Linking the Jet, Inner Disk, and Outer Disk of HD 163296

Scientific Category is a required field. Science Keywords: Select from 2 to 5 items. Instrument Setup(s) is a required field. Please specify your scheduling constraints or 'No Constraints' on all Observation forms. 0 Assigned ID: 1614 ----- Attempting Submission 1 (Wed Nov 15 16:43:44 GMT 2017) ----- HST Phase I Proposal 1614 (Rich.apt) successfully submitted. Receipt: # 1614-1 ----- Attempting Submission 2 (Wed Nov 15 16:52:26 GMT 2017) ----- Joint NRAO 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 Unschedulable Visit 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 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Submission aborted. ----- Attempting Submission 2 (Tue Mar 06 21:57:38 GMT 2018) ----- I am sending a message to Shelly w/ details. Linking the Jet, Inner Disk, and Outer Disk of HD 163296 Young protoplanetary disks serve both as the birthplace of planets and help to guide the accretion of material onto forming stars. The HD 163296 protoplanetary disk system has revealed substantial and often unexpected variability in its accretion, inner disk structure, outer disk appearance, "dipper" extinction events, and periodic HH knot ejections. The Herbig-Haro (HH) knots for HD 163296 are ejected every 16 years, and the next ejection is predicted to occur in 2018. Concurrent observations of the jet, inner disk, and outer disk during a knot ejection provide a unique opportunity to constrain the interplay between these three regions. We propose to monitor HD 163296 with the VLA to detect the next knot ejection event. Then when an HH knot ejection is detected, we will schedule observations with Hubble to monitor how the ejection of the HH knot affects the outer disk. These observations will anchor our efforts to use pre-existing radiative transfer codes to construct a self-consistent picture of the system's circumstellar environment. We will use 8 orbits of STIS coronagraphic imagery to study the disk and HH knots of HD 163296 after the VLA has performed monthly montoring of the system's jet to search for evidence of a 17-yr periodic jet activity event. We will use the 6 roll/PSF template subtraction strategy that has been successfuly demonstrated in previous programs. We will obtain a sequence of short and long coronagraphic exposures at 6 different spacecraft roll angles using the wedge A0.6 and A1.0 coronagraphic apertures. The 8 orbits will be broken up into two sets of 4 orbits with each set containing 3 orbits with relative orientations of -30D to -15D, 0D, and +15-30D (with loose tolerance) from off-nominal rolls to observe HD 163296 (science target) and one orbit to observe the PSF star. The two sets are each scheduled (typically at different epochs) at nominal roll relative orientations differing by 90-150Dto fully sample 360D around the star. VLA observations, which are scheduled ~every 3-4 weeks, will look for flux changes associated with the emission of an HH-knot, that is predicted based on a 17-yr periodic ejection timescale. Given the limited HST visibility windows, we a) only use the combination of Wedge A0.6 and A1.0 apertures, instead of BAR5 and Wedge A1.0 apertures, which will provide substantial increase in visibility window flexibility at nominal science impact; and b) be scheduled as close to the August/September 2018 time-frame as possible, such that our HST observations occur near the end of our VLA monitoring. Planets and Planet Formation 6 false false false false false false false AVAILABLE STAR HERBIG AE/BE This object was generated by the targetselector and retrieved from the SIMBAD database. J2000 J2000 B-V=0.08 STAR A0-A3 V-IV J2000 B-V=0.101 STIS/CCD Imaging Yes No WEDGEA1.0 STIS/CCD Imaging Yes No BAR5 1531156663265 Timing link suitability includes constraints ([02 After 01 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 26.0. CASM was run in Phase II mode. HD 163296 First of two sets of visits, each containing three visits of HD163296 at different relative orientations with one PSF calibration observation visit interleaved. This set of visits uses WedgeA. This is the first HD163296 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 have set the allowable orientation to range from -30 deg to -15 degrees from Visit 2, to allow a sufficiently large scheduling window. 1523744845000 254.68389640878002 (Tic-Visit :proposal-id 15437 :visit-id "01" :proposal-version -1 :trans-version "20180409" :date "09-Jul-2018 12:17:42.0" :trans-errors '(:WARNINGS 23 :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 169424 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15437 :visit-id "01" :obset-id "01" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15437 :visit-id "01" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2883 :al-overhead-at-end 0 :internal-dur-at-end 422 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3217 :pcs-gap 0 ) true 1 0 SNR=100, A1V, V=6.85, rounded to nearest 0.1 magnitude Exposure times scaled from 90% full well depth for GO-15219 WedgeA0.6 observations of AU Mic, HD198939, & HD191849. Use this for the "short" exposures, using 8 CR Splits and gain-4. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits 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 Exposure times scaled from 90% full well depth for GO-15219 WedgeA0.6 observations of AU Mic, HD198939, & HD191849. Use this for the "short" exposures, using 8 CR Splits and gain-4. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits 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 Exposure times scaled from 90% full well depth for GO-15219 WedgeA0.6 observations of AU Mic, HD198939, & HD191849. Use this for the "short" exposures, using 6 CR Splits and gain-4. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits 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 Exposure times scaled from 90% full well depth for GO-15219 WedgeA0.6 observations of AU Mic, HD198939, & HD191849. Use this for the "long" exposures, using 8 CR Splits and gain-4. 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. Exposure times scaled from 90% full well depth for GO-15219 WedgeA0.6 observations of AU Mic, HD198939, & HD191849. Use this for the "long" exposures, using 8 CR Splits and gain-4. 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. 1531156665820 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 26.0. CASM was run in Phase II mode. HD 163296 First of two sets of visits, each containing three visits of HD163296 at different relative orientations with one PSF calibration observation visit interleaved. This set of visits uses WedgeA. This is the second HD163296 visit in the first set. The four visits within each set MUST be executed sequentally in contiguous orbits interrupted only for Earth occultation. Orientation: This visit has NO orient constraints. Timing requirements: This visit MUST be executed in the subsequent orbit to visit #1. 1523750616000 269.68389640877996 (Tic-Visit :proposal-id 15437 :visit-id "02" :proposal-version -1 :trans-version "20180409" :date "09-Jul-2018 12:17:44.0" :trans-errors '(:WARNINGS 23 :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 169424 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15437 :visit-id "02" :obset-id "02" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15437 :visit-id "02" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2883 :al-overhead-at-end 0 :internal-dur-at-end 422 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3217 :pcs-gap 0 ) true 1 0 SNR=100, A1V, V=6.85, rounded to nearest 0.1 magnitude Exposure times scaled from 90% full well depth for GO-15219 WedgeA0.6 observations of AU Mic, HD198939, & HD191849. Use this for the "short" exposures, using 8 CR Splits and gain-4. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits 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 Exposure times scaled from 90% full well depth for GO-15219 WedgeA0.6 observations of AU Mic, HD198939, & HD191849. Use this for the "short" exposures, using 8 CR Splits and gain-4. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits 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 Exposure times scaled from 90% full well depth for GO-15219 WedgeA0.6 observations of AU Mic, HD198939, & HD191849. Use this for the "short" exposures, using 6 CR Splits and gain-4. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits 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 Exposure times scaled from 90% full well depth for GO-15219 WedgeA0.6 observations of AU Mic, HD198939, & HD191849. Use this for the "long" exposures, using 8 CR Splits and gain-4. 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. Exposure times scaled from 90% full well depth for GO-15219 WedgeA0.6 observations of AU Mic, HD198939, & HD191849. Use this for the "long" exposures, using 8 CR Splits and gain-4. 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. 1531156670645 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 26.0. CASM was run in Phase II mode. HD 145570 First of two sets of visits, each containing three visits of HD163296 at different relative orientations with one PSF calibration observation visit interleaved. This set of visits uses WedgeA. This is the PSF star visit in the first set. The four visits within each set MUST be executed sequentally in contiguous orbits interrupted only for Earth occultation. Orientation: This visit has NO orient constraints. Timing requirements: This visit MUST be executed in the subsequent orbit to visit #2. 1523755846000 273.0 (Tic-Visit :proposal-id 15437 :visit-id "03" :proposal-version -1 :trans-version "20180409" :date "09-Jul-2018 12:17:49.0" :trans-errors '(:WARNINGS 32 :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 319440 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15437 :visit-id "03" :obset-id "03" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15437 :visit-id "03" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2860 :al-overhead-at-end 0 :internal-dur-at-end 414 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3209 :pcs-gap 0 ) true 1 0 SNR=100; A1V; V=4.928; using F25ND5 filter Exposure times scaled from 90% full well depth for GO-15219 WedgeA0.6 observations of AU Mic, HD198939, & HD191849. Use this for the "short" exposures, using 8 CR Splits and gain-4. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits 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 Exposure times scaled from 90% full well depth for GO-15219 WedgeA0.6 observations of AU Mic, HD198939, & HD191849. Use this for the "short" exposures, using 8 CR Splits and gain-4. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits 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 Exposure times scaled from 90% full well depth for GO-15219 WedgeA0.6 observations of AU Mic, HD198939, & HD191849. Use this for the "short" exposures, using 8 CR Splits and gain-4. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits 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 Exposure times scaled from 90% full well depth for GO-15219 WedgeA0.6 observations of AU Mic, HD198939, & HD191849. Use this for the "short" exposures, using 8 CR Splits and gain-4. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits 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 Exposure times scaled from 90% full well depth for GO-15219 WedgeA0.6 observations of AU Mic, HD198939, & HD191849. Use this for the "long" exposures, using 8 CR Splits and gain-4. 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. Exposure times scaled from 90% full well depth for GO-15219 WedgeA0.6 observations of AU Mic, HD198939, & HD191849. Use this for the "long" exposures, using 8 CR Splits and gain-4. 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. Exposure times scaled from 90% full well depth for GO-15219 WedgeA0.6 observations of AU Mic, HD198939, & HD191849. Use this for the "long" exposures, using 8 CR Splits and gain-4. 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. Exposure times scaled from 90% full well depth for GO-15219 WedgeA0.6 observations of AU Mic, HD198939, & HD191849. Use this for the "long" exposures, using 8 CR Splits and gain-4. 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. 1531156673382 Timing link suitability includes constraints ([04 After 03 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 26.0. CASM was run in Phase II mode. HD 163296 First of two sets of visits, each containing three visits of HD163296 at different relative orientations with one PSF calibration observation visit interleaved. This set of visits uses WedgeA. This is the third and final HD163296 visit in the first set. The four visits within each set MUST be executed sequentally in contiguous orbits interrupted only for Earth occultation. Orientation: This visit should be oriented 15 degrees to 30 degrees from visit#2 Timing requirements: This visit MUST be executed in the subsequent orbit to visit #3. 1523762019000 284.6838964087799 (Tic-Visit :proposal-id 15437 :visit-id "04" :proposal-version -1 :trans-version "20180409" :date "09-Jul-2018 12:17:52.0" :trans-errors '(:WARNINGS 23 :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 169424 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15437 :visit-id "04" :obset-id "04" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15437 :visit-id "04" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2883 :al-overhead-at-end 0 :internal-dur-at-end 422 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3217 :pcs-gap 0 ) true 1 0 SNR=100, A1V, V=6.85, rounded to nearest 0.1 magnitude Exposure times scaled from 90% full well depth for GO-15219 WedgeA0.6 observations of AU Mic, HD198939, & HD191849. Use this for the "short" exposures, using 8 CR Splits and gain-4. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits 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 Exposure times scaled from 90% full well depth for GO-15219 WedgeA0.6 observations of AU Mic, HD198939, & HD191849. Use this for the "short" exposures, using 8 CR Splits and gain-4. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits 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 Exposure times scaled from 90% full well depth for GO-15219 WedgeA0.6 observations of AU Mic, HD198939, & HD191849. Use this for the "short" exposures, using 6 CR Splits and gain-4. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits 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 Exposure times scaled from 90% full well depth for GO-15219 WedgeA0.6 observations of AU Mic, HD198939, & HD191849. Use this for the "long" exposures, using 8 CR Splits and gain-4. 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. Exposure times scaled from 90% full well depth for GO-15219 WedgeA0.6 observations of AU Mic, HD198939, & HD191849. Use this for the "long" exposures, using 8 CR Splits and gain-4. 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. 1531156747481 Timing link suitability includes constraints ([06 After 05 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 26.0. CASM was run in Phase II mode. HD 163296 Second of two sets of visits, each containing three visits of HD163296 at different relative orientations with one PSF calibration observation visit interleaved. This set of visits uses WedgeA. This is the first HD163296 visit in the second set. The four visits within each set MUST be executed sequentally in contiguous orbits interrupted only for Earth occultation. Orientation: We have set the allowable orientation to range from -135 deg to -55 degrees from Visit 1, to allow a sufficiently large scheduling window. (Tic-Visit :proposal-id 15437 :visit-id "05" :proposal-version -1 :trans-version "20180409" :date "09-Jul-2018 12:19:04.0" :trans-errors '(:WARNINGS 23 :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 227088 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15437 :visit-id "05" :obset-id "05" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15437 :visit-id "05" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2860 :al-overhead-at-end 0 :internal-dur-at-end 419 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3217 :pcs-gap 0 ) true 1 0 SNR=100, A1V, V=6.85, rounded to nearest 0.1 magnitude Exposure times scaled from 90% full well depth for GO-15219 WedgeA0.6 observations of AU Mic, HD198939, & HD191849. Use this for the "short" exposures, using 8 CR Splits and gain-4. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits 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 Exposure times scaled from 90% full well depth for GO-15219 WedgeA0.6 observations of AU Mic, HD198939, & HD191849. Use this for the "short" exposures, using 8 CR Splits and gain-4. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits 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 Exposure times scaled from 90% full well depth for GO-15219 WedgeA0.6 observations of AU Mic, HD198939, & HD191849. Use this for the "short" exposures, using 6 CR Splits and gain-4. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits 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 Exposure times scaled from 90% full well depth for GO-15219 WedgeA0.6 observations of AU Mic, HD198939, & HD191849. Use this for the "long" exposures, using 8 CR Splits and gain-4. 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. Exposure times scaled from 90% full well depth for GO-15219 WedgeA0.6 observations of AU Mic, HD198939, & HD191849. Use this for the "long" exposures, using 8 CR Splits and gain-4. 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. 1531156806010 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 26.0. CASM was run in Phase II mode. HD 163296 Second of two sets of visits, each containing three visits of HD163296 at different relative orientations with one PSF calibration observation visit interleaved. This set of visits uses WedgeA. This is the second HD163296 visit in the second set. The four visits within each set MUST be executed sequentally in contiguous orbits interrupted only for Earth occultation. Orientation: We have set the allowable orientation to range from -30 deg to -15 degrees from Visit#5, to allow a sufficiently large scheduling window. Timing requirements: This visit MUST be executed in the subsequent orbit to visit #5. (Tic-Visit :proposal-id 15437 :visit-id "06" :proposal-version -1 :trans-version "20180409" :date "09-Jul-2018 12:20:04.0" :trans-errors '(:WARNINGS 23 :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 227088 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15437 :visit-id "06" :obset-id "06" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15437 :visit-id "06" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2860 :al-overhead-at-end 0 :internal-dur-at-end 419 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3217 :pcs-gap 0 ) true 1 0 SNR=100, A1V, V=6.85, rounded to nearest 0.1 magnitude Exposure times scaled from 90% full well depth for GO-15219 WedgeA0.6 observations of AU Mic, HD198939, & HD191849. Use this for the "short" exposures, using 8 CR Splits and gain-4. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits 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 Exposure times scaled from 90% full well depth for GO-15219 WedgeA0.6 observations of AU Mic, HD198939, & HD191849. Use this for the "short" exposures, using 8 CR Splits and gain-4. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits 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 Exposure times scaled from 90% full well depth for GO-15219 WedgeA0.6 observations of AU Mic, HD198939, & HD191849. Use this for the "short" exposures, using 6 CR Splits and gain-4. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits 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 Exposure times scaled from 90% full well depth for GO-15219 WedgeA0.6 observations of AU Mic, HD198939, & HD191849. Use this for the "long" exposures, using 8 CR Splits and gain-4. 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. Exposure times scaled from 90% full well depth for GO-15219 WedgeA0.6 observations of AU Mic, HD198939, & HD191849. Use this for the "long" exposures, using 8 CR Splits and gain-4. 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. 1531156682895 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 26.0. CASM was run in Phase II mode. HD 145570 Second of two sets of visits, each containing three visits of HD163296 at different relative orientations with one PSF calibration observation visit interleaved. This set of visits uses WedgeA. This is the PSF star visit in the second set. The four visits within each set MUST be executed sequentally in contiguous orbits interrupted only for Earth occultation. Orientation: This visit has NO orient constraints. Timing requirements: This visit MUST be executed in the subsequent orbit to visit #6. (Tic-Visit :proposal-id 15437 :visit-id "07" :proposal-version -1 :trans-version "20180409" :date "09-Jul-2018 12:17:58.0" :trans-errors '(:WARNINGS 32 :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 319440 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15437 :visit-id "07" :obset-id "07" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15437 :visit-id "07" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2860 :al-overhead-at-end 0 :internal-dur-at-end 414 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3209 :pcs-gap 0 ) true 1 0 SNR=100; A1V; V=4.928; using F25ND5 filter Exposure times scaled from 90% full well depth for GO-15219 WedgeA0.6 observations of AU Mic, HD198939, & HD191849. Use this for the "short" exposures, using 8 CR Splits and gain-4. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits 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 Exposure times scaled from 90% full well depth for GO-15219 WedgeA0.6 observations of AU Mic, HD198939, & HD191849. Use this for the "short" exposures, using 8 CR Splits and gain-4. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits 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 Exposure times scaled from 90% full well depth for GO-15219 WedgeA0.6 observations of AU Mic, HD198939, & HD191849. Use this for the "short" exposures, using 8 CR Splits and gain-4. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits 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 Exposure times scaled from 90% full well depth for GO-15219 WedgeA0.6 observations of AU Mic, HD198939, & HD191849. Use this for the "short" exposures, using 8 CR Splits and gain-4. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits 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 Exposure times scaled from 90% full well depth for GO-15219 WedgeA0.6 observations of AU Mic, HD198939, & HD191849. Use this for the "long" exposures, using 8 CR Splits and gain-4. 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. Exposure times scaled from 90% full well depth for GO-15219 WedgeA0.6 observations of AU Mic, HD198939, & HD191849. Use this for the "long" exposures, using 8 CR Splits and gain-4. 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. Exposure times scaled from 90% full well depth for GO-15219 WedgeA0.6 observations of AU Mic, HD198939, & HD191849. Use this for the "long" exposures, using 8 CR Splits and gain-4. 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. Exposure times scaled from 90% full well depth for GO-15219 WedgeA0.6 observations of AU Mic, HD198939, & HD191849. Use this for the "long" exposures, using 8 CR Splits and gain-4. 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. 1531161320967 Timing link suitability includes constraints ([08 After 07 by 0.0 to 0.1 days]) The scheduling data was generated by CASM 26.0. CASM was run in Phase II mode. /private/var/folders/bl/s7q0tqnn5gbcbyvcfnrhj2rh0004nc/T/OPVisit9065928605229761056.xml HD 163296 Second of two sets of visits, each containing three visits of HD163296 at different relative orientations with one PSF calibration observation visit interleaved. This set of visits uses WedgeA. This is the third and final HD163296 visit in the second set. The four visits within each set MUST be executed sequentally in contiguous orbits interrupted only for Earth occultation. Orientation: We have set the allowable orientation to range from -60 deg to -45 degrees from Visit#5, to allow a sufficiently large scheduling window. Timing requirements: This visit MUST be executed in the subsequent orbit to visit #7. (Tic-Visit :proposal-id 15437 :visit-id "08" :proposal-version -1 :trans-version "20180409" :date "09-Jul-2018 14:35:18.0" :trans-errors '(:WARNINGS 23 :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 227088 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15437 :visit-id "08" :obset-id "08" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15437 :visit-id "08" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2854 :al-overhead-at-end 0 :internal-dur-at-end 419 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3217 :pcs-gap 0 ) true 1 0 SNR=100, A1V, V=6.85, rounded to nearest 0.1 magnitude Exposure times scaled from 90% full well depth for GO-15219 WedgeA0.6 observations of AU Mic, HD198939, & HD191849. Use this for the "short" exposures, using 8 CR Splits and gain-4. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits 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 Exposure times scaled from 90% full well depth for GO-15219 WedgeA0.6 observations of AU Mic, HD198939, & HD191849. Use this for the "short" exposures, using 8 CR Splits and gain-4. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits 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 Exposure times scaled from 90% full well depth for GO-15219 WedgeA0.6 observations of AU Mic, HD198939, & HD191849. Use this for the "short" exposures, using 6 CR Splits and gain-4. SCALABLE PARAMETER FOR SUB-ARRAY Readout: SIZEAXIS2 = 20 is 1" in full extent (r = 0.5") For these "short" exposures we will image perpendicular to the wedge (symmetrically) centered on the target to the maximum extent permitted by the limits 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 Exposure times scaled from 90% full well depth for GO-15219 WedgeA0.6 observations of AU Mic, HD198939, & HD191849. Use this for the "long" exposures, using 8 CR Splits and gain-4. 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. Exposure times scaled from 90% full well depth for GO-15219 WedgeA0.6 observations of AU Mic, HD198939, & HD191849. Use this for the "long" exposures, using 8 CR Splits and gain-4. 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.