16236( 5) - 06-Oct-2022 20:30:32 - [ 1] HUBBLE SPACE TELESCOPE OBSERVING PROGRAM 16236 Version: 5 Check-in Time: 06-Oct-2022 20:30:32 STScI Edit Number: 3 Title The Life and Death of Ultra-Hot Jupiter WASP-12b ------------------------------------------------------------------------------------ Type Cycle GO 28 ------------------------------------------------------------------------------------ Investigators Contact? PI: Mr. Taylor James Bell Bay Area Environmental Research Institute Y CoI: Prof. Nicolas B Cowan McGill University N CoI: Ms. Lisa Dang McGill University N CoI: Dr. Kevin Stevenson The Johns Hopkins University Applied N Physics Laboratory CoI: Prof. David K. Sing The Johns Hopkins University N CoI: Dr. Laura Kreidberg Max Planck Institute for Astronomy N CoI: Michael Zhang University of Chicago N CoI: Dr. Ian Crossfield University of Kansas Center for Research, N Inc. CoI: Prof. Joshua Winn Princeton University N CoI: Prof. Jonathan Fortney University of California - Santa Cruz N CoI: Dr. Michael Line Arizona State University N CoI: Dr. Patricio E Cubillos Space Research Institute, Austrian Academy N of Sciences CoI: Dr. Drake Deming University of Maryland N CoI: Dr. Kamen Todorov Universiteit van Amsterdam N CoI: Dr. Ian M. Dobbs-Dixon New York University N CoI: Dr. Heather A. Knutson California Institute of Technology N CoI: Dr. Rob Zellem Jet Propulsion Laboratory N CoI: Dr. Luca Fossati Space Research Institute, Austrian Academy N of Sciences ------------------------------------------------------------------------------------ Abstract A new class of exoplanets called ultra-hot Jupiters has recently been recognized; these gas-giant exoplanets are on extremely close orbits around their host stars and have dayside atmospheres which reach >2500 K. Ultra-hot Jupiters are so strongly irradiated that many of the molecules, including the dominant constituent hydrogen, will thermally dissociate on their daysides and may recombine on their cooler nightsides. Significant mass loss and tidal distortion have also been predicted for some ultra-hot Jupiters. However, there are currently few ultra-hot Jupiters whose entire atmospheres are well characterized, and additional high precision observations are required to test recent model predictions. We therefore propose to collect one HST/WFC3 G141 spectroscopic full-orbit phasecurve of WASP-12b - the prototypical ultra-hot Jupiter - in order to create longitudinally resolved temperature and chemical maps, to understand the enormous ellipsoidal variations seen at 4.5 microns, and to better constrain the planet's orbital decay rate and the stellar tidal quality factor. ------------------------------------------------------------------------------------ Observations Description ------------------------ 16236( 5) - 06-Oct-2022 20:30:32 - [ 2] Full-orbit phasecurve observation of the exoplanet WASP-12b using WFC3 G141, containing two secondary eclipses and one transit. We have placed stringent orientation constraints which are necessary to avoid overlapping spectra from nearby stellar objects 1 and 10 arcsec away at PA=250 and 238, respectively. We intend to use the differences between individual non-destructive reads to remove the contamination from the nearby M-dwarfs, using the technique as was tested for HAT-P-32Ab using data from GO 14767 (Nikolov et al., 2018). To guarantee that we are able to subtract the companion spectra, we will also collect 10 staring mode observations during the first, stabilizing orbit (as was done by Kreidberg et al., 2015). We enforce a phase constraint on the first exposure of the first orbit to ensure that we acquire our two baseline orbits before the first secondary eclipse and two baseline orbits after the final secondary eclipse. We have placed our 22 orbits into 3 "visits" with timing constraints on the second and third visits to ensure they follow immediately after each other. We have had to use 3 visits instead of one to solve two error messages from the APT software: (PHASE CRITICAL VISIT HAS PHASE WINDOW LARGER THAN PERIOD; and TOO MANY SUBEXPOSURES IN ONE GROUP (REQUEST HELP FROM YOUR PC)). We have also placed a constraint on the second and third "visits" to ensure that all 22 orbits be collected at the same orientation angle as the first orbit to increase our ability to decorrelate detector systematics and to allow for subtraction of the nearby companion stars. We anticipate there being a need for gyro bias updates and SAA crossing(s), but have not entered any parameters related to this into the APT software. However, two good opportunities for brief interruptions in the observations are at the breaks between visits which are at times not expected to impact the transit, eclipse, or maximum/minimum points of the phasecurve. ------------------------------------------------------------------------------------ 16236( 5) - 06-Oct-2022 20:30:32 - [ 3] TARGET LIST Fixed Targets ------------------------------------------------------------------------------------------------------------------------------------ Tar| Target | Target | Target |Coord | Radial | Flux data No | Name | Description | Position |Eqnx | Vel. | ------------------------------------------------------------------------------------------------------------------------------------ 1 WASP-12 EXT-STAR, EXTRA-SOLAR RA=06H30M32.7967S +/- 0.0323", J2000 V = V = 11.57 +/- 0.16 PLANET, G V-IV DEC=+29D40'20.27" +/- 0.0285" 19.034 Reference Frame: ICRS Comments: This object was generated by the targetselector and retrieved from the SIMBAD database.This object was generated by the targetselector and retrieved from the SIMBAD database. Edited to include Proper Motion, RV, and Parallax Epoch of Position RA proper motion (seconds of time/yr) DEC Proper Motion (arcsec/yr) Annual Parallax (arcsec) 2000 -1.2123012165548467E-4 -0.006958 0.0023122 ------------------------------------------------------------------------------------------------------------------------------------ 16236( 5) - 06-Oct-2022 20:30:32 - [ 4] Visit: 01 (Companion Spec + Science) Visit Requirements: SCHED 70%; ORIENT 162.5D TO 247.5 D; ORIENT 342.7D TO 82.3 D; Period 1.09142030 D AND ZERO-PHASE HJD2456176.668258; SEQ 01, 02, 03, 04, 05, 06, 07 WITHIN 18 Orbits On Hold Comments: Additional Comments: The stringent orientation constraints are necessary to avoid overlapping spectra from nearby stellar objects 1 and 10 arcsec away at PA=250 and 238. We calculate the central values for our orient ranges using Detector Offset+PA=135+250=25 or 205. We calculate the width of our orient range to ensure that after each non-destructive read the two stars' spectra are still separated by >4 FWHM to try to allow for our mildly experimental technique to subtract the comanion flux using the differences between non-destructive reads (tested for HAT-P-32Ab using data from GO 14767; Nikolov et al., 2018). To guarantee that we are able to subtract the companion spectra, we will also collect 10 staring mode observations during the first, stabilizing orbit (as was done by Kreidberg et al., 2015); our orient ranges ensure that the spectra will be separated by >5.6 FWHM for these staring-mode spectra. We enforce a phase constraint on the first exposure to ensure that we acquire our two baseline orbits before the first secondary eclipse and two baseline orbits after the final secondary eclipse. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 1 WASP-12 WFC3/IR MULTIAC GRISM256 F126N SAMP-SEQ=RAPID, NSAMP=3 1 DEF (0.833 POS TARG 0, 0; PHASE CUM S) 0.31625 TO 0.35475; GS ACQ SCENARIO BASE1BE; SEQ 1-3 NON-INT Comments: F126N was selected as a narrow band filter to avoid saturation while determining the wavelength solution. This filter was also previously successfully used in GO program 13467 (Kreidberg et al., 2015). ------------------------------------------------------------------------------------------------------------------------------------ 2 WASP-12 WFC3/IR MULTIAC GRISM256 G141 SAMP-SEQ=SPARS10, NSAMP=2 9 DEF POS TARG 0, 0 CUM (68.619 S) Comments: No spatial scan desired here to ensure the separation between WASP-12A and the nearby M-dwarf companions WASP-12B, C. ------------------------------------------------------------------------------------------------------------------------------------ 16236( 5) - 06-Oct-2022 20:30:32 - [ 5] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 3 WASP-12 WFC3/IR MULTIAC GRISM256 G141 SAMP-SEQ=SPARS10, NSAMP=15 7 DEF POS TARG 0, 0; SPATIAL CUM (1443.801 SCAN 0.0325, 90.0 S) Degrees, Round trip Comments: Our scan rate, SAMP-SEQ, and NSAMP ere jointly optimized to provide high observing efficiency, a peak per-pixel count of ~35, 000 to ensure rapid charge-trapping equilibriation within the first orbit, and the ability to separate the contaminating flux from the nearby M-dwarf companions at PA=250 while also not excessively limiting the ORIENT range of the observations. ------------------------------------------------------------------------------------------------------------------------------------ 4 WASP-12 WFC3/IR MULTIAC GRISM256 F126N SAMP-SEQ=RAPID, NSAMP=3 1 DEF (0.833 POS TARG 0, 0; SEQ 4-5 CUM S) NON-INT Comments: F126N was selected as a narrow band filter to avoid saturation while determining the wavelength solution. This filter was also previously successfully used in GO program 13467 (Kreidberg et al., 2015). ------------------------------------------------------------------------------------------------------------------------------------ 5 WASP-12 WFC3/IR MULTIAC GRISM256 G141 SAMP-SEQ=SPARS10, NSAMP=15 8 DEF POS TARG 0, 0; SPATIAL CUM (1650.058 SCAN 0.0325, 90.0 S) Degrees, Round trip Comments: Our scan rate, SAMP-SEQ, and NSAMP ere jointly optimized to provide high observing efficiency, a peak per-pixel count of ~35, 000 to ensure rapid charge-trapping equilibriation within the first orbit, and the ability to separate the contaminating flux from the nearby M-dwarf companions at PA=250 while also not excessively limiting the ORIENT range of the observations. ------------------------------------------------------------------------------------------------------------------------------------ 6 WASP-12 WFC3/IR MULTIAC GRISM256 F126N SAMP-SEQ=RAPID, NSAMP=3 1 DEF (0.833 POS TARG 0, 0; SEQ 6-7 CUM S) NON-INT Comments: F126N was selected as a narrow band filter to avoid saturation while determining the wavelength solution. This filter was also previously successfully used in GO program 13467 (Kreidberg et al., 2015). ------------------------------------------------------------------------------------------------------------------------------------ 16236( 5) - 06-Oct-2022 20:30:32 - [ 6] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 7 WASP-12 WFC3/IR MULTIAC GRISM256 G141 SAMP-SEQ=SPARS10, NSAMP=15 8 DEF POS TARG 0, 0; SPATIAL CUM (1650.058 SCAN 0.0325, 90.0 S) Degrees, Round trip Comments: Our scan rate, SAMP-SEQ, and NSAMP ere jointly optimized to provide high observing efficiency, a peak per-pixel count of ~35, 000 to ensure rapid charge-trapping equilibriation within the first orbit, and the ability to separate the contaminating flux from the nearby M-dwarf companions at PA=250 while also not excessively limiting the ORIENT range of the observations. ------------------------------------------------------------------------------------------------------------------------------------ Sub Exposures ------------------------------------------------------------------------------------------------------------------------------------ Target | Exp |Instr | Oper. | Aper |Spectral|Cent.|Primary |Secondary |Iteration |CR-SPLIT |Orbit |Duration Name | Num |Config | Mode | or FOV |Element |Wave.|Pattern Pos |Pattern Pos |Num |Num |Number | ------------------------------------------------------------------------------------------------------------------------------------ WASP-12 1 WFC3/IR MULTIAC GRISM256 F126N none none none none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 1 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 2 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 3 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 4 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 5 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 6 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 7 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 8 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 9 none 1 N/A CUM WASP-12 3 WFC3/IR MULTIAC GRISM256 G141 none none 1 none 1 N/A CUM WASP-12 3 WFC3/IR MULTIAC GRISM256 G141 none none 1 none 1 N/A CUM WASP-12 3 WFC3/IR MULTIAC GRISM256 G141 none none 2 none 1 N/A CUM WASP-12 3 WFC3/IR MULTIAC GRISM256 G141 none none 2 none 1 N/A CUM 16236( 5) - 06-Oct-2022 20:30:32 - [ 7] Sub Exposures ------------------------------------------------------------------------------------------------------------------------------------ Target | Exp |Instr | Oper. | Aper |Spectral|Cent.|Primary |Secondary |Iteration |CR-SPLIT |Orbit |Duration Name | Num |Config | Mode | or FOV |Element |Wave.|Pattern Pos |Pattern Pos |Num |Num |Number | ------------------------------------------------------------------------------------------------------------------------------------ WASP-12 3 WFC3/IR MULTIAC GRISM256 G141 none none 3 none 1 N/A CUM WASP-12 3 WFC3/IR MULTIAC GRISM256 G141 none none 3 none 1 N/A CUM WASP-12 3 WFC3/IR MULTIAC GRISM256 G141 none none 4 none 1 N/A CUM WASP-12 3 WFC3/IR MULTIAC GRISM256 G141 none none 4 none 1 N/A CUM WASP-12 3 WFC3/IR MULTIAC GRISM256 G141 none none 5 none 1 N/A CUM WASP-12 3 WFC3/IR MULTIAC GRISM256 G141 none none 5 none 1 N/A CUM WASP-12 3 WFC3/IR MULTIAC GRISM256 G141 none none 6 none 1 N/A CUM WASP-12 3 WFC3/IR MULTIAC GRISM256 G141 none none 6 none 1 N/A CUM WASP-12 3 WFC3/IR MULTIAC GRISM256 G141 none none 7 none 1 N/A CUM WASP-12 3 WFC3/IR MULTIAC GRISM256 G141 none none 7 none 1 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 F126N none none none none 2 N/A CUM WASP-12 5 WFC3/IR MULTIAC GRISM256 G141 none none 1 none 2 N/A CUM WASP-12 5 WFC3/IR MULTIAC GRISM256 G141 none none 1 none 2 N/A CUM WASP-12 5 WFC3/IR MULTIAC GRISM256 G141 none none 2 none 2 N/A CUM WASP-12 5 WFC3/IR MULTIAC GRISM256 G141 none none 2 none 2 N/A CUM WASP-12 5 WFC3/IR MULTIAC GRISM256 G141 none none 3 none 2 N/A CUM WASP-12 5 WFC3/IR MULTIAC GRISM256 G141 none none 3 none 2 N/A CUM WASP-12 5 WFC3/IR MULTIAC GRISM256 G141 none none 4 none 2 N/A CUM WASP-12 5 WFC3/IR MULTIAC GRISM256 G141 none none 4 none 2 N/A CUM WASP-12 5 WFC3/IR MULTIAC GRISM256 G141 none none 5 none 2 N/A CUM WASP-12 5 WFC3/IR MULTIAC GRISM256 G141 none none 5 none 2 N/A CUM WASP-12 5 WFC3/IR MULTIAC GRISM256 G141 none none 6 none 2 N/A CUM WASP-12 5 WFC3/IR MULTIAC GRISM256 G141 none none 6 none 2 N/A CUM WASP-12 5 WFC3/IR MULTIAC GRISM256 G141 none none 7 none 2 N/A CUM 16236( 5) - 06-Oct-2022 20:30:32 - [ 8] Sub Exposures ------------------------------------------------------------------------------------------------------------------------------------ Target | Exp |Instr | Oper. | Aper |Spectral|Cent.|Primary |Secondary |Iteration |CR-SPLIT |Orbit |Duration Name | Num |Config | Mode | or FOV |Element |Wave.|Pattern Pos |Pattern Pos |Num |Num |Number | ------------------------------------------------------------------------------------------------------------------------------------ WASP-12 5 WFC3/IR MULTIAC GRISM256 G141 none none 7 none 2 N/A CUM WASP-12 5 WFC3/IR MULTIAC GRISM256 G141 none none 8 none 2 N/A CUM WASP-12 5 WFC3/IR MULTIAC GRISM256 G141 none none 8 none 2 N/A CUM WASP-12 6 WFC3/IR MULTIAC GRISM256 F126N none none none none 3 N/A CUM WASP-12 7 WFC3/IR MULTIAC GRISM256 G141 none none 1 none 3 N/A CUM WASP-12 7 WFC3/IR MULTIAC GRISM256 G141 none none 1 none 3 N/A CUM WASP-12 7 WFC3/IR MULTIAC GRISM256 G141 none none 2 none 3 N/A CUM WASP-12 7 WFC3/IR MULTIAC GRISM256 G141 none none 2 none 3 N/A CUM WASP-12 7 WFC3/IR MULTIAC GRISM256 G141 none none 3 none 3 N/A CUM WASP-12 7 WFC3/IR MULTIAC GRISM256 G141 none none 3 none 3 N/A CUM WASP-12 7 WFC3/IR MULTIAC GRISM256 G141 none none 4 none 3 N/A CUM WASP-12 7 WFC3/IR MULTIAC GRISM256 G141 none none 4 none 3 N/A CUM WASP-12 7 WFC3/IR MULTIAC GRISM256 G141 none none 5 none 3 N/A CUM WASP-12 7 WFC3/IR MULTIAC GRISM256 G141 none none 5 none 3 N/A CUM WASP-12 7 WFC3/IR MULTIAC GRISM256 G141 none none 6 none 3 N/A CUM WASP-12 7 WFC3/IR MULTIAC GRISM256 G141 none none 6 none 3 N/A CUM WASP-12 7 WFC3/IR MULTIAC GRISM256 G141 none none 7 none 3 N/A CUM WASP-12 7 WFC3/IR MULTIAC GRISM256 G141 none none 7 none 3 N/A CUM WASP-12 7 WFC3/IR MULTIAC GRISM256 G141 none none 8 none 3 N/A CUM WASP-12 7 WFC3/IR MULTIAC GRISM256 G141 none none 8 none 3 N/A CUM 16236( 5) - 06-Oct-2022 20:30:32 - [ 9] Visit: 02 (Companion Spec + Science (01)) Visit Requirements: SCHED 70%; SAME ORIENT AS 01; AFTER 01 On Hold Comments: Additional Comments: The stringent orientation constraints are necessary to avoid overlapping spectra from nearby stellar objects 1 and 10 arcsec away at PA=250 and 238. We calculate the central values for our orient ranges using Detector Offset+PA=135+250=25 or 205. We calculate the width of our orient range to ensure that after each non-destructive read the two stars' spectra are still separated by >4 FWHM to try to allow for our mildly experimental technique to subtract the comanion flux using the differences between non-destructive reads (tested for HAT-P-32Ab using data from GO 14767; Nikolov et al., 2018). To guarantee that we are able to subtract the companion spectra, we will also collect 10 staring mode observations during the first, stabilizing orbit (as was done by Kreidberg et al., 2015); our orient ranges ensure that the spectra will be separated by >5.6 FWHM for these staring-mode spectra. We enforce a phase constraint on the first exposure to ensure that we acquire our two baseline orbits before the first secondary eclipse and two baseline orbits after the final secondary eclipse. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 1 WASP-12 WFC3/IR MULTIAC GRISM256 F126N SAMP-SEQ=RAPID, NSAMP=3 1 DEF (0.833 POS TARG 0, 0; SEQ 1-2 CUM S) NON-INT Comments: F126N was selected as a narrow band filter to avoid saturation while determining the wavelength solution. This filter was also previously successfully used in GO program 13467 (Kreidberg et al., 2015). ------------------------------------------------------------------------------------------------------------------------------------ 2 WASP-12 WFC3/IR MULTIAC GRISM256 G141 SAMP-SEQ=SPARS10, NSAMP=15 8 DEF POS TARG 0, 0; SPATIAL CUM (1650.058 SCAN 0.0325, 90.0 S) Degrees, Round trip Comments: Our scan rate, SAMP-SEQ, and NSAMP ere jointly optimized to provide high observing efficiency, a peak per-pixel count of ~35, 000 to ensure rapid charge-trapping equilibriation within the first orbit, and the ability to separate the contaminating flux from the nearby M-dwarf companions at PA=250 while also not excessively limiting the ORIENT range of the observations. ------------------------------------------------------------------------------------------------------------------------------------ 3 WASP-12 WFC3/IR MULTIAC GRISM256 F126N SAMP-SEQ=RAPID, NSAMP=3 1 DEF (0.833 POS TARG 0, 0; SEQ 3-4 CUM S) NON-INT Comments: F126N was selected as a narrow band filter to avoid saturation while determining the wavelength solution. This filter was also previously successfully used in GO program 13467 (Kreidberg et al., 2015). 16236( 5) - 06-Oct-2022 20:30:32 - [ 10] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ ------------------------------------------------------------------------------------------------------------------------------------ 4 WASP-12 WFC3/IR MULTIAC GRISM256 G141 SAMP-SEQ=SPARS10, NSAMP=15 8 DEF POS TARG 0, 0; SPATIAL CUM (1650.058 SCAN 0.0325, 90.0 S) Degrees, Round trip Comments: Our scan rate, SAMP-SEQ, and NSAMP ere jointly optimized to provide high observing efficiency, a peak per-pixel count of ~35, 000 to ensure rapid charge-trapping equilibriation within the first orbit, and the ability to separate the contaminating flux from the nearby M-dwarf companions at PA=250 while also not excessively limiting the ORIENT range of the observations. ------------------------------------------------------------------------------------------------------------------------------------ 5 WASP-12 WFC3/IR MULTIAC GRISM256 F126N SAMP-SEQ=RAPID, NSAMP=3 1 DEF (0.833 POS TARG 0, 0; SEQ 5-6 CUM S) NON-INT Comments: F126N was selected as a narrow band filter to avoid saturation while determining the wavelength solution. This filter was also previously successfully used in GO program 13467 (Kreidberg et al., 2015). ------------------------------------------------------------------------------------------------------------------------------------ 6 WASP-12 WFC3/IR MULTIAC GRISM256 G141 SAMP-SEQ=SPARS10, NSAMP=15 8 DEF POS TARG 0, 0; SPATIAL CUM (1650.058 SCAN 0.0325, 90.0 S) Degrees, Round trip Comments: Our scan rate, SAMP-SEQ, and NSAMP ere jointly optimized to provide high observing efficiency, a peak per-pixel count of ~35, 000 to ensure rapid charge-trapping equilibriation within the first orbit, and the ability to separate the contaminating flux from the nearby M-dwarf companions at PA=250 while also not excessively limiting the ORIENT range of the observations. ------------------------------------------------------------------------------------------------------------------------------------ 7 WASP-12 WFC3/IR MULTIAC GRISM256 F126N SAMP-SEQ=RAPID, NSAMP=3 1 DEF (0.833 POS TARG 0, 0; SEQ 7-8 CUM S) NON-INT Comments: F126N was selected as a narrow band filter to avoid saturation while determining the wavelength solution. This filter was also previously successfully used in GO program 13467 (Kreidberg et al., 2015). ------------------------------------------------------------------------------------------------------------------------------------ 16236( 5) - 06-Oct-2022 20:30:32 - [ 11] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 8 WASP-12 WFC3/IR MULTIAC GRISM256 G141 SAMP-SEQ=SPARS10, NSAMP=15 8 DEF POS TARG 0, 0; SPATIAL CUM (1650.058 SCAN 0.0325, 90.0 S) Degrees, Round trip Comments: Our scan rate, SAMP-SEQ, and NSAMP ere jointly optimized to provide high observing efficiency, a peak per-pixel count of ~35, 000 to ensure rapid charge-trapping equilibriation within the first orbit, and the ability to separate the contaminating flux from the nearby M-dwarf companions at PA=250 while also not excessively limiting the ORIENT range of the observations. ------------------------------------------------------------------------------------------------------------------------------------ Sub Exposures ------------------------------------------------------------------------------------------------------------------------------------ Target | Exp |Instr | Oper. | Aper |Spectral|Cent.|Primary |Secondary |Iteration |CR-SPLIT |Orbit |Duration Name | Num |Config | Mode | or FOV |Element |Wave.|Pattern Pos |Pattern Pos |Num |Num |Number | ------------------------------------------------------------------------------------------------------------------------------------ WASP-12 1 WFC3/IR MULTIAC GRISM256 F126N none none none none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 1 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 1 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 2 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 2 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 3 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 3 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 4 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 4 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 5 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 5 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 6 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 6 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 7 none 1 N/A CUM 16236( 5) - 06-Oct-2022 20:30:32 - [ 12] Sub Exposures ------------------------------------------------------------------------------------------------------------------------------------ Target | Exp |Instr | Oper. | Aper |Spectral|Cent.|Primary |Secondary |Iteration |CR-SPLIT |Orbit |Duration Name | Num |Config | Mode | or FOV |Element |Wave.|Pattern Pos |Pattern Pos |Num |Num |Number | ------------------------------------------------------------------------------------------------------------------------------------ WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 7 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 8 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 8 none 1 N/A CUM WASP-12 3 WFC3/IR MULTIAC GRISM256 F126N none none none none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 1 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 1 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 2 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 2 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 3 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 3 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 4 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 4 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 5 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 5 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 6 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 6 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 7 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 7 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 8 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 8 none 2 N/A CUM WASP-12 5 WFC3/IR MULTIAC GRISM256 F126N none none none none 3 N/A CUM WASP-12 6 WFC3/IR MULTIAC GRISM256 G141 none none 1 none 3 N/A CUM WASP-12 6 WFC3/IR MULTIAC GRISM256 G141 none none 1 none 3 N/A CUM WASP-12 6 WFC3/IR MULTIAC GRISM256 G141 none none 2 none 3 N/A CUM 16236( 5) - 06-Oct-2022 20:30:32 - [ 13] Sub Exposures ------------------------------------------------------------------------------------------------------------------------------------ Target | Exp |Instr | Oper. | Aper |Spectral|Cent.|Primary |Secondary |Iteration |CR-SPLIT |Orbit |Duration Name | Num |Config | Mode | or FOV |Element |Wave.|Pattern Pos |Pattern Pos |Num |Num |Number | ------------------------------------------------------------------------------------------------------------------------------------ WASP-12 6 WFC3/IR MULTIAC GRISM256 G141 none none 2 none 3 N/A CUM WASP-12 6 WFC3/IR MULTIAC GRISM256 G141 none none 3 none 3 N/A CUM WASP-12 6 WFC3/IR MULTIAC GRISM256 G141 none none 3 none 3 N/A CUM WASP-12 6 WFC3/IR MULTIAC GRISM256 G141 none none 4 none 3 N/A CUM WASP-12 6 WFC3/IR MULTIAC GRISM256 G141 none none 4 none 3 N/A CUM WASP-12 6 WFC3/IR MULTIAC GRISM256 G141 none none 5 none 3 N/A CUM WASP-12 6 WFC3/IR MULTIAC GRISM256 G141 none none 5 none 3 N/A CUM WASP-12 6 WFC3/IR MULTIAC GRISM256 G141 none none 6 none 3 N/A CUM WASP-12 6 WFC3/IR MULTIAC GRISM256 G141 none none 6 none 3 N/A CUM WASP-12 6 WFC3/IR MULTIAC GRISM256 G141 none none 7 none 3 N/A CUM WASP-12 6 WFC3/IR MULTIAC GRISM256 G141 none none 7 none 3 N/A CUM WASP-12 6 WFC3/IR MULTIAC GRISM256 G141 none none 8 none 3 N/A CUM WASP-12 6 WFC3/IR MULTIAC GRISM256 G141 none none 8 none 3 N/A CUM WASP-12 7 WFC3/IR MULTIAC GRISM256 F126N none none none none 4 N/A CUM WASP-12 8 WFC3/IR MULTIAC GRISM256 G141 none none 1 none 4 N/A CUM WASP-12 8 WFC3/IR MULTIAC GRISM256 G141 none none 1 none 4 N/A CUM WASP-12 8 WFC3/IR MULTIAC GRISM256 G141 none none 2 none 4 N/A CUM WASP-12 8 WFC3/IR MULTIAC GRISM256 G141 none none 2 none 4 N/A CUM WASP-12 8 WFC3/IR MULTIAC GRISM256 G141 none none 3 none 4 N/A CUM WASP-12 8 WFC3/IR MULTIAC GRISM256 G141 none none 3 none 4 N/A CUM WASP-12 8 WFC3/IR MULTIAC GRISM256 G141 none none 4 none 4 N/A CUM WASP-12 8 WFC3/IR MULTIAC GRISM256 G141 none none 4 none 4 N/A CUM WASP-12 8 WFC3/IR MULTIAC GRISM256 G141 none none 5 none 4 N/A CUM WASP-12 8 WFC3/IR MULTIAC GRISM256 G141 none none 5 none 4 N/A CUM 16236( 5) - 06-Oct-2022 20:30:32 - [ 14] Sub Exposures ------------------------------------------------------------------------------------------------------------------------------------ Target | Exp |Instr | Oper. | Aper |Spectral|Cent.|Primary |Secondary |Iteration |CR-SPLIT |Orbit |Duration Name | Num |Config | Mode | or FOV |Element |Wave.|Pattern Pos |Pattern Pos |Num |Num |Number | ------------------------------------------------------------------------------------------------------------------------------------ WASP-12 8 WFC3/IR MULTIAC GRISM256 G141 none none 6 none 4 N/A CUM WASP-12 8 WFC3/IR MULTIAC GRISM256 G141 none none 6 none 4 N/A CUM WASP-12 8 WFC3/IR MULTIAC GRISM256 G141 none none 7 none 4 N/A CUM WASP-12 8 WFC3/IR MULTIAC GRISM256 G141 none none 7 none 4 N/A CUM WASP-12 8 WFC3/IR MULTIAC GRISM256 G141 none none 8 none 4 N/A CUM WASP-12 8 WFC3/IR MULTIAC GRISM256 G141 none none 8 none 4 N/A CUM 16236( 5) - 06-Oct-2022 20:30:32 - [ 15] Visit: 03 (Science (02)) Visit Requirements: SCHED 70%; SAME ORIENT AS 01; AFTER 02 On Hold Comments: Additional Comments: We must maintain the same orientation as in "visit" 1 to increase our ability to decorrelate the detector systematics and to allow us to subtract the companion star's spectrum. We also have placed an After Visit requirement to try to ensure that Visit 2 will follow immediately after Visit 1. See the Proposal Description for more details. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 1 WASP-12 WFC3/IR MULTIAC GRISM256 F126N SAMP-SEQ=RAPID, NSAMP=3 1 DEF (0.833 POS TARG 0, 0; SEQ 1-2 CUM S) NON-INT Comments: F126N was selected as a narrow band filter to avoid saturation while determining the wavelength solution. This filter was also previously successfully used in GO program 13467 (Kreidberg et al., 2015). ------------------------------------------------------------------------------------------------------------------------------------ 2 WASP-12 WFC3/IR MULTIAC GRISM256 G141 SAMP-SEQ=SPARS10, NSAMP=15 8 DEF POS TARG 0, 0; SPATIAL CUM (1650.058 SCAN 0.0325, 90.0 S) Degrees, Round trip Comments: Our scan rate, SAMP-SEQ, and NSAMP ere jointly optimized to provide high observing efficiency, a peak per-pixel count of ~35, 000 to ensure rapid charge-trapping equilibriation within the first orbit, and the ability to separate the contaminating flux from the nearby M-dwarf companions at PA=250 while also not excessively limiting the ORIENT range of the observations. ------------------------------------------------------------------------------------------------------------------------------------ 3 WASP-12 WFC3/IR MULTIAC GRISM256 F126N SAMP-SEQ=RAPID, NSAMP=3 1 DEF (0.833 POS TARG 0, 0; SEQ 3-4 CUM S) NON-INT Comments: F126N was selected as a narrow band filter to avoid saturation while determining the wavelength solution. This filter was also previously successfully used in GO program 13467 (Kreidberg et al., 2015). ------------------------------------------------------------------------------------------------------------------------------------ 16236( 5) - 06-Oct-2022 20:30:32 - [ 16] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 4 WASP-12 WFC3/IR MULTIAC GRISM256 G141 SAMP-SEQ=SPARS10, NSAMP=15 8 DEF POS TARG 0, 0; SPATIAL CUM (1650.058 SCAN 0.0325, 90.0 S) Degrees, Round trip Comments: Our scan rate, SAMP-SEQ, and NSAMP ere jointly optimized to provide high observing efficiency, a peak per-pixel count of ~35, 000 to ensure rapid charge-trapping equilibriation within the first orbit, and the ability to separate the contaminating flux from the nearby M-dwarf companions at PA=250 while also not excessively limiting the ORIENT range of the observations. ------------------------------------------------------------------------------------------------------------------------------------ Sub Exposures ------------------------------------------------------------------------------------------------------------------------------------ Target | Exp |Instr | Oper. | Aper |Spectral|Cent.|Primary |Secondary |Iteration |CR-SPLIT |Orbit |Duration Name | Num |Config | Mode | or FOV |Element |Wave.|Pattern Pos |Pattern Pos |Num |Num |Number | ------------------------------------------------------------------------------------------------------------------------------------ WASP-12 1 WFC3/IR MULTIAC GRISM256 F126N none none none none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 1 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 1 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 2 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 2 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 3 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 3 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 4 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 4 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 5 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 5 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 6 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 6 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 7 none 1 N/A CUM 16236( 5) - 06-Oct-2022 20:30:32 - [ 17] Sub Exposures ------------------------------------------------------------------------------------------------------------------------------------ Target | Exp |Instr | Oper. | Aper |Spectral|Cent.|Primary |Secondary |Iteration |CR-SPLIT |Orbit |Duration Name | Num |Config | Mode | or FOV |Element |Wave.|Pattern Pos |Pattern Pos |Num |Num |Number | ------------------------------------------------------------------------------------------------------------------------------------ WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 7 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 8 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 8 none 1 N/A CUM WASP-12 3 WFC3/IR MULTIAC GRISM256 F126N none none none none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 1 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 1 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 2 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 2 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 3 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 3 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 4 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 4 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 5 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 5 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 6 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 6 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 7 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 7 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 8 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 8 none 2 N/A CUM 16236( 5) - 06-Oct-2022 20:30:32 - [ 18] Visit: 04 (Science (02)) Visit Requirements: SCHED 70%; SAME ORIENT AS 01; AFTER 03 On Hold Comments: Additional Comments: We must maintain the same orientation as in "visit" 1 to increase our ability to decorrelate the detector systematics and to allow us to subtract the companion star's spectrum. We also have placed an After Visit requirement to try to ensure that Visit 2 will follow immediately after Visit 1. See the Proposal Description for more details. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 1 WASP-12 WFC3/IR MULTIAC GRISM256 F126N SAMP-SEQ=RAPID, NSAMP=3 1 DEF (0.833 POS TARG 0, 0; SEQ 1-2 CUM S) NON-INT Comments: F126N was selected as a narrow band filter to avoid saturation while determining the wavelength solution. This filter was also previously successfully used in GO program 13467 (Kreidberg et al., 2015). ------------------------------------------------------------------------------------------------------------------------------------ 2 WASP-12 WFC3/IR MULTIAC GRISM256 G141 SAMP-SEQ=SPARS10, NSAMP=15 8 DEF POS TARG 0, 0; SPATIAL CUM (1650.058 SCAN 0.0325, 90.0 S) Degrees, Round trip Comments: Our scan rate, SAMP-SEQ, and NSAMP ere jointly optimized to provide high observing efficiency, a peak per-pixel count of ~35, 000 to ensure rapid charge-trapping equilibriation within the first orbit, and the ability to separate the contaminating flux from the nearby M-dwarf companions at PA=250 while also not excessively limiting the ORIENT range of the observations. ------------------------------------------------------------------------------------------------------------------------------------ 3 WASP-12 WFC3/IR MULTIAC GRISM256 F126N SAMP-SEQ=RAPID, NSAMP=3 1 DEF (0.833 POS TARG 0, 0; SEQ 3-4 CUM S) NON-INT Comments: F126N was selected as a narrow band filter to avoid saturation while determining the wavelength solution. This filter was also previously successfully used in GO program 13467 (Kreidberg et al., 2015). ------------------------------------------------------------------------------------------------------------------------------------ 16236( 5) - 06-Oct-2022 20:30:32 - [ 19] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 4 WASP-12 WFC3/IR MULTIAC GRISM256 G141 SAMP-SEQ=SPARS10, NSAMP=15 8 DEF POS TARG 0, 0; SPATIAL CUM (1650.058 SCAN 0.0325, 90.0 S) Degrees, Round trip Comments: Our scan rate, SAMP-SEQ, and NSAMP ere jointly optimized to provide high observing efficiency, a peak per-pixel count of ~35, 000 to ensure rapid charge-trapping equilibriation within the first orbit, and the ability to separate the contaminating flux from the nearby M-dwarf companions at PA=250 while also not excessively limiting the ORIENT range of the observations. ------------------------------------------------------------------------------------------------------------------------------------ 5 WASP-12 WFC3/IR MULTIAC GRISM256 F126N SAMP-SEQ=RAPID, NSAMP=3 1 DEF (0.833 POS TARG 0, 0; SEQ 5-6 CUM S) NON-INT Comments: F126N was selected as a narrow band filter to avoid saturation while determining the wavelength solution. This filter was also previously successfully used in GO program 13467 (Kreidberg et al., 2015). ------------------------------------------------------------------------------------------------------------------------------------ 6 WASP-12 WFC3/IR MULTIAC GRISM256 G141 SAMP-SEQ=SPARS10, NSAMP=15 8 DEF POS TARG 0, 0; SPATIAL CUM (1650.058 SCAN 0.0325, 90.0 S) Degrees, Round trip Comments: Our scan rate, SAMP-SEQ, and NSAMP ere jointly optimized to provide high observing efficiency, a peak per-pixel count of ~35, 000 to ensure rapid charge-trapping equilibriation within the first orbit, and the ability to separate the contaminating flux from the nearby M-dwarf companions at PA=250 while also not excessively limiting the ORIENT range of the observations. ------------------------------------------------------------------------------------------------------------------------------------ Sub Exposures ------------------------------------------------------------------------------------------------------------------------------------ Target | Exp |Instr | Oper. | Aper |Spectral|Cent.|Primary |Secondary |Iteration |CR-SPLIT |Orbit |Duration Name | Num |Config | Mode | or FOV |Element |Wave.|Pattern Pos |Pattern Pos |Num |Num |Number | ------------------------------------------------------------------------------------------------------------------------------------ WASP-12 1 WFC3/IR MULTIAC GRISM256 F126N none none none none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 1 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 1 none 1 N/A CUM 16236( 5) - 06-Oct-2022 20:30:32 - [ 20] Sub Exposures ------------------------------------------------------------------------------------------------------------------------------------ Target | Exp |Instr | Oper. | Aper |Spectral|Cent.|Primary |Secondary |Iteration |CR-SPLIT |Orbit |Duration Name | Num |Config | Mode | or FOV |Element |Wave.|Pattern Pos |Pattern Pos |Num |Num |Number | ------------------------------------------------------------------------------------------------------------------------------------ WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 2 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 2 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 3 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 3 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 4 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 4 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 5 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 5 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 6 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 6 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 7 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 7 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 8 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 8 none 1 N/A CUM WASP-12 3 WFC3/IR MULTIAC GRISM256 F126N none none none none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 1 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 1 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 2 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 2 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 3 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 3 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 4 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 4 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 5 none 2 N/A CUM 16236( 5) - 06-Oct-2022 20:30:32 - [ 21] Sub Exposures ------------------------------------------------------------------------------------------------------------------------------------ Target | Exp |Instr | Oper. | Aper |Spectral|Cent.|Primary |Secondary |Iteration |CR-SPLIT |Orbit |Duration Name | Num |Config | Mode | or FOV |Element |Wave.|Pattern Pos |Pattern Pos |Num |Num |Number | ------------------------------------------------------------------------------------------------------------------------------------ WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 5 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 6 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 6 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 7 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 7 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 8 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 8 none 2 N/A CUM WASP-12 5 WFC3/IR MULTIAC GRISM256 F126N none none none none 3 N/A CUM WASP-12 6 WFC3/IR MULTIAC GRISM256 G141 none none 1 none 3 N/A CUM WASP-12 6 WFC3/IR MULTIAC GRISM256 G141 none none 1 none 3 N/A CUM WASP-12 6 WFC3/IR MULTIAC GRISM256 G141 none none 2 none 3 N/A CUM WASP-12 6 WFC3/IR MULTIAC GRISM256 G141 none none 2 none 3 N/A CUM WASP-12 6 WFC3/IR MULTIAC GRISM256 G141 none none 3 none 3 N/A CUM WASP-12 6 WFC3/IR MULTIAC GRISM256 G141 none none 3 none 3 N/A CUM WASP-12 6 WFC3/IR MULTIAC GRISM256 G141 none none 4 none 3 N/A CUM WASP-12 6 WFC3/IR MULTIAC GRISM256 G141 none none 4 none 3 N/A CUM WASP-12 6 WFC3/IR MULTIAC GRISM256 G141 none none 5 none 3 N/A CUM WASP-12 6 WFC3/IR MULTIAC GRISM256 G141 none none 5 none 3 N/A CUM WASP-12 6 WFC3/IR MULTIAC GRISM256 G141 none none 6 none 3 N/A CUM WASP-12 6 WFC3/IR MULTIAC GRISM256 G141 none none 6 none 3 N/A CUM WASP-12 6 WFC3/IR MULTIAC GRISM256 G141 none none 7 none 3 N/A CUM WASP-12 6 WFC3/IR MULTIAC GRISM256 G141 none none 7 none 3 N/A CUM WASP-12 6 WFC3/IR MULTIAC GRISM256 G141 none none 8 none 3 N/A CUM WASP-12 6 WFC3/IR MULTIAC GRISM256 G141 none none 8 none 3 N/A CUM 16236( 5) - 06-Oct-2022 20:30:32 - [ 22] Visit: 05 (Science (03)) Visit Requirements: SCHED 70%; SAME ORIENT AS 01; AFTER 04 On Hold Comments: Additional Comments: We must maintain the same orientation as in "visit" 1 to increase our ability to decorrelate the detector systematics and to allow us to subtract the companion star's spectrum. We also have placed an After Visit requirement to try to ensure that Visit 2 will follow immediately after Visit 1. See the Proposal Description for more details. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 1 WASP-12 WFC3/IR MULTIAC GRISM256 F126N SAMP-SEQ=RAPID, NSAMP=3 1 DEF (0.833 POS TARG 0, 0; GS ACQ CUM S) SCENARIO BASE1BE; SEQ 1-2 NON-INT Comments: F126N was selected as a narrow band filter to avoid saturation while determining the wavelength solution. This filter was also previously successfully used in GO program 13467 (Kreidberg et al., 2015). ------------------------------------------------------------------------------------------------------------------------------------ 2 WASP-12 WFC3/IR MULTIAC GRISM256 G141 SAMP-SEQ=SPARS10, NSAMP=15 8 DEF POS TARG 0, 0; SPATIAL CUM (1650.058 SCAN 0.0325, 90.0 S) Degrees, Round trip Comments: Our scan rate, SAMP-SEQ, and NSAMP ere jointly optimized to provide high observing efficiency, a peak per-pixel count of ~35, 000 to ensure rapid charge-trapping equilibriation within the first orbit, and the ability to separate the contaminating flux from the nearby M-dwarf companions at PA=250 while also not excessively limiting the ORIENT range of the observations. ------------------------------------------------------------------------------------------------------------------------------------ 3 WASP-12 WFC3/IR MULTIAC GRISM256 F126N SAMP-SEQ=RAPID, NSAMP=3 1 DEF (0.833 POS TARG 0, 0; SEQ 3-4 CUM S) NON-INT Comments: F126N was selected as a narrow band filter to avoid saturation while determining the wavelength solution. This filter was also previously successfully used in GO program 13467 (Kreidberg et al., 2015). ------------------------------------------------------------------------------------------------------------------------------------ 16236( 5) - 06-Oct-2022 20:30:32 - [ 23] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 4 WASP-12 WFC3/IR MULTIAC GRISM256 G141 SAMP-SEQ=SPARS10, NSAMP=15 8 DEF POS TARG 0, 0; SPATIAL CUM (1650.058 SCAN 0.0325, 90.0 S) Degrees, Round trip Comments: Our scan rate, SAMP-SEQ, and NSAMP ere jointly optimized to provide high observing efficiency, a peak per-pixel count of ~35, 000 to ensure rapid charge-trapping equilibriation within the first orbit, and the ability to separate the contaminating flux from the nearby M-dwarf companions at PA=250 while also not excessively limiting the ORIENT range of the observations. ------------------------------------------------------------------------------------------------------------------------------------ 5 WASP-12 WFC3/IR MULTIAC GRISM256 F126N SAMP-SEQ=RAPID, NSAMP=3 1 DEF (0.833 POS TARG 0, 0; SEQ 5-6 CUM S) NON-INT Comments: F126N was selected as a narrow band filter to avoid saturation while determining the wavelength solution. This filter was also previously successfully used in GO program 13467 (Kreidberg et al., 2015). ------------------------------------------------------------------------------------------------------------------------------------ 6 WASP-12 WFC3/IR MULTIAC GRISM256 G141 SAMP-SEQ=SPARS10, NSAMP=15 8 DEF POS TARG 0, 0; SPATIAL CUM (1650.058 SCAN 0.0325, 90.0 S) Degrees, Round trip Comments: Our scan rate, SAMP-SEQ, and NSAMP ere jointly optimized to provide high observing efficiency, a peak per-pixel count of ~35, 000 to ensure rapid charge-trapping equilibriation within the first orbit, and the ability to separate the contaminating flux from the nearby M-dwarf companions at PA=250 while also not excessively limiting the ORIENT range of the observations. ------------------------------------------------------------------------------------------------------------------------------------ Sub Exposures ------------------------------------------------------------------------------------------------------------------------------------ Target | Exp |Instr | Oper. | Aper |Spectral|Cent.|Primary |Secondary |Iteration |CR-SPLIT |Orbit |Duration Name | Num |Config | Mode | or FOV |Element |Wave.|Pattern Pos |Pattern Pos |Num |Num |Number | ------------------------------------------------------------------------------------------------------------------------------------ WASP-12 1 WFC3/IR MULTIAC GRISM256 F126N none none none none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 1 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 1 none 1 N/A CUM 16236( 5) - 06-Oct-2022 20:30:32 - [ 24] Sub Exposures ------------------------------------------------------------------------------------------------------------------------------------ Target | Exp |Instr | Oper. | Aper |Spectral|Cent.|Primary |Secondary |Iteration |CR-SPLIT |Orbit |Duration Name | Num |Config | Mode | or FOV |Element |Wave.|Pattern Pos |Pattern Pos |Num |Num |Number | ------------------------------------------------------------------------------------------------------------------------------------ WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 2 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 2 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 3 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 3 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 4 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 4 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 5 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 5 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 6 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 6 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 7 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 7 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 8 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 8 none 1 N/A CUM WASP-12 3 WFC3/IR MULTIAC GRISM256 F126N none none none none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 1 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 1 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 2 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 2 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 3 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 3 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 4 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 4 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 5 none 2 N/A CUM 16236( 5) - 06-Oct-2022 20:30:32 - [ 25] Sub Exposures ------------------------------------------------------------------------------------------------------------------------------------ Target | Exp |Instr | Oper. | Aper |Spectral|Cent.|Primary |Secondary |Iteration |CR-SPLIT |Orbit |Duration Name | Num |Config | Mode | or FOV |Element |Wave.|Pattern Pos |Pattern Pos |Num |Num |Number | ------------------------------------------------------------------------------------------------------------------------------------ WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 5 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 6 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 6 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 7 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 7 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 8 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 8 none 2 N/A CUM WASP-12 5 WFC3/IR MULTIAC GRISM256 F126N none none none none 3 N/A CUM WASP-12 6 WFC3/IR MULTIAC GRISM256 G141 none none 1 none 3 N/A CUM WASP-12 6 WFC3/IR MULTIAC GRISM256 G141 none none 1 none 3 N/A CUM WASP-12 6 WFC3/IR MULTIAC GRISM256 G141 none none 2 none 3 N/A CUM WASP-12 6 WFC3/IR MULTIAC GRISM256 G141 none none 2 none 3 N/A CUM WASP-12 6 WFC3/IR MULTIAC GRISM256 G141 none none 3 none 3 N/A CUM WASP-12 6 WFC3/IR MULTIAC GRISM256 G141 none none 3 none 3 N/A CUM WASP-12 6 WFC3/IR MULTIAC GRISM256 G141 none none 4 none 3 N/A CUM WASP-12 6 WFC3/IR MULTIAC GRISM256 G141 none none 4 none 3 N/A CUM WASP-12 6 WFC3/IR MULTIAC GRISM256 G141 none none 5 none 3 N/A CUM WASP-12 6 WFC3/IR MULTIAC GRISM256 G141 none none 5 none 3 N/A CUM WASP-12 6 WFC3/IR MULTIAC GRISM256 G141 none none 6 none 3 N/A CUM WASP-12 6 WFC3/IR MULTIAC GRISM256 G141 none none 6 none 3 N/A CUM WASP-12 6 WFC3/IR MULTIAC GRISM256 G141 none none 7 none 3 N/A CUM WASP-12 6 WFC3/IR MULTIAC GRISM256 G141 none none 7 none 3 N/A CUM WASP-12 6 WFC3/IR MULTIAC GRISM256 G141 none none 8 none 3 N/A CUM WASP-12 6 WFC3/IR MULTIAC GRISM256 G141 none none 8 none 3 N/A CUM 16236( 5) - 06-Oct-2022 20:30:32 - [ 26] Visit: 06 (Science (03)) Visit Requirements: SCHED 70%; SAME ORIENT AS 01; AFTER 05 On Hold Comments: Additional Comments: We must maintain the same orientation as in "visit" 1 to increase our ability to decorrelate the detector systematics and to allow us to subtract the companion star's spectrum. We also have placed an After Visit requirement to try to ensure that Visit 3 will follow immediately after Visit 2. See the Proposal Description for more details. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 1 WASP-12 WFC3/IR MULTIAC GRISM256 F126N SAMP-SEQ=RAPID, NSAMP=3 1 DEF (0.833 POS TARG 0, 0; GS ACQ CUM S) SCENARIO BASE1BE; SEQ 1-2 NON-INT Comments: F126N was selected as a narrow band filter to avoid saturation while determining the wavelength solution. This filter was also previously successfully used in GO program 13467 (Kreidberg et al., 2015). ------------------------------------------------------------------------------------------------------------------------------------ 2 WASP-12 WFC3/IR MULTIAC GRISM256 G141 SAMP-SEQ=SPARS10, NSAMP=15 8 DEF POS TARG 0, 0; SPATIAL CUM (1650.058 SCAN 0.0325, 90.0 S) Degrees, Round trip Comments: Our scan rate, SAMP-SEQ, and NSAMP ere jointly optimized to provide high observing efficiency, a peak per-pixel count of ~35, 000 to ensure rapid charge-trapping equilibriation within the first orbit, and the ability to separate the contaminating flux from the nearby M-dwarf companions at PA=250 while also not excessively limiting the ORIENT range of the observations. ------------------------------------------------------------------------------------------------------------------------------------ 3 WASP-12 WFC3/IR MULTIAC GRISM256 F126N SAMP-SEQ=RAPID, NSAMP=3 1 DEF (0.833 POS TARG 0, 0; SEQ 3-4 CUM S) NON-INT Comments: F126N was selected as a narrow band filter to avoid saturation while determining the wavelength solution. This filter was also previously successfully used in GO program 13467 (Kreidberg et al., 2015). ------------------------------------------------------------------------------------------------------------------------------------ 16236( 5) - 06-Oct-2022 20:30:32 - [ 27] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 4 WASP-12 WFC3/IR MULTIAC GRISM256 G141 SAMP-SEQ=SPARS10, NSAMP=15 8 DEF POS TARG 0, 0; SPATIAL CUM (1650.058 SCAN 0.0325, 90.0 S) Degrees, Round trip Comments: Our scan rate, SAMP-SEQ, and NSAMP ere jointly optimized to provide high observing efficiency, a peak per-pixel count of ~35, 000 to ensure rapid charge-trapping equilibriation within the first orbit, and the ability to separate the contaminating flux from the nearby M-dwarf companions at PA=250 while also not excessively limiting the ORIENT range of the observations. ------------------------------------------------------------------------------------------------------------------------------------ 5 WASP-12 WFC3/IR MULTIAC GRISM256 F126N SAMP-SEQ=RAPID, NSAMP=3 1 DEF (0.833 POS TARG 0, 0; SEQ 5-6 CUM S) NON-INT Comments: F126N was selected as a narrow band filter to avoid saturation while determining the wavelength solution. This filter was also previously successfully used in GO program 13467 (Kreidberg et al., 2015). ------------------------------------------------------------------------------------------------------------------------------------ 6 WASP-12 WFC3/IR MULTIAC GRISM256 G141 SAMP-SEQ=SPARS10, NSAMP=15 8 DEF POS TARG 0, 0; SPATIAL CUM (1650.058 SCAN 0.0325, 90.0 S) Degrees, Round trip Comments: Our scan rate, SAMP-SEQ, and NSAMP ere jointly optimized to provide high observing efficiency, a peak per-pixel count of ~35, 000 to ensure rapid charge-trapping equilibriation within the first orbit, and the ability to separate the contaminating flux from the nearby M-dwarf companions at PA=250 while also not excessively limiting the ORIENT range of the observations. ------------------------------------------------------------------------------------------------------------------------------------ Sub Exposures ------------------------------------------------------------------------------------------------------------------------------------ Target | Exp |Instr | Oper. | Aper |Spectral|Cent.|Primary |Secondary |Iteration |CR-SPLIT |Orbit |Duration Name | Num |Config | Mode | or FOV |Element |Wave.|Pattern Pos |Pattern Pos |Num |Num |Number | ------------------------------------------------------------------------------------------------------------------------------------ WASP-12 1 WFC3/IR MULTIAC GRISM256 F126N none none none none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 1 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 1 none 1 N/A CUM 16236( 5) - 06-Oct-2022 20:30:32 - [ 28] Sub Exposures ------------------------------------------------------------------------------------------------------------------------------------ Target | Exp |Instr | Oper. | Aper |Spectral|Cent.|Primary |Secondary |Iteration |CR-SPLIT |Orbit |Duration Name | Num |Config | Mode | or FOV |Element |Wave.|Pattern Pos |Pattern Pos |Num |Num |Number | ------------------------------------------------------------------------------------------------------------------------------------ WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 2 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 2 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 3 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 3 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 4 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 4 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 5 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 5 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 6 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 6 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 7 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 7 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 8 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 8 none 1 N/A CUM WASP-12 3 WFC3/IR MULTIAC GRISM256 F126N none none none none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 1 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 1 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 2 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 2 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 3 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 3 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 4 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 4 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 5 none 2 N/A CUM 16236( 5) - 06-Oct-2022 20:30:32 - [ 29] Sub Exposures ------------------------------------------------------------------------------------------------------------------------------------ Target | Exp |Instr | Oper. | Aper |Spectral|Cent.|Primary |Secondary |Iteration |CR-SPLIT |Orbit |Duration Name | Num |Config | Mode | or FOV |Element |Wave.|Pattern Pos |Pattern Pos |Num |Num |Number | ------------------------------------------------------------------------------------------------------------------------------------ WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 5 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 6 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 6 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 7 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 7 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 8 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 8 none 2 N/A CUM WASP-12 5 WFC3/IR MULTIAC GRISM256 F126N none none none none 3 N/A CUM WASP-12 6 WFC3/IR MULTIAC GRISM256 G141 none none 1 none 3 N/A CUM WASP-12 6 WFC3/IR MULTIAC GRISM256 G141 none none 1 none 3 N/A CUM WASP-12 6 WFC3/IR MULTIAC GRISM256 G141 none none 2 none 3 N/A CUM WASP-12 6 WFC3/IR MULTIAC GRISM256 G141 none none 2 none 3 N/A CUM WASP-12 6 WFC3/IR MULTIAC GRISM256 G141 none none 3 none 3 N/A CUM WASP-12 6 WFC3/IR MULTIAC GRISM256 G141 none none 3 none 3 N/A CUM WASP-12 6 WFC3/IR MULTIAC GRISM256 G141 none none 4 none 3 N/A CUM WASP-12 6 WFC3/IR MULTIAC GRISM256 G141 none none 4 none 3 N/A CUM WASP-12 6 WFC3/IR MULTIAC GRISM256 G141 none none 5 none 3 N/A CUM WASP-12 6 WFC3/IR MULTIAC GRISM256 G141 none none 5 none 3 N/A CUM WASP-12 6 WFC3/IR MULTIAC GRISM256 G141 none none 6 none 3 N/A CUM WASP-12 6 WFC3/IR MULTIAC GRISM256 G141 none none 6 none 3 N/A CUM WASP-12 6 WFC3/IR MULTIAC GRISM256 G141 none none 7 none 3 N/A CUM WASP-12 6 WFC3/IR MULTIAC GRISM256 G141 none none 7 none 3 N/A CUM WASP-12 6 WFC3/IR MULTIAC GRISM256 G141 none none 8 none 3 N/A CUM WASP-12 6 WFC3/IR MULTIAC GRISM256 G141 none none 8 none 3 N/A CUM 16236( 5) - 06-Oct-2022 20:30:32 - [ 30] Visit: 07 (Science (03)) Visit Requirements: SCHED 70%; SAME ORIENT AS 01; AFTER 06 On Hold Comments: Additional Comments: We must maintain the same orientation as in "visit" 1 to increase our ability to decorrelate the detector systematics and to allow us to subtract the companion star's spectrum. We also have placed an After Visit requirement to try to ensure that Visit 3 will follow immediately after Visit 2. See the Proposal Description for more details. Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 1 WASP-12 WFC3/IR MULTIAC GRISM256 F126N SAMP-SEQ=RAPID, NSAMP=3 1 DEF (0.833 POS TARG 0, 0; SEQ 1-2 CUM S) NON-INT Comments: F126N was selected as a narrow band filter to avoid saturation while determining the wavelength solution. This filter was also previously successfully used in GO program 13467 (Kreidberg et al., 2015). ------------------------------------------------------------------------------------------------------------------------------------ 2 WASP-12 WFC3/IR MULTIAC GRISM256 G141 SAMP-SEQ=SPARS10, NSAMP=15 8 DEF POS TARG 0, 0; SPATIAL CUM (1650.058 SCAN 0.0325, 90.0 S) Degrees, Round trip Comments: Our scan rate, SAMP-SEQ, and NSAMP ere jointly optimized to provide high observing efficiency, a peak per-pixel count of ~35, 000 to ensure rapid charge-trapping equilibriation within the first orbit, and the ability to separate the contaminating flux from the nearby M-dwarf companions at PA=250 while also not excessively limiting the ORIENT range of the observations. ------------------------------------------------------------------------------------------------------------------------------------ 3 WASP-12 WFC3/IR MULTIAC GRISM256 F126N SAMP-SEQ=RAPID, NSAMP=3 1 DEF (0.833 POS TARG 0, 0; SEQ 3-4 CUM S) NON-INT Comments: F126N was selected as a narrow band filter to avoid saturation while determining the wavelength solution. This filter was also previously successfully used in GO program 13467 (Kreidberg et al., 2015). ------------------------------------------------------------------------------------------------------------------------------------ 16236( 5) - 06-Oct-2022 20:30:32 - [ 31] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 4 WASP-12 WFC3/IR MULTIAC GRISM256 G141 SAMP-SEQ=SPARS10, NSAMP=15 8 DEF POS TARG 0, 0; SPATIAL CUM (1650.058 SCAN 0.0325, 90.0 S) Degrees, Round trip Comments: Our scan rate, SAMP-SEQ, and NSAMP ere jointly optimized to provide high observing efficiency, a peak per-pixel count of ~35, 000 to ensure rapid charge-trapping equilibriation within the first orbit, and the ability to separate the contaminating flux from the nearby M-dwarf companions at PA=250 while also not excessively limiting the ORIENT range of the observations. ------------------------------------------------------------------------------------------------------------------------------------ 5 WASP-12 WFC3/IR MULTIAC GRISM256 F126N SAMP-SEQ=RAPID, NSAMP=3 1 DEF (0.833 POS TARG 0, 0; SEQ 5-6 CUM S) NON-INT Comments: F126N was selected as a narrow band filter to avoid saturation while determining the wavelength solution. This filter was also previously successfully used in GO program 13467 (Kreidberg et al., 2015). ------------------------------------------------------------------------------------------------------------------------------------ 6 WASP-12 WFC3/IR MULTIAC GRISM256 G141 SAMP-SEQ=SPARS10, NSAMP=15 8 DEF POS TARG 0, 0; SPATIAL CUM (1650.058 SCAN 0.0325, 90.0 S) Degrees, Round trip Comments: Our scan rate, SAMP-SEQ, and NSAMP ere jointly optimized to provide high observing efficiency, a peak per-pixel count of ~35, 000 to ensure rapid charge-trapping equilibriation within the first orbit, and the ability to separate the contaminating flux from the nearby M-dwarf companions at PA=250 while also not excessively limiting the ORIENT range of the observations. ------------------------------------------------------------------------------------------------------------------------------------ 7 WASP-12 WFC3/IR MULTIAC GRISM256 F126N SAMP-SEQ=RAPID, NSAMP=3 1 DEF (0.833 POS TARG 0, 0; SEQ 7-8 CUM S) NON-INT Comments: F126N was selected as a narrow band filter to avoid saturation while determining the wavelength solution. This filter was also previously successfully used in GO program 13467 (Kreidberg et al., 2015). ------------------------------------------------------------------------------------------------------------------------------------ 16236( 5) - 06-Oct-2022 20:30:32 - [ 32] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 8 WASP-12 WFC3/IR MULTIAC GRISM256 G141 SAMP-SEQ=SPARS10, NSAMP=15 8 DEF POS TARG 0, 0; SPATIAL CUM (1650.058 SCAN 0.0325, 90.0 S) Degrees, Round trip Comments: Our scan rate, SAMP-SEQ, and NSAMP ere jointly optimized to provide high observing efficiency, a peak per-pixel count of ~35, 000 to ensure rapid charge-trapping equilibriation within the first orbit, and the ability to separate the contaminating flux from the nearby M-dwarf companions at PA=250 while also not excessively limiting the ORIENT range of the observations. ------------------------------------------------------------------------------------------------------------------------------------ Sub Exposures ------------------------------------------------------------------------------------------------------------------------------------ Target | Exp |Instr | Oper. | Aper |Spectral|Cent.|Primary |Secondary |Iteration |CR-SPLIT |Orbit |Duration Name | Num |Config | Mode | or FOV |Element |Wave.|Pattern Pos |Pattern Pos |Num |Num |Number | ------------------------------------------------------------------------------------------------------------------------------------ WASP-12 1 WFC3/IR MULTIAC GRISM256 F126N none none none none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 1 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 1 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 2 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 2 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 3 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 3 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 4 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 4 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 5 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 5 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 6 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 6 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 7 none 1 N/A CUM 16236( 5) - 06-Oct-2022 20:30:32 - [ 33] Sub Exposures ------------------------------------------------------------------------------------------------------------------------------------ Target | Exp |Instr | Oper. | Aper |Spectral|Cent.|Primary |Secondary |Iteration |CR-SPLIT |Orbit |Duration Name | Num |Config | Mode | or FOV |Element |Wave.|Pattern Pos |Pattern Pos |Num |Num |Number | ------------------------------------------------------------------------------------------------------------------------------------ WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 7 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 8 none 1 N/A CUM WASP-12 2 WFC3/IR MULTIAC GRISM256 G141 none none 8 none 1 N/A CUM WASP-12 3 WFC3/IR MULTIAC GRISM256 F126N none none none none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 1 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 1 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 2 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 2 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 3 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 3 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 4 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 4 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 5 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 5 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 6 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 6 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 7 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 7 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 8 none 2 N/A CUM WASP-12 4 WFC3/IR MULTIAC GRISM256 G141 none none 8 none 2 N/A CUM WASP-12 5 WFC3/IR MULTIAC GRISM256 F126N none none none none 3 N/A CUM WASP-12 6 WFC3/IR MULTIAC GRISM256 G141 none none 1 none 3 N/A CUM WASP-12 6 WFC3/IR MULTIAC GRISM256 G141 none none 1 none 3 N/A CUM WASP-12 6 WFC3/IR MULTIAC GRISM256 G141 none none 2 none 3 N/A CUM 16236( 5) - 06-Oct-2022 20:30:32 - [ 34] Sub Exposures ------------------------------------------------------------------------------------------------------------------------------------ Target | Exp |Instr | Oper. | Aper |Spectral|Cent.|Primary |Secondary |Iteration |CR-SPLIT |Orbit |Duration Name | Num |Config | Mode | or FOV |Element |Wave.|Pattern Pos |Pattern Pos |Num |Num |Number | ------------------------------------------------------------------------------------------------------------------------------------ WASP-12 6 WFC3/IR MULTIAC GRISM256 G141 none none 2 none 3 N/A CUM WASP-12 6 WFC3/IR MULTIAC GRISM256 G141 none none 3 none 3 N/A CUM WASP-12 6 WFC3/IR MULTIAC GRISM256 G141 none none 3 none 3 N/A CUM WASP-12 6 WFC3/IR MULTIAC GRISM256 G141 none none 4 none 3 N/A CUM WASP-12 6 WFC3/IR MULTIAC GRISM256 G141 none none 4 none 3 N/A CUM WASP-12 6 WFC3/IR MULTIAC GRISM256 G141 none none 5 none 3 N/A CUM WASP-12 6 WFC3/IR MULTIAC GRISM256 G141 none none 5 none 3 N/A CUM WASP-12 6 WFC3/IR MULTIAC GRISM256 G141 none none 6 none 3 N/A CUM WASP-12 6 WFC3/IR MULTIAC GRISM256 G141 none none 6 none 3 N/A CUM WASP-12 6 WFC3/IR MULTIAC GRISM256 G141 none none 7 none 3 N/A CUM WASP-12 6 WFC3/IR MULTIAC GRISM256 G141 none none 7 none 3 N/A CUM WASP-12 6 WFC3/IR MULTIAC GRISM256 G141 none none 8 none 3 N/A CUM WASP-12 6 WFC3/IR MULTIAC GRISM256 G141 none none 8 none 3 N/A CUM WASP-12 7 WFC3/IR MULTIAC GRISM256 F126N none none none none 4 N/A CUM WASP-12 8 WFC3/IR MULTIAC GRISM256 G141 none none 1 none 4 N/A CUM WASP-12 8 WFC3/IR MULTIAC GRISM256 G141 none none 1 none 4 N/A CUM WASP-12 8 WFC3/IR MULTIAC GRISM256 G141 none none 2 none 4 N/A CUM WASP-12 8 WFC3/IR MULTIAC GRISM256 G141 none none 2 none 4 N/A CUM WASP-12 8 WFC3/IR MULTIAC GRISM256 G141 none none 3 none 4 N/A CUM WASP-12 8 WFC3/IR MULTIAC GRISM256 G141 none none 3 none 4 N/A CUM WASP-12 8 WFC3/IR MULTIAC GRISM256 G141 none none 4 none 4 N/A CUM WASP-12 8 WFC3/IR MULTIAC GRISM256 G141 none none 4 none 4 N/A CUM WASP-12 8 WFC3/IR MULTIAC GRISM256 G141 none none 5 none 4 N/A CUM WASP-12 8 WFC3/IR MULTIAC GRISM256 G141 none none 5 none 4 N/A CUM 16236( 5) - 06-Oct-2022 20:30:32 - [ 35] Sub Exposures ------------------------------------------------------------------------------------------------------------------------------------ Target | Exp |Instr | Oper. | Aper |Spectral|Cent.|Primary |Secondary |Iteration |CR-SPLIT |Orbit |Duration Name | Num |Config | Mode | or FOV |Element |Wave.|Pattern Pos |Pattern Pos |Num |Num |Number | ------------------------------------------------------------------------------------------------------------------------------------ WASP-12 8 WFC3/IR MULTIAC GRISM256 G141 none none 6 none 4 N/A CUM WASP-12 8 WFC3/IR MULTIAC GRISM256 G141 none none 6 none 4 N/A CUM WASP-12 8 WFC3/IR MULTIAC GRISM256 G141 none none 7 none 4 N/A CUM WASP-12 8 WFC3/IR MULTIAC GRISM256 G141 none none 7 none 4 N/A CUM WASP-12 8 WFC3/IR MULTIAC GRISM256 G141 none none 8 none 4 N/A CUM WASP-12 8 WFC3/IR MULTIAC GRISM256 G141 none none 8 none 4 N/A CUM 16236( 5) - 06-Oct-2022 20:30:32 - [ 36] Summary Form for Proposal 16236 Item Used in this proposal ------------------------------------------------------------------------------------------------------------------------------------ Apertures GRISM256 ------------------------------------------------------------------------------------------------------------------------------------ Configurations WFC3/IR ------------------------------------------------------------------------------------------------------------------------------------ Opmodes MULTIACCUM ------------------------------------------------------------------------------------------------------------------------------------ Optional Parameters NSAMP=15, NSAMP=2, NSAMP=3, SAMP-SEQ=RAPID, SAMP-SEQ=SPARS10 ------------------------------------------------------------------------------------------------------------------------------------ Special Requirements AFTER 01, AFTER 02, AFTER 03, AFTER 04, AFTER 05, AFTER 06, GS ACQ SCENARIO BASE1BE, ORIENT 162.5D TO 247.5 D, ORIENT 342.7D TO 82.3 D, PHASE 0.31625 TO 0.35475, POS TARG 0, 0, Period 1.09142030 D AND ZERO-PHASE HJD2456176.668258, SAME ORIENT AS 01, SCHED 70%, SEQ 01, 02, 03, 04, 05, 06, 07 WITHIN 18 Orbits, SEQ 1-2 NON-INT, SEQ 1-3 NON-INT, SEQ 3-4 NON-INT, SEQ 4-5 NON-INT, SEQ 5-6 NON-INT, SEQ 6-7 NON-INT, SEQ 7-8 NON-INT, SPATIAL SCAN 0.0325, 90.0 Degrees, Round trip ------------------------------------------------------------------------------------------------------------------------------------ Spectral Elements F126N, G141 ------------------------------------------------------------------------------------------------------------------------------------ Target Names WASP-12 ------------------------------------------------------------------------------------------------------------------------------------