The last and final submission. Fingers crossed. -2054755503 Assigned ID: 30 ----- Attempting Submission 1 (Wed Apr 02 17:20:05 GMT 2014) ----- HST Phase I Proposal 30 (CYCLE22_STIS_DISKS_000_APT_MAIN.apt) successfully submitted. ----- Attempting Submission 2 (Fri Apr 04 20:29:37 GMT 2014) ----- HST Phase I Proposal 30 (CYCLE22_STIS_DISKS_003_MAIN.apt) successfully submitted. ----- Attempting Submission 3 (Fri Apr 04 20:37:14 GMT 2014) ----- HST Phase I Proposal 30 (CYCLE22_STIS_DISKS_003_MAIN.apt) successfully submitted. ----- Attempting Submission 4 (Tue Apr 08 18:25:36 GMT 2014) ----- HST Phase I Proposal 30 (CYCLE22_STIS_DISKS_004_MAIN.apt) successfully submitted. ----- Attempting Submission 5 (Tue Apr 08 20:53:36 GMT 2014) ----- HST Phase I Proposal 30 (CYCLE22_STIS_DISKS_006_MAIN.apt) successfully submitted. ----- Attempting Submission 6 (Wed Apr 09 19:11:46 GMT 2014) ----- HST Phase I Proposal 30 (CYCLE22_STIS_DISKS_007_MAIN.apt) successfully submitted. ----- Attempting Submission 7 (Wed Apr 09 21:47:41 GMT 2014) ----- HST Phase I Proposal 30 (CYCLE22_STIS_DISKS_008_MAIN.apt) successfully submitted. ----- Attempting Submission 8 (Fri Apr 11 22:17:13 GMT 2014) ----- SUBARRAY OFF OF DETECTOR SUBARRAY OFF OF DETECTOR SUBARRAY OFF OF DETECTOR SUBARRAY OFF OF DETECTOR SUBARRAY OFF OF DETECTOR SUBARRAY OFF OF DETECTOR SUBARRAY OFF OF DETECTOR SUBARRAY OFF OF DETECTOR SUBARRAY OFF OF DETECTOR SUBARRAY OFF OF DETECTOR SUBARRAY OFF OF DETECTOR SUBARRAY OFF OF DETECTOR SUBARRAY OFF OF DETECTOR SUBARRAY OFF OF DETECTOR SUBARRAY OFF OF DETECTOR SUBARRAY OFF OF DETECTOR SUBARRAY OFF OF DETECTOR SUBARRAY OFF OF DETECTOR SUBARRAY OFF OF DETECTOR SUBARRAY OFF OF DETECTOR SUBARRAY OFF OF DETECTOR SUBARRAY OFF OF DETECTOR SUBARRAY OFF OF DETECTOR SUBARRAY OFF OF DETECTOR SUBARRAY OFF OF DETECTOR SUBARRAY OFF OF DETECTOR STIS EXPOSURE TIME ROUNDED DOWN TO NEAREST 0.1 SECONDS STIS EXPOSURE TIME ROUNDED DOWN TO NEAREST 0.1 SECONDS STIS EXPOSURE TIME ROUNDED DOWN TO NEAREST 0.1 SECONDS STIS EXPOSURE TIME ROUNDED DOWN TO NEAREST 0.1 SECONDS STIS EXPOSURE TIME ROUNDED DOWN TO NEAREST 0.1 SECONDS STIS EXPOSURE TIME ROUNDED DOWN TO NEAREST 0.1 SECONDS STIS EXPOSURE TIME ROUNDED DOWN TO NEAREST 0.1 SECONDS STIS EXPOSURE TIME ROUNDED DOWN TO NEAREST 0.1 SECONDS STIS EXPOSURE TIME ROUNDED DOWN TO NEAREST 0.1 SECONDS STIS EXPOSURE TIME ROUNDED DOWN TO NEAREST 0.1 SECONDS SUBARRAY OFF OF DETECTOR SUBARRAY OFF OF DETECTOR SUBARRAY OFF OF DETECTOR SUBARRAY OFF OF DETECTOR SUBARRAY OFF OF DETECTOR SUBARRAY OFF OF DETECTOR SUBARRAY OFF OF DETECTOR SUBARRAY OFF OF DETECTOR SUBARRAY OFF OF DETECTOR ORBITAL VISIBILITY OVERRUN SUBARRAY OFF OF DETECTOR SUBARRAY OFF OF DETECTOR SUBARRAY OFF OF DETECTOR SUBARRAY OFF OF DETECTOR SUBARRAY OFF OF DETECTOR SUBARRAY OFF OF DETECTOR SUBARRAY OFF OF DETECTOR SUBARRAY OFF OF DETECTOR SUBARRAY OFF OF DETECTOR SUBARRAY OFF OF DETECTOR SUBARRAY OFF OF DETECTOR SUBARRAY OFF OF DETECTOR SUBARRAY OFF OF DETECTOR SUBARRAY OFF OF DETECTOR SUBARRAY OFF OF DETECTOR ORBITAL VISIBILITY OVERRUN SUBARRAY OFF OF DETECTOR SUBARRAY OFF OF DETECTOR SUBARRAY OFF OF DETECTOR SUBARRAY OFF OF DETECTOR SUBARRAY OFF OF DETECTOR STIS EXPOSURE TIME ROUNDED DOWN TO NEAREST 0.1 SECONDS SUBARRAY OFF OF DETECTOR ORBITAL VISIBILITY OVERRUN STIS EXPOSURE TIME ROUNDED DOWN TO NEAREST 0.1 SECONDS STIS EXPOSURE TIME ROUNDED DOWN TO NEAREST 0.1 SECONDS STIS EXPOSURE TIME ROUNDED DOWN TO NEAREST 0.1 SECONDS STIS EXPOSURE TIME ROUNDED DOWN TO NEAREST 0.1 SECONDS SUBARRAY OFF OF DETECTOR SUBARRAY OFF OF DETECTOR STIS EXPOSURE TIME ROUNDED DOWN TO NEAREST 0.1 SECONDS STIS EXPOSURE TIME ROUNDED DOWN TO NEAREST 0.1 SECONDS SUBARRAY OFF OF DETECTOR SUBARRAY OFF OF DETECTOR STIS EXPOSURE TIME ROUNDED DOWN TO NEAREST 0.1 SECONDS STIS EXPOSURE TIME ROUNDED DOWN TO NEAREST 0.1 SECONDS STIS EXPOSURE TIME ROUNDED DOWN TO NEAREST 0.1 SECONDS SUBARRAY OFF OF DETECTOR ORBITAL VISIBILITY OVERRUN SUBARRAY OFF OF DETECTOR SUBARRAY OFF OF DETECTOR SUBARRAY OFF OF DETECTOR SUBARRAY OFF OF DETECTOR SUBARRAY OFF OF DETECTOR SUBARRAY OFF OF DETECTOR SUBARRAY OFF OF DETECTOR Updates exposure time and number of repetitions for Wedge 1.0 imaging in Visit 53. Increased UNUSED back end portion of visibility window to 171 sec to enable mid-Oct schedualability 1684638448 ----- Attempting Submission 1 (Wed Jul 09 23:06:20 GMT 2014) ----- ----- Attempting Submission 2 (Mon Jun 01 19:58:17 GMT 2015) ----- ----- Attempting Submission 3 (Mon Aug 03 20:17:31 GMT 2015) ----- HST Phase II Proposal 13786 (GO3786_03AUG2015.apt) successfully submitted. Receipt: # 13786-3 ----- Attempting Submission 4 (Tue Aug 04 15:37:20 GMT 2015) ----- - Ran target conf. charts prior AND we preciously observed this target in these apertures. - Orbit and Visit planners were run on the linked visits set 51 - 58 and found AOK I didn't re-run it for the other visits previously exeucted or run prior for the other visits planned prior awaiting execution. - Warnings: Just the usual "sub-array out of aperture" (it is not), exposure time rounded dowen to nearest 0.1s - AOK, and a warning Visit 57 is too long - but that one already executed!for How do circumstellar (CS) disks evolve and form planetary systems? Is our solar system's two-component debris disk (DD) typical? Are planets implicated by evidence of dynamical stirring in disks? Are DD architectures correlated with stellar mass? To address these highly-compelling questions of fundamental astrophysical import, we propose follow-up STIS coronagraphy of five intermediate-inclination ring-like DDs. These images will provide unprecedented clarity, sensitivity, and photometric efficacy to: 1) Study the spatial distribution of dust as close as 0.2" from the host stars enabling us to infer the existence and properties of unseen co-orbiting planets, and to probe disk-planet interactions across stellar ages and spectral types; 2) Provide spatially resolved imaging within DD regions previously unsampled to significantly improve constraints on disk grain properties and radial segregation of grain populations as a function of stellocentric distance (and thus temperature); 3) Produce high-fidelity images of DD substructures for dynamical interpretation, constraining the possibilities for planetary system architectures; 4) Obtain deep images of regions beyond the primary, bright debris features to study small-grain populations that might be unbound from the system and affected by both extrinsic and intrinsic forces and may inform about the level of dynamical activity in the planetesimal belt; 5) Provide, through the HLA, the highest quality and most complete, value-added data products for a seminal legacy data set of spatially resolvable light-scattering DDs, thus enabling multi-wavelength investigations with new and future ground- and space-based facilities. TARGETS & OCCULTING APERTURES ============================= In GO 13786 we observe five debris disk hosting stars, and five B-V color-matched PSF template stars, in relatively close proximity on the sky (within ~ 10 deg) with STIS coronagraphy. The first three disk hosts (HD202628, HD207129, and HD202917) on the target list are G-type stars and we observe them and their paired PSF template stars with both the STIS WedgeA0.6 and Wedge1.0A occulting apertures. The last two disk hosts (HD14156 and HR4796) on the target list are A-type stars and we observe them and their paired PSF template stars with both the STIS BAR5 and Wedge1.0A occulting apertures. *** Note to PC and CS: The use of the BAR5 occulter was commissioned (by us) in GO program 12923, but is syntactically unavailable in APT 22.2. Additionally, its fiducial SIAF position as a result our astrometric calibrations has not (yet) been updated in the PDB SIAF.dat file or flowed down to other elements of the ground system. Therefore, to make use of the BAR5 aperture, we define our reference pointings using the BAR10 position mnemonically in APT with POS TARGs to offset to the mid-line and +/- 1/4-pixel dithered positions we use to observe with BAR5 in this program. *** NOTE TO PC: We assume *NO* BAR10 updates to its reference pixel position in the PDB/SIAF.dat file (or ground system population) since our GO program 12923. If this is altered, before GO 13786 executes, we must update our POS TARGs accordingly. If BAR5 becomes defined in the PDB SIAF.DAT and ground system S/W with the GO 12923 recommended position this proposal can be updated accordingly (but not necessary unless the BAR10 definition is changed). EIGHT SINGLE-ORBIT VISIT STRUCTURES FOR TARGET+PSF STARS ======================================================= Each disk-host target and its color-matched PSF star are observed in two sets of four sequential (back to back) single-orbit visits (eight orbits total per target+psf star). Within four orbits within each set of four must be "back to back" orbits, spaced only by Earth occultation (we use AFTER relative timing requirements to enforce this on the relevant visits). There is NO timing linkage requirement between the first set of four visits and the second set of four visits, but there are relative orientation requirements that will determine the schedualability. For each target we observe the disk-host first in two orbits (at different S/C orientation angles), then the PSF star (naturally at nominal roll), then the disk-host again at a third orientation angle. This defines the first set of four orbits. We then re-observe with this four-orbit sequence but at three additional S/C orientation angles for the disk-hosts with the PSF star interleaved in the same manner. RELATIVE ORIENTATIONS: By design, for each disk-host target and its matching PSF star the following relative orientations are optimal and desired (but not necessarily possible - this is our design goal). Here we use Visit numbers for each target as they are assigned within the observation plan for a representative target. VISITS V#1 - V#4 in Back-to-Back Orbits ======================================= V#1 DISK-HOST Orient from V#2 by -30 deg V#2 DISK-HOST Nominal (or other) Roll as Scheduled by STScI V#3 PSF-STAR Nominal (or other) Roll as Scheduled by STScI V#4 DISK-HOST Orient from V#2 by +30 deg VISITS V#5 - V#8 in Back-to-Back Orbits No Timing Linkage between the First (V#1-4) and Second (V#5-8) Set of Orbits ======================================= V#5 DISK-HOST Orient from V#1 by +90 deg *OR* -90 deg V#6 DISK-HOST Orient from V#5 by +30 deg V#7 PSF-STAR Nominal (or other) Roll as Scheduled by STScI V#8 DISK-HOST Orient from V#5 by +60 deg (Note: Information only: We expect the target/PSF imaging in V#2/V#3, and V#6/V#7, each to be at very similar celestial orientation (roll) angles due to the close proximity in the sky of the target/PSF stars and one-orbit timing linkages. Thus, we do not over-constrain the V#3 and V#7 roll angles (e.g., no "same orient as") as they naturally will be sufficiently similar so as not to induce inter-visit breathing modes.) *** NOTE TO PC: In V#5, a relative orientation w.r.t. V#1 of either +90 or -90 deg (between the two sets of visits) is acceptable. There is no way to specify this dual allowed relative orientation in APT 22.2. Thus we have used one or the other for which APT 22.2 first indicated link-set schedualbility for all eight linked visits (for each target). The PC is free to change the parity of the relative orientation in V#5 if scheduling is further constrained (unknown to APT) by guide stars or other issues. *** NOTE TO PC: While the relative 30-degree incremental orientation differences are optimal for our needs, we recognize across the link-set for each target this may not be schedulable in the face of guide star availabilities or other constraints not modeled by APT 22.2. We therefore specify only loose tolerances with allowable roll ranges as follows: VISITS V#1 - V#4 in Back-to-Back Orbits ======================================= V#1 DISK-HOST Orient from V#2 by -30 to -15 deg V#2 DISK-HOST Nominal (or other) Roll as Scheduled by STScI V#3 PSF-STAR Nominal (or other) Roll as Scheduled by STScI V#4 DISK-HOST Orient from V#2 by +15 to +30 deg VISITS V#5 - V#8 in Back-to-Back Orbits No Timing Linkage between the First (V#1-4) and Second (V#5-8) Set of Orbits ======================================= V#5 DISK-HOST Orient from V#1 by +75 to +105 deg *OR* -105 deg to -75 deg V#6 DISK-HOST Orient from V#5 by +15 to +30 deg V#7 PSF-STAR Nominal (or other) Roll as Scheduled by STScI V#8 DISK-HOST Orient from V#5 by +45 to +60 deg *** IMPORTANT NOTE **** TO PC: When scheduling, *PLEASE* select relative orientations as close to the optimal roll differentials as noted above and commented in the observing plan for each visit. I.e., -30, +30 from V#2 in V#1 and V#4, respectively; +30, +60 from V#5 in V#6 and V#8, respectively; and +90 from V#1 in V#5. EXCEPT for V3* (HD 141569) see immediately below. SPECIAL NOTE ON RELATIVE ORIENTATIONS FOR VISITS V31, V34, V35, V36, and V38 (HD 141569) ======================================================= SPECIAL NOTE ON RELATIVE ORIENTATIONS FOR VISITS V31, V34, V35, V36, and V38 (HD 141569) - Finding schedualability for this with APT 22.2 was a bear! But we did. Here we (necessarily) define our relative orientations except for Visit 35 in the negative domain. A positive domain solution was also found but was even more constraining on the possible roll ranges so we define what you see here. We would LIKE (if possible!) to increase the roll ranges on these target visits, and have put special notes of explanation/desire in the Visit level comments for our PC. Please see! We did not "tweak" (improve) further as this, we suspect, will be informed (or constrained) also by Guide Star selection. When these visits go to implementation we would wish to review the relative orientation possibilities, if found to be less constraining then we have now assumed using the APT 22.2 Visit Planner. ORBIT LAYOUTS ============= For each disk or PSF target, in each orbit (identically for each) we perform: (a) a coronagraphic (no peak-up) imaging target acquisition (b) a series of "short" 50CCD/CORON exposures with Wedge0.6A or BAR5 occulters (c) a series of "long" 50CCD/CORN exposures with the Wedge1.0A occulter We use the STIS TA/ETC to determine TA exposure times for all our targets. We predicate on SNR = 100 in the central pixel and confirm no saturation for the brightest targets. For imaging with the occulters, we determined from prior program data conservative expectations against soft-saturation at the edges of each of the occulting apertures, and plan individual exposure times at 90% of that conservative edge-saturation limit. We repeat those short exposures multiple times "filling" appx 1/3 of the visibility period (we use CR-split construct for convince). For the G-stars, using Wedge 0.6A, this is at a fixed location. For the A-stars using BOX5 we actually "dither" by +/- 1/4 pixel above and below the mid-line of the BAR5 "finger" in sets of eight short images. For the deeper Wedge1.0A images we plan for individual exposure times <= 20x the calculated 90% to soft-saturation depth for Wedge 0.6A -- and use that for our BAR5 short exposure targets as well. (For the faintest targets we cannot het quite that deep). These are repeated multiple times to fill the remainder of the target visibility period. NOTES ON CALCULATED EXPOSURE TIMES ================================== WEDGE 0.6/1.0 0.3SAT is time to saturation at wedge edge with Wedge 0.3 Scaled from VB mag based on V=3.55 for A0 star 0.3-90% is time to 90% full well. This is the time for each individual WedgeA0.6 exposure 20x is IDEALLY how deep to go (individual exptime) in each of at least 3 Wedge A0.6 exposures For faintest targets that cannot be achieved, but will fill orbit as best possible TARGET VMAG SPEC ETC TAs 0.3SAT 0.3-90% 20x HD-202628 6.75 G5V STIS.ta.617096 0.2 19.05s 17.15s 343.0s HD-207129 5.58 G2V STIS.ta.617422 0.1 6.49s 5.84s 116.8s HD-202917 8.67 G7V STIS.ta.618240 1.1 111.68s 100.52s 2010.4s HD-141569 7.12 A0V STIS.ta.618242 0.3 26.79s 24.11s 482.3s HR-4796A 5.78 A0V STIS.ta.618243 0.1 7.80s 7.02s 140.4s PSF01-BX-MIC-HD202628 6.82 G0IV STIS.ta.617137 0.2 20.32s 18.30s 365.8s PSF02-TAU01-GRU-HD207129 6.04 G0V STIS.ta.617449 0.1 9.91s 8.92s 178.4s PSF03-LTT8893-HD202917 7.22 G3V STIS.ta.618251 0.3 29.38s 26.43s 528.8s PSF04-HD135298-HD141569A 7.20 A0 STIS.ta.618246 0.4 28.84s 25.96s 519.1s PSF05-HR4735-HR4796A 5.57 B9V STIS.ta.618247 0.1 6.43s 5.78s 115.7s BAR5 BR5SAT is is time to saturation at wedge edge withBAR5 Scaled from Vmag based on V=5.0 for A0 star B%-50% is time to 90% full well. This is the time for each individual BAR5 exposure TARGET VMAG SPEC ETC TAs BR5SAT BR5-90% HD-141569 7.12 A0V STIS.ta.618242 0.3 7.05s 6.34s HR-4796A 5.78 A0V STIS.ta.618243 0.1 2.05s 1.85s PSF04-HD135298-HD141569A 7.20 A0 STIS.ta.618246 0.4 7.59s 6.83s PSF05-HR4735-HR4796A 5.57 B9V STIS.ta.618247 0.1 1.69s 1.52s BAR5 = BAR10 WITH POS TARGS =========================== For the BAR5 targets, as noted, we reference the pointings to BAR10 and use POS TARGs to effect a +/- 3 point dither centered on the bar as follows: BAR10 with POSTARG 17.48331, -7.43398 (below mid-line of BAR5) BAR10 with POSTARG 17.48579, -7.42153 (on mid-line of BAR5) BAR10 with POSTARG 17.48827, -7.40908 (above mid-line of BAR5) NOTES ON APT 22.2 "MODES" ========================= NOTE TO PC: (1) As ALWAYS for coronagraphy, all observations *MUST* be done with two-FGS fine-lock guiding with a 3-gyro on-board acquistion (3GOBAD) scenario. We have specified this along with setting the "Program Coordinator Use Only" flag in APT. NOTE TO PC AND CS: (2) In order to use the BAR5 occulter (referenced from the BAR10 position) we *MUST* set the CENTERAXIS2 location for sub-array readouts. This is an "available" mode, and so we have switched the "Availability" flag for this proposal from "Supported" to "Available" Our PC and CS are fully aware of our need for these capabilities. NOTES ON PSF STARS ================== Note: We have pre-selected an alternate, suitable, PSF template star for each target, if guide-stars are problematic for those we have used here. As these are at slightly different positions in the sky (all also < 10 deg from their targets) their visibility windows may be a bit different, as well as their brightnesses, so both the orientation angles and acquisition/exposure times amy have to be tweaked. DEBRIS DISKS 12 false false false false AVAILABLE STAR G V-IV This object was generated by the targetselector and retrieved from the SIMBAD database. J2000 J2000 B-V =+0.64, Spectral Type: G5V STAR G V-IV This object was generated by the targetselector and retrieved from the SIMBAD database. J2000 J2000 B-V =+0.60, Spectral Type: G2V STAR G V-IV This object was generated by the targetselector and retrieved from the SIMBAD database. J2000 J2000 B-V =+0.65, Spectral Type: G7V STAR A0-A3 V-IV USING BAR5 J2000 J2000 B-V =+0.08, Spectral Type: A0V. STAR A0-A3 V-IV Using BAR5 J2000 J2000 B-V =+0.08, Spectral Type: A0V. N.B. STAR G V-IV HD197482 J2000 J2000 B-V = +0.64. delta(B-V) = 0.00. Spectral Type G0IV. Slew to matched target 10.4 deg STAR G V-IV LTT9179 J2000 J2000 B-V = +0.62. delta(B-V) = -0.02. Spectral Type G0V. Slew to matched target 11.0 deg STAR G V-IV J2000 J2000 B-V = +0.66. delta(B-V) = +0.01. Spectral Type G3V. Slew to matched target 7.7 deg STAR A0-A3 III-I Using BAR 5 J2000 J2000 B-V = +0.08. delta(B-V) = 0.00. Spectral Type A0. Slew to matched target 8.9deg STAR A0-A3 V-IV Using BAR5 J2000 J2000 B-V = -0.01. delta(B-V) = 0.00. Spectral Type B9V. Slew to matched target 87.3 deg STAR G V-IV Replacement PSF for BX Mic (PSF01, Visit 03) due to 5" background contamination from faint field star. Ner-equal brightness star at angular separation 55" (OK). HD-200011 J2000 B = 7.32, B-V = +0.68 (delta(B-V) = -0.04, Spectral Type G3IV. Slew to matched target 3.0 deg 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 23.0. CASM was run in Phase II mode. 1433188475818 HD 202628 (V=6.75, B-V = +0.64). First of two sets of visits, each containing three visits of HD 202628 at different relative orientations with one PSF calibration observation interleaved. This is the first HD 202628 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. We allow a relative orientation tolerence from -15 deg to -30 deg to assist in guide star selection and scheduling. NOTE to PC: Schedule as close to -30 deg from Visit 02 as possible. Relative Timing: This visit (01) should immediately preceed visit (02). I.e., They should be executed sequentially in "back-to-back" orbits. (Tic-Visit :proposal-id 13786 :visit-id "01" :proposal-version -1 :trans-version "20150128" :date "01-Jun-2015 12:54:32.0" :trans-errors '(:WARNINGS 20 :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 86752 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13786 :visit-id "01" :obset-id "01" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13786 :visit-id "01" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2983 :al-overhead-at-end 0 :internal-dur-at-end 393 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3316 :pcs-gap 0 ) true 1 0 SNR = 100, V = 6.75, sp = G5V, Exptime rounded to nearest 0.1 second ETC Request ID: STIS.ta.617096 SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD 202628 is V = 6.75 so saturation in 19.05s. So 90% full well in appx 17.15s. 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 202628 is V = 6.75 so saturation in 19.05s. So 90% full well in appx 17.15s. 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 202628 is V = 6.75 so saturation in 19.05s. So 90% full well in appx 17.15s. 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" (Wedge0.6) from wings of stellar PSF in 1 second for V=3.55 HD 202628 is V = 6.75 so saturation in 19.05s in Wedge0.6 images So 90% full well in appx 17.15s. 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 ([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 23.0. CASM was run in Phase II mode. 1433188484305 HD 202628 (V=6.75, B-V = +0.64). First of two sets of visits, each containing three visits of HD 202628 at different relative orientations with one PSF calibration observation interleaved. This is the second HD 202628 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). This visit at nominal roll as scheduled by STScI. Visits 01, 04, 05, 06 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. (Tic-Visit :proposal-id 13786 :visit-id "02" :proposal-version -1 :trans-version "20150128" :date "01-Jun-2015 12:54:40.0" :trans-errors '(:WARNINGS 20 :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 86752 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13786 :visit-id "02" :obset-id "02" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13786 :visit-id "02" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2983 :al-overhead-at-end 0 :internal-dur-at-end 393 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3316 :pcs-gap 0 ) true 1 0 SNR = 100, V = 6.75, sp = G5V, Exptime rounded to nearest 0.1 second ETC Request ID: STIS.ta.617096 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 ([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 23.0. CASM was run in Phase II mode. 1433188493676 PSF01B (HR 8042). B = 7.32, B-V = +0.68 (delta(B-V) = -0.04, Spectral Type G3IV. Slew to matched target 3.0 deg 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) then 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. (Tic-Visit :proposal-id 13786 :visit-id "03" :proposal-version -1 :trans-version "20150128" :date "01-Jun-2015 12:54:50.0" :trans-errors '(:WARNINGS 20 :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 13786 :visit-id "03" :obset-id "03" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13786 :visit-id "03" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2980 :al-overhead-at-end 0 :internal-dur-at-end 402 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3316 :pcs-gap 0 ) true 1 0 SNR = 100, V = 6.64, sp = G3IV, Exptime (0.176s) rounded to nearest 0.1 second ETC Request ID: STIS.ta.710657 SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HR 8042 is V = 6.64, so saturation in 17.12s L So 90% full well in appx 15.50s. 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 SIZEAXIS2 = 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). HR 8042 is V = 6.64, so saturation in 17.12s L So 90% full well in appx 15.50s. 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 SIZEAXIS2 = 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). HR 8042 is V = 6.64, so saturation in 17.12s L So 90% full well in appx 15.50s. 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. HR 8042 is V = 6.64, so saturation in 17.12s L So 90% full well in appx 15.50s. For long exposures at WedgeA1.0 go 10-20x 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 23.0. CASM was run in Phase II mode. 1433188503371 HD 202628 (V=6.75, B-V = +0.64). First of two sets of visits, each containing three visits of HD 202628 at different relative orientations with one PSF calibration observation interleaved. This is the third HD 202628 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. We allow a relative orientation tolerence from +15 deg to +30 deg to assist in guide star selection and scheduling. NOTE to PC: Schedule as close to +30 deg from Visit 02 as possible. Relative Timing: This visit (04) should immediately follow Visit 03. I.e., They should be executed sequentially in "back-to-back" orbits. (Tic-Visit :proposal-id 13786 :visit-id "04" :proposal-version -1 :trans-version "20150128" :date "01-Jun-2015 12:55:00.0" :trans-errors '(:WARNINGS 20 :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 86752 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13786 :visit-id "04" :obset-id "04" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13786 :visit-id "04" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2983 :al-overhead-at-end 0 :internal-dur-at-end 393 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3316 :pcs-gap 0 ) true 1 0 SNR = 100, V = 6.75, sp = G5V, Exptime rounded to nearest 0.1 second ETC Request ID: STIS.ta.617096 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 (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 ~ 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 23.0. CASM was run in Phase II mode. 1433186776858 HD 202628 (V=6.75, B-V = +0.64). Second of two sets of visits, each containing three visits of HD 202628 at different relative orientations with one PSF calibration observation interleaved. This is the first HD 202628 visit in the first 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 (+ or -) is equally acceptable, but there is no way to specificy this via APT 22.2. Here we specify a range of positive relative orientations of -75 deg to -105 deg to assist in guide star selection and scheduling. NOTE to PC: Schedule as close to -90 deg from Visit 01 as possible. Note to PC: You may freely change the parity of the relative orientation to negative if needed for guise star selection and scheduling. Relative Timing: Schedule in orbit immediately before Visit 06, 1432978127000 288.0 (Tic-Visit :proposal-id 13786 :visit-id "05" :proposal-version -1 :trans-version "20150128" :date "01-Jun-2015 12:26:13.0" :trans-errors '(:WARNINGS 20 :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 86752 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13786 :visit-id "05" :obset-id "05" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13786 :visit-id "05" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2983 :al-overhead-at-end 0 :internal-dur-at-end 393 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3316 :pcs-gap 0 ) true 1 0 SNR = 100, V = 6.75, sp = G5V, Exptime rounded to nearest 0.1 second ETC Request ID: STIS.ta.617096 SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD 202628 is V = 6.75 so saturation in 19.05s. So 90% full well in appx 17.15s. 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 202628 is V = 6.75 so saturation in 19.05s. So 90% full well in appx 17.15s. 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 202628 is V = 6.75 so saturation in 19.05s. So 90% full well in appx 17.15s. 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" (Wedge0.6) from wings of stellar PSF in 1 second for V=3.55 HD 202628 is V = 6.75 so saturation in 19.05s in Wedge0.6 images So 90% full well in appx 17.15s. 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 ([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 23.0. CASM was run in Phase II mode. 1433186784922 HD 202628 (V=6.75, B-V = +0.64). First of two sets of visits, each containing three visits of HD 202628 at different relative orientations with one PSF calibration observation interleaved. This is the second HD 202628 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 (06) at -30 deg from Visit 05. We allow a relative orientation tolerence from -15 deg to -30 deg to assist in guide star selection and scheduling. NOTE to PC: Schedule as close to -30 deg from Visit 05 as possible. 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. 1432984018000 265.0 (Tic-Visit :proposal-id 13786 :visit-id "06" :proposal-version -1 :trans-version "20150128" :date "01-Jun-2015 12:26:22.0" :trans-errors '(:WARNINGS 20 :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 86752 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13786 :visit-id "06" :obset-id "06" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13786 :visit-id "06" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2983 :al-overhead-at-end 0 :internal-dur-at-end 393 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3316 :pcs-gap 0 ) true 1 0 SNR = 100, V = 6.75, sp = G5V, Exptime rounded to nearest 0.1 second ETC Request ID: STIS.ta.617096 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 ([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 23.0. CASM was run in Phase II mode. 1433186796809 PSF01 (MX MIC). PSF calibration target for HD 202628. V = 6.81. B - V = +0.46. Sp G0IV This is the PSF star calibrator for the flanking visits (04-08). 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 06 and 07 must be scheduled in sequential contiguous orbits, if scheduled at nominal roll (as we expect also Visit 06 will be) then 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. 1432989705000 260.0 (Tic-Visit :proposal-id 13786 :visit-id "07" :proposal-version -1 :trans-version "20150128" :date "01-Jun-2015 12:26:34.0" :trans-errors '(:WARNINGS 20 :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 86752 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13786 :visit-id "07" :obset-id "07" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13786 :visit-id "07" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2943 :al-overhead-at-end 0 :internal-dur-at-end 393 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3278 :pcs-gap 0 ) true 1 0 SNR = 100, V = 6.8.2, sp = G0IV, Exptime rounded to nearest 0.1 second ETC Request ID: STIS.ta.617137 SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). BX MIC is V = 6.82, so saturation in 20.32s. So 90% full well in appx 18.3s. 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 SIZEAXIS2 = 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). BX MIC is V = 6.82, so saturation in 20.32s. So 90% full well in appx 18.3s. 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 SIZEAXIS2 = 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). BX MIC is V = 6.82, so saturation in 20.32s. So 90% full well in appx 18.3s. 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. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). BX MIC is V = 6.82, so saturation in 20.32s. So 90% full well in appx 18.3s. 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 ([08 After 07 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 23.0. CASM was run in Phase II mode. 1433186806724 HD 202628 (V=6.75, B-V = +0.64). First of two sets of visits, each containing three visits of HD 202628 at different relative orientations with one PSF calibration observation interleaved. This is the third HD 202628 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 (08) at -60 deg from Visit 05. We allow a relative orientation tolerence from -45 deg to -60 deg to assist in guide star selection and scheduling. NOTE to PC: Schedule as close to -60 deg from Visit 05 as possible. Relative Timing: This visit (08) should immediately follow Visit 07. I.e., They should be executed sequentially in "back-to-back" orbits. 1432995301000 242.0 (Tic-Visit :proposal-id 13786 :visit-id "08" :proposal-version -1 :trans-version "20150128" :date "01-Jun-2015 12:26:44.0" :trans-errors '(:WARNINGS 20 :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 86752 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13786 :visit-id "08" :obset-id "08" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13786 :visit-id "08" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2983 :al-overhead-at-end 0 :internal-dur-at-end 393 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3316 :pcs-gap 0 ) true 1 0 SNR = 100, V = 6.75, sp = G5V, Exptime rounded to nearest 0.1 second ETC Request ID: STIS.ta.617096 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 (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 ~ 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 22.2. CASM was run in Phase II mode. 1404777944736 HD 207129 (V=5.58, B-V = +0.60). First of two sets of visits, each containing three visits of HD 207129 at different relative orientations with one PSF calibration observation interleaved. This is the first HD 207129 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. We allow a relative orientation tolerence from 15 deg to 30 deg to assist in guide star selection and scheduling. NOTE to PC: Schedule as close to 30 deg from Visit 12 as possible. Relative Timing: This visit (11) should immediately preceed visit (12). I.e., They should be executed sequentially in "back-to-back" orbits. 1438723437000 356.65999999999997 (Tic-Visit :proposal-id 13786 :visit-id "11" :proposal-version -1 :trans-version "20140605" :date "07-Jul-2014 17:05:42.0" :trans-errors '(:WARNINGS 48 :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 156784 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13786 :visit-id "11" :obset-id "11" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13786 :visit-id "11" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2965 :al-overhead-at-end 0 :internal-dur-at-end 381 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3358 :pcs-gap 0 ) false 1 0 SNR = 100, V = 5.58, sp = G2V, Exptime rounded to nearest 0.1 second Min exp time will not saturate, and will give SNR = 173 ETC Request ID: STIS.ta.617422 SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD 207129 is V = 5.58 so saturation in 6.49s. So 90% full well in appx 5.84s. 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 207129 is V = 5.58 so saturation in 6.49s. So 90% full well in appx 5.84s. 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 207129 is V = 5.58 so saturation in 6.49s. So 90% full well in appx 5.84s. 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" (Wedge0.6) 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 207129 is V = 5.58 so saturation in 6.49s. So 90% full well in appx 5.84s. 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. SCALABLE BENCHMARK: We expect full-well at r=0.3" (Wedge0.6) 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 207129 is V = 5.58 so saturation in 6.49s. So 90% full well in appx 5.84s. 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 ([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 22.2. CASM was run in Phase II mode. 1404777746181 HD 207129 (V=5.58, B-V = +0.60). First of two sets of visits, each containing three visits of HD 202628 at different relative orientations with one PSF calibration observation interleaved. This is the second HD 207129 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). This visit at nominal roll as scheduled by STScI. Visits 11, 14, 15, 16 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. 1438729166000 334.65999999999997 (Tic-Visit :proposal-id 13786 :visit-id "12" :proposal-version -1 :trans-version "20140605" :date "07-Jul-2014 17:02:23.0" :trans-errors '(:WARNINGS 48 :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 156784 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13786 :visit-id "12" :obset-id "12" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13786 :visit-id "12" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2965 :al-overhead-at-end 0 :internal-dur-at-end 381 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3358 :pcs-gap 0 ) false 1 0 SNR = 100, V = 5.58, sp = G2V, Exptime rounded to nearest 0.1 second Min exp time will not saturate, and will give SNR = 173 ETC Request ID: STIS.ta.617422 SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD 207129 is V = 5.58 so saturation in 6.49s. So 90% full well in appx 5.84s. 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 207129 is V = 5.58 so saturation in 6.49s. So 90% full well in appx 5.84s. 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 207129 is V = 5.58 so saturation in 6.49s. So 90% full well in appx 5.84s. 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" (Wedge0.6) 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 207129 is V = 5.58 so saturation in 6.49s. So 90% full well in appx 5.84s. 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. SCALABLE BENCHMARK: We expect full-well at r=0.3" (Wedge0.6) 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 207129 is V = 5.58 so saturation in 6.49s. So 90% full well in appx 5.84s. 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 ([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 22.2. CASM was run in Phase II mode. 1404777752166 PSF02 (Tau01 Gru). PSF calibration target for HD 202917. V = 6.04. B - V = +0.62. Sp G2V 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) then 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. 1438735207000 313.24899675099607 (Tic-Visit :proposal-id 13786 :visit-id "13" :proposal-version -1 :trans-version "20140605" :date "07-Jul-2014 17:02:29.0" :trans-errors '(:WARNINGS 46 :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 131728 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13786 :visit-id "13" :obset-id "13" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13786 :visit-id "13" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3023 :al-overhead-at-end 0 :internal-dur-at-end 442 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3358 :pcs-gap 0 ) false 1 0 SNR = 100, V = 6.04, sp = G0IV, Exptime rounded to nearest 0.1 second 0.1s yields non-saturated SNR 100 ETC Request ID:STIS.ta.617449 SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). Tau01 Gru is V = 6.04, so saturation in 9.91s. So 90% full well in appx 8.92s. 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 SIZEAXIS2 = 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). Tau01 Gru is V = 6.04, so saturation in 9.91s. So 90% full well in appx 8.92s. 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 SIZEAXIS2 = 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). Tau01 Gru is V = 6.04, so saturation in 9.91s. So 90% full well in appx 8.92s. 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 SIZEAXIS2 = 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). Tau01 Gru is V = 6.04, so saturation in 9.91s. So 90% full well in appx 8.92s. 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 (A0V). Tau01 Gru is V = 6.04, so saturation in 9.91s. So 90% full well in appx 8.92s. 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 ([14 After 13 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 22.2. CASM was run in Phase II mode. 1404777953216 HD 207129 (V=5.58, B-V = +0.60). First of two sets of visits, each containing three visits of HD207129 at different relative orientations with one PSF calibration observation interleaved. This is the third HD 207129 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. We allow a relative orientation tolerence from -15 deg to -30 deg to assist in guide star selection and scheduling. NOTE to PC: Schedule as close to -30 deg from Visit 12 as possible. Relative Timing: This visit (14) should immediately follow Visit 13. I.e., They should be executed sequentially in "back-to-back" orbits. 1438740624000 314.65999999999997 (Tic-Visit :proposal-id 13786 :visit-id "14" :proposal-version -1 :trans-version "20140605" :date "07-Jul-2014 17:05:50.0" :trans-errors '(:WARNINGS 48 :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 156784 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13786 :visit-id "14" :obset-id "14" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13786 :visit-id "14" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2965 :al-overhead-at-end 0 :internal-dur-at-end 381 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3358 :pcs-gap 0 ) false 1 0 SNR = 100, V = 5.58, sp = G2V, Exptime rounded to nearest 0.1 second Min exp time will not saturate, and will give SNR = 173 ETC Request ID: STIS.ta.617422 SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD 207129 is V = 5.58 so saturation in 6.49s. So 90% full well in appx 5.84s. 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 207129 is V = 5.58 so saturation in 6.49s. So 90% full well in appx 5.84s. 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 207129 is V = 5.58 so saturation in 6.49s. So 90% full well in appx 5.84s. 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" (Wedge0.6) 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 207129 is V = 5.58 so saturation in 6.49s. So 90% full well in appx 5.84s. 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. SCALABLE BENCHMARK: We expect full-well at r=0.3" (Wedge0.6) 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 207129 is V = 5.58 so saturation in 6.49s. So 90% full well in appx 5.84s. 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 ([16 After 15 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 22.2. CASM was run in Phase II mode. 1404777959445 HD 207129 (V=5.58, B-V = +0.60). Second of two sets of visits, each containing three visits of HD 207129 at different relative orientations with one PSF calibration observation interleaved. This is the first HD 207129 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 11. Either (+ or -) is equally acceptable, but there is no way to specificy this via APT 22.2. Here we specify a range of positive relative orientations of -75 deg to -105 deg to assist in guide star selection and scheduling. NOTE to PC: Schedule as close to -90 deg from Visit 11 as possible. Note to PC: You may freely change the parity of the relative orientation to negative if needed for guise star selection and scheduling. Relative Timing: Schedule in orbit immediately before Visit 26. 1432640356000 281.65999999999997 (Tic-Visit :proposal-id 13786 :visit-id "15" :proposal-version -1 :trans-version "20140605" :date "07-Jul-2014 17:05:56.0" :trans-errors '(:WARNINGS 48 :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 156784 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13786 :visit-id "15" :obset-id "15" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13786 :visit-id "15" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2965 :al-overhead-at-end 0 :internal-dur-at-end 381 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3358 :pcs-gap 0 ) false 1 0 SNR = 100, V = 5.58, sp = G2V, Exptime rounded to nearest 0.1 second Min exp time will not saturate, and will give SNR = 173 ETC Request ID: STIS.ta.617422 SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD 207129 is V = 5.58 so saturation in 6.49s. So 90% full well in appx 5.84s. 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 207129 is V = 5.58 so saturation in 6.49s. So 90% full well in appx 5.84s. 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 207129 is V = 5.58 so saturation in 6.49s. So 90% full well in appx 5.84s. 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" (Wedge0.6) 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 207129 is V = 5.58 so saturation in 6.49s. So 90% full well in appx 5.84s. 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. SCALABLE BENCHMARK: We expect full-well at r=0.3" (Wedge0.6) 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 207129 is V = 5.58 so saturation in 6.49s. So 90% full well in appx 5.84s. 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 ([16 After 15 by 0.0 to 0.1 days] [17 After 16 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 22.2. CASM was run in Phase II mode. 1404777966576 HD 207129 (V=5.58, B-V = +0.60). First of two sets of visits, each containing three visits of HD 207129 at different relative orientations with one PSF calibration observation interleaved. This is the second HD 207129 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 allow a relative orientation tolerence from -15 deg to -30 deg to assist in guide star selection and scheduling. NOTE to PC: Schedule as close to -30 deg from Visit 15 as possible. 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. 1432646124000 259.15999999999997 (Tic-Visit :proposal-id 13786 :visit-id "16" :proposal-version -1 :trans-version "20140605" :date "07-Jul-2014 17:06:03.0" :trans-errors '(:WARNINGS 48 :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 156784 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13786 :visit-id "16" :obset-id "16" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13786 :visit-id "16" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2965 :al-overhead-at-end 0 :internal-dur-at-end 381 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3358 :pcs-gap 0 ) false 1 0 SNR = 100, V = 5.58, sp = G2V, Exptime rounded to nearest 0.1 second Min exp time will not saturate, and will give SNR = 173 ETC Request ID: STIS.ta.617422 SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD 207129 is V = 5.58 so saturation in 6.49s. So 90% full well in appx 5.84s. 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 207129 is V = 5.58 so saturation in 6.49s. So 90% full well in appx 5.84s. 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 207129 is V = 5.58 so saturation in 6.49s. So 90% full well in appx 5.84s. 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" (Wedge0.6) 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 207129 is V = 5.58 so saturation in 6.49s. So 90% full well in appx 5.84s. 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. SCALABLE BENCHMARK: We expect full-well at r=0.3" (Wedge0.6) 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 207129 is V = 5.58 so saturation in 6.49s. So 90% full well in appx 5.84s. 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 ([17 After 16 by 0.0 to 0.1 days] [18 After 17 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 22.2. CASM was run in Phase II mode. 1404777777004 PSF02 (Tau01 Gru). PSF calibration target for HD 202917. V = 6.04. B - V = +0.62. Sp G2V This is the PSF star calibrator for the flanking visits (25-28). 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 26 and 27 must be scheduled in sequential contiguous orbits, if scheduled at nominal roll (as we expect also Visit 06 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. 1432652036000 248.0426422001574 (Tic-Visit :proposal-id 13786 :visit-id "17" :proposal-version -1 :trans-version "20140605" :date "07-Jul-2014 17:02:54.0" :trans-errors '(:WARNINGS 46 :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 131728 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13786 :visit-id "17" :obset-id "17" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13786 :visit-id "17" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3023 :al-overhead-at-end 0 :internal-dur-at-end 442 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3358 :pcs-gap 0 ) false 1 0 SNR = 100, V = 6.04, sp = G0IV, Exptime rounded to nearest 0.1 second 0.1s yields non-saturated SNR 100 ETC Request ID:STIS.ta.617449 SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). Tau01 Gru is V = 6.04, so saturation in 9.91s. So 90% full well in appx 8.92s. 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 SIZEAXIS2 = 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). Tau01 Gru is V = 6.04, so saturation in 9.91s. So 90% full well in appx 8.92s. 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 SIZEAXIS2 = 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). Tau01 Gru is V = 6.04, so saturation in 9.91s. So 90% full well in appx 8.92s. 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 SIZEAXIS2 = 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). Tau01 Gru is V = 6.04, so saturation in 9.91s. So 90% full well in appx 8.92s. 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 (A0V). Tau01 Gru is V = 6.04, so saturation in 9.91s. So 90% full well in appx 8.92s. 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 ([18 After 17 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 22.2. CASM was run in Phase II mode. 1404777973661 HD 207129 (V=5.58, B-V = +0.60). First of two sets of visits, each containing three visits of HD 207129 at different relative orientations with one PSF calibration observation interleaved. This is the third HD 207129 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 (08) at -60 deg from Visit 05. We allow a relative orientation tolerence from -45 deg to -60 deg to assist in guide star selection and scheduling. NOTE to PC: Schedule as close to -60 deg from Visit 05 as possible. Relative Timing: This visit (18) should immediately follow Visit 17. I.e., They should be executed sequentially in "back-to-back" orbits. 1432657526000 236.66 (Tic-Visit :proposal-id 13786 :visit-id "18" :proposal-version -1 :trans-version "20140605" :date "07-Jul-2014 17:06:11.0" :trans-errors '(:WARNINGS 48 :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 156784 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13786 :visit-id "18" :obset-id "18" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13786 :visit-id "18" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2965 :al-overhead-at-end 0 :internal-dur-at-end 381 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3358 :pcs-gap 0 ) false 1 0 SNR = 100, V = 5.58, sp = G2V, Exptime rounded to nearest 0.1 second Min exp time will not saturate, and will give SNR = 173 ETC Request ID: STIS.ta.617422 SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD 207129 is V = 5.58 so saturation in 6.49s. So 90% full well in appx 5.84s. 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 207129 is V = 5.58 so saturation in 6.49s. So 90% full well in appx 5.84s. 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 207129 is V = 5.58 so saturation in 6.49s. So 90% full well in appx 5.84s. 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" (Wedge0.6) 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 207129 is V = 5.58 so saturation in 6.49s. So 90% full well in appx 5.84s. 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. SCALABLE BENCHMARK: We expect full-well at r=0.3" (Wedge0.6) 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 207129 is V = 5.58 so saturation in 6.49s. So 90% full well in appx 5.84s. 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 ([22 After 21 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 22.2. CASM was run in Phase II mode. 1404835970498 HD 202917 (V=8.67, B-V = +0.65). First of two sets of visits, each containing three visits of HD 202917 at different relative orientations with one PSF calibration observation interleaved. This is the first HD 202917 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. We allow a relative orientation tolerence from 15 deg to 30 deg to assist in guide star selection and scheduling. NOTE to PC: Schedule as close to 30 deg from Visit 22 as possible. Relative Timing: This visit (21) should immediately preceed visit (22). I.e., They should be executed sequentially in "back-to-back" orbits. (Tic-Visit :proposal-id 13786 :visit-id "21" :proposal-version -1 :trans-version "20140605" :date "08-Jul-2014 09:12:49.0" :trans-errors '(:WARNINGS 8 :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 13786 :visit-id "21" :obset-id "21" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13786 :visit-id "21" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3074 :al-overhead-at-end 0 :internal-dur-at-end 346 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3409 :pcs-gap 0 ) false 1 0 SNR = 100, V = 8,67, sp = G7V, Exptime rounded to nearest 0.1 second ETC Request ID: STIS.ta.618240 SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD 202917 is V = 8.67 so saturation in 111.68s. So 90% full well in appx 100.52s. 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 202917 is V = 8.67 so saturation in 111.68s. So 90% full well in appx 100.52s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. For long exposures at WedgeA1.0 go (up to) 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 22.2. CASM was run in Phase II mode. 1404835974818 HD 202917 (V=8.67, B-V = +0.65). First of two sets of visits, each containing three visits of HD 202917 at different relative orientations with one PSF calibration observation interleaved. This is the second HD 202917 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). This visit at nominal roll as scheduled by STScI. Visits 21, 24, 25, 26 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. (Tic-Visit :proposal-id 13786 :visit-id "22" :proposal-version -1 :trans-version "20140605" :date "08-Jul-2014 09:12:53.0" :trans-errors '(:WARNINGS 8 :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 13786 :visit-id "22" :obset-id "22" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13786 :visit-id "22" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3074 :al-overhead-at-end 0 :internal-dur-at-end 346 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3409 :pcs-gap 0 ) false 1 0 SNR = 100, V = 8,67, sp = G7V, Exptime rounded to nearest 0.1 second ETC Request ID: STIS.ta.618240 SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD 202917 is V = 8.67 so saturation in 111.68s. So 90% full well in appx 100.52s. 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 202917 is V = 8.67 so saturation in 111.68s. So 90% full well in appx 100.52s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. For long exposures at WedgeA1.0 go (up to) 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 22.2. CASM was run in Phase II mode. 1404835980849 PSF03 (LTT 8893). PSF calibration target for HD 202917. V = 7.22. B - V = +0.66. Sp G3V 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) then we expect absolute orientations of Visits 22 and 23 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 22 and immediately precede visit 24. I.e., they should be executed sequentially in "back-to-back" orbits. (Tic-Visit :proposal-id 13786 :visit-id "23" :proposal-version -1 :trans-version "20140605" :date "08-Jul-2014 09:12:59.0" :trans-errors '(:WARNINGS 20 :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 54896 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13786 :visit-id "23" :obset-id "23" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13786 :visit-id "23" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3130 :al-overhead-at-end 0 :internal-dur-at-end 359 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3470 :pcs-gap 0 ) false 1 0 SNR = 100, V = 6.22, sp = G3V, Exptime rounded to nearest 0.1 second ETC Request ID: STIS.ta.618251 SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). LTT 8893 is V = 7.22, so saturation in 29.38s. So 90% full well in appx 26.43s. 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 SIZEAXIS2 = 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). LTT 8893 is V = 7.22, so saturation in 29.38s. So 90% full well in appx 26.43s. 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 SIZEAXIS2 = 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). LTT 8893 is V = 7.22, so saturation in 29.38s. So 90% full well in appx 26.43s. For long exposures at WedgeA1.0 go (at least (x20) 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 22.2. CASM was run in Phase II mode. 1404835986081 HD 202917 (V=8.67, B-V = +0.65). First of two sets of visits, each containing three visits of HD 202917 at different relative orientations with one PSF calibration observation interleaved. This is the third HD 202917 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. We allow a relative orientation tolerence from -15 deg to -30 deg to assist in guide star selection and scheduling. NOTE to PC: Schedule as close to -30 deg from Visit 22 as possible. Relative Timing: This visit (24) should immediately follow Visit 23. I.e., They should be executed sequentially in "back-to-back" orbits. (Tic-Visit :proposal-id 13786 :visit-id "24" :proposal-version -1 :trans-version "20140605" :date "08-Jul-2014 09:13:05.0" :trans-errors '(:WARNINGS 8 :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 13786 :visit-id "24" :obset-id "24" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13786 :visit-id "24" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3074 :al-overhead-at-end 0 :internal-dur-at-end 346 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3409 :pcs-gap 0 ) false 1 0 SNR = 100, V = 8,67, sp = G7V, Exptime rounded to nearest 0.1 second ETC Request ID: STIS.ta.618240 SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD 202917 is V = 8.67 so saturation in 111.68s. So 90% full well in appx 100.52s. 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 202917 is V = 8.67 so saturation in 111.68s. So 90% full well in appx 100.52s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. For long exposures at WedgeA1.0 go (up to) 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 22.2. CASM was run in Phase II mode. 1404835991559 HD 202917 (V=8.67, B-V = +0.65). Second of two sets of visits, each containing three visits of HD 202917 at different relative orientations with one PSF calibration observation interleaved. This is the first HD 202917 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 21. Either (+ or -) is equally acceptable, but there is no way to specificy this via APT 22.2. Here we specify a range of relative orientations of -75 deg to -105 deg to assist in guide star selection and scheduling. NOTE to PC: Schedule as close to -90 deg from Visit 21 as possible. Note to PC: You may freely change the parity of the relative orientation to positive if needed for guise star selection and scheduling. Relative Timing: Schedule in orbit immediately before Visit 26. 1433390801000 293.0 (Tic-Visit :proposal-id 13786 :visit-id "25" :proposal-version -1 :trans-version "20140605" :date "08-Jul-2014 09:13:10.0" :trans-errors '(:WARNINGS 8 :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 13786 :visit-id "25" :obset-id "25" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13786 :visit-id "25" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3074 :al-overhead-at-end 0 :internal-dur-at-end 346 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3409 :pcs-gap 0 ) false 1 0 SNR = 100, V = 8,67, sp = G7V, Exptime rounded to nearest 0.1 second ETC Request ID: STIS.ta.618240 SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD 202917 is V = 8.67 so saturation in 111.68s. So 90% full well in appx 100.52s. 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 202917 is V = 8.67 so saturation in 111.68s. So 90% full well in appx 100.52s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. For long exposures at WedgeA1.0 go (up to) 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 0.0 to 0.1 days]) The scheduling data was generated by CASM 22.2. CASM was run in Phase II mode. 1404835995791 HD 202917 (V=8.67, B-V = +0.65). Second of two sets of visits, each containing three visits of HD 202917 at different relative orientations with one PSF calibration observation interleaved. This is the second HD 202917 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 05. We allow a relative orientation tolerence from -15 deg to -30 deg to assist in guide star selection and scheduling. NOTE to PC: Schedule as close to -30 deg from Visit 25 as possible. 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. 1433396403000 272.5 (Tic-Visit :proposal-id 13786 :visit-id "26" :proposal-version -1 :trans-version "20140605" :date "08-Jul-2014 09:13:15.0" :trans-errors '(:WARNINGS 8 :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 13786 :visit-id "26" :obset-id "26" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13786 :visit-id "26" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3074 :al-overhead-at-end 0 :internal-dur-at-end 346 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3409 :pcs-gap 0 ) false 1 0 SNR = 100, V = 8,67, sp = G7V, Exptime rounded to nearest 0.1 second ETC Request ID: STIS.ta.618240 SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD 202917 is V = 8.67 so saturation in 111.68s. So 90% full well in appx 100.52s. 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 202917 is V = 8.67 so saturation in 111.68s. So 90% full well in appx 100.52s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. For long exposures at WedgeA1.0 go (up to) 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 0.0 to 0.1 days] [28 After 27 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 22.2. CASM was run in Phase II mode. 1404836001274 PSF03 (LTT 8893). PSF calibration target for HD 202917. V = 7.22. B - V = +0.66. Sp G3V 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. 1433400307000 263.9971884228152 (Tic-Visit :proposal-id 13786 :visit-id "27" :proposal-version -1 :trans-version "20140605" :date "08-Jul-2014 09:13:20.0" :trans-errors '(:WARNINGS 20 :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 54896 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13786 :visit-id "27" :obset-id "27" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13786 :visit-id "27" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3130 :al-overhead-at-end 0 :internal-dur-at-end 359 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3470 :pcs-gap 0 ) false 1 0 SNR = 100, V = 6.22, sp = G3V, Exptime rounded to nearest 0.1 second ETC Request ID: STIS.ta.618251 SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). LTT 8893 is V = 7.22, so saturation in 29.38s. So 90% full well in appx 26.43s. 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 SIZEAXIS2 = 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). LTT 8893 is V = 7.22, so saturation in 29.38s. So 90% full well in appx 26.43s. 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 SIZEAXIS2 = 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). LTT 8893 is V = 7.22, so saturation in 29.38s. So 90% full well in appx 26.43s. For long exposures at WedgeA1.0 go (at least (x20) 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 0.0 to 0.1 days]) The scheduling data was generated by CASM 22.2. CASM was run in Phase II mode. 1404836005236 HD 202917 (V=8.67, B-V = +0.65). Second of two sets of visits, each containing three visits of HD 202917 at different relative orientations with one PSF calibration observation interleaved. This is the third HD 202917 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 05. We allow a relative orientation tolerence from -41 deg to -60 deg to assist in guide star selection and scheduling. NOTE to PC: Schedule as close to -60 deg from Visit 25 as possible. Relative Timing: This visit (28) should immediately follow Visit 27. I.e., They should be executed sequentially in "back-to-back" orbits. 1433407566000 252.0 (Tic-Visit :proposal-id 13786 :visit-id "28" :proposal-version -1 :trans-version "20140605" :date "08-Jul-2014 09:13:24.0" :trans-errors '(:WARNINGS 8 :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 13786 :visit-id "28" :obset-id "28" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13786 :visit-id "28" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3074 :al-overhead-at-end 0 :internal-dur-at-end 346 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3409 :pcs-gap 0 ) false 1 0 SNR = 100, V = 8,67, sp = G7V, Exptime rounded to nearest 0.1 second ETC Request ID: STIS.ta.618240 SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD 202917 is V = 8.67 so saturation in 111.68s. So 90% full well in appx 100.52s. 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 202917 is V = 8.67 so saturation in 111.68s. So 90% full well in appx 100.52s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. For long exposures at WedgeA1.0 go (up to) 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 22.2. CASM was run in Phase II mode. 1404942883783 HD 141569 (V=7.12, B-V = +0.08). First of two sets of visits, each containing three visits of HD 141569 at different relative orientations with one PSF calibration observation interleaved. This is the first HD 141569 visit in the first set. The four visits within each set must be executed sequentally in contiguous orbits interrupted only for Earth occultation. Relative Orientation: Due to schedualability issues this target only is observed over a reduced foll range, and the relative orientations except for Visit 35 are defined with opposite partity as for our other targets. NOTE to PC: In Visit 31, the relative orient from range w.r.t. Visit 32 is specified as +10 to +20 deg. PLEASE schedule as close to +15 deg relative orientation as possible - but see note on Visit 35. Relative Timing: This visit (31) should immediately preceed visit (32). I.e., They should be executed sequentially in "back-to-back" orbits. (Tic-Visit :proposal-id 13786 :visit-id "31" :proposal-version -1 :trans-version "20140605" :date "09-Jul-2014 14:54:37.0" :trans-errors '(:WARNINGS 28 :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 73200 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13786 :visit-id "31" :obset-id "31" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13786 :visit-id "31" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2888 :al-overhead-at-end 0 :internal-dur-at-end 379 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3222 :pcs-gap 0 ) false 1 0 SNR = 100, V = 7.12, sp = A0V, Exptime rounded to nearest 0.1 second ETC Request ID: STIS.ta.618242 NOTE TO PC/CS: Here we use the BAR5 occulter (Aperture) that we comissioned in GO program 12923. This aperture is not available in APT Phase 2, *AND* the SIAF locations of the aperture fiducial we determined in GO 12923 is yet to be populated in SIAF.dat and flowed down to the ground system. We therefore call out BAR10 and use POS TARGs to move the target to the desired positions behind the BAR5 occulter. He we attempt to place the target on the mid-line of BAR5. We then use a subarray readout of CENTYERAXIS2 = 700 appopriate for BAR5 with a SIZEAXIS2 = 137 (the same ass we use elsewhere for Wedge0.6A). SCALABLE BENCHMARK: We expect full-well at r=0.15" with BAR10 from wings of stellar PSF in 1 second for V=5.0 (A0V) {**to be re-verified**}. HD 141569 is V = 7.12 so saturation in 7.05s. So 90% full well in appx 6.34s. Use this for the BAR5 exposures, repeated (8x) with multiple CR Splits. NOTE TO PC/CS: Here we use the BAR5 occulter (Aperture) that we comissioned in GO program 12923. This aperture is not available in APT Phase 2, *AND* the SIAF locations of the aperture fiducial we determined in GO 12923 is yet to be populated in SIAF.dat and flowed down to the ground system. We therefore call out BAR10 and use POS TARGs to move the target to the desired positions behind the BAR5 occulter. He we attempt to place the target 1/4 pixel above the midline mid-line of BAR5. We then use a subarray readout of CENTYERAXIS2 = 700 appopriate for BAR5 with a SIZEAXIS2 = 137 (the same ass we use elsewhere for Wedge0.6A). SCALABLE BENCHMARK: We expect full-well at r=0.15" with BAR10 from wings of stellar PSF in 1 second for V=5.0 (A0V) {**to be re-verified**}. HD 141569 is V = 7.12 so saturation in 7.05s. So 90% full well in appx 6.34s. Use this for the BAR5 exposures, repeated (8x) with multiple CR Splits. NOTE TO PC/CS: Here we use the BAR5 occulter (Aperture) that we comissioned in GO program 12923. This aperture is not available in APT Phase 2, *AND* the SIAF locations of the aperture fiducial we determined in GO 12923 is yet to be populated in SIAF.dat and flowed down to the ground system. We therefore call out BAR10 and use POS TARGs to move the target to the desired positions behind the BAR5 occulter. He we attempt to place the target 1/4 pixel below the midline mid-line of BAR5. We then use a subarray readout of CENTYERAXIS2 = 700 appopriate for BAR5 with a SIZEAXIS2 = 137 (the same ass we use elsewhere for Wedge0.6A). SCALABLE BENCHMARK: We expect full-well at r=0.15" with BAR10 from wings of stellar PSF in 1 second for V=5.0 (A0V) {**to be re-verified**}. HD 141569 is V = 7.12 so saturation in 7.05s. So 90% full well in appx 6.34s. Use this for the BAR5 exposures, repeated (8x) with multiple CR Splits. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD 141569 is V = 7.12 so saturation in 26.79s. So 90% full well in appx 24.11s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. For long exposures at WedgeA1.0 go (up to) 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] [33 After 32 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 22.2. CASM was run in Phase II mode. 1404779000650 HD 141569 (V=7.12, B-V = +0.08). First of two sets of visits, each containing three visits of HD 141569 at different relative orientations with one PSF calibration observation interleaved. This is the second HD 141569 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). This visit at nominal roll as scheduled by STScI. Visits 31, 34, 35, 36 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. (Tic-Visit :proposal-id 13786 :visit-id "32" :proposal-version -1 :trans-version "20140605" :date "07-Jul-2014 17:23:18.0" :trans-errors '(:WARNINGS 28 :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 73200 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13786 :visit-id "32" :obset-id "32" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13786 :visit-id "32" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2888 :al-overhead-at-end 0 :internal-dur-at-end 379 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3222 :pcs-gap 0 ) false 1 0 SNR = 100, V = 7.12, sp = A0V, Exptime rounded to nearest 0.1 second ETC Request ID: STIS.ta.618242 NOTE TO PC/CS: Here we use the BAR5 occulter (Aperture) that we comissioned in GO program 12923. This aperture is not available in APT Phase 2, *AND* the SIAF locations of the aperture fiducial we determined in GO 12923 is yet to be populated in SIAF.dat and flowed down to the ground system. We therefore call out BAR10 and use POS TARGs to move the target to the desired positions behind the BAR5 occulter. He we attempt to place the target on the mid-line of BAR5. We then use a subarray readout of CENTYERAXIS2 = 700 appopriate for BAR5 with a SIZEAXIS2 = 137 (the same ass we use elsewhere for Wedge0.6A). SCALABLE BENCHMARK: We expect full-well at r=0.15" with BAR10 from wings of stellar PSF in 1 second for V=5.0 (A0V) {**to be re-verified**}. HD 141569 is V = 7.12 so saturation in 7.05s. So 90% full well in appx 6.34s. Use this for the BAR5 exposures, repeated (8x) with multiple CR Splits. NOTE TO PC/CS: Here we use the BAR5 occulter (Aperture) that we comissioned in GO program 12923. This aperture is not available in APT Phase 2, *AND* the SIAF locations of the aperture fiducial we determined in GO 12923 is yet to be populated in SIAF.dat and flowed down to the ground system. We therefore call out BAR10 and use POS TARGs to move the target to the desired positions behind the BAR5 occulter. He we attempt to place the target 1/4 pixel above the midline mid-line of BAR5. We then use a subarray readout of CENTYERAXIS2 = 700 appopriate for BAR5 with a SIZEAXIS2 = 137 (the same ass we use elsewhere for Wedge0.6A). SCALABLE BENCHMARK: We expect full-well at r=0.15" with BAR10 from wings of stellar PSF in 1 second for V=5.0 (A0V) {**to be re-verified**}. HD 141569 is V = 7.12 so saturation in 7.05s. So 90% full well in appx 6.34s. Use this for the BAR5 exposures, repeated (8x) with multiple CR Splits. NOTE TO PC/CS: Here we use the BAR5 occulter (Aperture) that we comissioned in GO program 12923. This aperture is not available in APT Phase 2, *AND* the SIAF locations of the aperture fiducial we determined in GO 12923 is yet to be populated in SIAF.dat and flowed down to the ground system. We therefore call out BAR10 and use POS TARGs to move the target to the desired positions behind the BAR5 occulter. He we attempt to place the target 1/4 pixel below the midline mid-line of BAR5. We then use a subarray readout of CENTYERAXIS2 = 700 appopriate for BAR5 with a SIZEAXIS2 = 137 (the same ass we use elsewhere for Wedge0.6A). SCALABLE BENCHMARK: We expect full-well at r=0.15" with BAR10 from wings of stellar PSF in 1 second for V=5.0 (A0V) {**to be re-verified**}. HD 141569 is V = 7.12 so saturation in 7.05s. So 90% full well in appx 6.34s. Use this for the BAR5 exposures, repeated (8x) with multiple CR Splits. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD 141569 is V = 7.12 so saturation in 26.79s. So 90% full well in appx 24.11s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. For long exposures at WedgeA1.0 go (up to) 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 ([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 22.2. CASM was run in Phase II mode. 1404779004657 PSF04 (HD 135298. PSF calibration target for HD HD 141569. V = 7.20. B - V = +0.08. Sp A0 This is the PSF star calibrator for the flanking visits (31-34). We levy no orientation constraints on this visit (33). 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 06 will be) then 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 (33) should immediately follow visit 32 and immediately precede visit 34. I.e., they should be executed sequentially in "back-to-back" orbits. (Tic-Visit :proposal-id 13786 :visit-id "33" :proposal-version -1 :trans-version "20140605" :date "07-Jul-2014 17:23:22.0" :trans-errors '(:WARNINGS 24 :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 73200 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13786 :visit-id "33" :obset-id "33" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13786 :visit-id "33" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2888 :al-overhead-at-end 0 :internal-dur-at-end 379 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3222 :pcs-gap 0 ) false 1 0 SNR = 100, V = 7.20, sp = A0, Exptime rounded to nearest 0.1 second ETC Request ID: STIS.ta.618246 NOTE TO PC/CS: Here we use the BAR5 occulter (Aperture) that we comissioned in GO program 12923. This aperture is not available in APT Phase 2, *AND* the SIAF locations of the aperture fiducial we determined in GO 12923 is yet to be populated in SIAF.dat and flowed down to the ground system. We therefore call out BAR10 and use POS TARGs to move the target to the desired positions behind the BAR5 occulter. He we attempt to place the target on the mid-line of BAR5. We then use a subarray readout of CENTYERAXIS2 = 700 appopriate for BAR5 with a SIZEAXIS2 = 137 (the same ass we use elsewhere for Wedge0.6A). SCALABLE BENCHMARK: We expect full-well at r=0.15" with BAR10 from wings of stellar PSF in 1 second for V=5.0 (A0V) {**to be re-verified**}. HD 135298 is V = 7.20 so saturation in 7.59s. So 90% full well in appx 6.83s. Use this for the BAR5 exposures, repeated (8x) with multiple CR Splits. NOTE TO PC/CS: Here we use the BAR5 occulter (Aperture) that we comissioned in GO program 12923. This aperture is not available in APT Phase 2, *AND* the SIAF locations of the aperture fiducial we determined in GO 12923 is yet to be populated in SIAF.dat and flowed down to the ground system. We therefore call out BAR10 and use POS TARGs to move the target to the desired positions behind the BAR5 occulter. He we attempt to place the target on the mid-line of BAR5. We then use a subarray readout of CENTYERAXIS2 = 700 appopriate for BAR5 with a SIZEAXIS2 = 137 (the same ass we use elsewhere for Wedge0.6A). SCALABLE BENCHMARK: We expect full-well at r=0.15" with BAR10 from wings of stellar PSF in 1 second for V=5.0 (A0V) {**to be re-verified**}. HD 135298 is V = 7.20 so saturation in 7.59s. So 90% full well in appx 6.83s. Use this for the BAR5 exposures, repeated (8x) with multiple CR Splits. NOTE TO PC/CS: Here we use the BAR5 occulter (Aperture) that we comissioned in GO program 12923. This aperture is not available in APT Phase 2, *AND* the SIAF locations of the aperture fiducial we determined in GO 12923 is yet to be populated in SIAF.dat and flowed down to the ground system. We therefore call out BAR10 and use POS TARGs to move the target to the desired positions behind the BAR5 occulter. He we attempt to place the target on the mid-line of BAR5. We then use a subarray readout of CENTYERAXIS2 = 700 appopriate for BAR5 with a SIZEAXIS2 = 137 (the same ass we use elsewhere for Wedge0.6A). SCALABLE BENCHMARK: We expect full-well at r=0.15" with BAR10 from wings of stellar PSF in 1 second for V=5.0 (A0V) {**to be re-verified**}. HD 135298 is V = 7.20 so saturation in 7.59s. So 90% full well in appx 6.83s. Use this for the BAR5 exposures, repeated (8x) with multiple CR Splits. SCALABLE BENCHMARK: We expect full-well at r=0.3" (Wedge0.6) from wings of stellar PSF in 1 second for V=3.55 SCALABLE BENCHMARK: We expect full-well at r=0.15" with BAR10 from wings of stellar PSF in 1 second for V=5.0 (A0V) {**to be re-verified**}. HD 135298 is V = 7.20 so saturation in 7.59s. So 90% full well in appx 6.83s. 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 ([34 After 33 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 22.2. CASM was run in Phase II mode. 1404939697057 HD 141569 (V=7.12, B-V = +0.08). First of two sets of visits, each containing three visits of HD 141569 at different relative orientations with one PSF calibration observation interleaved. This is the third HD 141569 visit in the first set. The four visits within each set must be executed sequentally in contiguous orbits interrupted only for Earth occultation. Relative Orientation: Due to schedualability issues this target only is observed over a reduced foll range, and the relative orientations except for Visit 35 are defined with opposite partity as for our other targets. NOTE to PC: In Visit 31, the relative orient from range w.r.t. Visit 32 is specified as -20 to -10 deg. PLEASE schedule as close to -15 deg relative orientation as possible - but see note on Visit 35. Relative Timing: This visit (34) should immediately follow Visit 33. I.e., They should be executed sequentially in "back-to-back" orbits. (Tic-Visit :proposal-id 13786 :visit-id "34" :proposal-version -1 :trans-version "20140605" :date "09-Jul-2014 14:01:29.0" :trans-errors '(:WARNINGS 28 :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 73200 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13786 :visit-id "34" :obset-id "34" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13786 :visit-id "34" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2888 :al-overhead-at-end 0 :internal-dur-at-end 379 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3222 :pcs-gap 0 ) false 1 0 SNR = 100, V = 7.12, sp = A0V, Exptime rounded to nearest 0.1 second ETC Request ID: STIS.ta.618242 NOTE TO PC/CS: Here we use the BAR5 occulter (Aperture) that we comissioned in GO program 12923. This aperture is not available in APT Phase 2, *AND* the SIAF locations of the aperture fiducial we determined in GO 12923 is yet to be populated in SIAF.dat and flowed down to the ground system. We therefore call out BAR10 and use POS TARGs to move the target to the desired positions behind the BAR5 occulter. He we attempt to place the target on the mid-line of BAR5. We then use a subarray readout of CENTYERAXIS2 = 700 appopriate for BAR5 with a SIZEAXIS2 = 137 (the same ass we use elsewhere for Wedge0.6A). SCALABLE BENCHMARK: We expect full-well at r=0.15" with BAR10 from wings of stellar PSF in 1 second for V=5.0 (A0V) {**to be re-verified**}. HD 141569 is V = 7.12 so saturation in 7.05s. So 90% full well in appx 6.34s. Use this for the BAR5 exposures, repeated (8x) with multiple CR Splits. NOTE TO PC/CS: Here we use the BAR5 occulter (Aperture) that we comissioned in GO program 12923. This aperture is not available in APT Phase 2, *AND* the SIAF locations of the aperture fiducial we determined in GO 12923 is yet to be populated in SIAF.dat and flowed down to the ground system. We therefore call out BAR10 and use POS TARGs to move the target to the desired positions behind the BAR5 occulter. He we attempt to place the target 1/4 pixel above the midline mid-line of BAR5. We then use a subarray readout of CENTYERAXIS2 = 700 appopriate for BAR5 with a SIZEAXIS2 = 137 (the same ass we use elsewhere for Wedge0.6A). SCALABLE BENCHMARK: We expect full-well at r=0.15" with BAR10 from wings of stellar PSF in 1 second for V=5.0 (A0V) {**to be re-verified**}. HD 141569 is V = 7.12 so saturation in 7.05s. So 90% full well in appx 6.34s. Use this for the BAR5 exposures, repeated (8x) with multiple CR Splits. NOTE TO PC/CS: Here we use the BAR5 occulter (Aperture) that we comissioned in GO program 12923. This aperture is not available in APT Phase 2, *AND* the SIAF locations of the aperture fiducial we determined in GO 12923 is yet to be populated in SIAF.dat and flowed down to the ground system. We therefore call out BAR10 and use POS TARGs to move the target to the desired positions behind the BAR5 occulter. He we attempt to place the target 1/4 pixel below the midline mid-line of BAR5. We then use a subarray readout of CENTYERAXIS2 = 700 appopriate for BAR5 with a SIZEAXIS2 = 137 (the same ass we use elsewhere for Wedge0.6A). SCALABLE BENCHMARK: We expect full-well at r=0.15" with BAR10 from wings of stellar PSF in 1 second for V=5.0 (A0V) {**to be re-verified**}. HD 141569 is V = 7.12 so saturation in 7.05s. So 90% full well in appx 6.34s. Use this for the BAR5 exposures, repeated (8x) with multiple CR Splits. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD 141569 is V = 7.12 so saturation in 26.79s. So 90% full well in appx 24.11s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. For long exposures at WedgeA1.0 go (up to) 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 ([36 After 35 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 22.2. CASM was run in Phase II mode. 1404942464761 HD 141569 (V=7.12, B-V = +0.08). Second of two sets of visits, each containing three visits of HD 141569 at different relative orientations with one PSF calibration observation interleaved. This is the first HD 141569 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: Due to schedualability issues this target only is observed over a reduced foll range. Here, for Visit 55 we specify a relative orientation from Visit 31 of +55 to +100 deg. However, we do not expect schedualability with other link-set relative orientation constraints much larger than 55 deg. NOTE to PC: If it is possible to acheive an increaded relative orientation greater than appx +55 deg from Visit 31 we would like to do so (+90 deg would be ideal. We do NOT wish to do this, however, at the expense of further reucing the relative orientation minimum values on visits 31, 34, 36, or 38. Relative Timing: Schedule in orbit immediately before Visit 36. 1434077236000 156.473 (Tic-Visit :proposal-id 13786 :visit-id "35" :proposal-version -1 :trans-version "20140605" :date "09-Jul-2014 14:47:36.0" :trans-errors '(:WARNINGS 28 :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 73200 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13786 :visit-id "35" :obset-id "35" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13786 :visit-id "35" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2888 :al-overhead-at-end 0 :internal-dur-at-end 379 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3222 :pcs-gap 0 ) false 1 0 SNR = 100, V = 7.12, sp = A0V, Exptime rounded to nearest 0.1 second ETC Request ID: STIS.ta.618242 NOTE TO PC/CS: Here we use the BAR5 occulter (Aperture) that we comissioned in GO program 12923. This aperture is not available in APT Phase 2, *AND* the SIAF locations of the aperture fiducial we determined in GO 12923 is yet to be populated in SIAF.dat and flowed down to the ground system. We therefore call out BAR10 and use POS TARGs to move the target to the desired positions behind the BAR5 occulter. He we attempt to place the target on the mid-line of BAR5. We then use a subarray readout of CENTYERAXIS2 = 700 appopriate for BAR5 with a SIZEAXIS2 = 137 (the same ass we use elsewhere for Wedge0.6A). SCALABLE BENCHMARK: We expect full-well at r=0.15" with BAR10 from wings of stellar PSF in 1 second for V=5.0 (A0V) {**to be re-verified**}. HD 141569 is V = 7.12 so saturation in 7.05s. So 90% full well in appx 6.34s. Use this for the BAR5 exposures, repeated (8x) with multiple CR Splits. NOTE TO PC/CS: Here we use the BAR5 occulter (Aperture) that we comissioned in GO program 12923. This aperture is not available in APT Phase 2, *AND* the SIAF locations of the aperture fiducial we determined in GO 12923 is yet to be populated in SIAF.dat and flowed down to the ground system. We therefore call out BAR10 and use POS TARGs to move the target to the desired positions behind the BAR5 occulter. He we attempt to place the target 1/4 pixel above the midline mid-line of BAR5. We then use a subarray readout of CENTYERAXIS2 = 700 appopriate for BAR5 with a SIZEAXIS2 = 137 (the same ass we use elsewhere for Wedge0.6A). SCALABLE BENCHMARK: We expect full-well at r=0.15" with BAR10 from wings of stellar PSF in 1 second for V=5.0 (A0V) {**to be re-verified**}. HD 141569 is V = 7.12 so saturation in 7.05s. So 90% full well in appx 6.34s. Use this for the BAR5 exposures, repeated (8x) with multiple CR Splits. NOTE TO PC/CS: Here we use the BAR5 occulter (Aperture) that we comissioned in GO program 12923. This aperture is not available in APT Phase 2, *AND* the SIAF locations of the aperture fiducial we determined in GO 12923 is yet to be populated in SIAF.dat and flowed down to the ground system. We therefore call out BAR10 and use POS TARGs to move the target to the desired positions behind the BAR5 occulter. He we attempt to place the target 1/4 pixel below the midline mid-line of BAR5. We then use a subarray readout of CENTYERAXIS2 = 700 appopriate for BAR5 with a SIZEAXIS2 = 137 (the same ass we use elsewhere for Wedge0.6A). SCALABLE BENCHMARK: We expect full-well at r=0.15" with BAR10 from wings of stellar PSF in 1 second for V=5.0 (A0V) {**to be re-verified**}. HD 141569 is V = 7.12 so saturation in 7.05s. So 90% full well in appx 6.34s. Use this for the BAR5 exposures, repeated (8x) with multiple CR Splits. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD 141569 is V = 7.12 so saturation in 26.79s. So 90% full well in appx 24.11s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. For long exposures at WedgeA1.0 go (up to) 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 ([36 After 35 by 0.0 to 0.1 days] [37 After 36 by 0.5 to 1.5 days]) The scheduling data was generated by CASM 22.2. CASM was run in Phase II mode. 1404939717527 HD 141569 (V=7.12, B-V = +0.08). Second of two sets of visits, each containing three visits of HD 141569 at different relative orientations with one PSF calibration observation interleaved. This is the second HD 141569 visit in the first set. The four visits within each set must be executed sequentally in contiguous orbits interrupted only for Earth occultation. Relative Orientation: Due to schedualability issues this target only is observed over a reduced foll range, and the relative orientations except for Visit 35 are defined with opposite partity as for our other targets. NOTE to PC: In Visit 36, the relative orient from range w.r.t. Visit 35 is specified as -20 to -10 deg. PLEASE schedule as close to -15 deg relative orientation as possible - but see note on Visit 35. 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. 1434082964000 140.473 (Tic-Visit :proposal-id 13786 :visit-id "36" :proposal-version -1 :trans-version "20140605" :date "09-Jul-2014 14:01:51.0" :trans-errors '(:WARNINGS 28 :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 73200 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13786 :visit-id "36" :obset-id "36" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13786 :visit-id "36" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2888 :al-overhead-at-end 0 :internal-dur-at-end 379 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3222 :pcs-gap 0 ) false 1 0 SNR = 100, V = 7.12, sp = A0V, Exptime rounded to nearest 0.1 second ETC Request ID: STIS.ta.618242 NOTE TO PC/CS: Here we use the BAR5 occulter (Aperture) that we comissioned in GO program 12923. This aperture is not available in APT Phase 2, *AND* the SIAF locations of the aperture fiducial we determined in GO 12923 is yet to be populated in SIAF.dat and flowed down to the ground system. We therefore call out BAR10 and use POS TARGs to move the target to the desired positions behind the BAR5 occulter. He we attempt to place the target on the mid-line of BAR5. We then use a subarray readout of CENTYERAXIS2 = 700 appopriate for BAR5 with a SIZEAXIS2 = 137 (the same ass we use elsewhere for Wedge0.6A). SCALABLE BENCHMARK: We expect full-well at r=0.15" with BAR10 from wings of stellar PSF in 1 second for V=5.0 (A0V) {**to be re-verified**}. HD 141569 is V = 7.12 so saturation in 7.05s. So 90% full well in appx 6.34s. Use this for the BAR5 exposures, repeated (8x) with multiple CR Splits. NOTE TO PC/CS: Here we use the BAR5 occulter (Aperture) that we comissioned in GO program 12923. This aperture is not available in APT Phase 2, *AND* the SIAF locations of the aperture fiducial we determined in GO 12923 is yet to be populated in SIAF.dat and flowed down to the ground system. We therefore call out BAR10 and use POS TARGs to move the target to the desired positions behind the BAR5 occulter. He we attempt to place the target 1/4 pixel above the midline mid-line of BAR5. We then use a subarray readout of CENTYERAXIS2 = 700 appopriate for BAR5 with a SIZEAXIS2 = 137 (the same ass we use elsewhere for Wedge0.6A). SCALABLE BENCHMARK: We expect full-well at r=0.15" with BAR10 from wings of stellar PSF in 1 second for V=5.0 (A0V) {**to be re-verified**}. HD 141569 is V = 7.12 so saturation in 7.05s. So 90% full well in appx 6.34s. Use this for the BAR5 exposures, repeated (8x) with multiple CR Splits. NOTE TO PC/CS: Here we use the BAR5 occulter (Aperture) that we comissioned in GO program 12923. This aperture is not available in APT Phase 2, *AND* the SIAF locations of the aperture fiducial we determined in GO 12923 is yet to be populated in SIAF.dat and flowed down to the ground system. We therefore call out BAR10 and use POS TARGs to move the target to the desired positions behind the BAR5 occulter. He we attempt to place the target 1/4 pixel below the midline mid-line of BAR5. We then use a subarray readout of CENTYERAXIS2 = 700 appopriate for BAR5 with a SIZEAXIS2 = 137 (the same ass we use elsewhere for Wedge0.6A). SCALABLE BENCHMARK: We expect full-well at r=0.15" with BAR10 from wings of stellar PSF in 1 second for V=5.0 (A0V) {**to be re-verified**}. HD 141569 is V = 7.12 so saturation in 7.05s. So 90% full well in appx 6.34s. Use this for the BAR5 exposures, repeated (8x) with multiple CR Splits. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD 141569 is V = 7.12 so saturation in 26.79s. So 90% full well in appx 24.11s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. For long exposures at WedgeA1.0 go (up to) 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 ([37 After 36 by 0.5 to 1.5 days] [38 After 37 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 22.2. CASM was run in Phase II mode. 1404779021440 PSF04 (HD 135298. PSF calibration target for HD HD 141569. V = 7.20. B - V = +0.08. Sp A0 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) then 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. 1434088555000 125.95197272065178 (Tic-Visit :proposal-id 13786 :visit-id "37" :proposal-version -1 :trans-version "20140605" :date "07-Jul-2014 17:23:39.0" :trans-errors '(:WARNINGS 24 :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 73200 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13786 :visit-id "37" :obset-id "37" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13786 :visit-id "37" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2888 :al-overhead-at-end 0 :internal-dur-at-end 379 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3222 :pcs-gap 0 ) false 1 0 SNR = 100, V = 7.20, sp = A0, Exptime rounded to nearest 0.1 second ETC Request ID: STIS.ta.618246 NOTE TO PC/CS: Here we use the BAR5 occulter (Aperture) that we comissioned in GO program 12923. This aperture is not available in APT Phase 2, *AND* the SIAF locations of the aperture fiducial we determined in GO 12923 is yet to be populated in SIAF.dat and flowed down to the ground system. We therefore call out BAR10 and use POS TARGs to move the target to the desired positions behind the BAR5 occulter. He we attempt to place the target on the mid-line of BAR5. We then use a subarray readout of CENTYERAXIS2 = 700 appopriate for BAR5 with a SIZEAXIS2 = 137 (the same ass we use elsewhere for Wedge0.6A). SCALABLE BENCHMARK: We expect full-well at r=0.15" with BAR10 from wings of stellar PSF in 1 second for V=5.0 (A0V) {**to be re-verified**}. HD 135298 is V = 7.20 so saturation in 7.59s. So 90% full well in appx 6.83s. Use this for the BAR5 exposures, repeated (8x) with multiple CR Splits. NOTE TO PC/CS: Here we use the BAR5 occulter (Aperture) that we comissioned in GO program 12923. This aperture is not available in APT Phase 2, *AND* the SIAF locations of the aperture fiducial we determined in GO 12923 is yet to be populated in SIAF.dat and flowed down to the ground system. We therefore call out BAR10 and use POS TARGs to move the target to the desired positions behind the BAR5 occulter. He we attempt to place the target on the mid-line of BAR5. We then use a subarray readout of CENTYERAXIS2 = 700 appopriate for BAR5 with a SIZEAXIS2 = 137 (the same ass we use elsewhere for Wedge0.6A). SCALABLE BENCHMARK: We expect full-well at r=0.15" with BAR10 from wings of stellar PSF in 1 second for V=5.0 (A0V) {**to be re-verified**}. HD 135298 is V = 7.20 so saturation in 7.59s. So 90% full well in appx 6.83s. Use this for the BAR5 exposures, repeated (8x) with multiple CR Splits. NOTE TO PC/CS: Here we use the BAR5 occulter (Aperture) that we comissioned in GO program 12923. This aperture is not available in APT Phase 2, *AND* the SIAF locations of the aperture fiducial we determined in GO 12923 is yet to be populated in SIAF.dat and flowed down to the ground system. We therefore call out BAR10 and use POS TARGs to move the target to the desired positions behind the BAR5 occulter. He we attempt to place the target on the mid-line of BAR5. We then use a subarray readout of CENTYERAXIS2 = 700 appopriate for BAR5 with a SIZEAXIS2 = 137 (the same ass we use elsewhere for Wedge0.6A). SCALABLE BENCHMARK: We expect full-well at r=0.15" with BAR10 from wings of stellar PSF in 1 second for V=5.0 (A0V) {**to be re-verified**}. HD 135298 is V = 7.20 so saturation in 7.59s. So 90% full well in appx 6.83s. Use this for the BAR5 exposures, repeated (8x) with multiple CR Splits. SCALABLE BENCHMARK: We expect full-well at r=0.3" (Wedge0.6) from wings of stellar PSF in 1 second for V=3.55 SCALABLE BENCHMARK: We expect full-well at r=0.15" with BAR10 from wings of stellar PSF in 1 second for V=5.0 (A0V) {**to be re-verified**}. HD 135298 is V = 7.20 so saturation in 7.59s. So 90% full well in appx 6.83s. 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 ([38 After 37 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 22.2. CASM was run in Phase II mode. 1404939738479 HD 141569 (V=7.12, B-V = +0.08). Second of two sets of visits, each containing three visits of HD 141569 at different relative orientations with one PSF calibration observation interleaved. This is the third HD 141569 visit in the first set. The four visits within each set must be executed sequentally in contiguous orbits interrupted only for Earth occultation. Relative Orientation: Due to schedualability issues this target only is observed over a reduced foll range, and the relative orientations except for Visit 35 are defined with opposite partity as for our other targets. NOTE to PC: In Visit 36, the relative orient from range w.r.t. Visit 35 is specified as -35 to -30 deg. PLEASE schedule as close to -30 deg relative orientation as possible - but see note on Visit 35. Relative Timing: This visit (38) should immediately follow Visit 37. I.e., They should be executed sequentially in "back-to-back" orbits. 1434094418000 126.47300000000001 (Tic-Visit :proposal-id 13786 :visit-id "38" :proposal-version -1 :trans-version "20140605" :date "09-Jul-2014 14:02:11.0" :trans-errors '(:WARNINGS 28 :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 73200 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13786 :visit-id "38" :obset-id "38" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13786 :visit-id "38" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2888 :al-overhead-at-end 0 :internal-dur-at-end 379 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3222 :pcs-gap 0 ) false 1 0 SNR = 100, V = 7.12, sp = A0V, Exptime rounded to nearest 0.1 second ETC Request ID: STIS.ta.618242 NOTE TO PC/CS: Here we use the BAR5 occulter (Aperture) that we comissioned in GO program 12923. This aperture is not available in APT Phase 2, *AND* the SIAF locations of the aperture fiducial we determined in GO 12923 is yet to be populated in SIAF.dat and flowed down to the ground system. We therefore call out BAR10 and use POS TARGs to move the target to the desired positions behind the BAR5 occulter. He we attempt to place the target on the mid-line of BAR5. We then use a subarray readout of CENTYERAXIS2 = 700 appopriate for BAR5 with a SIZEAXIS2 = 137 (the same ass we use elsewhere for Wedge0.6A). SCALABLE BENCHMARK: We expect full-well at r=0.15" with BAR10 from wings of stellar PSF in 1 second for V=5.0 (A0V) {**to be re-verified**}. HD 141569 is V = 7.12 so saturation in 7.05s. So 90% full well in appx 6.34s. Use this for the BAR5 exposures, repeated (8x) with multiple CR Splits. NOTE TO PC/CS: Here we use the BAR5 occulter (Aperture) that we comissioned in GO program 12923. This aperture is not available in APT Phase 2, *AND* the SIAF locations of the aperture fiducial we determined in GO 12923 is yet to be populated in SIAF.dat and flowed down to the ground system. We therefore call out BAR10 and use POS TARGs to move the target to the desired positions behind the BAR5 occulter. He we attempt to place the target 1/4 pixel above the midline mid-line of BAR5. We then use a subarray readout of CENTYERAXIS2 = 700 appopriate for BAR5 with a SIZEAXIS2 = 137 (the same ass we use elsewhere for Wedge0.6A). SCALABLE BENCHMARK: We expect full-well at r=0.15" with BAR10 from wings of stellar PSF in 1 second for V=5.0 (A0V) {**to be re-verified**}. HD 141569 is V = 7.12 so saturation in 7.05s. So 90% full well in appx 6.34s. Use this for the BAR5 exposures, repeated (8x) with multiple CR Splits. NOTE TO PC/CS: Here we use the BAR5 occulter (Aperture) that we comissioned in GO program 12923. This aperture is not available in APT Phase 2, *AND* the SIAF locations of the aperture fiducial we determined in GO 12923 is yet to be populated in SIAF.dat and flowed down to the ground system. We therefore call out BAR10 and use POS TARGs to move the target to the desired positions behind the BAR5 occulter. He we attempt to place the target 1/4 pixel below the midline mid-line of BAR5. We then use a subarray readout of CENTYERAXIS2 = 700 appopriate for BAR5 with a SIZEAXIS2 = 137 (the same ass we use elsewhere for Wedge0.6A). SCALABLE BENCHMARK: We expect full-well at r=0.15" with BAR10 from wings of stellar PSF in 1 second for V=5.0 (A0V) {**to be re-verified**}. HD 141569 is V = 7.12 so saturation in 7.05s. So 90% full well in appx 6.34s. Use this for the BAR5 exposures, repeated (8x) with multiple CR Splits. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD 141569 is V = 7.12 so saturation in 26.79s. So 90% full well in appx 24.11s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. For long exposures at WedgeA1.0 go (up to) 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]) The scheduling data was generated by CASM 22.2. CASM was run in Phase II mode. 1404852429496 HR 4796 (V=5.78, B-V = +0.01). First of two sets of visits, each containing three visits of HR 4796 at different relative orientations with one PSF calibration observation interleaved. This is the first HD 4796 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 32, with the absolute orientation of Visit 42 unconstrained. We allow a relative orientation tolerence from -15 deg to -30 deg to assist in guide star selection and scheduling. NOTE to PC: Schedule as close to -30 deg from Visit 42 as possible. Relative Timing: This visit (3) should immediately preceed visit (42). I.e., They should be executed sequentially in "back-to-back" orbits. 1421714506000 277.59999999999997 (Tic-Visit :proposal-id 13786 :visit-id "41" :proposal-version -1 :trans-version "20140605" :date "08-Jul-2014 13:47:03.0" :trans-errors '(:WARNINGS 24 :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 125952 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13786 :visit-id "41" :obset-id "41" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13786 :visit-id "41" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2898 :al-overhead-at-end 0 :internal-dur-at-end 435 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3278 :pcs-gap 0 ) false 1 0 V = 5.78, sp = A0V, Exptime rounded to nearest 0.1 second ETC Request ID: STIS.ta.618243 NOTE TO PC/CS: Here we use the BAR5 occulter (Aperture) that we comissioned in GO program 12923. This aperture is not available in APT Phase 2, *AND* the SIAF locations of the aperture fiducial we determined in GO 12923 is yet to be populated in SIAF.dat and flowed down to the ground system. We therefore call out BAR10 and use POS TARGs to move the target to the desired positions behind the BAR5 occulter. He we attempt to place the target on the mid-line of BAR5. We then use a subarray readout of CENTYERAXIS2 = 700 appopriate for BAR5 with a SIZEAXIS2 = 137 (the same ass we use elsewhere for Wedge0.6A). SCALABLE BENCHMARK: We expect full-well at r=0.15" with BAR10 from wings of stellar PSF in 1 second for V=5.0 (A0V) {**to be re-verified**}. HR 4796 is V = 5.78 so saturation in 2.09s. So 90% full well in appx 1.85s. Use this for the BAR5 exposures, repeated (8x) with multiple CR Splits. NOTE TO PC/CS: Here we use the BAR5 occulter (Aperture) that we comissioned in GO program 12923. This aperture is not available in APT Phase 2, *AND* the SIAF locations of the aperture fiducial we determined in GO 12923 is yet to be populated in SIAF.dat and flowed down to the ground system. We therefore call out BAR10 and use POS TARGs to move the target to the desired positions behind the BAR5 occulter. He we attempt to place the target 1/4 pixel above the mid-line of BAR5. We then use a subarray readout of CENTYERAXIS2 = 700 appopriate for BAR5 with a SIZEAXIS2 = 137 (the same ass we use elsewhere for Wedge0.6A). SCALABLE BENCHMARK: We expect full-well at r=0.15" with BAR10 from wings of stellar PSF in 1 second for V=5.0 (A0V) {**to be re-verified**}. HR 4796 is V = 5.78 so saturation in 2.09s. So 90% full well in appx 1.85s. Use this for the BAR5 exposures, repeated (8x) with multiple CR Splits. NOTE TO PC/CS: Here we use the BAR5 occulter (Aperture) that we comissioned in GO program 12923. This aperture is not available in APT Phase 2, *AND* the SIAF locations of the aperture fiducial we determined in GO 12923 is yet to be populated in SIAF.dat and flowed down to the ground system. We therefore call out BAR10 and use POS TARGs to move the target to the desired positions behind the BAR5 occulter. He we attempt to place the target 1/4 pixel below the mid-line of BAR5. We then use a subarray readout of CENTYERAXIS2 = 700 appopriate for BAR5 with a SIZEAXIS2 = 137 (the same ass we use elsewhere for Wedge0.6A). SCALABLE BENCHMARK: We expect full-well at r=0.15" with BAR10 from wings of stellar PSF in 1 second for V=5.0 (A0V) {**to be re-verified**}. HR 4796 is V = 5.78 so saturation in 2.09s. So 90% full well in appx 1.85s. Use this for the BAR5 exposures, repeated (8x) with multiple CR Splits. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HR 4796 is V =5.78 so saturation in 7.80s. So 90% full well in appx 7.02s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. For long exposures at WedgeA1.0 go (up to) 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. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HR 4796 is V =5.78 so saturation in 7.80s. So 90% full well in appx 7.02s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. For long exposures at WedgeA1.0 go (up to) 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 22.2. CASM was run in Phase II mode. 1404852441577 HR 4796 (V=5.78, B-V = +0.01). First of two sets of visits, each containing three visits of HR 4796 at different relative orientations with one PSF calibration observation interleaved. This is the second HD 4796 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). This visit at nominal roll as scheduled by STScI. Visits 41, 44, 45, 46 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. 1421720239000 299.865 (Tic-Visit :proposal-id 13786 :visit-id "42" :proposal-version -1 :trans-version "20140605" :date "08-Jul-2014 13:47:15.0" :trans-errors '(:WARNINGS 24 :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 125952 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13786 :visit-id "42" :obset-id "42" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13786 :visit-id "42" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2898 :al-overhead-at-end 0 :internal-dur-at-end 435 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3278 :pcs-gap 0 ) false 1 0 V = 5.78, sp = A0V, Exptime rounded to nearest 0.1 second ETC Request ID: STIS.ta.618243 NOTE TO PC/CS: Here we use the BAR5 occulter (Aperture) that we comissioned in GO program 12923. This aperture is not available in APT Phase 2, *AND* the SIAF locations of the aperture fiducial we determined in GO 12923 is yet to be populated in SIAF.dat and flowed down to the ground system. We therefore call out BAR10 and use POS TARGs to move the target to the desired positions behind the BAR5 occulter. He we attempt to place the target on the mid-line of BAR5. We then use a subarray readout of CENTYERAXIS2 = 700 appopriate for BAR5 with a SIZEAXIS2 = 137 (the same ass we use elsewhere for Wedge0.6A). SCALABLE BENCHMARK: We expect full-well at r=0.15" with BAR10 from wings of stellar PSF in 1 second for V=5.0 (A0V) {**to be re-verified**}. HR 4796 is V = 5.78 so saturation in 2.09s. So 90% full well in appx 1.85s. Use this for the BAR5 exposures, repeated (8x) with multiple CR Splits. NOTE TO PC/CS: Here we use the BAR5 occulter (Aperture) that we comissioned in GO program 12923. This aperture is not available in APT Phase 2, *AND* the SIAF locations of the aperture fiducial we determined in GO 12923 is yet to be populated in SIAF.dat and flowed down to the ground system. We therefore call out BAR10 and use POS TARGs to move the target to the desired positions behind the BAR5 occulter. He we attempt to place the target 1/4 pixel above the mid-line of BAR5. We then use a subarray readout of CENTYERAXIS2 = 700 appopriate for BAR5 with a SIZEAXIS2 = 137 (the same ass we use elsewhere for Wedge0.6A). SCALABLE BENCHMARK: We expect full-well at r=0.15" with BAR10 from wings of stellar PSF in 1 second for V=5.0 (A0V) {**to be re-verified**}. HR 4796 is V = 5.78 so saturation in 2.09s. So 90% full well in appx 1.85s. Use this for the BAR5 exposures, repeated (8x) with multiple CR Splits. NOTE TO PC/CS: Here we use the BAR5 occulter (Aperture) that we comissioned in GO program 12923. This aperture is not available in APT Phase 2, *AND* the SIAF locations of the aperture fiducial we determined in GO 12923 is yet to be populated in SIAF.dat and flowed down to the ground system. We therefore call out BAR10 and use POS TARGs to move the target to the desired positions behind the BAR5 occulter. He we attempt to place the target 1/4 pixel below the mid-line of BAR5. We then use a subarray readout of CENTYERAXIS2 = 700 appopriate for BAR5 with a SIZEAXIS2 = 137 (the same ass we use elsewhere for Wedge0.6A). SCALABLE BENCHMARK: We expect full-well at r=0.15" with BAR10 from wings of stellar PSF in 1 second for V=5.0 (A0V) {**to be re-verified**}. HR 4796 is V = 5.78 so saturation in 2.09s. So 90% full well in appx 1.85s. Use this for the BAR5 exposures, repeated (8x) with multiple CR Splits. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HR 4796 is V =5.78 so saturation in 7.80s. So 90% full well in appx 7.02s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. For long exposures at WedgeA1.0 go (up to) 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. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HR 4796 is V =5.78 so saturation in 7.80s. So 90% full well in appx 7.02s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. For long exposures at WedgeA1.0 go (up to) 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 22.2. CASM was run in Phase II mode. 1404839731459 PSF05 (HR 4735). PSF calibration target for HD HD 4786. V = 5.57. B - V = +0.01. Spex. B9V. 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) then 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 (43) should immediately follow visit 42 and immediately precede visit 44. I.e., they should be executed sequentially in "back-to-back" orbits. 1421725881000 300.7448663048435 (Tic-Visit :proposal-id 13786 :visit-id "43" :proposal-version -1 :trans-version "20140605" :date "08-Jul-2014 10:15:29.0" :trans-errors '(:WARNINGS 24 :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 141040 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13786 :visit-id "43" :obset-id "43" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13786 :visit-id "43" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2913 :al-overhead-at-end 0 :internal-dur-at-end 365 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3257 :pcs-gap 0 ) false 1 0 V = 5.57, sp = B9V, Exptime rounded to nearest 0.1 second ETC Request ID: STIS.ta.618247 NOTE TO PC/CS: Here we use the BAR5 occulter (Aperture) that we comissioned in GO program 12923. This aperture is not available in APT Phase 2, *AND* the SIAF locations of the aperture fiducial we determined in GO 12923 is yet to be populated in SIAF.dat and flowed down to the ground system. We therefore call out BAR10 and use POS TARGs to move the target to the desired positions behind the BAR5 occulter. He we attempt to place the target on the mid-line of BAR5. We then use a subarray readout of CENTYERAXIS2 = 700 appopriate for BAR5 with a SIZEAXIS2 = 137 (the same ass we use elsewhere for Wedge0.6A). SCALABLE BENCHMARK: We expect full-well at r=0.15" with BAR10 from wings of stellar PSF in 1 second for V=5.0 (A0V) {**to be re-verified**}. HR 4735 is V = 5.57 so saturation in 1.69Ss. So 90% full well in appx 1.52s. Use this for the BAR5 exposures, repeated (8x) with multiple CR Splits. NOTE TO PC/CS: Here we use the BAR5 occulter (Aperture) that we comissioned in GO program 12923. This aperture is not available in APT Phase 2, *AND* the SIAF locations of the aperture fiducial we determined in GO 12923 is yet to be populated in SIAF.dat and flowed down to the ground system. We therefore call out BAR10 and use POS TARGs to move the target to the desired positions behind the BAR5 occulter. He we attempt to place the target on 1/4 PIXEL ABOVE the mid-line of BAR5. We then use a subarray readout of CENTYERAXIS2 = 700 appopriate for BAR5 with a SIZEAXIS2 = 137 (the same ass we use elsewhere for Wedge0.6A). SCALABLE BENCHMARK: We expect full-well at r=0.15" with BAR10 from wings of stellar PSF in 1 second for V=5.0 (A0V) {**to be re-verified**}. HR 4735 is V = 5.57 so saturation in 1.69Ss. So 90% full well in appx 1.52s. Use this for the BAR5 exposures, repeated (8x) with multiple CR Splits. NOTE TO PC/CS: Here we use the BAR5 occulter (Aperture) that we comissioned in GO program 12923. This aperture is not available in APT Phase 2, *AND* the SIAF locations of the aperture fiducial we determined in GO 12923 is yet to be populated in SIAF.dat and flowed down to the ground system. We therefore call out BAR10 and use POS TARGs to move the target to the desired positions behind the BAR5 occulter. He we attempt to place the target on 1/4 pixel below the mid-line of BAR5. We then use a subarray readout of CENTYERAXIS2 = 700 appropriate for BAR5 with a SIZEAXIS2 = 137 (the same ass we use elsewhere for Wedge0.6A). SCALABLE BENCHMARK: We expect full-well at r=0.15" with BAR10 from wings of stellar PSF in 1 second for V=5.0 (A0V) {**to be re-verified**}. HR 4735 is V = 5.57 so saturation in 1.69Ss. So 90% full well in appx 1.52s. Use this for the BAR5 exposures, repeated (8x) with multiple CR Splits. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HR 4725 is V =5.57 so saturation in 6.43s. So 90% full well in appx 5.78s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. For long exposures at WedgeA1.0 go (up to) 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. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HR 4725 is V =5.57 so saturation in 6.43s. So 90% full well in appx 5.78s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. For long exposures at WedgeA1.0 go (up to) 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 22.2. CASM was run in Phase II mode. 1404852459007 HR 4796 (V=5.78, B-V = +0.01). Firdst of two sets of visits, each containing three visits of HR 4796 at different relative orientations with one PSF calibration observation interleaved. This is the third HD 4796 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. We allow a relative orientation tolerence from +15 deg to +30 deg to assist in guide star selection and scheduling. NOTE to PC: Schedule as close to +30 deg from Visit 42 as possible. Relative Timing: This visit (44) should immediately follow Visit 43. I.e., They should be executed sequentially in "back-to-back" orbits. 1421731704000 321.865 (Tic-Visit :proposal-id 13786 :visit-id "44" :proposal-version -1 :trans-version "20140605" :date "08-Jul-2014 13:47:33.0" :trans-errors '(:WARNINGS 24 :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 125952 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13786 :visit-id "44" :obset-id "44" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13786 :visit-id "44" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2898 :al-overhead-at-end 0 :internal-dur-at-end 435 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3278 :pcs-gap 0 ) false 1 0 V = 5.78, sp = A0V, Exptime rounded to nearest 0.1 second ETC Request ID: STIS.ta.618243 NOTE TO PC/CS: Here we use the BAR5 occulter (Aperture) that we comissioned in GO program 12923. This aperture is not available in APT Phase 2, *AND* the SIAF locations of the aperture fiducial we determined in GO 12923 is yet to be populated in SIAF.dat and flowed down to the ground system. We therefore call out BAR10 and use POS TARGs to move the target to the desired positions behind the BAR5 occulter. He we attempt to place the target on the mid-line of BAR5. We then use a subarray readout of CENTYERAXIS2 = 700 appopriate for BAR5 with a SIZEAXIS2 = 137 (the same ass we use elsewhere for Wedge0.6A). SCALABLE BENCHMARK: We expect full-well at r=0.15" with BAR10 from wings of stellar PSF in 1 second for V=5.0 (A0V) {**to be re-verified**}. HR 4796 is V = 5.78 so saturation in 2.09s. So 90% full well in appx 1.85s. Use this for the BAR5 exposures, repeated (8x) with multiple CR Splits. NOTE TO PC/CS: Here we use the BAR5 occulter (Aperture) that we comissioned in GO program 12923. This aperture is not available in APT Phase 2, *AND* the SIAF locations of the aperture fiducial we determined in GO 12923 is yet to be populated in SIAF.dat and flowed down to the ground system. We therefore call out BAR10 and use POS TARGs to move the target to the desired positions behind the BAR5 occulter. He we attempt to place the target 1/4 pixel above the mid-line of BAR5. We then use a subarray readout of CENTYERAXIS2 = 700 appopriate for BAR5 with a SIZEAXIS2 = 137 (the same ass we use elsewhere for Wedge0.6A). SCALABLE BENCHMARK: We expect full-well at r=0.15" with BAR10 from wings of stellar PSF in 1 second for V=5.0 (A0V) {**to be re-verified**}. HR 4796 is V = 5.78 so saturation in 2.09s. So 90% full well in appx 1.85s. Use this for the BAR5 exposures, repeated (8x) with multiple CR Splits. NOTE TO PC/CS: Here we use the BAR5 occulter (Aperture) that we comissioned in GO program 12923. This aperture is not available in APT Phase 2, *AND* the SIAF locations of the aperture fiducial we determined in GO 12923 is yet to be populated in SIAF.dat and flowed down to the ground system. We therefore call out BAR10 and use POS TARGs to move the target to the desired positions behind the BAR5 occulter. He we attempt to place the target 1/4 pixel below the mid-line of BAR5. We then use a subarray readout of CENTYERAXIS2 = 700 appopriate for BAR5 with a SIZEAXIS2 = 137 (the same ass we use elsewhere for Wedge0.6A). SCALABLE BENCHMARK: We expect full-well at r=0.15" with BAR10 from wings of stellar PSF in 1 second for V=5.0 (A0V) {**to be re-verified**}. HR 4796 is V = 5.78 so saturation in 2.09s. So 90% full well in appx 1.85s. Use this for the BAR5 exposures, repeated (8x) with multiple CR Splits. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HR 4796 is V =5.78 so saturation in 7.80s. So 90% full well in appx 7.02s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. For long exposures at WedgeA1.0 go (up to) 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. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HR 4796 is V =5.78 so saturation in 7.80s. So 90% full well in appx 7.02s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. For long exposures at WedgeA1.0 go (up to) 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 22.2. CASM was run in Phase II mode. 1404842961142 HR 4796 (V=5.78, B-V = +0.01). Second of two sets of visits, each containing three visits of HR 4796 at different relative orientations with one PSF calibration observation interleaved. This is the first HR 4796 visit in the second set. The four visits within each set must be executed sequentally in contiguous orbits interrupted only for Earth occultation. Relative Timing: Schedule in orbit immediately before Visit 46. 1436442120000 90.46399999999988 (Tic-Visit :proposal-id 13786 :visit-id "45" :proposal-version -1 :trans-version "20140605" :date "08-Jul-2014 11:09:19.0" :trans-errors '(:WARNINGS 24 :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 125952 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13786 :visit-id "45" :obset-id "45" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13786 :visit-id "45" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2898 :al-overhead-at-end 0 :internal-dur-at-end 435 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3278 :pcs-gap 0 ) false 1 0 V = 5.78, sp = A0V, Exptime rounded to nearest 0.1 second ETC Request ID: STIS.ta.618243 NOTE TO PC/CS: Here we use the BAR5 occulter (Aperture) that we comissioned in GO program 12923. This aperture is not available in APT Phase 2, *AND* the SIAF locations of the aperture fiducial we determined in GO 12923 is yet to be populated in SIAF.dat and flowed down to the ground system. We therefore call out BAR10 and use POS TARGs to move the target to the desired positions behind the BAR5 occulter. He we attempt to place the target on the mid-line of BAR5. We then use a subarray readout of CENTYERAXIS2 = 700 appopriate for BAR5 with a SIZEAXIS2 = 137 (the same ass we use elsewhere for Wedge0.6A). SCALABLE BENCHMARK: We expect full-well at r=0.15" with BAR10 from wings of stellar PSF in 1 second for V=5.0 (A0V) {**to be re-verified**}. HR 4796 is V = 5.78 so saturation in 2.09s. So 90% full well in appx 1.85s. Use this for the BAR5 exposures, repeated (8x) with multiple CR Splits. NOTE TO PC/CS: Here we use the BAR5 occulter (Aperture) that we comissioned in GO program 12923. This aperture is not available in APT Phase 2, *AND* the SIAF locations of the aperture fiducial we determined in GO 12923 is yet to be populated in SIAF.dat and flowed down to the ground system. We therefore call out BAR10 and use POS TARGs to move the target to the desired positions behind the BAR5 occulter. He we attempt to place the target 1/4 pixel above the mid-line of BAR5. We then use a subarray readout of CENTYERAXIS2 = 700 appopriate for BAR5 with a SIZEAXIS2 = 137 (the same ass we use elsewhere for Wedge0.6A). SCALABLE BENCHMARK: We expect full-well at r=0.15" with BAR10 from wings of stellar PSF in 1 second for V=5.0 (A0V) {**to be re-verified**}. HR 4796 is V = 5.78 so saturation in 2.09s. So 90% full well in appx 1.85s. Use this for the BAR5 exposures, repeated (8x) with multiple CR Splits. NOTE TO PC/CS: Here we use the BAR5 occulter (Aperture) that we comissioned in GO program 12923. This aperture is not available in APT Phase 2, *AND* the SIAF locations of the aperture fiducial we determined in GO 12923 is yet to be populated in SIAF.dat and flowed down to the ground system. We therefore call out BAR10 and use POS TARGs to move the target to the desired positions behind the BAR5 occulter. He we attempt to place the target 1/4 pixel below the mid-line of BAR5. We then use a subarray readout of CENTYERAXIS2 = 700 appopriate for BAR5 with a SIZEAXIS2 = 137 (the same ass we use elsewhere for Wedge0.6A). SCALABLE BENCHMARK: We expect full-well at r=0.15" with BAR10 from wings of stellar PSF in 1 second for V=5.0 (A0V) {**to be re-verified**}. HR 4796 is V = 5.78 so saturation in 2.09s. So 90% full well in appx 1.85s. Use this for the BAR5 exposures, repeated (8x) with multiple CR Splits. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HR 4796 is V =5.78 so saturation in 7.80s. So 90% full well in appx 7.02s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. For long exposures at WedgeA1.0 go (up to) 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. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HR 4796 is V =5.78 so saturation in 7.80s. So 90% full well in appx 7.02s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. For long exposures at WedgeA1.0 go (up to) 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 22.2. CASM was run in Phase II mode. 1404842975233 HR 4796 (V=5.78, B-V = +0.01). Second of two sets of visits, each containing three visits of HR 4796 at different relative orientations with one PSF calibration observation interleaved. This is the second HR 4796 visit in the first set. The four visits within each set must be executed sequentally in contiguous orbits interrupted only for Earth occultation. 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. 1436447846000 112.96399999999988 (Tic-Visit :proposal-id 13786 :visit-id "46" :proposal-version -1 :trans-version "20140605" :date "08-Jul-2014 11:09:33.0" :trans-errors '(:WARNINGS 24 :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 125952 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13786 :visit-id "46" :obset-id "46" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13786 :visit-id "46" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2898 :al-overhead-at-end 0 :internal-dur-at-end 435 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3278 :pcs-gap 0 ) false 1 0 V = 5.78, sp = A0V, Exptime rounded to nearest 0.1 second ETC Request ID: STIS.ta.618243 NOTE TO PC/CS: Here we use the BAR5 occulter (Aperture) that we comissioned in GO program 12923. This aperture is not available in APT Phase 2, *AND* the SIAF locations of the aperture fiducial we determined in GO 12923 is yet to be populated in SIAF.dat and flowed down to the ground system. We therefore call out BAR10 and use POS TARGs to move the target to the desired positions behind the BAR5 occulter. He we attempt to place the target on the mid-line of BAR5. We then use a subarray readout of CENTYERAXIS2 = 700 appopriate for BAR5 with a SIZEAXIS2 = 137 (the same ass we use elsewhere for Wedge0.6A). SCALABLE BENCHMARK: We expect full-well at r=0.15" with BAR10 from wings of stellar PSF in 1 second for V=5.0 (A0V) {**to be re-verified**}. HR 4796 is V = 5.78 so saturation in 2.09s. So 90% full well in appx 1.85s. Use this for the BAR5 exposures, repeated (8x) with multiple CR Splits. NOTE TO PC/CS: Here we use the BAR5 occulter (Aperture) that we comissioned in GO program 12923. This aperture is not available in APT Phase 2, *AND* the SIAF locations of the aperture fiducial we determined in GO 12923 is yet to be populated in SIAF.dat and flowed down to the ground system. We therefore call out BAR10 and use POS TARGs to move the target to the desired positions behind the BAR5 occulter. He we attempt to place the target 1/4 pixel above the mid-line of BAR5. We then use a subarray readout of CENTYERAXIS2 = 700 appopriate for BAR5 with a SIZEAXIS2 = 137 (the same ass we use elsewhere for Wedge0.6A). SCALABLE BENCHMARK: We expect full-well at r=0.15" with BAR10 from wings of stellar PSF in 1 second for V=5.0 (A0V) {**to be re-verified**}. HR 4796 is V = 5.78 so saturation in 2.09s. So 90% full well in appx 1.85s. Use this for the BAR5 exposures, repeated (8x) with multiple CR Splits. NOTE TO PC/CS: Here we use the BAR5 occulter (Aperture) that we comissioned in GO program 12923. This aperture is not available in APT Phase 2, *AND* the SIAF locations of the aperture fiducial we determined in GO 12923 is yet to be populated in SIAF.dat and flowed down to the ground system. We therefore call out BAR10 and use POS TARGs to move the target to the desired positions behind the BAR5 occulter. He we attempt to place the target 1/4 pixel below the mid-line of BAR5. We then use a subarray readout of CENTYERAXIS2 = 700 appopriate for BAR5 with a SIZEAXIS2 = 137 (the same ass we use elsewhere for Wedge0.6A). SCALABLE BENCHMARK: We expect full-well at r=0.15" with BAR10 from wings of stellar PSF in 1 second for V=5.0 (A0V) {**to be re-verified**}. HR 4796 is V = 5.78 so saturation in 2.09s. So 90% full well in appx 1.85s. Use this for the BAR5 exposures, repeated (8x) with multiple CR Splits. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HR 4796 is V =5.78 so saturation in 7.80s. So 90% full well in appx 7.02s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. For long exposures at WedgeA1.0 go (up to) 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. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HR 4796 is V =5.78 so saturation in 7.80s. So 90% full well in appx 7.02s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. For long exposures at WedgeA1.0 go (up to) 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 22.2. CASM was run in Phase II mode. 1404842986096 PSF05 (HR 4735). PSF calibration target for HD HD 4786. V = 5.57. B - V = +0.01. Spex. B9V. TThis 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) then 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 46 and immediately precede visit 48. I.e., they should be executed sequentially in "back-to-back" orbits. 1436453480000 114.90192526457048 (Tic-Visit :proposal-id 13786 :visit-id "47" :proposal-version -1 :trans-version "20140605" :date "08-Jul-2014 11:09:43.0" :trans-errors '(:WARNINGS 24 :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 141040 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13786 :visit-id "47" :obset-id "47" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13786 :visit-id "47" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2913 :al-overhead-at-end 0 :internal-dur-at-end 365 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3257 :pcs-gap 0 ) false 1 0 V = 5.57, sp = B9V, Exptime rounded to nearest 0.1 second ETC Request ID: STIS.ta.618247 NOTE TO PC/CS: Here we use the BAR5 occulter (Aperture) that we comissioned in GO program 12923. This aperture is not available in APT Phase 2, *AND* the SIAF locations of the aperture fiducial we determined in GO 12923 is yet to be populated in SIAF.dat and flowed down to the ground system. We therefore call out BAR10 and use POS TARGs to move the target to the desired positions behind the BAR5 occulter. He we attempt to place the target on the mid-line of BAR5. We then use a subarray readout of CENTYERAXIS2 = 700 appopriate for BAR5 with a SIZEAXIS2 = 137 (the same ass we use elsewhere for Wedge0.6A). SCALABLE BENCHMARK: We expect full-well at r=0.15" with BAR10 from wings of stellar PSF in 1 second for V=5.0 (A0V) {**to be re-verified**}. HR 4735 is V = 5.57 so saturation in 1.69Ss. So 90% full well in appx 1.52s. Use this for the BAR5 exposures, repeated (8x) with multiple CR Splits. NOTE TO PC/CS: Here we use the BAR5 occulter (Aperture) that we comissioned in GO program 12923. This aperture is not available in APT Phase 2, *AND* the SIAF locations of the aperture fiducial we determined in GO 12923 is yet to be populated in SIAF.dat and flowed down to the ground system. We therefore call out BAR10 and use POS TARGs to move the target to the desired positions behind the BAR5 occulter. He we attempt to place the target on 1/4 PIXEL ABOVE the mid-line of BAR5. We then use a subarray readout of CENTYERAXIS2 = 700 appopriate for BAR5 with a SIZEAXIS2 = 137 (the same ass we use elsewhere for Wedge0.6A). SCALABLE BENCHMARK: We expect full-well at r=0.15" with BAR10 from wings of stellar PSF in 1 second for V=5.0 (A0V) {**to be re-verified**}. HR 4735 is V = 5.57 so saturation in 1.69Ss. So 90% full well in appx 1.52s. Use this for the BAR5 exposures, repeated (8x) with multiple CR Splits. NOTE TO PC/CS: Here we use the BAR5 occulter (Aperture) that we comissioned in GO program 12923. This aperture is not available in APT Phase 2, *AND* the SIAF locations of the aperture fiducial we determined in GO 12923 is yet to be populated in SIAF.dat and flowed down to the ground system. We therefore call out BAR10 and use POS TARGs to move the target to the desired positions behind the BAR5 occulter. He we attempt to place the target on 1/4 pixel below the mid-line of BAR5. We then use a subarray readout of CENTYERAXIS2 = 700 appropriate for BAR5 with a SIZEAXIS2 = 137 (the same ass we use elsewhere for Wedge0.6A). SCALABLE BENCHMARK: We expect full-well at r=0.15" with BAR10 from wings of stellar PSF in 1 second for V=5.0 (A0V) {**to be re-verified**}. HR 4735 is V = 5.57 so saturation in 1.69Ss. So 90% full well in appx 1.52s. Use this for the BAR5 exposures, repeated (8x) with multiple CR Splits. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HR 4725 is V =5.57 so saturation in 6.43s. So 90% full well in appx 5.78s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. For long exposures at WedgeA1.0 go (up to) 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. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HR 4725 is V =5.57 so saturation in 6.43s. So 90% full well in appx 5.78s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. For long exposures at WedgeA1.0 go (up to) 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 22.2. CASM was run in Phase II mode. 1404842995345 HR 4796 (V=5.78, B-V = +0.01). FSecond of two sets of visits, each containing three visits of HR 4735 at different relative orientations with one PSF calibration observation interleaved. This is the third HR 4735 visit in the first set. The four visits within each set must be executed sequentally in contiguous orbits interrupted only for Earth occultation. Relative Timing: This visit (48) should immediately follow Visit 47. I.e., They should be executed sequentially in "back-to-back" orbits. 1436459297000 135.46399999999988 (Tic-Visit :proposal-id 13786 :visit-id "48" :proposal-version -1 :trans-version "20140605" :date "08-Jul-2014 11:09:53.0" :trans-errors '(:WARNINGS 24 :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 125952 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13786 :visit-id "48" :obset-id "48" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13786 :visit-id "48" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2898 :al-overhead-at-end 0 :internal-dur-at-end 435 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3278 :pcs-gap 0 ) false 1 0 V = 5.78, sp = A0V, Exptime rounded to nearest 0.1 second ETC Request ID: STIS.ta.618243 NOTE TO PC/CS: Here we use the BAR5 occulter (Aperture) that we comissioned in GO program 12923. This aperture is not available in APT Phase 2, *AND* the SIAF locations of the aperture fiducial we determined in GO 12923 is yet to be populated in SIAF.dat and flowed down to the ground system. We therefore call out BAR10 and use POS TARGs to move the target to the desired positions behind the BAR5 occulter. He we attempt to place the target on the mid-line of BAR5. We then use a subarray readout of CENTYERAXIS2 = 700 appopriate for BAR5 with a SIZEAXIS2 = 137 (the same ass we use elsewhere for Wedge0.6A). SCALABLE BENCHMARK: We expect full-well at r=0.15" with BAR10 from wings of stellar PSF in 1 second for V=5.0 (A0V) {**to be re-verified**}. HR 4796 is V = 5.78 so saturation in 2.09s. So 90% full well in appx 1.85s. Use this for the BAR5 exposures, repeated (8x) with multiple CR Splits. NOTE TO PC/CS: Here we use the BAR5 occulter (Aperture) that we comissioned in GO program 12923. This aperture is not available in APT Phase 2, *AND* the SIAF locations of the aperture fiducial we determined in GO 12923 is yet to be populated in SIAF.dat and flowed down to the ground system. We therefore call out BAR10 and use POS TARGs to move the target to the desired positions behind the BAR5 occulter. He we attempt to place the target 1/4 pixel above the mid-line of BAR5. We then use a subarray readout of CENTYERAXIS2 = 700 appopriate for BAR5 with a SIZEAXIS2 = 137 (the same ass we use elsewhere for Wedge0.6A). SCALABLE BENCHMARK: We expect full-well at r=0.15" with BAR10 from wings of stellar PSF in 1 second for V=5.0 (A0V) {**to be re-verified**}. HR 4796 is V = 5.78 so saturation in 2.09s. So 90% full well in appx 1.85s. Use this for the BAR5 exposures, repeated (8x) with multiple CR Splits. NOTE TO PC/CS: Here we use the BAR5 occulter (Aperture) that we comissioned in GO program 12923. This aperture is not available in APT Phase 2, *AND* the SIAF locations of the aperture fiducial we determined in GO 12923 is yet to be populated in SIAF.dat and flowed down to the ground system. We therefore call out BAR10 and use POS TARGs to move the target to the desired positions behind the BAR5 occulter. He we attempt to place the target 1/4 pixel below the mid-line of BAR5. We then use a subarray readout of CENTYERAXIS2 = 700 appopriate for BAR5 with a SIZEAXIS2 = 137 (the same ass we use elsewhere for Wedge0.6A). SCALABLE BENCHMARK: We expect full-well at r=0.15" with BAR10 from wings of stellar PSF in 1 second for V=5.0 (A0V) {**to be re-verified**}. HR 4796 is V = 5.78 so saturation in 2.09s. So 90% full well in appx 1.85s. Use this for the BAR5 exposures, repeated (8x) with multiple CR Splits. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HR 4796 is V =5.78 so saturation in 7.80s. So 90% full well in appx 7.02s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. For long exposures at WedgeA1.0 go (up to) 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. SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HR 4796 is V =5.78 so saturation in 7.80s. So 90% full well in appx 7.02s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. For long exposures at WedgeA1.0 go (up to) 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 23.2. CASM was run in Phase II mode. 1438632508169 /Users/glenn/Desktop/GO13786_APT2/OP-cache/GO13786_03AUG2015-v51.xml HD 202917 (V=8.67, B-V = +0.65). First of two sets of visits, each containing three visits of HD 202917 at different relative orientations with one PSF calibration observation interleaved. This is the first HD 202917 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. We allow a relative orientation tolerence from 15 deg to 30 deg to assist in guide star selection and scheduling. NOTE to PC: Schedule as close to 30 deg from Visit 52 as possible. Relative Timing: This visit (51) should immediately preceed visit (52). I.e., They should be executed sequentially in "back-to-back" orbits. (Tic-Visit :proposal-id 13786 :visit-id "51" :proposal-version -1 :trans-version "20150609" :date "03-Aug-2015 13:08:27.0" :trans-errors '(:WARNINGS 8 :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 13786 :visit-id "51" :obset-id "51" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13786 :visit-id "51" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2954 :al-overhead-at-end 0 :internal-dur-at-end 346 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3403 :pcs-gap 0 ) true 1 0 SNR = 100, V = 8,67, sp = G7V, Exptime rounded to nearest 0.1 second ETC Request ID: STIS.ta.618240 SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD 202917 is V = 8.67 so saturation in 111.68s. So 90% full well in appx 100.52s. 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 202917 is V = 8.67 so saturation in 111.68s. So 90% full well in appx 100.52s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. For long exposures at WedgeA1.0 go (up to) 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] [53 After 52 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 23.2. CASM was run in Phase II mode. 1438632512505 /Users/glenn/Desktop/GO13786_APT2/OP-cache/GO13786_03AUG2015-v52.xml HD 202917 (V=8.67, B-V = +0.65). First of two sets of visits, each containing three visits of HD 202917 at different relative orientations with one PSF calibration observation interleaved. This is the second HD 202917 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). This visit at nominal roll as scheduled by STScI. Visits 51, 54, 55, 56 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. (Tic-Visit :proposal-id 13786 :visit-id "52" :proposal-version -1 :trans-version "20150609" :date "03-Aug-2015 13:08:31.0" :trans-errors '(:WARNINGS 8 :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 13786 :visit-id "52" :obset-id "52" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13786 :visit-id "52" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2954 :al-overhead-at-end 0 :internal-dur-at-end 346 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3403 :pcs-gap 0 ) true 1 0 SNR = 100, V = 8,67, sp = G7V, Exptime rounded to nearest 0.1 second ETC Request ID: STIS.ta.618240 SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD 202917 is V = 8.67 so saturation in 111.68s. So 90% full well in appx 100.52s. 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 202917 is V = 8.67 so saturation in 111.68s. So 90% full well in appx 100.52s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. For long exposures at WedgeA1.0 go (up to) 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 ([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 23.2. CASM was run in Phase II mode. 1438702141185 /private/var/folders/z3/1f1ry3tx34lf_81wtfblpwgw0000gn/T/OPVisit4160422241655904952.xml PSF03 (LTT 8893). PSF calibration target for HD 202917. V = 7.22. B - V = +0.66. Sp G3V 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) then 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. NOTE: W'ith Visit 53 resubmission on 04AUG2015, 171 seconds are left unused at the back end of this visibility window to assure schedualability into the mid-October timeframe to enable the relative rolls found acceptable. 152 second minimum unused was required per Beth P. email 04AUG2015. (Tic-Visit :proposal-id 13786 :visit-id "53" :proposal-version -1 :trans-version "20150609" :date "04-Aug-2015 08:28:59.0" :trans-errors '(:WARNINGS 20 :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 122720 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13786 :visit-id "53" :obset-id "53" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13786 :visit-id "53" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2952 :al-overhead-at-end 0 :internal-dur-at-end 432 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3456 :pcs-gap 0 ) true 1 0 SNR = 100, V = 6.22, sp = G3V, Exptime rounded to nearest 0.1 second ETC Request ID: STIS.ta.618251 SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). LTT 8893 is V = 7.22, so saturation in 29.38s. So 90% full well in appx 26.43s. 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 SIZEAXIS2 = 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). LTT 8893 is V = 7.22, so saturation in 29.38s. So 90% full well in appx 26.43s. 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 SIZEAXIS2 = 137, appropriate for the WedgeA0.6 position. NOTE ON EXPOSURE TIME: Was revised 04AUG2015 based upon prior executed Visit 57 observations to 129s per individual exposure (before CR splitting) to avoid saturation at Wedge 1.0 beyond the A wedge edge. 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. NOTE ON EXPOSURE TIME: Was revised 04AUG2015 based upon prior executed Visit 57 observations to 129s per individual exposure (before CR splitting) to avoid saturation at Wedge 1.0 beyond the A wedge edge. 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 23.2. CASM was run in Phase II mode. 1438632516841 /Users/glenn/Desktop/GO13786_APT2/OP-cache/GO13786_03AUG2015-v54.xml HD 202917 (V=8.67, B-V = +0.65). First of two sets of visits, each containing three visits of HD 202917 at different relative orientations with one PSF calibration observation interleaved. This is the third HD 202917 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. We allow a relative orientation tolerence from -15 deg to -30 deg to assist in guide star selection and scheduling. NOTE to PC: Schedule as close to -30 deg from Visit 52 as possible. Relative Timing: This visit (54) should immediately follow Visit 53. I.e., They should be executed sequentially in "back-to-back" orbits. (Tic-Visit :proposal-id 13786 :visit-id "54" :proposal-version -1 :trans-version "20150609" :date "03-Aug-2015 13:08:36.0" :trans-errors '(:WARNINGS 8 :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 13786 :visit-id "54" :obset-id "54" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13786 :visit-id "54" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2954 :al-overhead-at-end 0 :internal-dur-at-end 346 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3403 :pcs-gap 0 ) true 1 0 SNR = 100, V = 8,67, sp = G7V, Exptime rounded to nearest 0.1 second ETC Request ID: STIS.ta.618240 SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD 202917 is V = 8.67 so saturation in 111.68s. So 90% full well in appx 100.52s. 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 202917 is V = 8.67 so saturation in 111.68s. So 90% full well in appx 100.52s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. For long exposures at WedgeA1.0 go (up to) 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 ([56 After 55 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 23.2. CASM was run in Phase II mode. 1438632532813 /Users/glenn/Desktop/GO13786_APT2/OP-cache/GO13786_03AUG2015-v55.xml HD 202917 (V=8.67, B-V = +0.65). Second of two sets of visits, each containing three visits of HD 202917 at different relative orientations with one PSF calibration observation interleaved. This is the first HD 202917 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 (+ or -) is equally acceptable, but there is no way to specificy this via APT 22.2. Here we specify a range of relative orientations of -75 deg to -105 deg to assist in guide star selection and scheduling. NOTE to PC: Schedule as close to -90 deg from Visit 51 as possible. Note to PC: You may freely change the parity of the relative orientation to positive if needed for guise star selection and scheduling. Relative Timing: Schedule in orbit immediately before Visit 56. 1438471156000 6.0 (Tic-Visit :proposal-id 13786 :visit-id "55" :proposal-version -1 :trans-version "20150609" :date "03-Aug-2015 13:08:51.0" :trans-errors '(:WARNINGS 9 :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 13786 :visit-id "55" :obset-id "55" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13786 :visit-id "55" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3074 :al-overhead-at-end 0 :internal-dur-at-end 346 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3403 :pcs-gap 0 ) true 1 1 SNR = 100, V = 8,67, sp = G7V, Exptime rounded to nearest 0.1 second ETC Request ID: STIS.ta.618240 SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD 202917 is V = 8.67 so saturation in 111.68s. So 90% full well in appx 100.52s. 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 202917 is V = 8.67 so saturation in 111.68s. So 90% full well in appx 100.52s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. For long exposures at WedgeA1.0 go (up to) 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 ([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 23.2. CASM was run in Phase II mode. 1438632541998 /Users/glenn/Desktop/GO13786_APT2/OP-cache/GO13786_03AUG2015-v56.xml HD 202917 (V=8.67, B-V = +0.65). Second of two sets of visits, each containing three visits of HD 202917 at different relative orientations with one PSF calibration observation interleaved. This is the second HD 202917 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 (56) at -30 deg from Visit 55. We allow a relative orientation tolerence from -15 deg to -30 deg to assist in guide star selection and scheduling. NOTE to PC: Schedule as close to -30 deg from Visit 55 as possible. 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. 1438477292000 345.5 (Tic-Visit :proposal-id 13786 :visit-id "56" :proposal-version -1 :trans-version "20150609" :date "03-Aug-2015 13:09:01.0" :trans-errors '(:WARNINGS 9 :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 13786 :visit-id "56" :obset-id "56" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13786 :visit-id "56" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3074 :al-overhead-at-end 0 :internal-dur-at-end 346 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3403 :pcs-gap 0 ) true 1 1 SNR = 100, V = 8,67, sp = G7V, Exptime rounded to nearest 0.1 second ETC Request ID: STIS.ta.618240 SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD 202917 is V = 8.67 so saturation in 111.68s. So 90% full well in appx 100.52s. 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 202917 is V = 8.67 so saturation in 111.68s. So 90% full well in appx 100.52s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. For long exposures at WedgeA1.0 go (up to) 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 ([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 23.2. CASM was run in Phase II mode. 1438632545217 /Users/glenn/Desktop/GO13786_APT2/OP-cache/GO13786_03AUG2015-v57.xml PSF03 (LTT 8893). PSF calibration target for HD 202917. V = 7.22. B - V = +0.66. Sp G3V 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) then 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. 1438482800000 330.0 (Tic-Visit :proposal-id 13786 :visit-id "57" :proposal-version -1 :trans-version "20150609" :date "03-Aug-2015 13:09:03.0" :trans-errors '(:WARNINGS 21 :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 54896 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 13786 :visit-id "57" :obset-id "57" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13786 :visit-id "57" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3130 :al-overhead-at-end 0 :internal-dur-at-end 359 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3456 :pcs-gap 0 ) true 1 1 SNR = 100, V = 6.22, sp = G3V, Exptime rounded to nearest 0.1 second ETC Request ID: STIS.ta.618251 SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). LTT 8893 is V = 7.22, so saturation in 29.38s. So 90% full well in appx 26.43s. 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 SIZEAXIS2 = 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). LTT 8893 is V = 7.22, so saturation in 29.38s. So 90% full well in appx 26.43s. 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 SIZEAXIS2 = 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). LTT 8893 is V = 7.22, so saturation in 29.38s. So 90% full well in appx 26.43s. For long exposures at WedgeA1.0 go (at least (x20) 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 23.2. CASM was run in Phase II mode. 1438632548085 /Users/glenn/Desktop/GO13786_APT2/OP-cache/GO13786_03AUG2015-v58.xml HD 202917 (V=8.67, B-V = +0.65). Second of two sets of visits, each containing three visits of HD 202917 at different relative orientations with one PSF calibration observation interleaved. This is the third HD 202917 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 (58) at -60 deg from Visit 55. We allow a relative orientation tolerence from -41 deg to -60 deg to assist in guide star selection and scheduling. NOTE to PC: Schedule as close to -60 deg from Visit 55 as possible. Relative Timing: This visit (58) should immediately follow Visit 57. I.e., They should be executed sequentially in "back-to-back" orbits. 1438488422000 325.0 (Tic-Visit :proposal-id 13786 :visit-id "58" :proposal-version -1 :trans-version "20150609" :date "03-Aug-2015 13:09:07.0" :trans-errors '(:WARNINGS 9 :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 13786 :visit-id "58" :obset-id "58" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 13786 :visit-id "58" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3074 :al-overhead-at-end 0 :internal-dur-at-end 346 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3403 :pcs-gap 0 ) true 1 1 SNR = 100, V = 8,67, sp = G7V, Exptime rounded to nearest 0.1 second ETC Request ID: STIS.ta.618240 SCALABLE BENCHMARK: We expect full-well at r=0.3" from wings of stellar PSF in 1 second for V=3.55 (A0V). HD 202917 is V = 8.67 so saturation in 111.68s. So 90% full well in appx 100.52s. 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 202917 is V = 8.67 so saturation in 111.68s. So 90% full well in appx 100.52s. Use this for the "short" exposures, repeated (8x) with multiple CR Splits. For long exposures at WedgeA1.0 go (up to) 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.