115 at different relative orientations with one PSF calibration observation interleaved. This is the first HD15115 visit in the second set. The four visits within each set must be executed sequentally in contiguous orbits interrupted only for Earth occultation. Relative Orientation: We wish to schedule this visit (35) at EITHER -90 deg OR +90 deg from Visit 31. Either is equally acceptable, but there is no way to specifich this via APT 18.2, so we arbitraily specify an acceptable Orinet From in the positive range (becasuse it worked) of +70 to +110 deg (to aid in schedulability and acceptable to our needs). If guide stars or other scheduling issues arise which APT is not cognizant of that makes these linked visits unschedualable she may freely change the parity of the relative orientation to -110 deg to -70 deg from Visit 31 Schedule in orbit immediately before Visit 36. 1281320133000 356.0 (Tic-Visit :proposal-id 12228 :visit-id "35" :proposal-version -1 :trans-version "20100505" :date "28-Jun-2010 16:50:23.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 52224 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "35" :obset-id "35" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "35" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2940 :al-overhead-at-end 0 :internal-dur-at-end 358 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3275 :pcs-gap 0 ) false 1 0 SNR = 100, V = 8.61, sp = M1Ve, Exptime rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. AU MIC is V = 8.61 so saturation in 50.6s. So 90% full well in appx 45.5s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. AU MIC is V = 8.61 so saturation in 50.6s. So 90% full well in appx 45.5s. Use this for the "short" exposures, repeated with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. AU MIC is V = 8.61 so saturation in 50.6s. So 90% full well in appx 45.5s. For long exposures at WedgeA1.0 go > 10x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. Timing link suitability includes constraints ([36 After 35 by 0.0 to 0.1 days] [37 After 36 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. AU MIC (V=8.61, B-V = + 1.45). Second of two sets of visits, each containing three visits of AU MIC at different relative orientations with one PSF calibration observation interleaved. This is the second AU MIC visit in the second set. The four visits within each set must be executed sequentally in contiguous orbits interrupted only for Earth occultation. Orientation: We wish to schedule this visit (36) at +30 deg from Visit 35. We specify this exactly, and would relax this relative orientation requirment only if a suitable guide stars cannot be found. Relative Timing: This visit (36) should immediately follow visit 35 and immediately precede visit 37. I.e., They should be executed sequentially in "back-to-back" orbits. 1281325886000 26.0 (Tic-Visit :proposal-id 12228 :visit-id "36" :proposal-version -1 :trans-version "20100505" :date "28-Jun-2010 16:50:25.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 52224 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "36" :obset-id "36" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "36" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2940 :al-overhead-at-end 0 :internal-dur-at-end 358 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3275 :pcs-gap 0 ) false 1 0 SNR = 100, V = 8.61, sp = M1Ve, Exptime rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. AU MIC is V = 8.61 so saturation in 50.6s. So 90% full well in appx 45.5s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. AU MIC is V = 8.61 so saturation in 50.6s. So 90% full well in appx 45.5s. Use this for the "short" exposures, repeated with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. AU MIC is V = 8.61 so saturation in 50.6s. So 90% full well in appx 45.5s. For long exposures at WedgeA1.0 go > 10x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. Timing link suitability includes constraints ([37 After 36 by 0.0 to 0.1 days] [38 After 37 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. PSF04A (HD191849). PSF calibration target for AU MIC. V = 7.97. B-V = +1.46. This is the PSF star calibrator for the flanking visits (35-38). We levy no orientation constraints on this visit (37). However, we choose this target very close in the sky to its paired science target. So as Visits 36 and 37 must be scheduled in sequential contiguous orbits, if scheduled at nominal roll (as we expect also Visit 36 will be) the we expect absolute orientations of Visits 36 and 37 to be very similar (within a few degrees). This is important so we maintain similar Sun and Beta angles for the science target and its PSF calibrator Relative Timing: This visit (37) should immediately follow visit 36 and immediately precede visit 38. I.e., They should be executed sequentially in "back-to-back" orbits. 1281331189000 28.875989332710787 (Tic-Visit :proposal-id 12228 :visit-id "37" :proposal-version -1 :trans-version "20100505" :date "28-Jun-2010 16:50:26.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 61952 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "37" :obset-id "37" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "37" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3056 :al-overhead-at-end 0 :internal-dur-at-end 369 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3391 :pcs-gap 0 ) false 1 0 SNR = 100, V = 7.97, sp = M0Ve, Exptime rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. V = 7.97 so saturation in 34.0s. So 90% full well in appx 30.6s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. V = 7.97 so saturation in 34.0s. So 90% full well in appx 30.6s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. V = 6.26 so saturation in 12.1s. So 90% full well in appx 10.9s. For long exposures at WedgeA1.0 go < = 20x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. Timing link suitability includes constraints ([38 After 37 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. AU MIC (V=8.61, B-V = + 1.45). Second of two sets of visits, each containing three visits of AU MIC at different relative orientations with one PSF calibration observation interleaved. This is the third AU MIC visit in the second set. The four visits within each set must be executed sequentally in contiguous orbits interrupted only for Earth occultation. Orientation: We wish to schedule this visit (38) at +60 deg from Visit 35. We specify this exactly, and would relax this relative orientation requirment only if a suitable guide stars cannot be found. Relative Timing: This visit (38) should immediately follow Visit 37. I.e., They should be executed sequentially in "back-to-back" orbits. 1281337391000 55.0 (Tic-Visit :proposal-id 12228 :visit-id "38" :proposal-version -1 :trans-version "20100505" :date "28-Jun-2010 16:50:28.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 52224 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "38" :obset-id "38" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "38" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2940 :al-overhead-at-end 0 :internal-dur-at-end 358 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3275 :pcs-gap 0 ) false 1 0 SNR = 100, V = 6.80, sp = F2, Exptimne rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. AU MIC is V = 8.61 so saturation in 50.6s. So 90% full well in appx 45.5s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. AU MIC is V = 8.61 so saturation in 50.6s. So 90% full well in appx 45.5s. Use this for the "short" exposures, repeated with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. AU MIC is V = 8.61 so saturation in 50.6s. So 90% full well in appx 45.5s. For long exposures at WedgeA1.0 go > 10x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. Timing link suitability includes constraints ([42 After 41 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. HD15115 (V=6.80, B-V = + 0.35). First of two sets of visits, each containing three visits of HD15115 at different relative orientations with one PSF calibration observation interleaved. This is the first HD15115 visit in the first set. The four visits within each set must be executed sequentally in contiguous orbits interrupted only for Earth occultation. Orientation: We wish to schedule this visit (41) at -30 deg from Visit 42, with the absolute orientation of Visit 42 unconstrained. Relative Timing: This visit (41) should immediately preceed visit (42). I.e., They should be executed sequentially in "back-to-back" orbits. 1318041027000 240.0 (Tic-Visit :proposal-id 12228 :visit-id "41" :proposal-version -1 :trans-version "20100505" :date "28-Jun-2010 16:50:31.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 76784 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "41" :obset-id "41" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "41" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2812 :al-overhead-at-end 0 :internal-dur-at-end 385 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3242 :pcs-gap 0 ) false 1 0 SNR = 100, V = 6.80, sp = F2, Exptimne rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD15115 is V = 6.80 so saturation in 20.0s. So 90% full well in appx 18.0s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD15115 is V = 6.80 so saturation in 20.0s. So 90% full well in appx 18.0s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. ts. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD15115 is V = 6.80 so saturation in 20.0s. So 90% full well in appx 18.0s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. ts. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD15115 is V = 6.80 so saturation in 20.0s. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. So 90% full well in appx 18.0s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. For long exposures at WedgeA1.0 go ~ 20x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. Timing link suitability includes constraints ([42 After 41 by 0.0 to 0.1 days] [43 After 42 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. HD15115 (V=6.80, B-V = + 0.35). First of two sets of visits, each containing three visits of HD15115 at different relative orientations with one PSF calibration observation interleaved. This is the second HD15115 visit in the first set. The four visits within each set must be executed sequentally in contiguous orbits interrupted only for Earth occultation. Orientation: There are no orientation constraints on this visit (42). Visits 41, 43, 44, 45, and 48 carry relative orientation constraints w.r.t. this visit. Relative Timing: This visit (42) should immediately follow Visit 41 and immediately preceed Visit 43 in back-to-back orbits. 1318046777000 265.0 (Tic-Visit :proposal-id 12228 :visit-id "42" :proposal-version -1 :trans-version "20100505" :date "28-Jun-2010 16:50:33.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 76784 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "42" :obset-id "42" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "42" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2808 :al-overhead-at-end 0 :internal-dur-at-end 385 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3242 :pcs-gap 0 ) false 1 0 SNR = 100, V = 6.80, sp = F2, Exptimne rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD15115 is V = 6.80 so saturation in 20.0s. So 90% full well in appx 18.0s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD15115 is V = 6.80 so saturation in 20.0s. So 90% full well in appx 18.0s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD15115 is V = 6.80 so saturation in 20.0s. So 90% full well in appx 18.0s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. ts. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. So 90% full well in appx 18.0s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. For long exposures at WedgeA1.0 go < = 20x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. Timing link suitability includes constraints ([43 After 42 by 0.0 to 0.1 days] [44 After 43 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. PSF5A (HD16647). PSF calibration target for HD15115. V = 6.26. B-V = +0.37. This is the PSF star calibrator for the flanking visits (41-44). We levy no orientation constraints on this visit (43). However, we choose this target very close in the sky to its paired science target. So as Visits 42 and 43 must be scheduled in sequential contiguous orbits, if scheduled at nominal roll (as we expect also Visit 42 will be) the we expect absolute orientations of Visits 42 and 43 to be very similar (within a few degrees). This is important so we maintain similar Sun and Beta angles for the science target and its PSF calibrator Relative Timing: This visit (43) should immediately follow visit 42 and immediately precede visit 44. I.e., They should be executed sequentially in "back-to-back" orbits. 1318052568000 266.67968308462423 (Tic-Visit :proposal-id 12228 :visit-id "43" :proposal-version -1 :trans-version "20100505" :date "28-Jun-2010 16:50:36.0" :trans-errors '(:WARNINGS 7 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 111552 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "43" :obset-id "43" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "43" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2845 :al-overhead-at-end 0 :internal-dur-at-end 422 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3242 :pcs-gap 0 ) false 1 0 SNR = 100, V =6.26, sp = F3V, Exptime rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. V = 6.26 so saturation in 12.1s. So 90% full well in appx 10.9s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. V = 6.26 so saturation in 12.1s. So 90% full well in appx 10.9s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. V = 6.26 so saturation in 12.1s. So 90% full well in appx 10.9s. Use this for the "short" exposures, repeated with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. V = 6.26 so saturation in 12.1s. So 90% full well in appx 10.9s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. For long exposures at WedgeA1.0 go <=20x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. Timing link suitability includes constraints ([44 After 43 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. HD15115 (V=6.80, B-V = + 0.35). First of two sets of visits, each containing three visits of HD15115 at different relative orientations with one PSF calibration observation interleaved. This is the third HD15115 visit in the first set. The four visits within each set must be executed sequentally in contiguous orbits interrupted only for Earth occultation. Orientation: We wish to schedule this visit (44) at +30 deg from Visit 42, with the absolute orientation of Visit 42 unconstrained. Relative Timing: This visit (44) should immediately follow Visit 43. I.e., They should be executed sequentially in "back-to-back" orbits. 1318058276000 290.0 (Tic-Visit :proposal-id 12228 :visit-id "44" :proposal-version -1 :trans-version "20100505" :date "28-Jun-2010 16:50:39.0" :trans-errors '(:WARNINGS 4 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 76784 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "44" :obset-id "44" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "44" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2800 :al-overhead-at-end 0 :internal-dur-at-end 385 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3242 :pcs-gap 0 ) false 1 0 SNR = 100, V = 6.80, sp = F2, Exptimne rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD15115 is V = 6.80 so saturation in 20.0s. So 90% full well in appx 18.0s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD15115 is V = 6.80 so saturation in 20.0s. So 90% full well in appx 18.0s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD15115 is V = 6.80 so saturation in 20.0s. So 90% full well in appx 18.0s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. ts. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. So 90% full well in appx 18.0s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. For long exposures at WedgeA1.0 go < = 20x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. Timing link suitability includes constraints ([46 After 45 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. HD15115 (V=6.80, B-V = + 0.35). Second of two sets of visits, each containing three visits of HD15115 at different relative orientations with one PSF calibration observation interleaved. This is the first HD15115 visit in the second set. The four visits within each set must be executed sequentally in contiguous orbits interrupted only for Earth occultation. Relative Orientation: We wish to schedule this visit (45) at EITHER -90 deg OR +90 deg from Visit 41. Either is equally acceptable, but there is no way to specifich this via APT 18.2, so we arbitraily specify an acceptable Orient From in the positive range (becasuse it worked) of +70 to +110 deg (to aid in schedulability and acceptable to our needs). If guide stars or other scheduling issues arise which APT is not cognizant of that makes these linked visits unschedualable she may freely change the parity of the relative orientation to -110 deg to -70 deg from Visit 41 Schedule in orbit immediately before Visit 46. 1292732979000 45.0 (Tic-Visit :proposal-id 12228 :visit-id "45" :proposal-version -1 :trans-version "20100505" :date "28-Jun-2010 16:50:41.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 76784 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "45" :obset-id "45" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "45" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2908 :al-overhead-at-end 0 :internal-dur-at-end 385 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3242 :pcs-gap 0 ) false 1 0 SNR = 100, V = 6.80, sp = F2, Exptimne rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD15115 is V = 6.80 so saturation in 20.0s. So 90% full well in appx 18.0s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD15115 is V = 6.80 so saturation in 20.0s. So 90% full well in appx 18.0s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD15115 is V = 6.80 so saturation in 20.0s. So 90% full well in appx 18.0s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. So 90% full well in appx 18.0s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. For long exposures at WedgeA1.0 go < = 20x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. Timing link suitability includes constraints ([46 After 45 by 0.0 to 0.1 days] [47 After 46 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. HD15115 (V=6.80, B-V = + 0.35). Second of two sets of visits, each containing three visits of HD15115 at different relative orientations with one PSF calibration observation interleaved. This is the second HD15115 visit in the second set. The four visits within each set must be executed sequentally in contiguous orbits interrupted only for Earth occultation. Orientation: We wish to schedule this visit (46) at +30 deg from Visit 45. We specify this exactly, and would relax this relative orientation requirment only if a suitable guide stars cannot be found. Relative Timing: This visit (46) should immediately follow visit 45 and immediately precede visit 47. I.e., They should be executed sequentially in "back-to-back" orbits. 1292738731000 72.5 (Tic-Visit :proposal-id 12228 :visit-id "46" :proposal-version -1 :trans-version "20100505" :date "28-Jun-2010 16:50:44.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 76784 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "46" :obset-id "46" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "46" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2908 :al-overhead-at-end 0 :internal-dur-at-end 385 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3242 :pcs-gap 0 ) false 1 0 SNR = 100, V = 6.80, sp = F2, Exptimne rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD15115 is V = 6.80 so saturation in 20.0s. So 90% full well in appx 18.0s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD15115 is V = 6.80 so saturation in 20.0s. So 90% full well in appx 18.0s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD15115 is V = 6.80 so saturation in 20.0s. So 90% full well in appx 18.0s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. So 90% full well in appx 18.0s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. For long exposures at WedgeA1.0 go < = 20x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. Timing link suitability includes constraints ([47 After 46 by 0.0 to 0.1 days] [48 After 47 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. PSF5A (HD16647). PSF calibration target for HD15115. V = 6.26. B-V = +0.37. This is the PSF star calibrator for the flanking visits (45-48). We levy no orientation constraints on this visit (47). However, we choose this target very close in the sky to its paired science target. So as Visits 46 and 47 must be scheduled in sequential contiguous orbits, if scheduled at nominal roll (as we expect also Visit 06 will be) the we expect absolute orientations of Visits 46 and 47 to be very similar (within a few degrees). This is important so we maintain similar Sun and Beta angles for the science target and its PSF calibrator Relative Timing: This visit (47) should immediately follow visit 06 and immediately precede visit 48. I.e., They should be executed sequentially in "back-to-back" orbits. 1292744551000 63.9305291380891 (Tic-Visit :proposal-id 12228 :visit-id "47" :proposal-version -1 :trans-version "20100505" :date "28-Jun-2010 16:50:47.0" :trans-errors '(:WARNINGS 7 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 111552 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "47" :obset-id "47" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "47" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2845 :al-overhead-at-end 0 :internal-dur-at-end 422 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3242 :pcs-gap 0 ) false 1 0 SNR = 100, V =6.26, sp = F3V, Exptime rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. V = 6.26 so saturation in 12.1s. So 90% full well in appx 10.9s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. V = 6.26 so saturation in 12.1s. So 90% full well in appx 10.9s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. V = 6.26 so saturation in 12.1s. So 90% full well in appx 10.9s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. V = 6.26 so saturation in 12.1s. So 90% full well in appx 10.9s. For long exposures at WedgeA1.0 go < = 20x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. Timing link suitability includes constraints ([48 After 47 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. HD15115 (V=6.80, B-V = + 0.35). Second of two sets of visits, each containing three visits of HD15115 at different relative orientations with one PSF calibration observation interleaved. This is the third HD15115 visit in the second set. The four visits within each set must be executed sequentally in contiguous orbits interrupted only for Earth occultation. Orientation: We wish to schedule this visit (48) at +60 deg from Visit 45. We specify this exactly, and would relax this relative orientation requirment only if a suitable guide stars cannot be found. Relative Timing: This visit (48) should immediately follow Visit 47. I.e., They should be executed sequentially in "back-to-back" orbits. 1292750237000 85.0 (Tic-Visit :proposal-id 12228 :visit-id "48" :proposal-version -1 :trans-version "20100505" :date "28-Jun-2010 16:50:50.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 76784 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "48" :obset-id "48" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "48" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2908 :al-overhead-at-end 0 :internal-dur-at-end 385 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3242 :pcs-gap 0 ) false 1 0 SNR = 100, V = 6.80, sp = F2, Exptimne rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD15115 is V = 6.80 so saturation in 20.0s. So 90% full well in appx 18.0s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD15115 is V = 6.80 so saturation in 20.0s. So 90% full well in appx 18.0s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD15115 is V = 6.80 so saturation in 20.0s. So 90% full well in appx 18.0s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. So 90% full well in appx 18.0s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. For long exposures at WedgeA1.0 go < = 20x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. Timing link suitability includes constraints ([52 After 51 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. HD 61005 (V=8.22, B-V = +0.71). First of two sets of visits, each containing three visits of HD 61005 at different relative orientations with one PSF calibration observation interleaved. This is the first HD 61005 visit in the first set. The four visits within each set must be executed sequentally in contiguous orbits interrupted only for Earth occultation. Orientation: We wish to schedule this visit (51) at -30 deg from Visit 52, with the absolute orientation of Visit 52 unconstrained. Relative Timing: This visit (51) should immediately preceed visit (52). I.e., They should be executed sequentially in "back-to-back" orbits. 1323130229000 295.0 (Tic-Visit :proposal-id 12228 :visit-id "51" :proposal-version -1 :trans-version "20100505" :date "28-Jun-2010 16:50:52.0" :trans-errors '(:WARNINGS 11 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 47360 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "51" :obset-id "51" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "51" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2941 :al-overhead-at-end 0 :internal-dur-at-end 353 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3275 :pcs-gap 0 ) false 1 0 SNR = 100, V = 8.22, sp = G8V, Exptime rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD 61005 is V = 8.22 (G8V) so saturation in 70.2s. So 90% full well in appx 63.2s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD 61005 is V = 8.22 (G8V) so saturation in 70.2s. So 90% full well in appx 63.2s. Use this for the "short" exposures, repeated (2x) with CR Split. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD 61005 is V = 8.22 (G8V) so saturation in 70.2s. So 90% full well in appx 63.2s. For long exposures at WedgeA1.0 go as deep as possible to fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. Timing link suitability includes constraints ([52 After 51 by 0.0 to 0.1 days] [53 After 52 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. HHD 61005 (V=8.22, B-V = +0.71). First of two sets of visits, each containing three visits of HD 61005 at different relative orientations with one PSF calibration observation interleaved. This is the second HD 61005 visit in the first set. The four visits within each set must be executed sequentally in contiguous orbits interrupted only for Earth occultation. Orientation: There are no orientation constraints on this visit (52). Visits 51, 53, 54, 55, and 58 carry relative orientation constraints w.r.t. this visit. Relative Timing: This visit (52) should immediately follow Visit 51 and immediately preceed Visit 53 in back-to-back orbits. 1323135979000 315.0 (Tic-Visit :proposal-id 12228 :visit-id "52" :proposal-version -1 :trans-version "20100505" :date "28-Jun-2010 16:50:53.0" :trans-errors '(:WARNINGS 11 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 47360 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "52" :obset-id "52" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "52" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2941 :al-overhead-at-end 0 :internal-dur-at-end 353 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3275 :pcs-gap 0 ) false 1 0 SNR = 100, V = 8.22, sp = G8V, Exptime rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD 61005 is V = 8.22 (G8V) so saturation in 70.2s. So 90% full well in appx 63.2s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD 61005 is V = 8.22 (G8V) so saturation in 70.2s. So 90% full well in appx 63.2s. Use this for the "short" exposures, repeated (2x) with CR Split. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD 61005 is V = 8.22 (G8V) so saturation in 70.2s. So 90% full well in appx 63.2s. For long exposures at WedgeA1.0 go as deep as possible to fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. Timing link suitability includes constraints ([53 After 52 by 0.0 to 0.1 days] [54 After 53 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. PSF06A (HD56161). PSF calibration target for HD 61005 . V = 6.937. B - V = +0.75. This is the PSF star calibrator for the flanking visits (51-54). We levy no orientation constraints on this visit (53). However, we choose this target very close in the sky to its paired science target. So as Visits 52 and 53 must be scheduled in sequential contiguous orbits, if scheduled at nominal roll (as we expect also Visit 52 will be) the we expect absolute orientations of Visits 52 and 53 to be very similar (within a few degrees). This is important so we maintain similar Sun and Beta angles for the science target and its PSF calibrator Relative Timing: This visit (53) should immediately follow visit 52 and immediately precede visit 54. I.e., They should be executed sequentially in "back-to-back" orbits. 1323141612000 322.0892879743782 (Tic-Visit :proposal-id 12228 :visit-id "53" :proposal-version -1 :trans-version "20100505" :date "28-Jun-2010 16:50:56.0" :trans-errors '(:WARNINGS 16 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 61952 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "53" :obset-id "53" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "53" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2940 :al-overhead-at-end 0 :internal-dur-at-end 369 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3275 :pcs-gap 0 ) false 1 0 SNR >~ 100, V = 6.973, sp = G5IV, Exptime rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. V = 6.94 so saturation in 21.8s. So 90% full well in appx 19.6s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. V = 6.94 so saturation in 21.8s. So 90% full well in appx 19.6s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. V = 7.74 so saturation in 47.4.0s. So 90% full well in appx 42.7s. For long exposures at WedgeA1.0 go <=20x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. Timing link suitability includes constraints ([54 After 53 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. HD 61005 (V=8.22, B-V = +0.71). First of two sets of visits, each containing three visits of HD 61005 at different relative orientations with one PSF calibration observation interleaved. This is the third HD 61005 visit in the first set. The four visits within each set must be executed sequentally in contiguous orbits interrupted only for Earth occultation. Orientation: We wish to schedule this visit (54) at +30 deg from Visit 52, with the absolute orientation of Visit 52 unconstrained. Relative Timing: This visit (54) should immediately follow Visit 53. I.e., They should be executed sequentially in "back-to-back" orbits. 1323147479000 335.0 (Tic-Visit :proposal-id 12228 :visit-id "54" :proposal-version -1 :trans-version "20100505" :date "28-Jun-2010 16:50:58.0" :trans-errors '(:WARNINGS 11 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 47360 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "54" :obset-id "54" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "54" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2941 :al-overhead-at-end 0 :internal-dur-at-end 353 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3275 :pcs-gap 0 ) false 1 0 SNR >~ 100, V = 8.22, sp = G8V, Exptime rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD 61005 is V = 8.22 (G8V) so saturation in 70.2s. So 90% full well in appx 63.2s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD 61005 is V = 8.22 (G8V) so saturation in 70.2s. So 90% full well in appx 63.2s. Use this for the "short" exposures, repeated (2x) with CR Split. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD 61005 is V = 8.22 (G8V) so saturation in 70.2s. So 90% full well in appx 63.2s. For long exposures at WedgeA1.0 go as deep as possible to fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. Timing link suitability includes constraints ([56 After 55 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. HD 61005 (V=8.22, B-V = +0.71). Second of two sets of visits, each containing three visits of HD 61005 at different relative orientations with one PSF calibration observation interleaved. This is the first HD 61005 visit in the second set. The four visits within each set must be executed sequentally in contiguous orbits interrupted only for Earth occultation. Relative Orientation: We wish to schedule this visit (55) at EITHER -90 deg OR +90 deg from Visit 51. Either is equally acceptable, but there is no way to specifich this via APT 18.2. Here we specify the positive exact value of +90 deg only. If guide stars or other scheduling issues arise which APT is not cognizant of that makes these linked visits unschedualable our PC may freely change the parity of the relative orientation to -110 deg to -70 deg from Visit 51 to seek schedualability. Schedule in orbit immediately before Visit 56. 1297984691000 25.0 (Tic-Visit :proposal-id 12228 :visit-id "55" :proposal-version -1 :trans-version "20100505" :date "28-Jun-2010 16:51:00.0" :trans-errors '(:WARNINGS 11 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 47360 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "55" :obset-id "55" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "55" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2941 :al-overhead-at-end 0 :internal-dur-at-end 353 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3275 :pcs-gap 0 ) false 1 0 SNR = 100, V = 8.22, sp = G8V, Exptime rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD 61005 is V = 8.22 (G8V) so saturation in 70.2s. So 90% full well in appx 63.2s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD 61005 is V = 8.22 (G8V) so saturation in 70.2s. So 90% full well in appx 63.2s. Use this for the "short" exposures, repeated (2x) with CR Split. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD 61005 is V = 8.22 (G8V) so saturation in 70.2s. So 90% full well in appx 63.2s. For long exposures at WedgeA1.0 go as deep as possible to fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. Timing link suitability includes constraints ([56 After 55 by 0.0 to 0.1 days] [57 After 56 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. HD 61005 (V=8.22, B-V = +0.71). Second of two sets of visits, each containing three visits of HD 61005 at different relative orientations with one PSF calibration observation interleaved. This is the second HD 61005 visit in the second set. The four visits within each set must be executed sequentally in contiguous orbits interrupted only for Earth occultation. Orientation: We wish to schedule this visit (56) at +30 deg from Visit 35. We specify this exactly, and would relax this relative orientation requirment only if a suitable guide stars cannot be found. Relative Timing: This visit (56) should immediately follow visit 55 and immediately precede visit 57. I.e., They should be executed sequentially in "back-to-back" orbits. 1297990441000 55.0 (Tic-Visit :proposal-id 12228 :visit-id "56" :proposal-version -1 :trans-version "20100505" :date "28-Jun-2010 16:51:02.0" :trans-errors '(:WARNINGS 11 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 47360 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "56" :obset-id "56" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "56" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2941 :al-overhead-at-end 0 :internal-dur-at-end 353 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3275 :pcs-gap 0 ) false 1 0 SNR = 100, V = 8.22, sp = G8V, Exptime rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD 61005 is V = 8.22 (G8V) so saturation in 70.2s. So 90% full well in appx 63.2s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD 61005 is V = 8.22 (G8V) so saturation in 70.2s. So 90% full well in appx 63.2s. Use this for the "short" exposures, repeated (2x) with CR Split. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD 61005 is V = 8.22 (G8V) so saturation in 70.2s. So 90% full well in appx 63.2s. For long exposures at WedgeA1.0 go as deep as possible to fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. Timing link suitability includes constraints ([57 After 56 by 0.0 to 0.1 days] [58 After 57 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. PSF06A (HD56161). PSF calibration target for HD 61005 . V = 6.937. B - V = +0.75. This is the PSF star calibrator for the flanking visits (55-58). We levy no orientation constraints on this visit (57). However, we choose this target very close in the sky to its paired science target. So as Visits 56 and 57 must be scheduled in sequential contiguous orbits, if scheduled at nominal roll (as we expect also Visit 56 will be) the we expect absolute orientations of Visits 56 and 57 to be very similar (within a few degrees). This is important so we maintain similar Sun and Beta angles for the science target and its PSF calibrator Relative Timing: This visit (57) should immediately follow visit 56 and immediately precede visit 58. I.e., They should be executed sequentially in "back-to-back" orbits. 1297996139000 50.4820680346204 (Tic-Visit :proposal-id 12228 :visit-id "57" :proposal-version -1 :trans-version "20100505" :date "28-Jun-2010 16:51:04.0" :trans-errors '(:WARNINGS 16 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 61952 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "57" :obset-id "57" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "57" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2940 :al-overhead-at-end 0 :internal-dur-at-end 369 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3275 :pcs-gap 0 ) false 1 0 SNR >~ 100, V = 6.973, sp = G5IV, Exptime rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. V = 6.94 so saturation in 21.8s. So 90% full well in appx 19.6s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. V = 6.94 so saturation in 21.8s. So 90% full well in appx 19.6s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. V = 7.74 so saturation in 47.4.0s. So 90% full well in appx 42.7s. For long exposures at WedgeA1.0 go < = 20x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. Timing link suitability includes constraints ([58 After 57 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. HD 61005 (V=8.22, B-V = +0.71). Second of two sets of visits, each containing three visits of HD 61005 at different relative orientations with one PSF calibration observation interleaved. This is the third HD 61005 visit in the second set. The four visits within each set must be executed sequentally in contiguous orbits interrupted only for Earth occultation. Orientation: We wish to schedule this visit (78) at +60 deg from Visit 75. We specify this exactly, and would relax this relative orientation requirment only if a suitable guide stars cannot be found. Relative Timing: This visit (78) should immediately follow Visit 77. I.e., They should be executed sequentially in "back-to-back" orbits. 1298001943000 65.0 (Tic-Visit :proposal-id 12228 :visit-id "58" :proposal-version -1 :trans-version "20100505" :date "28-Jun-2010 16:51:07.0" :trans-errors '(:WARNINGS 11 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 47360 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "58" :obset-id "58" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "58" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2941 :al-overhead-at-end 0 :internal-dur-at-end 353 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3275 :pcs-gap 0 ) false 1 0 SNR >~ 100, V = 8.22, sp = G8V, Exptime rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD 61005 is V = 8.22 (G8V) so saturation in 70.2s. So 90% full well in appx 63.2s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD 61005 is V = 8.22 (G8V) so saturation in 70.2s. So 90% full well in appx 63.2s. Use this for the "short" exposures, repeated (2x) with CR Split. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD 61005 is V = 8.22 (G8V) so saturation in 70.2s. So 90% full well in appx 63.2s. For long exposures at WedgeA1.0 go as deep as possible to fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. Timing link suitability includes constraints ([62 After 61 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. HD92945 (V=7.76, B-V = + 0.89). First of two sets of visits, each containing three visits of HD92945 at different relative orientations with one PSF calibration observation interleaved. This is the first HD92945 visit in the first set. The four visits within each set must be executed sequentally in contiguous orbits interrupted only for Earth occultation. Orientation: We wish to schedule this visit (61) at -30 deg from Visit 62, with the absolute orientation of Visit 42 unconstrained. Here we allow -30 to -20 to aid in scheduling, but as close to -30 deg as possible is preferential. Relative Timing: This visit (61) should immediately preceed visit (62). I.e., They should be executed sequentially in "back-to-back" orbits. 1330481748000 341.0 (Tic-Visit :proposal-id 12228 :visit-id "61" :proposal-version -1 :trans-version "20100505" :date "28-Jun-2010 16:51:09.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 57088 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "61" :obset-id "61" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "61" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2922 :al-overhead-at-end 0 :internal-dur-at-end 364 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3257 :pcs-gap 0 ) false 1 0 SNR = 100, V = 7.76 sp = K1V, Exptime rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD92945 is V = 7.76 so saturation in 41.7s. So 90% full well in appx 37.5s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD92945 is V = 7.76 so saturation in 41.7s. So 90% full well in appx 37.5s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD92945 is V = 7.76 so saturation in 41.7s. So 90% full well in appx 37.5s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. For long exposures at WedgeA1.0 go ~ 20x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. Timing link suitability includes constraints ([62 After 61 by 0.0 to 0.1 days] [63 After 62 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. HD92945 (V=7.76, B-V = + 0.89). First of two sets of visits, each containing three visits of HD92945 at different relative orientations with one PSF calibration observation interleaved. This is the second HD92945 visit in the first set. The four visits within each set must be executed sequentally in contiguous orbits interrupted only for Earth occultation. Orientation: There are no orientation constraints on this visit (62). Visits 61, 63, 64, 65, and 68 carry relative orientation constraints w.r.t. this visit. Relative Timing: This visit (62) should immediately follow Visit 61 and immediately preceed Visit 63 in back-to-back orbits. 1330487494000 1.0 (Tic-Visit :proposal-id 12228 :visit-id "62" :proposal-version -1 :trans-version "20100505" :date "28-Jun-2010 16:51:11.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 57088 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "62" :obset-id "62" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "62" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2922 :al-overhead-at-end 0 :internal-dur-at-end 364 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3257 :pcs-gap 0 ) false 1 0 SNR = 100, V = 7.76 sp = K1V, Exptime rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD92945 is V = 7.76 so saturation in 41.7s. So 90% full well in appx 37.5s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD92945 is V = 7.76 so saturation in 41.7s. So 90% full well in appx 37.5s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD92945 is V = 7.76 so saturation in 41.7s. So 90% full well in appx 37.5s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. For long exposures at WedgeA1.0 go < = 20x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. Timing link suitability includes constraints ([63 After 62 by 0.0 to 0.1 days] [64 After 63 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. PSF07A (HD89585). PSF calibration target for HD92945. V = 7.41. B-V = +0.88. This is the PSF star calibrator for the flanking visits (61-64). We levy no orientation constraints on this visit (63). However, we choose this target very close in the sky to its paired science target. So as Visits 62 and 63 must be scheduled in sequential contiguous orbits, if scheduled at nominal roll (as we expect also Visit 62 will be) the we expect absolute orientations of Visits 62 and 63 to be very similar (within a few degrees). This is important so we maintain similar Sun and Beta angles for the science target and its PSF calibrator Relative Timing: This visit (63) should immediately follow visit 62 and immediately precede visit 64. I.e., They should be executed sequentially in "back-to-back" orbits. 1330493137000 10.240415359341313 (Tic-Visit :proposal-id 12228 :visit-id "63" :proposal-version -1 :trans-version "20100505" :date "28-Jun-2010 16:51:13.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 61952 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "63" :obset-id "63" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "63" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2941 :al-overhead-at-end 0 :internal-dur-at-end 369 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3275 :pcs-gap 0 ) false 1 0 SNR = 100, V =7.41, sp =G5III, Exptime rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. V = 7.41 so saturation in 33.0s. So 90% full well in appx 29.7s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. V = 7.41 so saturation in 33.0s. So 90% full well in appx 29.7s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. V = 7.41 so saturation in 33.0s. So 90% full well in appx 29.7s. For long exposures at WedgeA1.0 go <=20x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. Timing link suitability includes constraints ([64 After 63 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. HD92945 (V=7.76, B-V = + 0.89). First of two sets of visits, each containing three visits of HD92945 at different relative orientations with one PSF calibration observation interleaved. This is the third HD92945 visit in the first set. The four visits within each set must be executed sequentally in contiguous orbits interrupted only for Earth occultation. Orientation: We wish to schedule this visit (64) at +30 deg from Visit 62, with the absolute orientation of Visit 62 unconstrained. To aid in scheduling we alow an Orient From range of +20 to +30 deg, though as close to +30 deg as possibke is ppreferred. Relative Timing: This visit (64) should immediately follow Visit 63. I.e., They should be executed sequentially in "back-to-back" orbits. 1330498986000 21.0 (Tic-Visit :proposal-id 12228 :visit-id "64" :proposal-version -1 :trans-version "20100505" :date "28-Jun-2010 16:51:15.0" :trans-errors '(:WARNINGS 3 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 57088 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "64" :obset-id "64" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "64" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2877 :al-overhead-at-end 0 :internal-dur-at-end 364 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3257 :pcs-gap 0 ) false 1 0 SNR = 100, V = 7.76 sp = K1V, Exptime rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD92945 is V = 7.76 so saturation in 41.7s. So 90% full well in appx 37.5s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD92945 is V = 7.76 so saturation in 41.7s. So 90% full well in appx 37.5s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD92945 is V = 7.76 so saturation in 41.7s. So 90% full well in appx 37.5s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. For long exposures at WedgeA1.0 go < = 20x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. Timing link suitability includes constraints ([66 After 65 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. HD92945 (V=7.76, B-V = + 0.89). Second of two sets of visits, each containing three visits of HD15115 at different relative orientations with one PSF calibration observation interleaved. This is the first HD15115 visit in the second set. The four visits within each set must be executed sequentally in contiguous orbits interrupted only for Earth occultation. Relative Orientation: We wish to schedule this visit (65) at EITHER -90 deg OR +90 deg from Visit 41. Either is equally acceptable, but there is no way to specifich this via APT 18.2. Here we specify the positive exact value of +90 deg only. If guide stars or other scheduling issues arise which APT is not cognizant of that makes these linked visits unschedualable our PC may freely change the parity of the relative orientation to -110 deg to -70 deg from Visit 61 to seek schedualability. Schedule in orbit immediately before Visit 66. From 61 by 70 to 110 1304668442000 71.0 (Tic-Visit :proposal-id 12228 :visit-id "65" :proposal-version -1 :trans-version "20100505" :date "28-Jun-2010 16:51:17.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 57088 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "65" :obset-id "65" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "65" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2922 :al-overhead-at-end 0 :internal-dur-at-end 364 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3257 :pcs-gap 0 ) false 1 0 SNR = 100, V = 7.76 sp = K1V, Exptime rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD92945 is V = 7.76 so saturation in 41.7s. So 90% full well in appx 37.5s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD92945 is V = 7.76 so saturation in 41.7s. So 90% full well in appx 37.5s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD92945 is V = 7.76 so saturation in 41.7s. So 90% full well in appx 37.5s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. Timing link suitability includes constraints ([66 After 65 by 0.0 to 0.1 days] [67 After 66 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. HD92945 (V=7.76, B-V = + 0.89). Second of two sets of visits, each containing three visits of HD15115 at different relative orientations with one PSF calibration observation interleaved. This is the second HD92945 visit in the second set. The four visits within each set must be executed sequentally in contiguous orbits interrupted only for Earth occultation. Orientation: We wish to schedule this visit (66) at +30 deg from Visit 65. Here we specify +22 deg exactly for schedualability, We would reduce this further by a few degrees only if a suitable guide stars cannot be found. Relative Timing: This visit (66) should immediately follow visit 65 and immediately precede visit 67. I.e., They should be executed sequentially in "back-to-back" orbits. 1304674191000 93.0 (Tic-Visit :proposal-id 12228 :visit-id "66" :proposal-version -1 :trans-version "20100505" :date "28-Jun-2010 16:51:19.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 57088 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "66" :obset-id "66" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "66" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2922 :al-overhead-at-end 0 :internal-dur-at-end 364 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3257 :pcs-gap 0 ) false 1 0 SNR = 100, V = 7.76 sp = K1V, Exptime rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD92945 is V = 7.76 so saturation in 41.7s. So 90% full well in appx 37.5s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD92945 is V = 7.76 so saturation in 41.7s. So 90% full well in appx 37.5s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD92945 is V = 7.76 so saturation in 41.7s. So 90% full well in appx 37.5s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. For long exposures at WedgeA1.0 go < = 20x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. Timing link suitability includes constraints ([67 After 66 by 0.0 to 0.1 days] [68 After 67 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. PSF07A (HD89585). PSF calibration target for HD92945. V = 7.41. B-V = +0.88. This is the PSF star calibrator for the flanking visits (65-68). We levy no orientation constraints on this visit (67). However, we choose this target very close in the sky to its paired science target. So as Visits 66 and 67 must be scheduled in sequential contiguous orbits, if scheduled at nominal roll (as we expect also Visit 06 will be) the we expect absolute orientations of Visits 66 and 47 to be very similar (within a few degrees). This is important so we maintain similar Sun and Beta angles for the science target and its PSF calibrator Relative Timing: This visit (67) should immediately follow visit 66 and immediately precede visit 68. I.e., They should be executed sequentially in "back-to-back" orbits. 1304679870000 93.78305671268117 (Tic-Visit :proposal-id 12228 :visit-id "67" :proposal-version -1 :trans-version "20100505" :date "28-Jun-2010 16:51:21.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 61952 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "67" :obset-id "67" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "67" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2941 :al-overhead-at-end 0 :internal-dur-at-end 369 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3275 :pcs-gap 0 ) false 1 0 SNR = 100, V =7.41, sp =G5III, Exptime rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. V = 7.41 so saturation in 33.0s. So 90% full well in appx 29.7s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. V = 7.41 so saturation in 33.0s. So 90% full well in appx 29.7s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD92945 is V = 7.76 so saturation in 41.7s. So 90% full well in appx 37.5s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. For long exposures at WedgeA1.0 go < = 20x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. Timing link suitability includes constraints ([68 After 67 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. HD92945 (V=7.76, B-V = + 0.89). Second of two sets of visits, each containing three visits of HD92945 at different relative orientations with one PSF calibration observation interleaved. This is the third HD92945 visit in the second set. The four visits within each set must be executed sequentally in contiguous orbits interrupted only for Earth occultation. Orientation: We wish to schedule this visit (68) at +60 deg from Visit 65. Here we specify +22 deg exactly for schedualability, We would reduce this further by a few degrees only if a suitable guide stars cannot be found. Relative Timing: This visit (68) should immediately follow Visit 67. I.e., They should be executed sequentially in "back-to-back" orbits. 1304685690000 113.0 (Tic-Visit :proposal-id 12228 :visit-id "68" :proposal-version -1 :trans-version "20100505" :date "28-Jun-2010 16:51:23.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 57088 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "68" :obset-id "68" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "68" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2922 :al-overhead-at-end 0 :internal-dur-at-end 364 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3257 :pcs-gap 0 ) false 1 0 SNR = 100, V = 7.76 sp = K1V, Exptime rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD92945 is V = 7.76 so saturation in 41.7s. So 90% full well in appx 37.5s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD92945 is V = 7.76 so saturation in 41.7s. So 90% full well in appx 37.5s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD92945 is V = 7.76 so saturation in 41.7s. So 90% full well in appx 37.5s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. Timing link suitability includes constraints ([72 After 71 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. HD 15745 (V=7.50, B-V = +0.32). First of two sets of visits, each containing three visits of HD 15745 at different relative orientations with one PSF calibration observation interleaved. This is the first HD 15745 visit in the first set. The four visits within each set must be executed sequentally in contiguous orbits interrupted only for Earth occultation. Orientation: We wish to schedule this visit (71) at -30 deg from Visit 72, with the absolute orientation of Visit 72 unconstrained. Here we specify -20 deg exactly due to apparent schedualability limitations, though a value closer to -30 deg is preferable. Relative Timing: This visit (71) should immediately preceed visit (72). I.e., They should be executed sequentially in "back-to-back" orbits. 1325502361000 65.0 (Tic-Visit :proposal-id 12228 :visit-id "71" :proposal-version -1 :trans-version "20100505" :date "28-Jun-2010 16:51:25.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 57088 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "71" :obset-id "71" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "71" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2967 :al-overhead-at-end 0 :internal-dur-at-end 364 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3301 :pcs-gap 0 ) false 1 0 SNR = 100, V = 7.50, sp = F2V, Exptime rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD 15745 is V = 7.50 so saturation in 38.0s. So 90% full well in appx 34.2s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD 15745 is V = 7.50 so saturation in 38.0s. So 90% full well in appx 34.2s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD 15745 is V = 7.50 so saturation in 38.0s. So 90% full well in appx 34.2s.For long exposures at WedgeA1.0 go > 10x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. Timing link suitability includes constraints ([72 After 71 by 0.0 to 0.1 days] [73 After 72 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. HD 15745 (V=7.50, B-V = +0.32). First of two sets of visits, each containing three visits of HD 15745 at different relative orientations with one PSF calibration observation interleaved. This is the second HD 15745 visit in the first set. The four visits within each set must be executed sequentally in contiguous orbits interrupted only for Earth occultation. Orientation: There are no orientation constraints on this visit (72). Visits 71, 73, 74, 75, and 78 carry relative orientation constraints w.r.t. this visit. Relative Timing: This visit (72) should immediately follow Visit 71 and immediately preceed Visit 73 in back-to-back orbits. 1325508110000 85.0 (Tic-Visit :proposal-id 12228 :visit-id "72" :proposal-version -1 :trans-version "20100505" :date "28-Jun-2010 16:51:27.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 57088 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "72" :obset-id "72" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "72" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2967 :al-overhead-at-end 0 :internal-dur-at-end 364 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3301 :pcs-gap 0 ) false 1 0 SNR = 100, V = 7.50, sp = F2V, Exptime rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD 15745 is V = 7.50 so saturation in 38.0s. So 90% full well in appx 34.2s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD 15745 is V = 7.50 so saturation in 38.0s. So 90% full well in appx 34.2s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD 15745 is V = 7.50 so saturation in 38.0s. So 90% full well in appx 34.2s.For long exposures at WedgeA1.0 go > 10x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. Timing link suitability includes constraints ([73 After 72 by 0.0 to 0.1 days] [74 After 73 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. PSF08A (HD16199). PSF calibration target for HD 15745 . V = 7.47. B - V = +0.35. This is the PSF star calibrator for the flanking visits (71-74). We levy no orientation constraints on this visit (43). However, we choose this target very close in the sky to its paired science target. So as Visits 72 and 73 must be scheduled in sequential contiguous orbits, if scheduled at nominal roll (as we expect also Visit 32 will be) the we expect absolute orientations of Visits 72 and 73 to be very similar (within a few degrees). This is important so we maintain similar Sun and Beta angles for the science target and its PSF calibrator Relative Timing: This visit (73) should immediately follow visit 72 and immediately precede visit 74. I.e., They should be executed sequentially in "back-to-back" orbits. 1325514227000 46.684 (Tic-Visit :proposal-id 12228 :visit-id "73" :proposal-version -1 :trans-version "20120712" :date "20-Aug-2012 11:30:43.0" :trans-errors '(:WARNINGS 15 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 49792 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "73" :obset-id "73" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "73" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2908 :al-overhead-at-end 0 :internal-dur-at-end 354 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3233 :pcs-gap 0 ) false 1 1 SNR = 100, V = 7.74, sp = F2V, Exptime rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. V = 7.74 so saturation in 47.4.0s. So 90% full well in appx 42.7s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. V = 7.74 so saturation in 47.4.0s. So 90% full well in appx 42.7s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. V = 7.74 so saturation in 47.4.0s. So 90% full well in appx 42.7s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. For long exposures at WedgeA1.0 go <=20x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. Timing link suitability includes constraints ([74 After 73 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. HD 15745 (V=7.50, B-V = +0.32). First of two sets of visits, each containing three visits of HD 15745 at different relative orientations with one PSF calibration observation interleaved. This is the third HD 15745 visit in the first set. The four visits within each set must be executed sequentally in contiguous orbits interrupted only for Earth occultation. Orientation: We wish to schedule this visit (74) at +30 deg from Visit 72, with the absolute orientation of Visit 72 unconstrained. Here we specify -20 deg exactly due to apparent schedualability limitations, though a value closer to -30 deg is preferable. Relative Timing: This visit (74) should immediately follow Visit 73. I.e., They should be executed sequentially in "back-to-back" orbits. 1325519610000 105.0 (Tic-Visit :proposal-id 12228 :visit-id "74" :proposal-version -1 :trans-version "20100505" :date "28-Jun-2010 16:51:31.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 57088 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "74" :obset-id "74" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "74" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2967 :al-overhead-at-end 0 :internal-dur-at-end 364 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3301 :pcs-gap 0 ) false 1 0 SNR = 100, V = 7.50, sp = F2V, Exptime rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD 15745 is V = 7.50 so saturation in 38.0s. So 90% full well in appx 34.2s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD 15745 is V = 7.50 so saturation in 38.0s. So 90% full well in appx 34.2s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD 15745 is V = 7.50 so saturation in 38.0s. So 90% full well in appx 34.2s.For long exposures at WedgeA1.0 go > 10x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. Timing link suitability includes constraints ([76 After 75 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. HD 15745 (V=7.50, B-V = +0.32). Second of two sets of visits, each containing three visits of HD 15745 at different relative orientations with one PSF calibration observation interleaved. This is the first HD 15745 visit in the second set. The four visits within each set must be executed sequentally in contiguous orbits interrupted only for Earth occultation. Relative Orientation: We wish to schedule this visit (35) at EITHER -90 deg OR +90 deg from Visit 71. Either is equally acceptable, but there is no way to specifich this via APT 18.2. Here we specify an acceptable Orient From range of +85 to +95 deg to aid in schedulability and acceptable to our needs (but the closer to +90 which can be scheduled the better). If guide stars or other scheduling issues arise which APT is not cognizant of that makes these linked visits unschedualable our the parity and range of the relative orientation to -110 deg to -70 deg from Visit 71 Schedule in orbit immediately before Visit 76. 1320495610000 150.0 (Tic-Visit :proposal-id 12228 :visit-id "75" :proposal-version -1 :trans-version "20100505" :date "28-Jun-2010 16:51:33.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 57088 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "75" :obset-id "75" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "75" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2967 :al-overhead-at-end 0 :internal-dur-at-end 364 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3301 :pcs-gap 0 ) false 1 0 SNR = 100, V = 7.50, sp = F2V, Exptime rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD 15745 is V = 7.50 so saturation in 38.0s. So 90% full well in appx 34.2s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD 15745 is V = 7.50 so saturation in 38.0s. So 90% full well in appx 34.2s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD 15745 is V = 7.50 so saturation in 38.0s. So 90% full well in appx 34.2s. For long exposures at WedgeA1.0 go > 10x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. Timing link suitability includes constraints ([76 After 75 by 0.0 to 0.1 days] [77 After 76 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. HD 15745 (V=7.50, B-V = +0.32). Second of two sets of visits, each containing three visits of HD 15745 at different relative orientations with one PSF calibration observation interleaved. This is the second HD 15745 visit in the second set. The four visits within each set must be executed sequentally in contiguous orbits interrupted only for Earth occultation. Orientation: We wish to schedule this visit (76) at +30 deg from Visit 35. Here we specify an allowble range of +25 to +30 deg, though as close to +30 deg as possible is preferable. Relative Timing: This visit (76) should immediately follow visit 35 and immediately precede visit 77. I.e., They should be executed sequentially in "back-to-back" orbits. 1320501359000 172.0 (Tic-Visit :proposal-id 12228 :visit-id "76" :proposal-version -1 :trans-version "20100505" :date "28-Jun-2010 16:51:35.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 57088 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "76" :obset-id "76" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "76" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2967 :al-overhead-at-end 0 :internal-dur-at-end 364 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3301 :pcs-gap 0 ) false 1 0 SNR = 100, V = 7.50, sp = F2V, Exptime rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD 15745 is V = 7.50 so saturation in 38.0s. So 90% full well in appx 34.2s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. AU MIC is V = 8.61 so saturation in 50.6s. So 90% full well in appx 45.5s. Use this for the "short" exposures, repeated with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD 15745 is V = 7.50 so saturation in 38.0s. So 90% full well in appx 34.2s. For long exposures at WedgeA1.0 go > 10x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. Timing link suitability includes constraints ([77 After 76 by 0.0 to 0.1 days] [78 After 77 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. PSF08A (HD16199). PSF calibration target for HD 15745 . V = 7.47. B - V = +0.35. This is the PSF star calibrator for the flanking visits (75-78). We levy no orientation constraints on this visit (37). However, we choose this target very close in the sky to its paired science target. So as Visits 76 and 77 must be scheduled in sequential contiguous orbits, if scheduled at nominal roll (as we expect also Visit 36 will be) the we expect absolute orientations of Visits 76 and 77 to be very similar (within a few degrees). This is important so we maintain similar Sun and Beta angles for the science target and its PSF calibrator Relative Timing: This visit (77) should immediately follow visit 36 and immediately precede visit 78. I.e., They should be executed sequentially in "back-to-back" orbits. 1320507480000 14.34758763930671 (Tic-Visit :proposal-id 12228 :visit-id "77" :proposal-version -1 :trans-version "20120712" :date "20-Aug-2012 11:06:48.0" :trans-errors '(:WARNINGS 11 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 49792 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "77" :obset-id "77" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "77" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2767 :al-overhead-at-end 0 :internal-dur-at-end 354 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3233 :pcs-gap 0 ) false 1 0 SNR = 100, V = 7.74, sp = F2V, Exptime rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. V = 7.74 so saturation in 47.4.0s. So 90% full well in appx 42.7s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. V = 7.74 so saturation in 47.4.0s. So 90% full well in appx 42.7s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. V = 7.74 so saturation in 47.4.0s. So 90% full well in appx 42.7s. For long exposures at WedgeA1.0 go < = 20x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. Timing link suitability includes constraints ([78 After 77 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. HD 15745 (V=7.50, B-V = +0.32). Second of two sets of visits, each containing three visits of HD 15745 at different relative orientations with one PSF calibration observation interleaved. This is the third HD 15745 visit in the second set. The four visits within each set must be executed sequentally in contiguous orbits interrupted only for Earth occultation. Orientation: We wish to schedule this visit (78) at +60 deg from Visit 75. We specify this exactly, and would relax this relative orientation requirment only if a suitable guide stars cannot be found. Here we specify an allowble range of +25 to +30 deg, though as close to +30 deg as possible is preferable. Relative Timing: This visit (78) should immediately follow Visit 77. I.e., They should be executed sequentially in "back-to-back" orbits. 1320514690000 199.0 (Tic-Visit :proposal-id 12228 :visit-id "78" :proposal-version -1 :trans-version "20100505" :date "28-Jun-2010 16:51:39.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 57088 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "78" :obset-id "78" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "78" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2967 :al-overhead-at-end 0 :internal-dur-at-end 364 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3301 :pcs-gap 0 ) false 1 0 SNR = 100, V = 7.50, sp = F2V, Exptime rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD 15745 is V = 7.50 so saturation in 38.0s. So 90% full well in appx 34.2s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD 15745 is V = 7.50 so saturation in 38.0s. So 90% full well in appx 34.2s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD 15745 is V = 7.50 so saturation in 38.0s. So 90% full well in appx 34.2s. For long exposures at WedgeA1.0 go > 10x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. Timing link suitability includes constraints ([82 After 81 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. HD 53143 (V=6.81, B-V = +0.20). First of two sets of visits, each containing three visits of HD 53143 at different relative orientations with one PSF calibration observation interleaved. This is the first HD 53143 visit in the first set. The four visits within each set must be executed sequentally in contiguous orbits interrupted only for Earth occultation. Orientation: We wish to schedule this visit (81) at -30 deg from Visit 82, with the absolute orientation of Visit 82 unconstrained. Relative Timing: This visit (81) should immediately preceed visit (82). I.e., They should be executed sequentially in "back-to-back" orbits. 1294672673000 346.0 (Tic-Visit :proposal-id 12228 :visit-id "81" :proposal-version -1 :trans-version "20100505" :date "02-Mar-2011 09:47:40.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 89056 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "81" :obset-id "81" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "81" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3169 :al-overhead-at-end 0 :internal-dur-at-end 398 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3516 :pcs-gap 0 ) false 1 0 SNR = 100, V = 6.81, sp = G9V, Exptime rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD 53143 is V = 6.81 so saturation in 19.2s. So 90% full well in appx 17.2s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD 53143 is V = 6.81 so saturation in 19.2s. So 90% full well in appx 17.2s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD 53143 is V = 6.81 so saturation in 19.2s. So 90% full well in appx 17.2s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD 53143 is V = 6.81 so saturation in 19.2s. So 90% full well in appx 17.2s. For long exposures at WedgeA1.0 go > 10x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. This is different... For all OTHER tragets we use target acquition images to establish the target:PSF template flux density ratios under the broad STIS 50CCD bandpass. In those cases target and template stars are both acquired with F25ND3. In THIS case the PSF template star for HD53143 is too bright to acquire without using F25ND5, which we do. While "neutral" we do not believe it is sufficiently so to assume no color transformation is needed for accurate photometry with F25ND3 transformed to F25ND5 - ans such a spectral calibration to high precision does not seem to exist. Hene we take a DIRECT (unocculted) image of the target star with F25ND5 (same as used for the ACQ imaging using Alpha Pic) so we can directly ratio the stellar brightnesses in the same spectral element. We only do this in one (istit 81) of the HD 53143 visits in the Visit 81-84 link set. SNR = 100 (each of two CR Split), V = 6.81, sp = G9V (F25ND5), Exptime rounded to nearest 0.1 second. SNR = 100, V = 6.81, sp = G9V, Exptime rounded to nearest 0.1 second Timing link suitability includes constraints ([82 After 81 by 0.0 to 0.1 days] [83 After 82 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. HD 53143 (V=6.81, B-V = +0.20). First of two sets of visits, each containing three visits of HD 53143 at different relative orientations with one PSF calibration observation interleaved. This is the second HD 53143 visit in the first set. The four visits within each set must be executed sequentally in contiguous orbits interrupted only for Earth occultation. Orientation: There are no orientation constraints on this visit (82). Visits 81, 83, 84, 85, and 88 carry relative orientation constraints w.r.t. this visit. Relative Timing: This visit (82) should immediately follow Visit 81 and immediately preceed Visit 83 in back-to-back orbits. 1294678604000 3.5 (Tic-Visit :proposal-id 12228 :visit-id "82" :proposal-version -1 :trans-version "20100505" :date "02-Mar-2011 09:47:42.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 94288 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "82" :obset-id "82" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "82" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3182 :al-overhead-at-end 0 :internal-dur-at-end 404 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3516 :pcs-gap 0 ) false 1 0 SNR = 100, V = 6.81, sp = G9V, Exptime rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD 53143 is V = 7.50 so saturation in 19.2s. So 90% full well in appx 17.2s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD 53143 is V = 6.81 so saturation in 19.2s. So 90% full well in appx 17.2s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD 53143 is V = 6.81 so saturation in 19.2s. So 90% full well in appx 17.2s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD 15745 is V = 7.50 so saturation in 38.0s. So 90% full well in appx 34.2s.For long exposures at WedgeA1.0 go > 10x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. Timing link suitability includes constraints ([83 After 82 by 0.0 to 0.1 days] [84 After 83 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. PSF09A (ALPHA PIC). PSF calibration target for ALPHA PIC . V = 3.30. B - V = +0.28. Sp A8V This is the PSF star calibrator for the flanking visits (81-84). We levy no orientation constraints on this visit (43). However, we choose this target very close in the sky to its paired science target. So as Visits 82 and 83 must be scheduled in sequential contiguous orbits, if scheduled at nominal roll (as we expect also Visit 32 will be) the we expect absolute orientations of Visits 82 and 83 to be very similar (within a few degrees). This is important so we maintain similar Sun and Beta angles for the science target and its PSF calibrator Relative Timing: This visit (83) should immediately follow visit 82 and immediately precede visit 84. I.e., they should be executed sequentially in "back-to-back" orbits. 1294684179000 8.9503486842259 (Tic-Visit :proposal-id 12228 :visit-id "83" :proposal-version -1 :trans-version "20100505" :date "02-Mar-2011 09:47:46.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 205152 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "83" :obset-id "83" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "83" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3173 :al-overhead-at-end 0 :internal-dur-at-end 383 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3516 :pcs-gap 0 ) false 1 0 SNR = 100, V = 3.30, sp = A8V, Exptime rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. V =3.30 so saturation in 0.812s. So ~ 90% full well in appx 0.7s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. V = 3.30 so saturation in 0.812s. So ~ 90% full well in appx 0.7s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. V =3.30 so saturation in 0.812s. So ~ 90% full well in appx 0.7s. Use this for the medium exposures, repeated (8x) with multiple CR Splits. For medium exposures at WedgeA1.0 go 20x deeper in each. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. V =3.30 so saturation in 0.812s. So ~ 90% full well in appx 0.7s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. For long exposures at WedgeA1.0 go <=20x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. V =3.30 so saturation in 0.812s. So ~ 90% full well in appx 0.7s.. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. For medium exposures at WedgeA1.0 go 20x deeper in each. These are in this orber (broken off from the first set) to mitigate dead-time that otherwise arises from non-parallel buffer dumps. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. Timing link suitability includes constraints ([84 After 83 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. HD 53143 (V=6.81, B-V = +0.20). First of two sets of visits, each containing three visits of HD 53143 at different relative orientations with one PSF calibration observation interleaved. This is the third HD 53143 visit in the first set. The four visits within each set must be executed sequentally in contiguous orbits interrupted only for Earth occultation. Orientation: We wish to schedule this visit (84) at +30 deg from Visit 82, with the absolute orientation of Visit 82 unconstrained. Relative Timing: This visit (84) should immediately follow Visit 83. I.e., They should be executed sequentially in "back-to-back" orbits. 1294689927000 21.0 (Tic-Visit :proposal-id 12228 :visit-id "84" :proposal-version -1 :trans-version "20100505" :date "02-Mar-2011 09:47:49.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 94288 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "84" :obset-id "84" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "84" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3182 :al-overhead-at-end 0 :internal-dur-at-end 404 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3516 :pcs-gap 0 ) false 1 0 SNR = 100, V = 6.81, sp = G9V, Exptime rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD 53143 is V = 7.50 so saturation in 19.2s. So 90% full well in appx 17.2s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD 53143 is V = 6.81 so saturation in 19.2s. So 90% full well in appx 17.2s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD 53143 is V = 6.81 so saturation in 19.2s. So 90% full well in appx 17.2s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD 15745 is V = 7.50 so saturation in 38.0s. So 90% full well in appx 34.2s.For long exposures at WedgeA1.0 go > 10x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. Timing link suitability includes constraints ([86 After 85 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. HD 53143 (V=6.81, B-V = +0.80, G9V). Second of two sets of visits, each containing three visits of HD 53143 at different relative orientations with one PSF calibration observation interleaved. This is the first HD 53143 visit in the second set. The four visits within each set must be executed sequentally in contiguous orbits interrupted only for Earth occultation. Relative Orientation: We wish to schedule this visit (85) at EITHER -90 deg OR +90 deg from Visit 78. Either is equally acceptable, but there is no way to specifich this via APT 18.2, so we arbitraily specify an acceptable Orinet From in the positive range (becasuse it worked) of +70 to +110 deg (to aid in schedulability and acceptable to our needs). If guide stars or other scheduling issues arise which APT is not cognizant of that makes these linked visits unschedualable she may freely change the parity of the relative orientation to -110 deg to -70 deg from Visit 71 Schedule in orbit immediately before Visit 86. N.B. On March 02, 2011 we removed the "HD53143_NDSCALE" exposures from the back end of this orbit (no longer needed with a replacement PSF template star in Visit 87) and revised the exposure level content to be identical with Visit 86. 1302392380000 76.0 (Tic-Visit :proposal-id 12228 :visit-id "85" :proposal-version -1 :trans-version "20100505" :date "02-Mar-2011 09:47:51.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 94288 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "85" :obset-id "85" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "85" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3182 :al-overhead-at-end 0 :internal-dur-at-end 404 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3516 :pcs-gap 0 ) false 1 0 SNR = 100, V = 6.81, sp = G9V, Exptime rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD 53143 is V = 6.81 so saturation in 19.2s. So 90% full well in appx 17.2s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD 53143 is V = 6.81 so saturation in 19.2s. So 90% full well in appx 17.2s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD 53143 is V = 6.81 so saturation in 19.2s. So 90% full well in appx 17.2s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD 53143 is V = 6.81 so saturation in 19.2s. So 90% full well in appx 17.2s. For long exposures at WedgeA1.0 go > 10x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. Timing link suitability includes constraints ([86 After 85 by 0.0 to 0.1 days] [87 After 86 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. HD 53143 (V=6.81, B-V = +0.80, G9V). Second of two sets of visits, each containing three visits of HD 53143 at different relative orientations with one PSF calibration observation interleaved. This is the second HD 53143 visit in the second set. The four visits within each set must be executed sequentally in contiguous orbits interrupted only for Earth occultation. Orientation: We wish to schedule this visit (86) at +30 deg from Visit 85. We specify this exactly, and would relax this relative orientation requirment only if a suitable guide stars cannot be found. Relative Timing: This visit (86) should immediately follow visit 85 and immediately precede visit 87. I.e., They should be executed sequentially in "back-to-back" orbits. 1302400932000 93.5 (Tic-Visit :proposal-id 12228 :visit-id "86" :proposal-version -1 :trans-version "20100505" :date "02-Mar-2011 09:46:09.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 94288 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "86" :obset-id "86" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "86" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3182 :al-overhead-at-end 0 :internal-dur-at-end 404 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3516 :pcs-gap 0 ) false 1 0 SNR = 100, V = 6.81, sp = G9V, Exptime rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD 53143 is V = 6.81 so saturation in 19.2s. So 90% full well in appx 17.2s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD 53143 is V = 6.81 so saturation in 19.2s. So 90% full well in appx 17.2s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD 53143 is V = 6.81 so saturation in 19.2s. So 90% full well in appx 17.2s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD 53143 is V = 6.81 so saturation in 38.0s. So 90% full well in appx 34.2s.For long exposures at WedgeA1.0 go > 10x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. Timing link suitability includes constraints ([87 After 86 by 0.0 to 0.1 days] [88 After 87 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. PSF09B (HD59780; V = 6.522. B - V = +0.919, G8III). PSF calibration target for HD 53143 . This is the PSF star calibrator for the flanking visits (85-88). We levy no orientation constraints on this visit (87). However, we choose this target very close in the sky to its paired science target. So as Visits 86 and 87 must be scheduled in sequential contiguous orbits, if scheduled at nominal roll (as we expect also Visit 36 will be) the we expect absolute orientations of Visits 86 and 87 to be very similar (within a few degrees). This is important so we maintain similar Sun and Beta angles for the science target and its PSF calibrator Relative Timing: This visit (87) should immediately follow visit 36 and immediately precede visit 88. I.e., They should be executed sequentially in "back-to-back" orbits. 1302406799000 90.91547490421868 (Tic-Visit :proposal-id 12228 :visit-id "87" :proposal-version -1 :trans-version "20100505" :date "02-Mar-2011 09:45:34.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 119088 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "87" :obset-id "87" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "87" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3176 :al-overhead-at-end 0 :internal-dur-at-end 430 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3511 :pcs-gap 0 ) false 1 0 Goal: SNR = 100, V = 6.522, sp = G8III. Exptime rounded (up) to nearest 0.1 second ETC: SNR = 100 in 0.134s; in 0.2s SNR = 169 SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD 59780 is V = 6.522 so saturation in 15.445s. So 90% full well in appx 13.9s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD 59780 is V = 6.522 so saturation in 15.445s. So 90% full well in appx 13.9s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD 59780 is V = 6.522 so saturation in 15.445s. So 90% full well in appx 13.9s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD 59780 is V = 6.522 so we expect saturation in 20.137s. So 90% full well in appx 18.125s. For long exposures at WedgeA1.0 go > 10x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. Timing link suitability includes constraints ([88 After 87 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. HD 53143 (V=6.81, B-V = +0.80, G9V). Second of two sets of visits, each containing three visits of HD 53143 at different relative orientations with one PSF calibration observation interleaved. This is the third HD 53143 visit in the second set. The four visits within each set must be executed sequentally in contiguous orbits interrupted only for Earth occultation. Orientation: We wish to schedule this visit (88) at +60 deg from Visit 85. We specify this exactly, and would relax this relative orientation requirment only if a suitable guide stars cannot be found. Relative Timing: This visit (88) should immediately follow Visit 87. I.e., They should be executed sequentially in "back-to-back" orbits. 1302412425000 111.0 (Tic-Visit :proposal-id 12228 :visit-id "88" :proposal-version -1 :trans-version "20100505" :date "02-Mar-2011 09:47:55.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 94288 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "88" :obset-id "88" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "88" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3182 :al-overhead-at-end 0 :internal-dur-at-end 404 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3516 :pcs-gap 0 ) false 1 0 SNR = 100, V = 6.81, sp = G9V, Exptime rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD 53143 is V = 6.81 so saturation in 19.2s. So 90% full well in appx 17.2s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD 53143 is V = 6.81 so saturation in 19.2s. So 90% full well in appx 17.2s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD 53143 is V = 6.81 so saturation in 19.2s. So 90% full well in appx 17.2s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD 53143 is V = 6.81 so saturation in 38.0s. So 90% full well in appx 34.2s.For long exposures at WedgeA1.0 go > 10x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. Timing link suitability includes constraints ([92 After 91 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. HD 139664 (V=4.64, B-V = +0.40). First of two sets of visits, each containing three visits of HD 139664 at different relative orientations with one PSF calibration observation interleaved. This is the first HD 139664 visit in the first set. The four visits within each set must be executed sequentally in contiguous orbits interrupted only for Earth occultation. Orientation: We wish to schedule this visit (91) at -30 deg from Visit 92, with the absolute orientation of Visit 92 unconstrained. Here w specifiy an exact value of -25 deg due to schedlability limitations. Relative Timing: This visit (91) should immediately preceed visit (92). I.e., They should be executed sequentially in "back-to-back" orbits. 1312110840000 69.0 (Tic-Visit :proposal-id 12228 :visit-id "91" :proposal-version -1 :trans-version "20100505" :date "28-Jun-2010 16:52:05.0" :trans-errors '(:WARNINGS 3 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 122240 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "91" :obset-id "91" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "91" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3002 :al-overhead-at-end 0 :internal-dur-at-end 433 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3341 :pcs-gap 0 ) false 1 0 SNR = 188, V = 4.64, sp = F5V, Exptime rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD 139664 is V = 4.64 (F5V) so saturation in 2.7s. So 90% full well in appx 2.4s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD 139664 is V = 4.64 (F5V) so saturation in 2.7s. So 90% full well in appx 2.4s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD 139664 is V = 4.64 (F5V) so saturation in 2.7s. So 90% full well in appx 2.4s. For long exposures at WedgeA1.0 go > 10x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD 139664 is V = 4.64 (F5V) so saturation in 2.7s. So 90% full well in appx 2.4s. For long exposures at WedgeA1.0 go > 10x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. Timing link suitability includes constraints ([92 After 91 by 0.0 to 0.1 days] [93 After 92 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. HD 139664 (V=4.64, B-V = +0.40). First of two sets of visits, each containing three visits of HD 139664 at different relative orientations with one PSF calibration observation interleaved. This is the second HD 139664 visit in the first set. The four visits within each set must be executed sequentally in contiguous orbits interrupted only for Earth occultation. Orientation: There are no orientation constraints on this visit (92). Visits 91, 93, 94, 95, and 98 carry relative orientation constraints w.r.t. this visit. Relative Timing: This visit (92) should immediately follow Visit 91 and immediately preceed Visit 93 in back-to-back orbits. 1312119080000 93.0 (Tic-Visit :proposal-id 12228 :visit-id "92" :proposal-version -1 :trans-version "20100505" :date "28-Jun-2010 16:52:08.0" :trans-errors '(:WARNINGS 3 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 122240 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "92" :obset-id "92" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "92" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3002 :al-overhead-at-end 0 :internal-dur-at-end 433 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3341 :pcs-gap 0 ) false 1 0 SNR = 188, V = 4.64, sp = F5V, Exptime rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD 139664 is V = 4.64 (F5V) so saturation in 2.7s. So 90% full well in appx 2.4s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD 139664 is V = 4.64 (F5V) so saturation in 2.7s. So 90% full well in appx 2.4s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD 139664 is V = 4.64 (F5V) so saturation in 2.7s. So 90% full well in appx 2.4s. For long exposures at WedgeA1.0 go > 10x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD 139664 is V = 4.64 (F5V) so saturation in 2.7s. So 90% full well in appx 2.4s. For long exposures at WedgeA1.0 go > 10x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. Timing link suitability includes constraints ([93 After 92 by 0.0 to 0.1 days] [94 After 93 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. PSF10A (HD99453). PSF calibration target for HD 139664 . V = 5.17. B - V = +0.50. This is the PSF star calibrator for the flanking visits (91-94). We levy no orientation constraints on this visit (43). However, we choose this target very close in the sky to its paired science target. So as Visits 92 and 93 must be scheduled in sequential contiguous orbits, if scheduled at nominal roll (as we expect also Visit 32 will be) the we expect absolute orientations of Visits 92 and 93 to be very similar (within a few degrees). This is important so we maintain similar Sun and Beta angles for the science target and its PSF calibrator Relative Timing: This visit (93) should immediately follow visit 92 and immediately precede visit 94. I.e., They should be executed sequentially in "back-to-back" orbits. 1312125858000 141.36509503380353 (Tic-Visit :proposal-id 12228 :visit-id "93" :proposal-version -1 :trans-version "20100505" :date "28-Jun-2010 16:52:10.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 122240 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "93" :obset-id "93" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "93" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3177 :al-overhead-at-end 0 :internal-dur-at-end 433 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3516 :pcs-gap 0 ) false 1 0 SNR = 148, V = 5.17, sp = F7V, Exptime rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0). V = 5.17 (F7V) so saturation in 4.4s. So 90% full well in appx 3.9s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0). V = 5.17 (F7V) so saturation in 4.4s. So 90% full well in appx 3.9s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. V = 7.74 so saturation in 47.4.0s. So 90% full well in appx 42.7s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. For long exposures at WedgeA1.0 go <=20x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. V = 7.74 so saturation in 47.4.0s. So 90% full well in appx 42.7s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. For long exposures at WedgeA1.0 go <=20x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. Timing link suitability includes constraints ([94 After 93 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. HD 139664 (V=4.64, B-V = +0.40). First of two sets of visits, each containing three visits of HD 139664 at different relative orientations with one PSF calibration observation interleaved. This is the third HD 139664 visit in the first set. The four visits within each set must be executed sequentally in contiguous orbits interrupted only for Earth occultation. Orientation: We wish to schedule this visit (94) at +30 deg from Visit 92, with the absolute orientation of Visit 92 unconstrained. However, only smaller Orient Froms were found t be schedulable. Here we specify exactly +18 deg as the minimum for this offset. Further reduction may be possible but only with changes in the relative orientations of other visits. Relative Timing: This visit (94) should immediately follow Visit 93. I.e., They should be executed sequentially in "back-to-back" orbits. 1312130574000 111.0 (Tic-Visit :proposal-id 12228 :visit-id "94" :proposal-version -1 :trans-version "20100505" :date "28-Jun-2010 16:52:13.0" :trans-errors '(:WARNINGS 3 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 122240 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "94" :obset-id "94" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "94" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3002 :al-overhead-at-end 0 :internal-dur-at-end 433 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3341 :pcs-gap 0 ) false 1 0 SNR = 188, V = 4.64, sp = F5V, Exptime rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD 139664 is V = 4.64 (F5V) so saturation in 2.7s. So 90% full well in appx 2.4s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD 139664 is V = 4.64 (F5V) so saturation in 2.7s. So 90% full well in appx 2.4s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD 139664 is V = 4.64 (F5V) so saturation in 2.7s. So 90% full well in appx 2.4s. For long exposures at WedgeA1.0 go > 10x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD 139664 is V = 4.64 (F5V) so saturation in 2.7s. So 90% full well in appx 2.4s. For long exposures at WedgeA1.0 go > 10x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. Timing link suitability includes constraints ([96 After 95 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. HD 139664 (V=4.64, B-V = +0.40). Second of two sets of visits, each containing three visits of HD 139664 at different relative orientations with one PSF calibration observation interleaved. This is the first HD 139664 visit in the second set. The four visits within each set must be executed sequentally in contiguous orbits interrupted only for Earth occultation. Relative Orientation: We wish to schedule this visit (95) at EITHER -90 deg OR +90 deg from Visit 91. Either is equally acceptable, but there is no way to specifich this via APT 18.2. Here we specify an acceptable Orient From in the positive range of +80 to +90 deg (to aid in schedulability and acceptable to our needs). If guide stars or other scheduling issues arise which APT is not cognizant of that makes these linked visits unschedualable she may freely change the parity of the relative orientation to -80 deg to -90 deg from Visit 91 Schedule in orbit immediately before Visit 96. 1306192698000 348.0 (Tic-Visit :proposal-id 12228 :visit-id "95" :proposal-version -1 :trans-version "20100505" :date "28-Jun-2010 16:52:16.0" :trans-errors '(:WARNINGS 3 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 122240 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "95" :obset-id "95" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "95" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3002 :al-overhead-at-end 0 :internal-dur-at-end 433 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3341 :pcs-gap 0 ) false 1 0 SNR = 188, V = 4.64, sp = F5V, Exptime rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD 139664 is V = 4.64 (F5V) so saturation in 2.7s. So 90% full well in appx 2.4s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD 139664 is V = 4.64 (F5V) so saturation in 2.7s. So 90% full well in appx 2.4s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD 139664 is V = 4.64 (F5V) so saturation in 2.7s. So 90% full well in appx 2.4s. For long exposures at WedgeA1.0 go > 10x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD 139664 is V = 4.64 (F5V) so saturation in 2.7s. So 90% full well in appx 2.4s. For long exposures at WedgeA1.0 go > 10x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. Timing link suitability includes constraints ([96 After 95 by 0.0 to 0.1 days] [97 After 96 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. HD 139664 (V=4.64, B-V = +0.40). Second of two sets of visits, each containing three visits of HD 15745 at different relative orientations with one PSF calibration observation interleaved. This is the second HD 139664 visit in the second set. The four visits within each set must be executed sequentally in contiguous orbits interrupted only for Earth occultation. Orientation: We wish to schedule this visit (96) at +30 deg from Visit 95. Here we specify +24 deg exactly due to scheduling limitation, though closer to +30 deg would be preferable. Relative Timing: This visit (96) should immediately follow visit 95 and immediately precede visit 97. I.e., They should be executed sequentially in "back-to-back" orbits. 1306200931000 12.0 (Tic-Visit :proposal-id 12228 :visit-id "96" :proposal-version -1 :trans-version "20100505" :date "28-Jun-2010 16:52:19.0" :trans-errors '(:WARNINGS 3 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 122240 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "96" :obset-id "96" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "96" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3002 :al-overhead-at-end 0 :internal-dur-at-end 433 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3341 :pcs-gap 0 ) false 1 0 SNR = 188, V = 4.64, sp = F5V, Exptime rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD 139664 is V = 4.64 (F5V) so saturation in 2.7s. So 90% full well in appx 2.4s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD 139664 is V = 4.64 (F5V) so saturation in 2.7s. So 90% full well in appx 2.4s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD 139664 is V = 4.64 (F5V) so saturation in 2.7s. So 90% full well in appx 2.4s. For long exposures at WedgeA1.0 go > 10x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD 139664 is V = 4.64 (F5V) so saturation in 2.7s. So 90% full well in appx 2.4s. For long exposures at WedgeA1.0 go > 10x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. Timing link suitability includes constraints ([97 After 96 by 0.0 to 0.1 days] [98 After 97 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. PSF10A (HD99453). PSF calibration target for HD 139664 . V = 5.17. B - V = +0.50. This is the PSF star calibrator for the flanking visits (95-98). We levy no orientation constraints on this visit (97). However, we choose this target very close in the sky to its paired science target. So as Visits 96 and 97 must be scheduled in sequential contiguous orbits, if scheduled at nominal roll (as we expect also Visit 36 will be) the we expect absolute orientations of Visits 76 and 77 to be very similar (within a few degrees). This is important so we maintain similar Sun and Beta angles for the science target and its PSF calibrator Relative Timing: This visit (97) should immediately follow visit 36 and immediately precede visit 98. I.e., They should be executed sequentially in "back-to-back" orbits. 1306208849000 80.51329986441078 (Tic-Visit :proposal-id 12228 :visit-id "97" :proposal-version -1 :trans-version "20100505" :date "28-Jun-2010 16:52:22.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 122240 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "97" :obset-id "97" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "97" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3177 :al-overhead-at-end 0 :internal-dur-at-end 433 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3516 :pcs-gap 0 ) false 1 0 SNR = 148, V = 5.17, sp = F7V, Exptime rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0). V = 5.17 (F7V) so saturation in 4.4s. So 90% full well in appx 3.9s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0). V = 5.17 (F7V) so saturation in 4.4s. So 90% full well in appx 3.9s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. V = 7.74 so saturation in 47.4.0s. So 90% full well in appx 42.7s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. For long exposures at WedgeA1.0 go <=20x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. V = 7.74 so saturation in 47.4.0s. So 90% full well in appx 42.7s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. For long exposures at WedgeA1.0 go <=20x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. Timing link suitability includes constraints ([98 After 97 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. HD 139664 (V=4.64, B-V = +0.40). Second of two sets of visits, each containing three visits of HD 139664 at different relative orientations with one PSF calibration observation interleaved. This is the third HD 139664 visit in the second set. The four visits within each set must be executed sequentally in contiguous orbits interrupted only for Earth occultation. Orientation: We wish to schedule this visit (98) at +60 deg from Visit 95. Here we specifiy exactly +48 deg , fue to scheduling limitations, though closer to +60 deg is preferable. Relative Timing: This visit (98) should immediately follow Visit 97. I.e., They should be executed sequentially in "back-to-back" orbits. 1306215701000 36.0 (Tic-Visit :proposal-id 12228 :visit-id "98" :proposal-version -1 :trans-version "20100505" :date "28-Jun-2010 16:52:24.0" :trans-errors '(:WARNINGS 3 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 122240 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "98" :obset-id "98" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "98" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3002 :al-overhead-at-end 0 :internal-dur-at-end 433 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3341 :pcs-gap 0 ) false 1 0 SNR = 188, V = 4.64, sp = F5V, Exptime rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD 139664 is V = 4.64 (F5V) so saturation in 2.7s. So 90% full well in appx 2.4s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD 139664 is V = 4.64 (F5V) so saturation in 2.7s. So 90% full well in appx 2.4s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD 139664 is V = 4.64 (F5V) so saturation in 2.7s. So 90% full well in appx 2.4s. For long exposures at WedgeA1.0 go > 10x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD 139664 is V = 4.64 (F5V) so saturation in 2.7s. So 90% full well in appx 2.4s. For long exposures at WedgeA1.0 go > 10x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. Timing link suitability includes constraints ([A2 After A1 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. PDS66 (V=10.30, B-V = +1.01, K1V). First of two sets of visits, each containing three visits of PDS 66 at different relative orientations with one PSF calibration observation interleaved. This is the first PDS 66 visit in the first set. The four visits within each set must be executed sequentally in contiguous orbits interrupted only for Earth occultation. Orientation: We wish to schedule this visit (A1) at -30 deg from Visit A2, with the absolute orientation of Visit A2 unconstrained. Relative Timing: This visit (A1) should immediately preceed visit (A2). I.e., They should be executed sequentially in "back-to-back" orbits. 1301554012000 324.0 (Tic-Visit :proposal-id 12228 :visit-id "A1" :proposal-version -1 :trans-version "20100505" :date "28-Jun-2010 16:52:26.0" :trans-errors '(:WARNINGS 7 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 17456 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "A1" :obset-id "A1" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "A1" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3266 :al-overhead-at-end 0 :internal-dur-at-end 321 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3599 :pcs-gap 0 ) false 1 0 SNR = 100, V = 10.35, sp = K1V. Exptime rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. PDS 66 is V = 10.35 so saturation in 452.6s. So 90% full well in appx 407.3s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. Timing link suitability includes constraints ([A2 After A1 by 0.0 to 0.1 days] [A3 After A2 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. PDS66 (V=10.30, B-V = +1.01, K1V). First of two sets of visits, each containing three visits of PDS 66 at different relative orientations with one PSF calibration observation interleaved. This is the second PDS 66 visit in the first set. The four visits within each set must be executed sequentally in contiguous orbits interrupted only for Earth occultation. Orientation: There are no orientation constraints on this visit (A2). Visits A1, A3, A4, A5, and A8 carry relative orientation constraints w.r.t. this visit. Relative Timing: This visit (A2) should immediately follow Visit A1 and immediately preceed Visit A3 in back-to-back orbits. 1301562089000 345.0 (Tic-Visit :proposal-id 12228 :visit-id "A2" :proposal-version -1 :trans-version "20100505" :date "28-Jun-2010 16:52:27.0" :trans-errors '(:WARNINGS 7 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 17456 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "A2" :obset-id "A2" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "A2" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3256 :al-overhead-at-end 0 :internal-dur-at-end 321 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3599 :pcs-gap 0 ) false 1 0 SNR = 100, V = 10.35, sp = K1V. Exptime rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. PDS 66 is V = 10.35 so saturation in 452.6s. So 90% full well in appx 407.3s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. Timing link suitability includes constraints ([A3 After A2 by 0.0 to 0.1 days] [A4 After A3 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. PSF0AA (CD-701017). PSF calibration target for PDS 66 . V = 9.58. B - V = +1.08. This is the PSF star calibrator for the flanking visits (A1-A4). We levy no orientation constraints on this visit (A3). However, we choose this target very close in the sky to its paired science target. So as Visits A2 and A3 must be scheduled in sequential contiguous orbits, if scheduled at nominal roll (as we expect also Visit 32 will be) the we expect absolute orientations of Visits A2 and A3 to be very similar (within a few degrees). This is important so we maintain similar Sun and Beta angles for the science target and its PSF calibrator Relative Timing: This visit (A3) should immediately follow visit A2 and immediately precede visit A4. I.e., They should be executed sequentially in "back-to-back" orbits. 1301567795000 350.6491146221458 (Tic-Visit :proposal-id 12228 :visit-id "A3" :proposal-version -1 :trans-version "20100505" :date "28-Jun-2010 16:52:29.0" :trans-errors '(:WARNINGS 11 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 27184 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "A3" :obset-id "A3" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "A3" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3309 :al-overhead-at-end 0 :internal-dur-at-end 332 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3645 :pcs-gap 0 ) false 1 0 SNR = 100, V = 9.58, sp = uncertain - assume M star form B-V Exptime rounded to nearest 0.1 secondsecond SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. V = 9.58 so saturation in 123.6s. So 90% full well in appx 111.2s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. V = 9.58 so saturation in 123.6s. So 90% full well in appx 111.2s. For long exposures go <=20x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. In THIS case only (and in Visit A7) we use Wedge0.6A for the long exposures (commensurate with the science target PDS-66). SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. Timing link suitability includes constraints ([A4 After A3 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. PDS66 (V=10.30, B-V = +1.01, K1V). First of two sets of visits, each containing three visits of PDS 66 at different relative orientations with one PSF calibration observation interleaved. This is the third PDS 66 visit in the first set. The four visits within each set must be executed sequentally in contiguous orbits interrupted only for Earth occultation. Orientation: We wish to schedule this visit (A4) at +30 deg from Visit A2, with the absolute orientation of Visit A2 unconstrained. Relative Timing: This visit (A4) should immediately follow Visit A3. I.e., They should be executed sequentially in "back-to-back" orbits. 1301573572000 6.0 (Tic-Visit :proposal-id 12228 :visit-id "A4" :proposal-version -1 :trans-version "20100505" :date "28-Jun-2010 16:52:30.0" :trans-errors '(:WARNINGS 7 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 17456 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "A4" :obset-id "A4" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "A4" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3266 :al-overhead-at-end 0 :internal-dur-at-end 321 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3599 :pcs-gap 0 ) false 1 0 SNR = 100, V = 10.35, sp = K1V. Exptime rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. PDS 66 is V = 10.35 so saturation in 452.6s. So 90% full well in appx 407.3s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. Timing link suitability includes constraints ([A6 After A5 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. PDS66 (V=10.30, B-V = +1.01, K1V). Second of two sets of visits, each containing three visits of PDS 66 at different relative orientations with one PSF calibration observation interleaved. This is the first PDS 66 visit in the second set. The four visits within each set must be executed sequentally in contiguous orbits interrupted only for Earth occultation. Relative Orientation: We wish to schedule this visit (A5) at EITHER -90 deg OR +90 deg from Visit 71. Either is equally acceptable, but there is no way to specifich this via APT 18.2, so we arbitraily specify an acceptable Orinet From in the positive range (becasuse it worked) of +70 to +110 deg (to aid in schedulability and acceptable to our needs). If guide stars or other scheduling issues arise which APT is not cognizant of that makes these linked visits unschedualable she may freely change the parity of the relative orientation to -110 deg to -70 deg from Visit A1 Schedule in orbit immediately before Visit A6. 1307206322000 44.0 (Tic-Visit :proposal-id 12228 :visit-id "A5" :proposal-version -1 :trans-version "20100505" :date "28-Jun-2010 16:52:32.0" :trans-errors '(:WARNINGS 7 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 17456 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "A5" :obset-id "A5" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "A5" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3266 :al-overhead-at-end 0 :internal-dur-at-end 321 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3599 :pcs-gap 0 ) false 1 0 SNR = 100, V = 10.35, sp = K1V. Exptime rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. PDS 66 is V = 10.35 so saturation in 452.6s. So 90% full well in appx 407.3s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. Timing link suitability includes constraints ([A6 After A5 by 0.0 to 0.1 days] [A7 After A6 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. PDS66 (V=10.30, B-V = +1.01, K1V). Second of two sets of visits, each containing three visits of HD 15745 at different relative orientations with one PSF calibration observation interleaved. This is the second PDS 66 visit in the second set. The four visits within each set must be executed sequentally in contiguous orbits interrupted only for Earth occultation. Orientation: We wish to schedule this visit (A6) at +30 deg from Visit A5. We specify this exactly, and would relax this relative orientation requirment only if a suitable guide stars cannot be found. Relative Timing: This visit (76) should immediately follow visit A5 and immediately precede visit 77. I.e., They should be executed sequentially in "back-to-back" orbits. 1307212332000 62.5 (Tic-Visit :proposal-id 12228 :visit-id "A6" :proposal-version -1 :trans-version "20100505" :date "28-Jun-2010 16:52:33.0" :trans-errors '(:WARNINGS 7 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 17456 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "A6" :obset-id "A6" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "A6" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3266 :al-overhead-at-end 0 :internal-dur-at-end 321 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3599 :pcs-gap 0 ) false 1 0 SNR = 100, V = 10.35, sp = K1V. Exptime rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. PDS 66 is V = 10.35 so saturation in 452.6s. So 90% full well in appx 407.3s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. Timing link suitability includes constraints ([A7 After A6 by 0.0 to 0.1 days] [A8 After A7 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. PSF0AA (CD-701017). PSF calibration target for PDS 66 . V = 9.58. B - V = +1.08. This is the PSF star calibrator for the flanking visits (A5-A8). We levy no orientation constraints on this visit (A7). However, we choose this target very close in the sky to its paired science target. So as Visits A6 and A7 must be scheduled in sequential contiguous orbits, if scheduled at nominal roll (as we expect also Visit 36 will be) the we expect absolute orientations of Visits A6 and A7 to be very similar (within a few degrees). This is important so we maintain similar Sun and Beta angles for the science target and its PSF calibrator Relative Timing: This visit (A7) should immediately follow visit 36 and immediately precede visit A8. I.e., They should be executed sequentially in "back-to-back" orbits. 1307217695000 62.97719024309981 (Tic-Visit :proposal-id 12228 :visit-id "A7" :proposal-version -1 :trans-version "20100505" :date "28-Jun-2010 16:52:34.0" :trans-errors '(:WARNINGS 11 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 27184 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "A7" :obset-id "A7" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "A7" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3309 :al-overhead-at-end 0 :internal-dur-at-end 332 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3645 :pcs-gap 0 ) false 1 0 SNR = 100, V = 9.58, sp = uncertain - assume M star form B-V Exptime rounded to nearest 0.1 secondsecond SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. V = 9.58 so saturation in 123.6s. So 90% full well in appx 111.2s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. V = 9.58 so saturation in 123.6s. So 90% full well in appx 111.2s. For long exposures go <=20x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. In THIS case only (and in Visit A7) we use Wedge0.6A for the long exposures (commensurate with the science target PDS-66). SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. Timing link suitability includes constraints ([A8 After A7 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 18.3.1. CASM was run in Phase II mode. PDS66 (V=10.30, B-V = +1.01, K1V). Second of two sets of visits, each containing three visits of PDS 66 at different relative orientations with one PSF calibration observation interleaved. This is the third PDS 66 visit in the second set. The four visits within each set must be executed sequentally in contiguous orbits interrupted only for Earth occultation. Orientation: We wish to schedule this visit (A8) at +60 deg from Visit A5. We specify this exactly, and would relax this relative orientation requirment only if a suitable guide stars cannot be found. Relative Timing: This visit (A8) should immediately follow Visit A7. I.e., They should be executed sequentially in "back-to-back" orbits. 1307223959000 81.0 (Tic-Visit :proposal-id 12228 :visit-id "A8" :proposal-version -1 :trans-version "20100505" :date "28-Jun-2010 16:52:36.0" :trans-errors '(:WARNINGS 7 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 17456 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "A8" :obset-id "A8" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "A8" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3266 :al-overhead-at-end 0 :internal-dur-at-end 321 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3599 :pcs-gap 0 ) false 1 0 SNR = 100, V = 10.35, sp = K1V. Exptime rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. PDS 66 is V = 10.35 so saturation in 452.6s. So 90% full well in appx 407.3s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. Timing link suitability includes constraints ([B6 After B5 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 20.2. CASM was run in Phase II mode. HD 15745 (V=7.50, B-V = +0.32). Second of two sets of visits, each containing three visits of HD 15745 at different relative orientations with one PSF calibration observation interleaved. This is the first HD 15745 visit in the second set. The four visits within each set must be executed sequentally in contiguous orbits interrupted only for Earth occultation. Relative Orientation: We wish to schedule this visit (B5) at EITHER -90 deg OR +90 deg from Visit 71. Either is equally acceptable, but there is no way to specifich this via APT 18.2. Here we specify an acceptable Orient From range of +85 to +95 deg to aid in schedulability and acceptable to our needs (but the closer to +90 which can be scheduled the better). If guide stars or other scheduling issues arise which APT is not cognizant of that makes these linked visits unschedualable our the parity and range of the relative orientation to -110 deg to -70 deg from Visit 71 Schedule in orbit immediately before Visit B6. (Tic-Visit :proposal-id 12228 :visit-id "B5" :proposal-version -1 :trans-version "20120712" :date "20-Aug-2012 11:50:21.0" :trans-errors '(:WARNINGS 17 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 57088 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "B5" :obset-id "B5" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "B5" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2694 :al-overhead-at-end 0 :internal-dur-at-end 362 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3287 :pcs-gap 0 ) true 1 0 SNR = 100, V = 7.50, sp = F2V, Exptime rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD 15745 is V = 7.50 so saturation in 38.0s. So 90% full well in appx 34.2s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD 15745 is V = 7.50 so saturation in 38.0s. So 90% full well in appx 34.2s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD 15745 is V = 7.50 so saturation in 38.0s. So 90% full well in appx 34.2s. For long exposures at WedgeA1.0 go > 10x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. Timing link suitability includes constraints ([B6 After B5 by 0.0 to 0.1 days] [B7 After B6 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 20.2. CASM was run in Phase II mode. HD 15745 (V=7.50, B-V = +0.32). Second of two sets of visits, each containing three visits of HD 15745 at different relative orientations with one PSF calibration observation interleaved. This is the second HD 15745 visit in the second set. The four visits within each set must be executed sequentally in contiguous orbits interrupted only for Earth occultation. Orientation: We wish to schedule this visit (76) at +30 deg from Visit B5. Here we specify an allowble range of +25 to +30 deg, though as close to +30 deg as possible is preferable. Relative Timing: This visit (B6) should immediately follow visit B5 and immediately precede visit B7. I.e., They should be executed sequentially in "back-to-back" orbits. (Tic-Visit :proposal-id 12228 :visit-id "B6" :proposal-version -1 :trans-version "20120712" :date "20-Aug-2012 11:50:25.0" :trans-errors '(:WARNINGS 17 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 57088 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "B6" :obset-id "B6" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "B6" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2694 :al-overhead-at-end 0 :internal-dur-at-end 362 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3287 :pcs-gap 0 ) true 1 0 SNR = 100, V = 7.50, sp = F2V, Exptime rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD 15745 is V = 7.50 so saturation in 38.0s. So 90% full well in appx 34.2s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. AU MIC is V = 8.61 so saturation in 50.6s. So 90% full well in appx 45.5s. Use this for the "short" exposures, repeated with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD 15745 is V = 7.50 so saturation in 38.0s. So 90% full well in appx 34.2s. For long exposures at WedgeA1.0 go > 10x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. Timing link suitability includes constraints ([B7 After B6 by 0.0 to 0.1 days] [B8 After B7 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 20.2. CASM was run in Phase II mode. PSF08A (HD16199). PSF calibration target for HD 15745 . V = 7.47. B - V = +0.35. This is the PSF star calibrator for the flanking visits (B5-B8). We levy no orientation constraints on this visit (B7). However, we choose this target very close in the sky to its paired science target. So as Visits B6 and B7 must be scheduled in sequential contiguous orbits, if scheduled at nominal roll (as we expect also Visit B6 will be) the we expect absolute orientations of Visits B6 and B7 to be very similar (within a few degrees). This is important so we maintain similar Sun and Beta angles for the science target and its PSF calibrator Relative Timing: This visit (B7) should immediately follow visit B6 and immediately precede visit B8. I.e., They should be executed sequentially in "back-to-back" orbits. (Tic-Visit :proposal-id 12228 :visit-id "B7" :proposal-version -1 :trans-version "20120802" :date "21-Aug-2012 07:40:20.0" :trans-errors '(:WARNINGS 15 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 57328 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "B7" :obset-id "B7" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "B7" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2722 :al-overhead-at-end 0 :internal-dur-at-end 362 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3287 :pcs-gap 0 ) true 1 0 SNR = 100, V = 7.27, sp = F2V, Exptime rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. V = 7.27 so saturation in 30.8s. So 90% full well in appx 27.7s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. V = 7.27 so saturation in 30.8s. So 90% full well in appx 27.7s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. V = 7.27 so saturation in 30.8s. So 90% full well in appx 27.7 For long exposures at WedgeA1.0 go < = 20x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position. Timing link suitability includes constraints ([B8 After B7 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 20.2. CASM was run in Phase II mode. HD 15745 (V=7.50, B-V = +0.32). Second of two sets of visits, each containing three visits of HD 15745 at different relative orientations with one PSF calibration observation interleaved. This is the third HD 15745 visit in the second set. The four visits within each set must be executed sequentally in contiguous orbits interrupted only for Earth occultation. Orientation: We wish to schedule this visit (B8) at +60 deg from Visit B5. We specify this exactly, and would relax this relative orientation requirment only if a suitable guide stars cannot be found. Here we specify an allowble range of +25 to +30 deg, though as close to +30 deg as possible is preferable. Relative Timing: This visit (B8) should immediately follow Visit B7. I.e., They should be executed sequentially in "back-to-back" orbits. (Tic-Visit :proposal-id 12228 :visit-id "B8" :proposal-version -1 :trans-version "20120712" :date "20-Aug-2012 11:50:33.0" :trans-errors '(:WARNINGS 17 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "24" :si-bright-earth-limb-angle 20.0 :data-volume 57088 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12228 :visit-id "B8" :obset-id "B8" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12228 :visit-id "B8" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2694 :al-overhead-at-end 0 :internal-dur-at-end 362 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3287 :pcs-gap 0 ) true 1 0 SNR = 100, V = 7.50, sp = F2V, Exptime rounded to nearest 0.1 second SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD 15745 is V = 7.50 so saturation in 38.0s. So 90% full well in appx 34.2s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD 15745 is V = 7.50 so saturation in 38.0s. So 90% full well in appx 34.2s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 137, appropriate for the WedgeA0.6 position. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55. HD 15745 is V = 7.50 so saturation in 38.0s. So 90% full well in appx 34.2s. For long exposures at WedgeA1.0 go > 10x deeper in each that will fit into remainer of visibility period CR-SPLIT at least 3 times - and trim exposure time to fit in visibility window. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "long" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits of the FOV (edge of the detector) on the "small" side of the Wedge A taper. Thus, for these short exposures we use SIZEAXIS12 = 427, appropriate for the WedgeA1.0 position.