16108( 6) - 02-Nov-2021 13:03:24 - [ 1] HUBBLE SPACE TELESCOPE OBSERVING PROGRAM 16108 Version: 6 Check-in Time: 02-Nov-2021 13:03:24 STScI Edit Number: 1 Title ULLYSES Monitoring Observations of the T Tauri Star GM Aur: First Epoch ------------------------------------------------------------------------------------ Type Cycle GO/DD 28 ------------------------------------------------------------------------------------ Investigators Contact? PI: Dr. Julia Christine Roman-Duval Space Telescope Science Institute Y CoI: Dr. Kenneth Sembach Space Telescope Science Institute N CoI: Dr. TalaWanda R. Monroe Space Telescope Science Institute Y CoI: Joanna Taylor Space Telescope Science Institute N CoI: Dr. Travis C Fischer Space Telescope Science Institute - ESA N CoI: Dr. Charles R. Proffitt Space Telescope Science Institute Y CoI: Dr. William J. Fischer Space Telescope Science Institute Y CoI: Dr. Alexander W. Fullerton Space Telescope Science Institute N CoI: Dr. Alessandra Aloisi Space Telescope Science Institute N CoI: Christopher Britt Space Telescope Science Institute N CoI: Dr. Thomas M. Brown Space Telescope Science Institute N CoI: Ivo Busko Space Telescope Science Institute N CoI: Dr. Joleen Carlberg Space Telescope Science Institute N CoI: Dr. Gisella De Rosa Space Telescope Science Institute N CoI: Elaine M Frazer Space Telescope Science Institute Y CoI: Dr. Svea S Hernandez Space Telescope Science Institute - ESA - N JWST CoI: Dr. Alec S. Hirschauer Space Telescope Science Institute Y CoI: Dr. Bethan Lesley James Space Telescope Science Institute - ESA - N JWST CoI: Robert Jedrzejewski Space Telescope Science Institute N CoI: Sean Lockwood Space Telescope Science Institute N CoI: Dr. Cristina Oliveira Space Telescope Science Institute N CoI: Rachel Plesha Space Telescope Science Institute N CoI: Dr. I. Neill Reid Space Telescope Science Institute N CoI: Dr. Adric R. Riedel Space Telescope Science Institute N CoI: Allyssa Riley Space Telescope Science Institute N CoI: Dr. David J. Sahnow Space Telescope Science Institute N CoI: Dr. Ravi Sankrit Space Telescope Science Institute N CoI: Dr. Richard Shaw Space Telescope Science Institute N CoI: Dr. Linda J. Smith Space Telescope Science Institute - ESA N CoI: Dr. Sangmo Tony Sohn Space Telescope Science Institute N CoI: Dr. Debopam Som Space Telescope Science Institute Y CoI: Dr. Leonardo Ubeda Space Telescope Science Institute N CoI: Dr. Daniel E. Welty Space Telescope Science Institute N CoI: Brian York Space Telescope Science Institute N ------------------------------------------------------------------------------------ Abstract The Space Telescope Science Institute (STScI) Director has decided to devote up to 1000 orbits of Director's Discretionary time in observing Cycles 27-29 to a new Hubble Ultraviolet Legacy program focused on star formation and associated stellar physics. This new program, ULLYSES (UV Legacy Library of Young Stars as Essential 16108( 6) - 02-Nov-2021 13:03:24 - [ 2] Standards), will provide a UV spectroscopic reference sample of young (< 10 Myr) high- and low-mass stars. It will target ~165 OB stars in the Magellanic Clouds and lower metallicity galaxies in the Local Group, and ~67 T Tauri stars and brown dwarfs in the Milky Way. In addition, ULLYSES will monitor 4 typical T Tauri stars over different rotational phases through at least three rotation periods, and over timescales of months to years. The resulting library will provide template spectra of massive stars at metallicities substantially below the well studied, while the low mass sample will cover a wide range of ages, accretion rates, and masses, including objects down to well below 0.5 M_sun. The legacy of this large UV dataset on the first 10 Myr of stellar evolution will be enhanced by complementary datasets obtained by the scientific community. In addition to the core goals of the program related to stellar astrophysics of low and high mass stars, this data will also enable exciting science in the fields of ISM, CGM, jets, and exoplanets. ULLYSES will be modeled after the Frontier Fields program: all data obtained will be non-proprietary. The implementation team at STScI is developing high-level science data products and a sophisticated database and website for disseminating data from the ULLYSES program and ancillary datasets for the ULLYSES target sample from space and ground-based facilities. ------------------------------------------------------------------------------------ Observations Description ------------------------ Observations use COS NUV + FUV and all visits are single orbit with SCHED=100. This target will be in the TESS field of view for Sectors 43 and 44. Furthermore, ground-based observers have requested that HST observations begin after October 1. For the purpose of coordinated observations, we set BETWEENs for all visits. 01 Oct 2021 00:00 - 11 Oct 2021 08:10 12 Oct 2021 17:00 - 24 Oct 2021 04:15 25 Oct 2021 17:20 - 05 Nov 2021 21:10 The rotation period of the target is 6.1 days = 92.2 orbits. We want to schedule 4 visits/period over three consecutive rotation periods, but we don't care about zero point shifts in the whole pattern. Ideal visit spacing would be 23.1 orbits. If we allow windows that are multiples of 23.1 +/- 4.1 orbits after visit 1 the required AFTER BY orbit values are as follows Visit 2 3 4 5 6 7 8 9 10 11 12 Start 19.0 42.0 65.1 88.2 111.2 134.3 157.4 180.4 203.5 226.6 249.6 End 27.2 50.2 73.3 96.4 119.4 142.5 165.6 188.6 211.7 234.8 257.8 The windows could be widened a bit if needed to facilitate scheduling. If possible, we would like to schedule visits during the period from roughly 0h to 16h UT every day when the target will be visible from LCOGT telescopes. More precise windows can be provided, and these can be enforced manually instead of as rigid BETWEENs. ------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [ 3] TARGET LIST Fixed Targets ------------------------------------------------------------------------------------------------------------------------------------ Tar| Target | Target | Target |Coord | Radial | Flux data No | Name | Description | Position |Eqnx | Vel. | ------------------------------------------------------------------------------------------------------------------------------------ 1 V-GM-AUR STAR, PRE-MAIN SEQUENCE RA=04H55M10.9860S +/- 0.00002", J2000 V = 12.242 SpT=K3, U=14.59, B=13.35, STAR, T TAURI STAR DEC=+30D21'59.00" +/- 0.00002" V=12.24, R=11.80, G=11.70, J=9.34, H=8.60, K=8.28 Reference Frame: ICRS Extended: NO Comments: tstatus; V-GM-AUR ; P/COS approved for submission; S/ins not started; P/AH 19/07/21; S/xx DD/MM/YY tcheck; APT/SIMBAD target names: ; V-GM-AUR ... Default SIMBAD name is V* GM Aur, aka 2MASS J04551098+3021595 tcheck; Target info verification status?; OK ... spectral type and magnitudes seem to be consistent Flam(B) = 2.6e-10 at 4444 Angstroms and Flam(V) = 4.7e-10 at 5540 Angstroms from Vizier photometry viewer linked from SIMBAD tcheck; Coordinates & P.M. verified, epoch checked?; OK ... SIMBAD coordinates check out with what's here, SIMBAD PM values check out with what's here tcheck; Adopted SED compared to Observations?; Yes ... located at: box/ullyses_tech/ullyses_proposals/monitor/16018/seds/ Epoch of Position RA proper motion (seconds of time/yr) DEC Proper Motion (arcsec/yr) Annual Parallax (arcsec) 2015.5 3.012635677084487E-4 -0.02445099994474731 0.0 ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [ 4] Visit: 1C (V-GM-AUR-COS-1) Visit Requirements: SCHED 100%; BETWEEN 01-OCT-2021:00:00:00 AND 11-OCT-2021:08:10:00; BETWEEN 12-OCT-2021:17:00:00 AND 24-OCT-2021:04:15:00; BETWEEN 25-OCT-2021:17:20:00 AND 05-NOV-2021:21:10:00 On Hold Comments: Additional Comments: vstatus; 1C; V-GM-AUR; P/COS approved for submission; P/AH 19/07/21 ; intrev: complete ; P/WF 19/07/21 vcheck; Enter targ name & Inst. & Resp. Sci.; GM Aur ; COS ; AH vcheck; ETC numbers entered in APT?; Yes vcheck; Any screening violations?; No vcheck; M-dwarf check complete and added to box folder?; N/A vcheck; S/N ETC calcs done & documented?; Yes vcheck; Field images checked & saved?; Yes ... located at: box/ullyses_tech/ullyses_proposals/monitor/16018/images/ vcheck; Selected ACQ strategy?; Double ACQ/PeakXD+ACQ/PeakD, G230L, S/N = 40 vcheck; Possible ACQ or Sci spoilers?; No vcheck; Field BOT clear?; Yes vcheck; Visual BOT check for stars not in catalog?; Yes vcheck; Orbit packing finalized?; Yes vcheck; Buffer times optimized?; Yes vcheck; Verify visit grouping correct; Yes vcheck; phase constraint for ground based observations added?; N/A vcheck; BETWEENS for coordinated observations added?; Yes ... 01 OCT 2021 00:00 to 11 OCT 2021 08:10 and 12 OCT 2021 17:00 to 24 OCT 2021 04:15 and 25 OCT 2021 17:20 to 05 NOV 2021 21:10 vcheck; Is visit ready for int. review?; Yes Allocated COS orbits = 12 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 V-GM-AUR COS/NUV ACQ/PEA PSA G230L 2950 STRIPE=DEF 1 5.8 S (5.8 KXD S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC (COS.sa.1522537) in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/PEAKXD with PSA takes 5.8 seconds for S/N=40. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sa.1522540) in order to determine bright object safety. ACQ/PEAKXD with PSA has peak pixel rate of 5.943 counts per second and global rate of 2997.808, so it is safe. This is the first of two ACQ/PEAKXD+ACQ/PEAKD used in order to improve the likelihood of a successful acquisition. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [ 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 ------------------------------------------------------------------------------------------------------------------------------------ 2 V-GM-AUR COS/NUV ACQ/PEA PSA G230L 2950 CENTER=FLUX-WT-FLR, NUM-POS=5, 1 5.3 S (5.3 KD STEP-SIZE=0.9 S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC (COS.sa.1522538) in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/PEAKD with PSA takes 5.3 seconds for S/N=40. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sa.1522541) in order to determine bright object safety. ACQ/PEAKD with PSA has peak pixel rate of 5.943 counts per second and global rate of 2997.808, so it is safe. This is the first of two ACQ/PEAKXD+ACQ/PEAKD used in order to improve the likelihood of a successful acquisition. ------------------------------------------------------------------------------------------------------------------------------------ 3 V-GM-AUR COS/NUV ACQ/PEA PSA G230L 2950 STRIPE=DEF 1 5.8 S (5.8 KXD S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC (COS.sa.1522537) in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/PEAKXD with PSA takes 5.8 seconds for S/N=40. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sa.1522540) in order to determine bright object safety. ACQ/PEAKXD with PSA has peak pixel rate of 5.943 counts per second and global rate of 2997.808, so it is safe. This is the second of two ACQ/PEAKXD+ACQ/PEAKD used in order to improve the likelihood of a successful acquisition. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [ 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 ------------------------------------------------------------------------------------------------------------------------------------ 4 V-GM-AUR COS/NUV ACQ/PEA PSA G230L 2950 CENTER=FLUX-WT-FLR, NUM-POS=5, 1 5.3 S (5.3 KD STEP-SIZE=0.9 S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC (COS.sa.1522538) in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/PEAKD with PSA takes 5.3 seconds for S/N=40. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sa.1522541) in order to determine bright object safety. ACQ/PEAKD with PSA has peak pixel rate of 5.943 counts per second and global rate of 2997.808, so it is safe. This is the second of two ACQ/PEAKXD+ACQ/PEAKD used in order to improve the likelihood of a successful acquisition. ------------------------------------------------------------------------------------------------------------------------------------ 5 V-GM-AUR COS/NUV TIME-TA PSA G230L 2950 FP-POS=4, BUFFER-TIME=524 1 184 S (184 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522552). 362.4388 seconds to achieve S/N = 20 at 2825 A. This time is halved (= 181.2194 seconds) to account for the other G230L cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522735) uses the expanded exposure time to fill the orbit (184 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is minimal. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522691) in order to determine bright object safety. Peak local rate of 5.943 counts per second and global rate of 2997.808, so it is safe. Buffer fill time = 786 seconds, and 2/3 of this is 524 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [ 7] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 6 V-GM-AUR COS/NUV TIME-TA PSA G230L 2635 FP-POS=1, BUFFER-TIME=448 1 184 S (184 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522553). 364.1707 seconds to achieve S/N = 20 at 2825 A. This time is halved (= 182.08535 seconds) to account for the other G230L cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522737) uses the expanded exposure time to fill the orbit (184 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is minimal. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522690) in order to determine bright object safety. Peak local rate of 5.927 counts per second and global rate of 2199.263, so it is safe. Buffer fill time = 672 seconds, and 2/3 of this is 448 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [ 8] 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 V-GM-AUR COS/FUV TIME-TA PSA G160M 1589 FP-POS=3, BUFFER-TIME=2865 1 186 S (186 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522544). 376.7304 seconds to achieve S/N = 30 at 1548.5 A. This time is quartered (= 94.1826 seconds) to account for both the other G160M cenwave and the two FP-POS settings per cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522739) uses the expanded exposure time to fill the orbit (186 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is significant compared to the G230L exposures. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522682) in order to determine bright object safety. Peak local rate of 0.315 counts per second and global rate of 548.875, so it is safe. Buffer fill time = 4297 seconds, and 2/3 of this is 2864.667 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [ 9] 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 V-GM-AUR COS/FUV TIME-TA PSA G160M 1589 FP-POS=4, BUFFER-TIME=2865 1 186 S (186 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522544). 376.7304 seconds to achieve S/N = 30 at 1548.5 A. This time is quartered (= 94.1826 seconds) to account for both the other G160M cenwave and the two FP-POS settings per cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522739) uses the expanded exposure time to fill the orbit (186 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is significant compared to the G230L exposures. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522682) in order to determine bright object safety. Peak local rate of 0.315 counts per second and global rate of 548.875, so it is safe. Buffer fill time = 4297 seconds, and 2/3 of this is 2864.667 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [ 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 ------------------------------------------------------------------------------------------------------------------------------------ 9 V-GM-AUR COS/FUV TIME-TA PSA G160M 1623 FP-POS=1, BUFFER-TIME=3154 1 186 S (186 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522545). 393.2034 seconds to achieve S/N = 30 at 1548.5 A. This time is quartered (= 98.30085 seconds) to account for both the other G160M cenwave and the two FP-POS settings per cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522741) uses the expanded exposure time to fill the orbit (186 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is significant compared to the G230L exposures. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522683) in order to determine bright object safety. Peak local rate of 0.317 counts per second and global rate of 498.525, so it is safe. Buffer fill time = 4731 seconds, and 2/3 of this is 3154 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [ 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 ------------------------------------------------------------------------------------------------------------------------------------ 10 V-GM-AUR COS/FUV TIME-TA PSA G160M 1623 FP-POS=2, BUFFER-TIME=3154 1 186 S (186 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522545). 393.2034 seconds to achieve S/N = 30 at 1548.5 A. This time is quartered (= 98.30085 seconds) to account for both the other G160M cenwave and the two FP-POS settings per cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522741) uses the expanded exposure time to fill the orbit (186 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is significant compared to the G230L exposures. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522683) in order to determine bright object safety. Peak local rate of 0.317 counts per second and global rate of 498.525, so it is safe. Buffer fill time = 4731 seconds, and 2/3 of this is 3154 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 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 | ------------------------------------------------------------------------------------------------------------------------------------ V-GM-AUR 1 COS/NUV ACQ/PEA PSA G230L 2950 none none none none 1 N/A KXD V-GM-AUR 2 COS/NUV ACQ/PEA PSA G230L 2950 none none none none 1 N/A KD V-GM-AUR 3 COS/NUV ACQ/PEA PSA G230L 2950 none none none none 1 N/A KXD V-GM-AUR 4 COS/NUV ACQ/PEA PSA G230L 2950 none none none none 1 N/A KD V-GM-AUR 5 COS/NUV TIME-TA PSA G230L 2950 none none none none 1 N/A G V-GM-AUR 6 COS/NUV TIME-TA PSA G230L 2635 none none none none 1 N/A G V-GM-AUR 7 COS/FUV TIME-TA PSA G160M 1589 none none none none 1 N/A G 16108( 6) - 02-Nov-2021 13:03:24 - [ 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 | ------------------------------------------------------------------------------------------------------------------------------------ V-GM-AUR 8 COS/FUV TIME-TA PSA G160M 1589 none none none none 1 N/A G V-GM-AUR 9 COS/FUV TIME-TA PSA G160M 1623 none none none none 1 N/A G V-GM-AUR 10 COS/FUV TIME-TA PSA G160M 1623 none none none none 1 N/A G 16108( 6) - 02-Nov-2021 13:03:24 - [ 13] Visit: 1D (V-GM-AUR-COS-2) Visit Requirements: SCHED 100%; AFTER 1C BY 19.0 Orbits TO 27.2 Orbits; BETWEEN 01-OCT-2021:00:00:00 AND 11-OCT-2021:08:10:00; BETWEEN 12-OCT-2021:17:00:00 AND 24-OCT-2021:04:15:00; BETWEEN 25-OCT-2021:17:20:00 AND 05-NOV-2021:21:10:00 On Hold Comments: Additional Comments: vstatus; 1D; V-GM-AUR; P/COS approved for submission; P/AH 19/07/21 ; intrev: complete ; P/WF 19/07/21 vcheck; Enter targ name & Inst. & Resp. Sci.; GM Aur ; COS ; AH vcheck; ETC numbers entered in APT?; Yes vcheck; Any screening violations?; No vcheck; M-dwarf check complete and added to box folder?; N/A vcheck; S/N ETC calcs done & documented?; Yes vcheck; Field images checked & saved?; Yes ... located at: box/ullyses_tech/ullyses_proposals/monitor/16018/images/ vcheck; Selected ACQ strategy?; Double ACQ/PeakXD+ACQ/PeakD, G230L, S/N = 40 vcheck; Possible ACQ or Sci spoilers?; No vcheck; Field BOT clear?; Yes vcheck; Visual BOT check for stars not in catalog?; Yes vcheck; Orbit packing finalized?; Yes vcheck; Buffer times optimized?; Yes vcheck; Verify visit grouping correct; Yes vcheck; phase constraint for ground based observations added?; N/A vcheck; BETWEENS for coordinated observations added?; Yes ... 01 OCT 2021 00:00 to 11 OCT 2021 08:10 and 12 OCT 2021 17:00 to 24 OCT 2021 04:15 and 25 OCT 2021 17:20 to 05 NOV 2021 21:10 vcheck; Is visit ready for int. review?; Yes Allocated COS orbits = 12 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 V-GM-AUR COS/NUV ACQ/PEA PSA G230L 2950 STRIPE=DEF 1 5.8 S (5.8 KXD S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC (COS.sa.1522537) in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/PEAKXD with PSA takes 5.8 seconds for S/N=40. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sa.1522540) in order to determine bright object safety. ACQ/PEAKXD with PSA has peak pixel rate of 5.943 counts per second and global rate of 2997.808, so it is safe. This is the first of two ACQ/PEAKXD+ACQ/PEAKD used in order to improve the likelihood of a successful acquisition. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [ 14] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 2 V-GM-AUR COS/NUV ACQ/PEA PSA G230L 2950 CENTER=FLUX-WT-FLR, NUM-POS=5, 1 5.3 S (5.3 KD STEP-SIZE=0.9 S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC (COS.sa.1522538) in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/PEAKD with PSA takes 5.3 seconds for S/N=40. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sa.1522541) in order to determine bright object safety. ACQ/PEAKD with PSA has peak pixel rate of 5.943 counts per second and global rate of 2997.808, so it is safe. This is the first of two ACQ/PEAKXD+ACQ/PEAKD used in order to improve the likelihood of a successful acquisition. ------------------------------------------------------------------------------------------------------------------------------------ 3 V-GM-AUR COS/NUV ACQ/PEA PSA G230L 2950 STRIPE=DEF 1 5.8 S (5.8 KXD S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC (COS.sa.1522537) in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/PEAKXD with PSA takes 5.8 seconds for S/N=40. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sa.1522540) in order to determine bright object safety. ACQ/PEAKXD with PSA has peak pixel rate of 5.943 counts per second and global rate of 2997.808, so it is safe. This is the second of two ACQ/PEAKXD+ACQ/PEAKD used in order to improve the likelihood of a successful acquisition. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [ 15] 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 V-GM-AUR COS/NUV ACQ/PEA PSA G230L 2950 CENTER=FLUX-WT-FLR, NUM-POS=5, 1 5.3 S (5.3 KD STEP-SIZE=0.9 S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC (COS.sa.1522538) in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/PEAKD with PSA takes 5.3 seconds for S/N=40. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sa.1522541) in order to determine bright object safety. ACQ/PEAKD with PSA has peak pixel rate of 5.943 counts per second and global rate of 2997.808, so it is safe. This is the second of two ACQ/PEAKXD+ACQ/PEAKD used in order to improve the likelihood of a successful acquisition. ------------------------------------------------------------------------------------------------------------------------------------ 5 V-GM-AUR COS/NUV TIME-TA PSA G230L 2950 FP-POS=4, BUFFER-TIME=524 1 184 S (184 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522552). 362.4388 seconds to achieve S/N = 20 at 2825 A. This time is halved (= 181.2194 seconds) to account for the other G230L cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522735) uses the expanded exposure time to fill the orbit (184 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is minimal. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522691) in order to determine bright object safety. Peak local rate of 5.943 counts per second and global rate of 2997.808, so it is safe. Buffer fill time = 786 seconds, and 2/3 of this is 524 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [ 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 ------------------------------------------------------------------------------------------------------------------------------------ 6 V-GM-AUR COS/NUV TIME-TA PSA G230L 2635 FP-POS=1, BUFFER-TIME=448 1 184 S (184 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522553). 364.1707 seconds to achieve S/N = 20 at 2825 A. This time is halved (= 182.08535 seconds) to account for the other G230L cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522737) uses the expanded exposure time to fill the orbit (184 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is minimal. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522690) in order to determine bright object safety. Peak local rate of 5.927 counts per second and global rate of 2199.263, so it is safe. Buffer fill time = 672 seconds, and 2/3 of this is 448 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [ 17] 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 V-GM-AUR COS/FUV TIME-TA PSA G160M 1589 FP-POS=3, BUFFER-TIME=2865 1 186 S (186 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522544). 376.7304 seconds to achieve S/N = 30 at 1548.5 A. This time is quartered (= 94.1826 seconds) to account for both the other G160M cenwave and the two FP-POS settings per cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522739) uses the expanded exposure time to fill the orbit (186 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is significant compared to the G230L exposures. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522682) in order to determine bright object safety. Peak local rate of 0.315 counts per second and global rate of 548.875, so it is safe. Buffer fill time = 4297 seconds, and 2/3 of this is 2864.667 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [ 18] 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 V-GM-AUR COS/FUV TIME-TA PSA G160M 1589 FP-POS=4, BUFFER-TIME=2865 1 186 S (186 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522544). 376.7304 seconds to achieve S/N = 30 at 1548.5 A. This time is quartered (= 94.1826 seconds) to account for both the other G160M cenwave and the two FP-POS settings per cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522739) uses the expanded exposure time to fill the orbit (186 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is significant compared to the G230L exposures. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522682) in order to determine bright object safety. Peak local rate of 0.315 counts per second and global rate of 548.875, so it is safe. Buffer fill time = 4297 seconds, and 2/3 of this is 2864.667 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [ 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 ------------------------------------------------------------------------------------------------------------------------------------ 9 V-GM-AUR COS/FUV TIME-TA PSA G160M 1623 FP-POS=1, BUFFER-TIME=3154 1 186 S (186 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522545). 393.2034 seconds to achieve S/N = 30 at 1548.5 A. This time is quartered (= 98.30085 seconds) to account for both the other G160M cenwave and the two FP-POS settings per cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522741) uses the expanded exposure time to fill the orbit (186 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is significant compared to the G230L exposures. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522683) in order to determine bright object safety. Peak local rate of 0.317 counts per second and global rate of 498.525, so it is safe. Buffer fill time = 4731 seconds, and 2/3 of this is 3154 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [ 20] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 10 V-GM-AUR COS/FUV TIME-TA PSA G160M 1623 FP-POS=2, BUFFER-TIME=3154 1 186 S (186 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522545). 393.2034 seconds to achieve S/N = 30 at 1548.5 A. This time is quartered (= 98.30085 seconds) to account for both the other G160M cenwave and the two FP-POS settings per cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522741) uses the expanded exposure time to fill the orbit (186 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is significant compared to the G230L exposures. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522683) in order to determine bright object safety. Peak local rate of 0.317 counts per second and global rate of 498.525, so it is safe. Buffer fill time = 4731 seconds, and 2/3 of this is 3154 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 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 | ------------------------------------------------------------------------------------------------------------------------------------ V-GM-AUR 1 COS/NUV ACQ/PEA PSA G230L 2950 none none none none 1 N/A KXD V-GM-AUR 2 COS/NUV ACQ/PEA PSA G230L 2950 none none none none 1 N/A KD V-GM-AUR 3 COS/NUV ACQ/PEA PSA G230L 2950 none none none none 1 N/A KXD V-GM-AUR 4 COS/NUV ACQ/PEA PSA G230L 2950 none none none none 1 N/A KD V-GM-AUR 5 COS/NUV TIME-TA PSA G230L 2950 none none none none 1 N/A G V-GM-AUR 6 COS/NUV TIME-TA PSA G230L 2635 none none none none 1 N/A G V-GM-AUR 7 COS/FUV TIME-TA PSA G160M 1589 none none none none 1 N/A G 16108( 6) - 02-Nov-2021 13:03:24 - [ 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 | ------------------------------------------------------------------------------------------------------------------------------------ V-GM-AUR 8 COS/FUV TIME-TA PSA G160M 1589 none none none none 1 N/A G V-GM-AUR 9 COS/FUV TIME-TA PSA G160M 1623 none none none none 1 N/A G V-GM-AUR 10 COS/FUV TIME-TA PSA G160M 1623 none none none none 1 N/A G 16108( 6) - 02-Nov-2021 13:03:24 - [ 22] Visit: 1E (V-GM-AUR-COS-3) Visit Requirements: SCHED 100%; AFTER 1C BY 42.0 Orbits TO 50.2 Orbits; BETWEEN 01-OCT-2021:00:00:00 AND 11-OCT-2021:08:10:00; BETWEEN 12-OCT-2021:17:00:00 AND 24-OCT-2021:04:15:00; BETWEEN 25-OCT-2021:17:20:00 AND 05-NOV-2021:21:10:00 On Hold Comments: Additional Comments: vstatus; 1E; V-GM-AUR; P/COS approved for submission; P/AH 19/07/21 ; intrev: complete ; P/WF 19/07/21 vcheck; Enter targ name & Inst. & Resp. Sci.; GM Aur ; COS ; AH vcheck; ETC numbers entered in APT?; Yes vcheck; Any screening violations?; No vcheck; M-dwarf check complete and added to box folder?; N/A vcheck; S/N ETC calcs done & documented?; Yes vcheck; Field images checked & saved?; Yes ... located at: box/ullyses_tech/ullyses_proposals/monitor/16018/images/ vcheck; Selected ACQ strategy?; Double ACQ/PeakXD+ACQ/PeakD, G230L, S/N = 40 vcheck; Possible ACQ or Sci spoilers?; No vcheck; Field BOT clear?; Yes vcheck; Visual BOT check for stars not in catalog?; Yes vcheck; Orbit packing finalized?; Yes vcheck; Buffer times optimized?; Yes vcheck; Verify visit grouping correct; Yes vcheck; phase constraint for ground based observations added?; N/A vcheck; BETWEENS for coordinated observations added?; Yes ... 01 OCT 2021 00:00 to 11 OCT 2021 08:10 and 12 OCT 2021 17:00 to 24 OCT 2021 04:15 and 25 OCT 2021 17:20 to 05 NOV 2021 21:10 vcheck; Is visit ready for int. review?; Yes Allocated COS orbits = 12 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 V-GM-AUR COS/NUV ACQ/PEA PSA G230L 2950 STRIPE=DEF 1 5.8 S (5.8 KXD S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC (COS.sa.1522537) in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/PEAKXD with PSA takes 5.8 seconds for S/N=40. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sa.1522540) in order to determine bright object safety. ACQ/PEAKXD with PSA has peak pixel rate of 5.943 counts per second and global rate of 2997.808, so it is safe. This is the first of two ACQ/PEAKXD+ACQ/PEAKD used in order to improve the likelihood of a successful acquisition. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [ 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 ------------------------------------------------------------------------------------------------------------------------------------ 2 V-GM-AUR COS/NUV ACQ/PEA PSA G230L 2950 CENTER=FLUX-WT-FLR, NUM-POS=5, 1 5.3 S (5.3 KD STEP-SIZE=0.9 S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC (COS.sa.1522538) in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/PEAKD with PSA takes 5.3 seconds for S/N=40. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sa.1522541) in order to determine bright object safety. ACQ/PEAKD with PSA has peak pixel rate of 5.943 counts per second and global rate of 2997.808, so it is safe. This is the first of two ACQ/PEAKXD+ACQ/PEAKD used in order to improve the likelihood of a successful acquisition. ------------------------------------------------------------------------------------------------------------------------------------ 3 V-GM-AUR COS/NUV ACQ/PEA PSA G230L 2950 STRIPE=DEF 1 5.8 S (5.8 KXD S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC (COS.sa.1522537) in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/PEAKXD with PSA takes 5.8 seconds for S/N=40. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sa.1522540) in order to determine bright object safety. ACQ/PEAKXD with PSA has peak pixel rate of 5.943 counts per second and global rate of 2997.808, so it is safe. This is the second of two ACQ/PEAKXD+ACQ/PEAKD used in order to improve the likelihood of a successful acquisition. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [ 24] 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 V-GM-AUR COS/NUV ACQ/PEA PSA G230L 2950 CENTER=FLUX-WT-FLR, NUM-POS=5, 1 5.3 S (5.3 KD STEP-SIZE=0.9 S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC (COS.sa.1522538) in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/PEAKD with PSA takes 5.3 seconds for S/N=40. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sa.1522541) in order to determine bright object safety. ACQ/PEAKD with PSA has peak pixel rate of 5.943 counts per second and global rate of 2997.808, so it is safe. This is the second of two ACQ/PEAKXD+ACQ/PEAKD used in order to improve the likelihood of a successful acquisition. ------------------------------------------------------------------------------------------------------------------------------------ 5 V-GM-AUR COS/NUV TIME-TA PSA G230L 2950 FP-POS=4, BUFFER-TIME=524 1 184 S (184 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522552). 362.4388 seconds to achieve S/N = 20 at 2825 A. This time is halved (= 181.2194 seconds) to account for the other G230L cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522735) uses the expanded exposure time to fill the orbit (184 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is minimal. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522691) in order to determine bright object safety. Peak local rate of 5.943 counts per second and global rate of 2997.808, so it is safe. Buffer fill time = 786 seconds, and 2/3 of this is 524 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [ 25] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 6 V-GM-AUR COS/NUV TIME-TA PSA G230L 2635 FP-POS=1, BUFFER-TIME=448 1 184 S (184 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522553). 364.1707 seconds to achieve S/N = 20 at 2825 A. This time is halved (= 182.08535 seconds) to account for the other G230L cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522737) uses the expanded exposure time to fill the orbit (184 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is minimal. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522690) in order to determine bright object safety. Peak local rate of 5.927 counts per second and global rate of 2199.263, so it is safe. Buffer fill time = 672 seconds, and 2/3 of this is 448 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [ 26] 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 V-GM-AUR COS/FUV TIME-TA PSA G160M 1589 FP-POS=3, BUFFER-TIME=2865 1 186 S (186 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522544). 376.7304 seconds to achieve S/N = 30 at 1548.5 A. This time is quartered (= 94.1826 seconds) to account for both the other G160M cenwave and the two FP-POS settings per cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522739) uses the expanded exposure time to fill the orbit (186 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is significant compared to the G230L exposures. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522682) in order to determine bright object safety. Peak local rate of 0.315 counts per second and global rate of 548.875, so it is safe. Buffer fill time = 4297 seconds, and 2/3 of this is 2864.667 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [ 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 ------------------------------------------------------------------------------------------------------------------------------------ 8 V-GM-AUR COS/FUV TIME-TA PSA G160M 1589 FP-POS=4, BUFFER-TIME=2865 1 186 S (186 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522544). 376.7304 seconds to achieve S/N = 30 at 1548.5 A. This time is quartered (= 94.1826 seconds) to account for both the other G160M cenwave and the two FP-POS settings per cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522739) uses the expanded exposure time to fill the orbit (186 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is significant compared to the G230L exposures. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522682) in order to determine bright object safety. Peak local rate of 0.315 counts per second and global rate of 548.875, so it is safe. Buffer fill time = 4297 seconds, and 2/3 of this is 2864.667 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [ 28] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 9 V-GM-AUR COS/FUV TIME-TA PSA G160M 1623 FP-POS=1, BUFFER-TIME=3154 1 186 S (186 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522545). 393.2034 seconds to achieve S/N = 30 at 1548.5 A. This time is quartered (= 98.30085 seconds) to account for both the other G160M cenwave and the two FP-POS settings per cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522741) uses the expanded exposure time to fill the orbit (186 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is significant compared to the G230L exposures. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522683) in order to determine bright object safety. Peak local rate of 0.317 counts per second and global rate of 498.525, so it is safe. Buffer fill time = 4731 seconds, and 2/3 of this is 3154 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [ 29] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 10 V-GM-AUR COS/FUV TIME-TA PSA G160M 1623 FP-POS=2, BUFFER-TIME=3154 1 186 S (186 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522545). 393.2034 seconds to achieve S/N = 30 at 1548.5 A. This time is quartered (= 98.30085 seconds) to account for both the other G160M cenwave and the two FP-POS settings per cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522741) uses the expanded exposure time to fill the orbit (186 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is significant compared to the G230L exposures. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522683) in order to determine bright object safety. Peak local rate of 0.317 counts per second and global rate of 498.525, so it is safe. Buffer fill time = 4731 seconds, and 2/3 of this is 3154 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 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 | ------------------------------------------------------------------------------------------------------------------------------------ V-GM-AUR 1 COS/NUV ACQ/PEA PSA G230L 2950 none none none none 1 N/A KXD V-GM-AUR 2 COS/NUV ACQ/PEA PSA G230L 2950 none none none none 1 N/A KD V-GM-AUR 3 COS/NUV ACQ/PEA PSA G230L 2950 none none none none 1 N/A KXD V-GM-AUR 4 COS/NUV ACQ/PEA PSA G230L 2950 none none none none 1 N/A KD V-GM-AUR 5 COS/NUV TIME-TA PSA G230L 2950 none none none none 1 N/A G V-GM-AUR 6 COS/NUV TIME-TA PSA G230L 2635 none none none none 1 N/A G V-GM-AUR 7 COS/FUV TIME-TA PSA G160M 1589 none none none none 1 N/A G 16108( 6) - 02-Nov-2021 13:03:24 - [ 30] 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 | ------------------------------------------------------------------------------------------------------------------------------------ V-GM-AUR 8 COS/FUV TIME-TA PSA G160M 1589 none none none none 1 N/A G V-GM-AUR 9 COS/FUV TIME-TA PSA G160M 1623 none none none none 1 N/A G V-GM-AUR 10 COS/FUV TIME-TA PSA G160M 1623 none none none none 1 N/A G 16108( 6) - 02-Nov-2021 13:03:24 - [ 31] Visit: 1F (V-GM-AUR-COS-4) Visit Requirements: SCHED 100%; AFTER 1C BY 65.1 Orbits TO 73.3 Orbits; BETWEEN 01-OCT-2021:00:00:00 AND 11-OCT-2021:08:10:00; BETWEEN 12-OCT-2021:17:00:00 AND 24-OCT-2021:04:15:00; BETWEEN 25-OCT-2021:17:20:00 AND 05-NOV-2021:21:10:00 On Hold Comments: Additional Comments: vstatus; 1F; V-GM-AUR; P/COS approved for submission; P/AH 19/07/21 ; intrev: complete ; P/WF 19/07/21 vcheck; Enter targ name & Inst. & Resp. Sci.; GM Aur ; COS ; AH vcheck; ETC numbers entered in APT?; Yes vcheck; Any screening violations?; No vcheck; M-dwarf check complete and added to box folder?; N/A vcheck; S/N ETC calcs done & documented?; Yes vcheck; Field images checked & saved?; Yes ... located at: box/ullyses_tech/ullyses_proposals/monitor/16018/images/ vcheck; Selected ACQ strategy?; Double ACQ/PeakXD+ACQ/PeakD, G230L, S/N = 40 vcheck; Possible ACQ or Sci spoilers?; No vcheck; Field BOT clear?; Yes vcheck; Visual BOT check for stars not in catalog?; Yes vcheck; Orbit packing finalized?; Yes vcheck; Buffer times optimized?; Yes vcheck; Verify visit grouping correct; Yes vcheck; phase constraint for ground based observations added?; N/A vcheck; BETWEENS for coordinated observations added?; Yes ... 01 OCT 2021 00:00 to 11 OCT 2021 08:10 and 12 OCT 2021 17:00 to 24 OCT 2021 04:15 and 25 OCT 2021 17:20 to 05 NOV 2021 21:10 vcheck; Is visit ready for int. review?; Yes Allocated COS orbits = 12 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 V-GM-AUR COS/NUV ACQ/PEA PSA G230L 2950 STRIPE=DEF 1 5.8 S (5.8 KXD S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC (COS.sa.1522537) in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/PEAKXD with PSA takes 5.8 seconds for S/N=40. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sa.1522540) in order to determine bright object safety. ACQ/PEAKXD with PSA has peak pixel rate of 5.943 counts per second and global rate of 2997.808, so it is safe. This is the first of two ACQ/PEAKXD+ACQ/PEAKD used in order to improve the likelihood of a successful acquisition. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [ 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 ------------------------------------------------------------------------------------------------------------------------------------ 2 V-GM-AUR COS/NUV ACQ/PEA PSA G230L 2950 CENTER=FLUX-WT-FLR, NUM-POS=5, 1 5.3 S (5.3 KD STEP-SIZE=0.9 S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC (COS.sa.1522538) in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/PEAKD with PSA takes 5.3 seconds for S/N=40. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sa.1522541) in order to determine bright object safety. ACQ/PEAKD with PSA has peak pixel rate of 5.943 counts per second and global rate of 2997.808, so it is safe. This is the first of two ACQ/PEAKXD+ACQ/PEAKD used in order to improve the likelihood of a successful acquisition. ------------------------------------------------------------------------------------------------------------------------------------ 3 V-GM-AUR COS/NUV ACQ/PEA PSA G230L 2950 STRIPE=DEF 1 5.8 S (5.8 KXD S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC (COS.sa.1522537) in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/PEAKXD with PSA takes 5.8 seconds for S/N=40. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sa.1522540) in order to determine bright object safety. ACQ/PEAKXD with PSA has peak pixel rate of 5.943 counts per second and global rate of 2997.808, so it is safe. This is the second of two ACQ/PEAKXD+ACQ/PEAKD used in order to improve the likelihood of a successful acquisition. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [ 33] 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 V-GM-AUR COS/NUV ACQ/PEA PSA G230L 2950 CENTER=FLUX-WT-FLR, NUM-POS=5, 1 5.3 S (5.3 KD STEP-SIZE=0.9 S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC (COS.sa.1522538) in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/PEAKD with PSA takes 5.3 seconds for S/N=40. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sa.1522541) in order to determine bright object safety. ACQ/PEAKD with PSA has peak pixel rate of 5.943 counts per second and global rate of 2997.808, so it is safe. This is the second of two ACQ/PEAKXD+ACQ/PEAKD used in order to improve the likelihood of a successful acquisition. ------------------------------------------------------------------------------------------------------------------------------------ 5 V-GM-AUR COS/NUV TIME-TA PSA G230L 2950 FP-POS=4, BUFFER-TIME=524 1 184 S (184 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522552). 362.4388 seconds to achieve S/N = 20 at 2825 A. This time is halved (= 181.2194 seconds) to account for the other G230L cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522735) uses the expanded exposure time to fill the orbit (184 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is minimal. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522691) in order to determine bright object safety. Peak local rate of 5.943 counts per second and global rate of 2997.808, so it is safe. Buffer fill time = 786 seconds, and 2/3 of this is 524 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [ 34] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 6 V-GM-AUR COS/NUV TIME-TA PSA G230L 2635 FP-POS=1, BUFFER-TIME=448 1 184 S (184 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522553). 364.1707 seconds to achieve S/N = 20 at 2825 A. This time is halved (= 182.08535 seconds) to account for the other G230L cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522737) uses the expanded exposure time to fill the orbit (184 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is minimal. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522690) in order to determine bright object safety. Peak local rate of 5.927 counts per second and global rate of 2199.263, so it is safe. Buffer fill time = 672 seconds, and 2/3 of this is 448 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [ 35] 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 V-GM-AUR COS/FUV TIME-TA PSA G160M 1589 FP-POS=3, BUFFER-TIME=2865 1 186 S (186 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522544). 376.7304 seconds to achieve S/N = 30 at 1548.5 A. This time is quartered (= 94.1826 seconds) to account for both the other G160M cenwave and the two FP-POS settings per cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522739) uses the expanded exposure time to fill the orbit (186 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is significant compared to the G230L exposures. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522682) in order to determine bright object safety. Peak local rate of 0.315 counts per second and global rate of 548.875, so it is safe. Buffer fill time = 4297 seconds, and 2/3 of this is 2864.667 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [ 36] 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 V-GM-AUR COS/FUV TIME-TA PSA G160M 1589 FP-POS=4, BUFFER-TIME=2865 1 186 S (186 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522544). 376.7304 seconds to achieve S/N = 30 at 1548.5 A. This time is quartered (= 94.1826 seconds) to account for both the other G160M cenwave and the two FP-POS settings per cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522739) uses the expanded exposure time to fill the orbit (186 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is significant compared to the G230L exposures. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522682) in order to determine bright object safety. Peak local rate of 0.315 counts per second and global rate of 548.875, so it is safe. Buffer fill time = 4297 seconds, and 2/3 of this is 2864.667 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [ 37] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 9 V-GM-AUR COS/FUV TIME-TA PSA G160M 1623 FP-POS=1, BUFFER-TIME=3154 1 186 S (186 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522545). 393.2034 seconds to achieve S/N = 30 at 1548.5 A. This time is quartered (= 98.30085 seconds) to account for both the other G160M cenwave and the two FP-POS settings per cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522741) uses the expanded exposure time to fill the orbit (186 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is significant compared to the G230L exposures. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522683) in order to determine bright object safety. Peak local rate of 0.317 counts per second and global rate of 498.525, so it is safe. Buffer fill time = 4731 seconds, and 2/3 of this is 3154 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [ 38] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 10 V-GM-AUR COS/FUV TIME-TA PSA G160M 1623 FP-POS=2, BUFFER-TIME=3154 1 186 S (186 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522545). 393.2034 seconds to achieve S/N = 30 at 1548.5 A. This time is quartered (= 98.30085 seconds) to account for both the other G160M cenwave and the two FP-POS settings per cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522741) uses the expanded exposure time to fill the orbit (186 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is significant compared to the G230L exposures. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522683) in order to determine bright object safety. Peak local rate of 0.317 counts per second and global rate of 498.525, so it is safe. Buffer fill time = 4731 seconds, and 2/3 of this is 3154 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 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 | ------------------------------------------------------------------------------------------------------------------------------------ V-GM-AUR 1 COS/NUV ACQ/PEA PSA G230L 2950 none none none none 1 N/A KXD V-GM-AUR 2 COS/NUV ACQ/PEA PSA G230L 2950 none none none none 1 N/A KD V-GM-AUR 3 COS/NUV ACQ/PEA PSA G230L 2950 none none none none 1 N/A KXD V-GM-AUR 4 COS/NUV ACQ/PEA PSA G230L 2950 none none none none 1 N/A KD V-GM-AUR 5 COS/NUV TIME-TA PSA G230L 2950 none none none none 1 N/A G V-GM-AUR 6 COS/NUV TIME-TA PSA G230L 2635 none none none none 1 N/A G V-GM-AUR 7 COS/FUV TIME-TA PSA G160M 1589 none none none none 1 N/A G 16108( 6) - 02-Nov-2021 13:03:24 - [ 39] 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 | ------------------------------------------------------------------------------------------------------------------------------------ V-GM-AUR 8 COS/FUV TIME-TA PSA G160M 1589 none none none none 1 N/A G V-GM-AUR 9 COS/FUV TIME-TA PSA G160M 1623 none none none none 1 N/A G V-GM-AUR 10 COS/FUV TIME-TA PSA G160M 1623 none none none none 1 N/A G 16108( 6) - 02-Nov-2021 13:03:24 - [ 40] Visit: 1G (V-GM-AUR-COS-5) Visit Requirements: SCHED 100%; AFTER 1C BY 88.2 Orbits TO 96.4 Orbits; BETWEEN 01-OCT-2021:00:00:00 AND 11-OCT-2021:08:10:00; BETWEEN 12-OCT-2021:17:00:00 AND 24-OCT-2021:04:15:00; BETWEEN 25-OCT-2021:17:20:00 AND 05-NOV-2021:21:10:00 On Hold Comments: Additional Comments: vstatus; 1G; V-GM-AUR; P/COS approved for submission; P/AH 19/07/21 ; intrev: complete ; P/WF 19/07/21 vcheck; Enter targ name & Inst. & Resp. Sci.; GM Aur ; COS ; AH vcheck; ETC numbers entered in APT?; Yes vcheck; Any screening violations?; No vcheck; M-dwarf check complete and added to box folder?; N/A vcheck; S/N ETC calcs done & documented?; Yes vcheck; Field images checked & saved?; Yes ... located at: box/ullyses_tech/ullyses_proposals/monitor/16018/images/ vcheck; Selected ACQ strategy?; Double ACQ/PeakXD+ACQ/PeakD, G230L, S/N = 40 vcheck; Possible ACQ or Sci spoilers?; No vcheck; Field BOT clear?; Yes vcheck; Visual BOT check for stars not in catalog?; Yes vcheck; Orbit packing finalized?; Yes vcheck; Buffer times optimized?; Yes vcheck; Verify visit grouping correct; Yes vcheck; phase constraint for ground based observations added?; N/A vcheck; BETWEENS for coordinated observations added?; Yes ... 01 OCT 2021 00:00 to 11 OCT 2021 08:10 and 12 OCT 2021 17:00 to 24 OCT 2021 04:15 and 25 OCT 2021 17:20 to 05 NOV 2021 21:10 vcheck; Is visit ready for int. review?; Yes Allocated COS orbits = 12 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 V-GM-AUR COS/NUV ACQ/PEA PSA G230L 2950 STRIPE=DEF 1 5.8 S (5.8 KXD S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC (COS.sa.1522537) in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/PEAKXD with PSA takes 5.8 seconds for S/N=40. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sa.1522540) in order to determine bright object safety. ACQ/PEAKXD with PSA has peak pixel rate of 5.943 counts per second and global rate of 2997.808, so it is safe. This is the first of two ACQ/PEAKXD+ACQ/PEAKD used in order to improve the likelihood of a successful acquisition. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [ 41] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 2 V-GM-AUR COS/NUV ACQ/PEA PSA G230L 2950 CENTER=FLUX-WT-FLR, NUM-POS=5, 1 5.3 S (5.3 KD STEP-SIZE=0.9 S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC (COS.sa.1522538) in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/PEAKD with PSA takes 5.3 seconds for S/N=40. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sa.1522541) in order to determine bright object safety. ACQ/PEAKD with PSA has peak pixel rate of 5.943 counts per second and global rate of 2997.808, so it is safe. This is the first of two ACQ/PEAKXD+ACQ/PEAKD used in order to improve the likelihood of a successful acquisition. ------------------------------------------------------------------------------------------------------------------------------------ 3 V-GM-AUR COS/NUV ACQ/PEA PSA G230L 2950 STRIPE=DEF 1 5.8 S (5.8 KXD S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC (COS.sa.1522537) in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/PEAKXD with PSA takes 5.8 seconds for S/N=40. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sa.1522540) in order to determine bright object safety. ACQ/PEAKXD with PSA has peak pixel rate of 5.943 counts per second and global rate of 2997.808, so it is safe. This is the second of two ACQ/PEAKXD+ACQ/PEAKD used in order to improve the likelihood of a successful acquisition. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [ 42] 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 V-GM-AUR COS/NUV ACQ/PEA PSA G230L 2950 CENTER=FLUX-WT-FLR, NUM-POS=5, 1 5.3 S (5.3 KD STEP-SIZE=0.9 S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC (COS.sa.1522538) in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/PEAKD with PSA takes 5.3 seconds for S/N=40. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sa.1522541) in order to determine bright object safety. ACQ/PEAKD with PSA has peak pixel rate of 5.943 counts per second and global rate of 2997.808, so it is safe. This is the second of two ACQ/PEAKXD+ACQ/PEAKD used in order to improve the likelihood of a successful acquisition. ------------------------------------------------------------------------------------------------------------------------------------ 5 V-GM-AUR COS/NUV TIME-TA PSA G230L 2950 FP-POS=4, BUFFER-TIME=524 1 184 S (184 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522552). 362.4388 seconds to achieve S/N = 20 at 2825 A. This time is halved (= 181.2194 seconds) to account for the other G230L cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522735) uses the expanded exposure time to fill the orbit (184 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is minimal. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522691) in order to determine bright object safety. Peak local rate of 5.943 counts per second and global rate of 2997.808, so it is safe. Buffer fill time = 786 seconds, and 2/3 of this is 524 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [ 43] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 6 V-GM-AUR COS/NUV TIME-TA PSA G230L 2635 FP-POS=1, BUFFER-TIME=448 1 184 S (184 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522553). 364.1707 seconds to achieve S/N = 20 at 2825 A. This time is halved (= 182.08535 seconds) to account for the other G230L cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522737) uses the expanded exposure time to fill the orbit (184 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is minimal. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522690) in order to determine bright object safety. Peak local rate of 5.927 counts per second and global rate of 2199.263, so it is safe. Buffer fill time = 672 seconds, and 2/3 of this is 448 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [ 44] 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 V-GM-AUR COS/FUV TIME-TA PSA G160M 1589 FP-POS=3, BUFFER-TIME=2865 1 186 S (186 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522544). 376.7304 seconds to achieve S/N = 30 at 1548.5 A. This time is quartered (= 94.1826 seconds) to account for both the other G160M cenwave and the two FP-POS settings per cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522739) uses the expanded exposure time to fill the orbit (186 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is significant compared to the G230L exposures. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522682) in order to determine bright object safety. Peak local rate of 0.315 counts per second and global rate of 548.875, so it is safe. Buffer fill time = 4297 seconds, and 2/3 of this is 2864.667 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [ 45] 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 V-GM-AUR COS/FUV TIME-TA PSA G160M 1589 FP-POS=4, BUFFER-TIME=2865 1 186 S (186 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522544). 376.7304 seconds to achieve S/N = 30 at 1548.5 A. This time is quartered (= 94.1826 seconds) to account for both the other G160M cenwave and the two FP-POS settings per cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522739) uses the expanded exposure time to fill the orbit (186 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is significant compared to the G230L exposures. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522682) in order to determine bright object safety. Peak local rate of 0.315 counts per second and global rate of 548.875, so it is safe. Buffer fill time = 4297 seconds, and 2/3 of this is 2864.667 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [ 46] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 9 V-GM-AUR COS/FUV TIME-TA PSA G160M 1623 FP-POS=1, BUFFER-TIME=3154 1 186 S (186 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522545). 393.2034 seconds to achieve S/N = 30 at 1548.5 A. This time is quartered (= 98.30085 seconds) to account for both the other G160M cenwave and the two FP-POS settings per cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522741) uses the expanded exposure time to fill the orbit (186 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is significant compared to the G230L exposures. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522683) in order to determine bright object safety. Peak local rate of 0.317 counts per second and global rate of 498.525, so it is safe. Buffer fill time = 4731 seconds, and 2/3 of this is 3154 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [ 47] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 10 V-GM-AUR COS/FUV TIME-TA PSA G160M 1623 FP-POS=2, BUFFER-TIME=3154 1 186 S (186 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522545). 393.2034 seconds to achieve S/N = 30 at 1548.5 A. This time is quartered (= 98.30085 seconds) to account for both the other G160M cenwave and the two FP-POS settings per cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522741) uses the expanded exposure time to fill the orbit (186 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is significant compared to the G230L exposures. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522683) in order to determine bright object safety. Peak local rate of 0.317 counts per second and global rate of 498.525, so it is safe. Buffer fill time = 4731 seconds, and 2/3 of this is 3154 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 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 | ------------------------------------------------------------------------------------------------------------------------------------ V-GM-AUR 1 COS/NUV ACQ/PEA PSA G230L 2950 none none none none 1 N/A KXD V-GM-AUR 2 COS/NUV ACQ/PEA PSA G230L 2950 none none none none 1 N/A KD V-GM-AUR 3 COS/NUV ACQ/PEA PSA G230L 2950 none none none none 1 N/A KXD V-GM-AUR 4 COS/NUV ACQ/PEA PSA G230L 2950 none none none none 1 N/A KD V-GM-AUR 5 COS/NUV TIME-TA PSA G230L 2950 none none none none 1 N/A G V-GM-AUR 6 COS/NUV TIME-TA PSA G230L 2635 none none none none 1 N/A G V-GM-AUR 7 COS/FUV TIME-TA PSA G160M 1589 none none none none 1 N/A G 16108( 6) - 02-Nov-2021 13:03:24 - [ 48] 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 | ------------------------------------------------------------------------------------------------------------------------------------ V-GM-AUR 8 COS/FUV TIME-TA PSA G160M 1589 none none none none 1 N/A G V-GM-AUR 9 COS/FUV TIME-TA PSA G160M 1623 none none none none 1 N/A G V-GM-AUR 10 COS/FUV TIME-TA PSA G160M 1623 none none none none 1 N/A G 16108( 6) - 02-Nov-2021 13:03:24 - [ 49] Visit: 1H (V-GM-AUR-COS-6) Visit Requirements: SCHED 100%; AFTER 1C BY 111.2 Orbits TO 119.4 Orbits; BETWEEN 01-OCT-2021:00:00:00 AND 11-OCT-2021:08:10:00; BETWEEN 12-OCT-2021:17:00:00 AND 24-OCT-2021:04:15:00; BETWEEN 25-OCT-2021:17:20:00 AND 05-NOV-2021:21:10:00 On Hold Comments: Additional Comments: vstatus; 1H; V-GM-AUR; P/COS approved for submission; P/AH 19/07/21 ; intrev: complete ; P/WF 19/07/21 vcheck; Enter targ name & Inst. & Resp. Sci.; GM Aur ; COS ; AH vcheck; ETC numbers entered in APT?; Yes vcheck; Any screening violations?; No vcheck; M-dwarf check complete and added to box folder?; N/A vcheck; S/N ETC calcs done & documented?; Yes vcheck; Field images checked & saved?; Yes ... located at: box/ullyses_tech/ullyses_proposals/monitor/16018/images/ vcheck; Selected ACQ strategy?; Double ACQ/PeakXD+ACQ/PeakD, G230L, S/N = 40 vcheck; Possible ACQ or Sci spoilers?; No vcheck; Field BOT clear?; Yes vcheck; Visual BOT check for stars not in catalog?; Yes vcheck; Orbit packing finalized?; Yes vcheck; Buffer times optimized?; Yes vcheck; Verify visit grouping correct; Yes vcheck; phase constraint for ground based observations added?; N/A vcheck; BETWEENS for coordinated observations added?; Yes ... 01 OCT 2021 00:00 to 11 OCT 2021 08:10 and 12 OCT 2021 17:00 to 24 OCT 2021 04:15 and 25 OCT 2021 17:20 to 05 NOV 2021 21:10 vcheck; Is visit ready for int. review?; Yes Allocated COS orbits = 12 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 V-GM-AUR COS/NUV ACQ/PEA PSA G230L 2950 STRIPE=DEF 1 5.8 S (5.8 KXD S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC (COS.sa.1522537) in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/PEAKXD with PSA takes 5.8 seconds for S/N=40. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sa.1522540) in order to determine bright object safety. ACQ/PEAKXD with PSA has peak pixel rate of 5.943 counts per second and global rate of 2997.808, so it is safe. This is the first of two ACQ/PEAKXD+ACQ/PEAKD used in order to improve the likelihood of a successful acquisition. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [ 50] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 2 V-GM-AUR COS/NUV ACQ/PEA PSA G230L 2950 CENTER=FLUX-WT-FLR, NUM-POS=5, 1 5.3 S (5.3 KD STEP-SIZE=0.9 S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC (COS.sa.1522538) in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/PEAKD with PSA takes 5.3 seconds for S/N=40. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sa.1522541) in order to determine bright object safety. ACQ/PEAKD with PSA has peak pixel rate of 5.943 counts per second and global rate of 2997.808, so it is safe. This is the first of two ACQ/PEAKXD+ACQ/PEAKD used in order to improve the likelihood of a successful acquisition. ------------------------------------------------------------------------------------------------------------------------------------ 3 V-GM-AUR COS/NUV ACQ/PEA PSA G230L 2950 STRIPE=DEF 1 5.8 S (5.8 KXD S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC (COS.sa.1522537) in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/PEAKXD with PSA takes 5.8 seconds for S/N=40. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sa.1522540) in order to determine bright object safety. ACQ/PEAKXD with PSA has peak pixel rate of 5.943 counts per second and global rate of 2997.808, so it is safe. This is the second of two ACQ/PEAKXD+ACQ/PEAKD used in order to improve the likelihood of a successful acquisition. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [ 51] 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 V-GM-AUR COS/NUV ACQ/PEA PSA G230L 2950 CENTER=FLUX-WT-FLR, NUM-POS=5, 1 5.3 S (5.3 KD STEP-SIZE=0.9 S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC (COS.sa.1522538) in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/PEAKD with PSA takes 5.3 seconds for S/N=40. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sa.1522541) in order to determine bright object safety. ACQ/PEAKD with PSA has peak pixel rate of 5.943 counts per second and global rate of 2997.808, so it is safe. This is the second of two ACQ/PEAKXD+ACQ/PEAKD used in order to improve the likelihood of a successful acquisition. ------------------------------------------------------------------------------------------------------------------------------------ 5 V-GM-AUR COS/NUV TIME-TA PSA G230L 2950 FP-POS=4, BUFFER-TIME=524 1 184 S (184 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522552). 362.4388 seconds to achieve S/N = 20 at 2825 A. This time is halved (= 181.2194 seconds) to account for the other G230L cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522735) uses the expanded exposure time to fill the orbit (184 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is minimal. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522691) in order to determine bright object safety. Peak local rate of 5.943 counts per second and global rate of 2997.808, so it is safe. Buffer fill time = 786 seconds, and 2/3 of this is 524 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [ 52] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 6 V-GM-AUR COS/NUV TIME-TA PSA G230L 2635 FP-POS=1, BUFFER-TIME=448 1 184 S (184 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522553). 364.1707 seconds to achieve S/N = 20 at 2825 A. This time is halved (= 182.08535 seconds) to account for the other G230L cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522737) uses the expanded exposure time to fill the orbit (184 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is minimal. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522690) in order to determine bright object safety. Peak local rate of 5.927 counts per second and global rate of 2199.263, so it is safe. Buffer fill time = 672 seconds, and 2/3 of this is 448 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [ 53] 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 V-GM-AUR COS/FUV TIME-TA PSA G160M 1589 FP-POS=3, BUFFER-TIME=2865 1 186 S (186 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522544). 376.7304 seconds to achieve S/N = 30 at 1548.5 A. This time is quartered (= 94.1826 seconds) to account for both the other G160M cenwave and the two FP-POS settings per cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522739) uses the expanded exposure time to fill the orbit (186 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is significant compared to the G230L exposures. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522682) in order to determine bright object safety. Peak local rate of 0.315 counts per second and global rate of 548.875, so it is safe. Buffer fill time = 4297 seconds, and 2/3 of this is 2864.667 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [ 54] 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 V-GM-AUR COS/FUV TIME-TA PSA G160M 1589 FP-POS=4, BUFFER-TIME=2865 1 186 S (186 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522544). 376.7304 seconds to achieve S/N = 30 at 1548.5 A. This time is quartered (= 94.1826 seconds) to account for both the other G160M cenwave and the two FP-POS settings per cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522739) uses the expanded exposure time to fill the orbit (186 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is significant compared to the G230L exposures. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522682) in order to determine bright object safety. Peak local rate of 0.315 counts per second and global rate of 548.875, so it is safe. Buffer fill time = 4297 seconds, and 2/3 of this is 2864.667 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [ 55] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 9 V-GM-AUR COS/FUV TIME-TA PSA G160M 1623 FP-POS=1, BUFFER-TIME=3154 1 186 S (186 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522545). 393.2034 seconds to achieve S/N = 30 at 1548.5 A. This time is quartered (= 98.30085 seconds) to account for both the other G160M cenwave and the two FP-POS settings per cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522741) uses the expanded exposure time to fill the orbit (186 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is significant compared to the G230L exposures. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522683) in order to determine bright object safety. Peak local rate of 0.317 counts per second and global rate of 498.525, so it is safe. Buffer fill time = 4731 seconds, and 2/3 of this is 3154 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [ 56] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 10 V-GM-AUR COS/FUV TIME-TA PSA G160M 1623 FP-POS=2, BUFFER-TIME=3154 1 186 S (186 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522545). 393.2034 seconds to achieve S/N = 30 at 1548.5 A. This time is quartered (= 98.30085 seconds) to account for both the other G160M cenwave and the two FP-POS settings per cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522741) uses the expanded exposure time to fill the orbit (186 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is significant compared to the G230L exposures. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522683) in order to determine bright object safety. Peak local rate of 0.317 counts per second and global rate of 498.525, so it is safe. Buffer fill time = 4731 seconds, and 2/3 of this is 3154 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 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 | ------------------------------------------------------------------------------------------------------------------------------------ V-GM-AUR 1 COS/NUV ACQ/PEA PSA G230L 2950 none none none none 1 N/A KXD V-GM-AUR 2 COS/NUV ACQ/PEA PSA G230L 2950 none none none none 1 N/A KD V-GM-AUR 3 COS/NUV ACQ/PEA PSA G230L 2950 none none none none 1 N/A KXD V-GM-AUR 4 COS/NUV ACQ/PEA PSA G230L 2950 none none none none 1 N/A KD V-GM-AUR 5 COS/NUV TIME-TA PSA G230L 2950 none none none none 1 N/A G V-GM-AUR 6 COS/NUV TIME-TA PSA G230L 2635 none none none none 1 N/A G V-GM-AUR 7 COS/FUV TIME-TA PSA G160M 1589 none none none none 1 N/A G 16108( 6) - 02-Nov-2021 13:03:24 - [ 57] 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 | ------------------------------------------------------------------------------------------------------------------------------------ V-GM-AUR 8 COS/FUV TIME-TA PSA G160M 1589 none none none none 1 N/A G V-GM-AUR 9 COS/FUV TIME-TA PSA G160M 1623 none none none none 1 N/A G V-GM-AUR 10 COS/FUV TIME-TA PSA G160M 1623 none none none none 1 N/A G 16108( 6) - 02-Nov-2021 13:03:24 - [ 58] Visit: 1I (V-GM-AUR-COS-7) Visit Requirements: SCHED 100%; AFTER 1C BY 134.3 Orbits TO 142.5 Orbits; BETWEEN 01-OCT-2021:00:00:00 AND 11-OCT-2021:08:10:00; BETWEEN 12-OCT-2021:17:00:00 AND 24-OCT-2021:04:15:00; BETWEEN 25-OCT-2021:17:20:00 AND 05-NOV-2021:21:10:00 On Hold Comments: Additional Comments: vstatus; 1I; V-GM-AUR; P/COS approved for submission; P/AH 19/07/21 ; intrev: complete ; P/WF 19/07/21 vcheck; Enter targ name & Inst. & Resp. Sci.; GM Aur ; COS ; AH vcheck; ETC numbers entered in APT?; Yes vcheck; Any screening violations?; No vcheck; M-dwarf check complete and added to box folder?; N/A vcheck; S/N ETC calcs done & documented?; Yes vcheck; Field images checked & saved?; Yes ... located at: box/ullyses_tech/ullyses_proposals/monitor/16018/images/ vcheck; Selected ACQ strategy?; Double ACQ/PeakXD+ACQ/PeakD, G230L, S/N = 40 vcheck; Possible ACQ or Sci spoilers?; No vcheck; Field BOT clear?; Yes vcheck; Visual BOT check for stars not in catalog?; Yes vcheck; Orbit packing finalized?; Yes vcheck; Buffer times optimized?; Yes vcheck; Verify visit grouping correct; Yes vcheck; phase constraint for ground based observations added?; N/A vcheck; BETWEENS for coordinated observations added?; Yes ... 01 OCT 2021 00:00 to 11 OCT 2021 08:10 and 12 OCT 2021 17:00 to 24 OCT 2021 04:15 and 25 OCT 2021 17:20 to 05 NOV 2021 21:10 vcheck; Is visit ready for int. review?; Yes Allocated COS orbits = 12 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 V-GM-AUR COS/NUV ACQ/PEA PSA G230L 2950 STRIPE=DEF 1 5.8 S (5.8 KXD S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC (COS.sa.1522537) in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/PEAKXD with PSA takes 5.8 seconds for S/N=40. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sa.1522540) in order to determine bright object safety. ACQ/PEAKXD with PSA has peak pixel rate of 5.943 counts per second and global rate of 2997.808, so it is safe. This is the first of two ACQ/PEAKXD+ACQ/PEAKD used in order to improve the likelihood of a successful acquisition. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [ 59] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 2 V-GM-AUR COS/NUV ACQ/PEA PSA G230L 2950 CENTER=FLUX-WT-FLR, NUM-POS=5, 1 5.3 S (5.3 KD STEP-SIZE=0.9 S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC (COS.sa.1522538) in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/PEAKD with PSA takes 5.3 seconds for S/N=40. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sa.1522541) in order to determine bright object safety. ACQ/PEAKD with PSA has peak pixel rate of 5.943 counts per second and global rate of 2997.808, so it is safe. This is the first of two ACQ/PEAKXD+ACQ/PEAKD used in order to improve the likelihood of a successful acquisition. ------------------------------------------------------------------------------------------------------------------------------------ 3 V-GM-AUR COS/NUV ACQ/PEA PSA G230L 2950 STRIPE=DEF 1 5.8 S (5.8 KXD S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC (COS.sa.1522537) in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/PEAKXD with PSA takes 5.8 seconds for S/N=40. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sa.1522540) in order to determine bright object safety. ACQ/PEAKXD with PSA has peak pixel rate of 5.943 counts per second and global rate of 2997.808, so it is safe. This is the second of two ACQ/PEAKXD+ACQ/PEAKD used in order to improve the likelihood of a successful acquisition. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [ 60] 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 V-GM-AUR COS/NUV ACQ/PEA PSA G230L 2950 CENTER=FLUX-WT-FLR, NUM-POS=5, 1 5.3 S (5.3 KD STEP-SIZE=0.9 S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC (COS.sa.1522538) in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/PEAKD with PSA takes 5.3 seconds for S/N=40. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sa.1522541) in order to determine bright object safety. ACQ/PEAKD with PSA has peak pixel rate of 5.943 counts per second and global rate of 2997.808, so it is safe. This is the second of two ACQ/PEAKXD+ACQ/PEAKD used in order to improve the likelihood of a successful acquisition. ------------------------------------------------------------------------------------------------------------------------------------ 5 V-GM-AUR COS/NUV TIME-TA PSA G230L 2950 FP-POS=4, BUFFER-TIME=524 1 184 S (184 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522552). 362.4388 seconds to achieve S/N = 20 at 2825 A. This time is halved (= 181.2194 seconds) to account for the other G230L cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522735) uses the expanded exposure time to fill the orbit (184 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is minimal. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522691) in order to determine bright object safety. Peak local rate of 5.943 counts per second and global rate of 2997.808, so it is safe. Buffer fill time = 786 seconds, and 2/3 of this is 524 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [ 61] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 6 V-GM-AUR COS/NUV TIME-TA PSA G230L 2635 FP-POS=1, BUFFER-TIME=448 1 184 S (184 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522553). 364.1707 seconds to achieve S/N = 20 at 2825 A. This time is halved (= 182.08535 seconds) to account for the other G230L cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522737) uses the expanded exposure time to fill the orbit (184 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is minimal. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522690) in order to determine bright object safety. Peak local rate of 5.927 counts per second and global rate of 2199.263, so it is safe. Buffer fill time = 672 seconds, and 2/3 of this is 448 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [ 62] 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 V-GM-AUR COS/FUV TIME-TA PSA G160M 1589 FP-POS=3, BUFFER-TIME=2865 1 186 S (186 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522544). 376.7304 seconds to achieve S/N = 30 at 1548.5 A. This time is quartered (= 94.1826 seconds) to account for both the other G160M cenwave and the two FP-POS settings per cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522739) uses the expanded exposure time to fill the orbit (186 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is significant compared to the G230L exposures. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522682) in order to determine bright object safety. Peak local rate of 0.315 counts per second and global rate of 548.875, so it is safe. Buffer fill time = 4297 seconds, and 2/3 of this is 2864.667 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [ 63] 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 V-GM-AUR COS/FUV TIME-TA PSA G160M 1589 FP-POS=4, BUFFER-TIME=2865 1 186 S (186 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522544). 376.7304 seconds to achieve S/N = 30 at 1548.5 A. This time is quartered (= 94.1826 seconds) to account for both the other G160M cenwave and the two FP-POS settings per cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522739) uses the expanded exposure time to fill the orbit (186 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is significant compared to the G230L exposures. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522682) in order to determine bright object safety. Peak local rate of 0.315 counts per second and global rate of 548.875, so it is safe. Buffer fill time = 4297 seconds, and 2/3 of this is 2864.667 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [ 64] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 9 V-GM-AUR COS/FUV TIME-TA PSA G160M 1623 FP-POS=1, BUFFER-TIME=3154 1 186 S (186 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522545). 393.2034 seconds to achieve S/N = 30 at 1548.5 A. This time is quartered (= 98.30085 seconds) to account for both the other G160M cenwave and the two FP-POS settings per cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522741) uses the expanded exposure time to fill the orbit (186 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is significant compared to the G230L exposures. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522683) in order to determine bright object safety. Peak local rate of 0.317 counts per second and global rate of 498.525, so it is safe. Buffer fill time = 4731 seconds, and 2/3 of this is 3154 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [ 65] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 10 V-GM-AUR COS/FUV TIME-TA PSA G160M 1623 FP-POS=2, BUFFER-TIME=3154 1 186 S (186 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522545). 393.2034 seconds to achieve S/N = 30 at 1548.5 A. This time is quartered (= 98.30085 seconds) to account for both the other G160M cenwave and the two FP-POS settings per cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522741) uses the expanded exposure time to fill the orbit (186 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is significant compared to the G230L exposures. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522683) in order to determine bright object safety. Peak local rate of 0.317 counts per second and global rate of 498.525, so it is safe. Buffer fill time = 4731 seconds, and 2/3 of this is 3154 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 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 | ------------------------------------------------------------------------------------------------------------------------------------ V-GM-AUR 1 COS/NUV ACQ/PEA PSA G230L 2950 none none none none 1 N/A KXD V-GM-AUR 2 COS/NUV ACQ/PEA PSA G230L 2950 none none none none 1 N/A KD V-GM-AUR 3 COS/NUV ACQ/PEA PSA G230L 2950 none none none none 1 N/A KXD V-GM-AUR 4 COS/NUV ACQ/PEA PSA G230L 2950 none none none none 1 N/A KD V-GM-AUR 5 COS/NUV TIME-TA PSA G230L 2950 none none none none 1 N/A G V-GM-AUR 6 COS/NUV TIME-TA PSA G230L 2635 none none none none 1 N/A G V-GM-AUR 7 COS/FUV TIME-TA PSA G160M 1589 none none none none 1 N/A G 16108( 6) - 02-Nov-2021 13:03:24 - [ 66] 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 | ------------------------------------------------------------------------------------------------------------------------------------ V-GM-AUR 8 COS/FUV TIME-TA PSA G160M 1589 none none none none 1 N/A G V-GM-AUR 9 COS/FUV TIME-TA PSA G160M 1623 none none none none 1 N/A G V-GM-AUR 10 COS/FUV TIME-TA PSA G160M 1623 none none none none 1 N/A G 16108( 6) - 02-Nov-2021 13:03:24 - [ 67] Visit: 1J (V-GM-AUR-COS-8) Visit Requirements: SCHED 100%; AFTER 1C BY 157.4 Orbits TO 165.6 Orbits; BETWEEN 01-OCT-2021:00:00:00 AND 11-OCT-2021:08:10:00; BETWEEN 12-OCT-2021:17:00:00 AND 24-OCT-2021:04:15:00; BETWEEN 25-OCT-2021:17:20:00 AND 05-NOV-2021:21:10:00 On Hold Comments: Additional Comments: vstatus; 1J; V-GM-AUR; P/COS approved for submission; P/AH 19/07/21 ; intrev: complete ; P/WF 19/07/21 vcheck; Enter targ name & Inst. & Resp. Sci.; GM Aur ; COS ; AH vcheck; ETC numbers entered in APT?; Yes vcheck; Any screening violations?; No vcheck; M-dwarf check complete and added to box folder?; N/A vcheck; S/N ETC calcs done & documented?; Yes vcheck; Field images checked & saved?; Yes ... located at: box/ullyses_tech/ullyses_proposals/monitor/16018/images/ vcheck; Selected ACQ strategy?; Double ACQ/PeakXD+ACQ/PeakD, G230L, S/N = 40 vcheck; Possible ACQ or Sci spoilers?; No vcheck; Field BOT clear?; Yes vcheck; Visual BOT check for stars not in catalog?; Yes vcheck; Orbit packing finalized?; Yes vcheck; Buffer times optimized?; Yes vcheck; Verify visit grouping correct; Yes vcheck; phase constraint for ground based observations added?; N/A vcheck; BETWEENS for coordinated observations added?; Yes ... 01 OCT 2021 00:00 to 11 OCT 2021 08:10 and 12 OCT 2021 17:00 to 24 OCT 2021 04:15 and 25 OCT 2021 17:20 to 05 NOV 2021 21:10 vcheck; Is visit ready for int. review?; Yes Allocated COS orbits = 12 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 V-GM-AUR COS/NUV ACQ/PEA PSA G230L 2950 STRIPE=DEF 1 5.8 S (5.8 KXD S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC (COS.sa.1522537) in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/PEAKXD with PSA takes 5.8 seconds for S/N=40. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sa.1522540) in order to determine bright object safety. ACQ/PEAKXD with PSA has peak pixel rate of 5.943 counts per second and global rate of 2997.808, so it is safe. This is the first of two ACQ/PEAKXD+ACQ/PEAKD used in order to improve the likelihood of a successful acquisition. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [ 68] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 2 V-GM-AUR COS/NUV ACQ/PEA PSA G230L 2950 CENTER=FLUX-WT-FLR, NUM-POS=5, 1 5.3 S (5.3 KD STEP-SIZE=0.9 S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC (COS.sa.1522538) in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/PEAKD with PSA takes 5.3 seconds for S/N=40. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sa.1522541) in order to determine bright object safety. ACQ/PEAKD with PSA has peak pixel rate of 5.943 counts per second and global rate of 2997.808, so it is safe. This is the first of two ACQ/PEAKXD+ACQ/PEAKD used in order to improve the likelihood of a successful acquisition. ------------------------------------------------------------------------------------------------------------------------------------ 3 V-GM-AUR COS/NUV ACQ/PEA PSA G230L 2950 STRIPE=DEF 1 5.8 S (5.8 KXD S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC (COS.sa.1522537) in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/PEAKXD with PSA takes 5.8 seconds for S/N=40. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sa.1522540) in order to determine bright object safety. ACQ/PEAKXD with PSA has peak pixel rate of 5.943 counts per second and global rate of 2997.808, so it is safe. This is the second of two ACQ/PEAKXD+ACQ/PEAKD used in order to improve the likelihood of a successful acquisition. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [ 69] 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 V-GM-AUR COS/NUV ACQ/PEA PSA G230L 2950 CENTER=FLUX-WT-FLR, NUM-POS=5, 1 5.3 S (5.3 KD STEP-SIZE=0.9 S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC (COS.sa.1522538) in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/PEAKD with PSA takes 5.3 seconds for S/N=40. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sa.1522541) in order to determine bright object safety. ACQ/PEAKD with PSA has peak pixel rate of 5.943 counts per second and global rate of 2997.808, so it is safe. This is the second of two ACQ/PEAKXD+ACQ/PEAKD used in order to improve the likelihood of a successful acquisition. ------------------------------------------------------------------------------------------------------------------------------------ 5 V-GM-AUR COS/NUV TIME-TA PSA G230L 2950 FP-POS=4, BUFFER-TIME=524 1 184 S (184 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522552). 362.4388 seconds to achieve S/N = 20 at 2825 A. This time is halved (= 181.2194 seconds) to account for the other G230L cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522735) uses the expanded exposure time to fill the orbit (184 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is minimal. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522691) in order to determine bright object safety. Peak local rate of 5.943 counts per second and global rate of 2997.808, so it is safe. Buffer fill time = 786 seconds, and 2/3 of this is 524 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [ 70] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 6 V-GM-AUR COS/NUV TIME-TA PSA G230L 2635 FP-POS=1, BUFFER-TIME=448 1 184 S (184 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522553). 364.1707 seconds to achieve S/N = 20 at 2825 A. This time is halved (= 182.08535 seconds) to account for the other G230L cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522737) uses the expanded exposure time to fill the orbit (184 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is minimal. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522690) in order to determine bright object safety. Peak local rate of 5.927 counts per second and global rate of 2199.263, so it is safe. Buffer fill time = 672 seconds, and 2/3 of this is 448 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [ 71] 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 V-GM-AUR COS/FUV TIME-TA PSA G160M 1589 FP-POS=3, BUFFER-TIME=2865 1 186 S (186 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522544). 376.7304 seconds to achieve S/N = 30 at 1548.5 A. This time is quartered (= 94.1826 seconds) to account for both the other G160M cenwave and the two FP-POS settings per cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522739) uses the expanded exposure time to fill the orbit (186 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is significant compared to the G230L exposures. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522682) in order to determine bright object safety. Peak local rate of 0.315 counts per second and global rate of 548.875, so it is safe. Buffer fill time = 4297 seconds, and 2/3 of this is 2864.667 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [ 72] 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 V-GM-AUR COS/FUV TIME-TA PSA G160M 1589 FP-POS=4, BUFFER-TIME=2865 1 186 S (186 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522544). 376.7304 seconds to achieve S/N = 30 at 1548.5 A. This time is quartered (= 94.1826 seconds) to account for both the other G160M cenwave and the two FP-POS settings per cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522739) uses the expanded exposure time to fill the orbit (186 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is significant compared to the G230L exposures. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522682) in order to determine bright object safety. Peak local rate of 0.315 counts per second and global rate of 548.875, so it is safe. Buffer fill time = 4297 seconds, and 2/3 of this is 2864.667 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [ 73] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 9 V-GM-AUR COS/FUV TIME-TA PSA G160M 1623 FP-POS=1, BUFFER-TIME=3154 1 186 S (186 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522545). 393.2034 seconds to achieve S/N = 30 at 1548.5 A. This time is quartered (= 98.30085 seconds) to account for both the other G160M cenwave and the two FP-POS settings per cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522741) uses the expanded exposure time to fill the orbit (186 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is significant compared to the G230L exposures. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522683) in order to determine bright object safety. Peak local rate of 0.317 counts per second and global rate of 498.525, so it is safe. Buffer fill time = 4731 seconds, and 2/3 of this is 3154 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [ 74] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 10 V-GM-AUR COS/FUV TIME-TA PSA G160M 1623 FP-POS=2, BUFFER-TIME=3154 1 186 S (186 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522545). 393.2034 seconds to achieve S/N = 30 at 1548.5 A. This time is quartered (= 98.30085 seconds) to account for both the other G160M cenwave and the two FP-POS settings per cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522741) uses the expanded exposure time to fill the orbit (186 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is significant compared to the G230L exposures. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522683) in order to determine bright object safety. Peak local rate of 0.317 counts per second and global rate of 498.525, so it is safe. Buffer fill time = 4731 seconds, and 2/3 of this is 3154 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 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 | ------------------------------------------------------------------------------------------------------------------------------------ V-GM-AUR 1 COS/NUV ACQ/PEA PSA G230L 2950 none none none none 1 N/A KXD V-GM-AUR 2 COS/NUV ACQ/PEA PSA G230L 2950 none none none none 1 N/A KD V-GM-AUR 3 COS/NUV ACQ/PEA PSA G230L 2950 none none none none 1 N/A KXD V-GM-AUR 4 COS/NUV ACQ/PEA PSA G230L 2950 none none none none 1 N/A KD V-GM-AUR 5 COS/NUV TIME-TA PSA G230L 2950 none none none none 1 N/A G V-GM-AUR 6 COS/NUV TIME-TA PSA G230L 2635 none none none none 1 N/A G V-GM-AUR 7 COS/FUV TIME-TA PSA G160M 1589 none none none none 1 N/A G 16108( 6) - 02-Nov-2021 13:03:24 - [ 75] 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 | ------------------------------------------------------------------------------------------------------------------------------------ V-GM-AUR 8 COS/FUV TIME-TA PSA G160M 1589 none none none none 1 N/A G V-GM-AUR 9 COS/FUV TIME-TA PSA G160M 1623 none none none none 1 N/A G V-GM-AUR 10 COS/FUV TIME-TA PSA G160M 1623 none none none none 1 N/A G 16108( 6) - 02-Nov-2021 13:03:24 - [ 76] Visit: 1K (V-GM-AUR-COS-9) Visit Requirements: SCHED 100%; AFTER 1C BY 180.4 Orbits TO 188.6 Orbits; BETWEEN 01-OCT-2021:00:00:00 AND 11-OCT-2021:08:10:00; BETWEEN 12-OCT-2021:17:00:00 AND 24-OCT-2021:04:15:00; BETWEEN 25-OCT-2021:17:20:00 AND 05-NOV-2021:21:10:00 On Hold Comments: Additional Comments: vstatus; 1K; V-GM-AUR; P/COS approved for submission; P/AH 19/07/21 ; intrev: complete ; P/WF 19/07/21 vcheck; Enter targ name & Inst. & Resp. Sci.; GM Aur ; COS ; AH vcheck; ETC numbers entered in APT?; Yes vcheck; Any screening violations?; No vcheck; M-dwarf check complete and added to box folder?; N/A vcheck; S/N ETC calcs done & documented?; Yes vcheck; Field images checked & saved?; Yes ... located at: box/ullyses_tech/ullyses_proposals/monitor/16018/images/ vcheck; Selected ACQ strategy?; Double ACQ/PeakXD+ACQ/PeakD, G230L, S/N = 40 vcheck; Possible ACQ or Sci spoilers?; No vcheck; Field BOT clear?; Yes vcheck; Visual BOT check for stars not in catalog?; Yes vcheck; Orbit packing finalized?; Yes vcheck; Buffer times optimized?; Yes vcheck; Verify visit grouping correct; Yes vcheck; phase constraint for ground based observations added?; N/A vcheck; BETWEENS for coordinated observations added?; Yes ... 01 OCT 2021 00:00 to 11 OCT 2021 08:10 and 12 OCT 2021 17:00 to 24 OCT 2021 04:15 and 25 OCT 2021 17:20 to 05 NOV 2021 21:10 vcheck; Is visit ready for int. review?; Yes Allocated COS orbits = 12 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 V-GM-AUR COS/NUV ACQ/PEA PSA G230L 2950 STRIPE=DEF 1 5.8 S (5.8 KXD S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC (COS.sa.1522537) in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/PEAKXD with PSA takes 5.8 seconds for S/N=40. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sa.1522540) in order to determine bright object safety. ACQ/PEAKXD with PSA has peak pixel rate of 5.943 counts per second and global rate of 2997.808, so it is safe. This is the first of two ACQ/PEAKXD+ACQ/PEAKD used in order to improve the likelihood of a successful acquisition. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [ 77] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 2 V-GM-AUR COS/NUV ACQ/PEA PSA G230L 2950 CENTER=FLUX-WT-FLR, NUM-POS=5, 1 5.3 S (5.3 KD STEP-SIZE=0.9 S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC (COS.sa.1522538) in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/PEAKD with PSA takes 5.3 seconds for S/N=40. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sa.1522541) in order to determine bright object safety. ACQ/PEAKD with PSA has peak pixel rate of 5.943 counts per second and global rate of 2997.808, so it is safe. This is the first of two ACQ/PEAKXD+ACQ/PEAKD used in order to improve the likelihood of a successful acquisition. ------------------------------------------------------------------------------------------------------------------------------------ 3 V-GM-AUR COS/NUV ACQ/PEA PSA G230L 2950 STRIPE=DEF 1 5.8 S (5.8 KXD S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC (COS.sa.1522537) in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/PEAKXD with PSA takes 5.8 seconds for S/N=40. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sa.1522540) in order to determine bright object safety. ACQ/PEAKXD with PSA has peak pixel rate of 5.943 counts per second and global rate of 2997.808, so it is safe. This is the second of two ACQ/PEAKXD+ACQ/PEAKD used in order to improve the likelihood of a successful acquisition. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [ 78] 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 V-GM-AUR COS/NUV ACQ/PEA PSA G230L 2950 CENTER=FLUX-WT-FLR, NUM-POS=5, 1 5.3 S (5.3 KD STEP-SIZE=0.9 S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC (COS.sa.1522538) in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/PEAKD with PSA takes 5.3 seconds for S/N=40. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sa.1522541) in order to determine bright object safety. ACQ/PEAKD with PSA has peak pixel rate of 5.943 counts per second and global rate of 2997.808, so it is safe. This is the second of two ACQ/PEAKXD+ACQ/PEAKD used in order to improve the likelihood of a successful acquisition. ------------------------------------------------------------------------------------------------------------------------------------ 5 V-GM-AUR COS/NUV TIME-TA PSA G230L 2950 FP-POS=4, BUFFER-TIME=524 1 184 S (184 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522552). 362.4388 seconds to achieve S/N = 20 at 2825 A. This time is halved (= 181.2194 seconds) to account for the other G230L cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522735) uses the expanded exposure time to fill the orbit (184 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is minimal. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522691) in order to determine bright object safety. Peak local rate of 5.943 counts per second and global rate of 2997.808, so it is safe. Buffer fill time = 786 seconds, and 2/3 of this is 524 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [ 79] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 6 V-GM-AUR COS/NUV TIME-TA PSA G230L 2635 FP-POS=1, BUFFER-TIME=448 1 184 S (184 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522553). 364.1707 seconds to achieve S/N = 20 at 2825 A. This time is halved (= 182.08535 seconds) to account for the other G230L cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522737) uses the expanded exposure time to fill the orbit (184 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is minimal. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522690) in order to determine bright object safety. Peak local rate of 5.927 counts per second and global rate of 2199.263, so it is safe. Buffer fill time = 672 seconds, and 2/3 of this is 448 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [ 80] 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 V-GM-AUR COS/FUV TIME-TA PSA G160M 1589 FP-POS=3, BUFFER-TIME=2865 1 186 S (186 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522544). 376.7304 seconds to achieve S/N = 30 at 1548.5 A. This time is quartered (= 94.1826 seconds) to account for both the other G160M cenwave and the two FP-POS settings per cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522739) uses the expanded exposure time to fill the orbit (186 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is significant compared to the G230L exposures. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522682) in order to determine bright object safety. Peak local rate of 0.315 counts per second and global rate of 548.875, so it is safe. Buffer fill time = 4297 seconds, and 2/3 of this is 2864.667 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [ 81] 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 V-GM-AUR COS/FUV TIME-TA PSA G160M 1589 FP-POS=4, BUFFER-TIME=2865 1 186 S (186 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522544). 376.7304 seconds to achieve S/N = 30 at 1548.5 A. This time is quartered (= 94.1826 seconds) to account for both the other G160M cenwave and the two FP-POS settings per cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522739) uses the expanded exposure time to fill the orbit (186 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is significant compared to the G230L exposures. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522682) in order to determine bright object safety. Peak local rate of 0.315 counts per second and global rate of 548.875, so it is safe. Buffer fill time = 4297 seconds, and 2/3 of this is 2864.667 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [ 82] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 9 V-GM-AUR COS/FUV TIME-TA PSA G160M 1623 FP-POS=1, BUFFER-TIME=3154 1 186 S (186 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522545). 393.2034 seconds to achieve S/N = 30 at 1548.5 A. This time is quartered (= 98.30085 seconds) to account for both the other G160M cenwave and the two FP-POS settings per cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522741) uses the expanded exposure time to fill the orbit (186 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is significant compared to the G230L exposures. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522683) in order to determine bright object safety. Peak local rate of 0.317 counts per second and global rate of 498.525, so it is safe. Buffer fill time = 4731 seconds, and 2/3 of this is 3154 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [ 83] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 10 V-GM-AUR COS/FUV TIME-TA PSA G160M 1623 FP-POS=2, BUFFER-TIME=3154 1 186 S (186 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522545). 393.2034 seconds to achieve S/N = 30 at 1548.5 A. This time is quartered (= 98.30085 seconds) to account for both the other G160M cenwave and the two FP-POS settings per cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522741) uses the expanded exposure time to fill the orbit (186 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is significant compared to the G230L exposures. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522683) in order to determine bright object safety. Peak local rate of 0.317 counts per second and global rate of 498.525, so it is safe. Buffer fill time = 4731 seconds, and 2/3 of this is 3154 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 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 | ------------------------------------------------------------------------------------------------------------------------------------ V-GM-AUR 1 COS/NUV ACQ/PEA PSA G230L 2950 none none none none 1 N/A KXD V-GM-AUR 2 COS/NUV ACQ/PEA PSA G230L 2950 none none none none 1 N/A KD V-GM-AUR 3 COS/NUV ACQ/PEA PSA G230L 2950 none none none none 1 N/A KXD V-GM-AUR 4 COS/NUV ACQ/PEA PSA G230L 2950 none none none none 1 N/A KD V-GM-AUR 5 COS/NUV TIME-TA PSA G230L 2950 none none none none 1 N/A G V-GM-AUR 6 COS/NUV TIME-TA PSA G230L 2635 none none none none 1 N/A G V-GM-AUR 7 COS/FUV TIME-TA PSA G160M 1589 none none none none 1 N/A G 16108( 6) - 02-Nov-2021 13:03:24 - [ 84] 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 | ------------------------------------------------------------------------------------------------------------------------------------ V-GM-AUR 8 COS/FUV TIME-TA PSA G160M 1589 none none none none 1 N/A G V-GM-AUR 9 COS/FUV TIME-TA PSA G160M 1623 none none none none 1 N/A G V-GM-AUR 10 COS/FUV TIME-TA PSA G160M 1623 none none none none 1 N/A G 16108( 6) - 02-Nov-2021 13:03:24 - [ 85] Visit: 1L (V-GM-AUR-COS-10) Visit Requirements: SCHED 100%; AFTER 1C BY 203.5 Orbits TO 213.2 Orbits; BETWEEN 01-OCT-2021:00:00:00 AND 11-OCT-2021:08:10:00; BETWEEN 12-OCT-2021:17:00:00 AND 24-OCT-2021:04:15:00; BETWEEN 25-OCT-2021:17:20:00 AND 05-NOV-2021:21:10:00 On Hold Comments: Additional Comments: vstatus; 1L; V-GM-AUR; P/COS approved for submission; P/AH 19/07/21 ; intrev: complete ; P/WF 19/07/21 vcheck; Enter targ name & Inst. & Resp. Sci.; GM Aur ; COS ; AH vcheck; ETC numbers entered in APT?; Yes vcheck; Any screening violations?; No vcheck; M-dwarf check complete and added to box folder?; N/A vcheck; S/N ETC calcs done & documented?; Yes vcheck; Field images checked & saved?; Yes ... located at: box/ullyses_tech/ullyses_proposals/monitor/16018/images/ vcheck; Selected ACQ strategy?; Double ACQ/PeakXD+ACQ/PeakD, G230L, S/N = 40 vcheck; Possible ACQ or Sci spoilers?; No vcheck; Field BOT clear?; Yes vcheck; Visual BOT check for stars not in catalog?; Yes vcheck; Orbit packing finalized?; Yes vcheck; Buffer times optimized?; Yes vcheck; Verify visit grouping correct; Yes vcheck; phase constraint for ground based observations added?; N/A vcheck; BETWEENS for coordinated observations added?; Yes ... 01 OCT 2021 00:00 to 11 OCT 2021 08:10 and 12 OCT 2021 17:00 to 24 OCT 2021 04:15 and 25 OCT 2021 17:20 to 05 NOV 2021 21:10 vcheck; Is visit ready for int. review?; Yes Allocated COS orbits = 12 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 V-GM-AUR COS/NUV ACQ/PEA PSA G230L 2950 STRIPE=DEF 1 5.8 S (5.8 KXD S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC (COS.sa.1522537) in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/PEAKXD with PSA takes 5.8 seconds for S/N=40. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sa.1522540) in order to determine bright object safety. ACQ/PEAKXD with PSA has peak pixel rate of 5.943 counts per second and global rate of 2997.808, so it is safe. This is the first of two ACQ/PEAKXD+ACQ/PEAKD used in order to improve the likelihood of a successful acquisition. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [ 86] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 2 V-GM-AUR COS/NUV ACQ/PEA PSA G230L 2950 CENTER=FLUX-WT-FLR, NUM-POS=5, 1 5.3 S (5.3 KD STEP-SIZE=0.9 S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC (COS.sa.1522538) in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/PEAKD with PSA takes 5.3 seconds for S/N=40. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sa.1522541) in order to determine bright object safety. ACQ/PEAKD with PSA has peak pixel rate of 5.943 counts per second and global rate of 2997.808, so it is safe. This is the first of two ACQ/PEAKXD+ACQ/PEAKD used in order to improve the likelihood of a successful acquisition. ------------------------------------------------------------------------------------------------------------------------------------ 3 V-GM-AUR COS/NUV ACQ/PEA PSA G230L 2950 STRIPE=DEF 1 5.8 S (5.8 KXD S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC (COS.sa.1522537) in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/PEAKXD with PSA takes 5.8 seconds for S/N=40. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sa.1522540) in order to determine bright object safety. ACQ/PEAKXD with PSA has peak pixel rate of 5.943 counts per second and global rate of 2997.808, so it is safe. This is the second of two ACQ/PEAKXD+ACQ/PEAKD used in order to improve the likelihood of a successful acquisition. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [ 87] 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 V-GM-AUR COS/NUV ACQ/PEA PSA G230L 2950 CENTER=FLUX-WT-FLR, NUM-POS=5, 1 5.3 S (5.3 KD STEP-SIZE=0.9 S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC (COS.sa.1522538) in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/PEAKD with PSA takes 5.3 seconds for S/N=40. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sa.1522541) in order to determine bright object safety. ACQ/PEAKD with PSA has peak pixel rate of 5.943 counts per second and global rate of 2997.808, so it is safe. This is the second of two ACQ/PEAKXD+ACQ/PEAKD used in order to improve the likelihood of a successful acquisition. ------------------------------------------------------------------------------------------------------------------------------------ 5 V-GM-AUR COS/NUV TIME-TA PSA G230L 2950 FP-POS=4, BUFFER-TIME=524 1 184 S (184 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522552). 362.4388 seconds to achieve S/N = 20 at 2825 A. This time is halved (= 181.2194 seconds) to account for the other G230L cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522735) uses the expanded exposure time to fill the orbit (184 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is minimal. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522691) in order to determine bright object safety. Peak local rate of 5.943 counts per second and global rate of 2997.808, so it is safe. Buffer fill time = 786 seconds, and 2/3 of this is 524 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [ 88] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 6 V-GM-AUR COS/NUV TIME-TA PSA G230L 2635 FP-POS=1, BUFFER-TIME=448 1 184 S (184 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522553). 364.1707 seconds to achieve S/N = 20 at 2825 A. This time is halved (= 182.08535 seconds) to account for the other G230L cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522737) uses the expanded exposure time to fill the orbit (184 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is minimal. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522690) in order to determine bright object safety. Peak local rate of 5.927 counts per second and global rate of 2199.263, so it is safe. Buffer fill time = 672 seconds, and 2/3 of this is 448 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [ 89] 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 V-GM-AUR COS/FUV TIME-TA PSA G160M 1589 FP-POS=3, BUFFER-TIME=2865 1 186 S (186 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522544). 376.7304 seconds to achieve S/N = 30 at 1548.5 A. This time is quartered (= 94.1826 seconds) to account for both the other G160M cenwave and the two FP-POS settings per cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522739) uses the expanded exposure time to fill the orbit (186 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is significant compared to the G230L exposures. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522682) in order to determine bright object safety. Peak local rate of 0.315 counts per second and global rate of 548.875, so it is safe. Buffer fill time = 4297 seconds, and 2/3 of this is 2864.667 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [ 90] 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 V-GM-AUR COS/FUV TIME-TA PSA G160M 1589 FP-POS=4, BUFFER-TIME=2865 1 186 S (186 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522544). 376.7304 seconds to achieve S/N = 30 at 1548.5 A. This time is quartered (= 94.1826 seconds) to account for both the other G160M cenwave and the two FP-POS settings per cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522739) uses the expanded exposure time to fill the orbit (186 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is significant compared to the G230L exposures. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522682) in order to determine bright object safety. Peak local rate of 0.315 counts per second and global rate of 548.875, so it is safe. Buffer fill time = 4297 seconds, and 2/3 of this is 2864.667 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [ 91] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 9 V-GM-AUR COS/FUV TIME-TA PSA G160M 1623 FP-POS=1, BUFFER-TIME=3154 1 186 S (186 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522545). 393.2034 seconds to achieve S/N = 30 at 1548.5 A. This time is quartered (= 98.30085 seconds) to account for both the other G160M cenwave and the two FP-POS settings per cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522741) uses the expanded exposure time to fill the orbit (186 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is significant compared to the G230L exposures. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522683) in order to determine bright object safety. Peak local rate of 0.317 counts per second and global rate of 498.525, so it is safe. Buffer fill time = 4731 seconds, and 2/3 of this is 3154 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [ 92] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 10 V-GM-AUR COS/FUV TIME-TA PSA G160M 1623 FP-POS=2, BUFFER-TIME=3154 1 186 S (186 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522545). 393.2034 seconds to achieve S/N = 30 at 1548.5 A. This time is quartered (= 98.30085 seconds) to account for both the other G160M cenwave and the two FP-POS settings per cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522741) uses the expanded exposure time to fill the orbit (186 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is significant compared to the G230L exposures. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522683) in order to determine bright object safety. Peak local rate of 0.317 counts per second and global rate of 498.525, so it is safe. Buffer fill time = 4731 seconds, and 2/3 of this is 3154 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 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 | ------------------------------------------------------------------------------------------------------------------------------------ V-GM-AUR 1 COS/NUV ACQ/PEA PSA G230L 2950 none none none none 1 N/A KXD V-GM-AUR 2 COS/NUV ACQ/PEA PSA G230L 2950 none none none none 1 N/A KD V-GM-AUR 3 COS/NUV ACQ/PEA PSA G230L 2950 none none none none 1 N/A KXD V-GM-AUR 4 COS/NUV ACQ/PEA PSA G230L 2950 none none none none 1 N/A KD V-GM-AUR 5 COS/NUV TIME-TA PSA G230L 2950 none none none none 1 N/A G V-GM-AUR 6 COS/NUV TIME-TA PSA G230L 2635 none none none none 1 N/A G V-GM-AUR 7 COS/FUV TIME-TA PSA G160M 1589 none none none none 1 N/A G 16108( 6) - 02-Nov-2021 13:03:24 - [ 93] 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 | ------------------------------------------------------------------------------------------------------------------------------------ V-GM-AUR 8 COS/FUV TIME-TA PSA G160M 1589 none none none none 1 N/A G V-GM-AUR 9 COS/FUV TIME-TA PSA G160M 1623 none none none none 1 N/A G V-GM-AUR 10 COS/FUV TIME-TA PSA G160M 1623 none none none none 1 N/A G 16108( 6) - 02-Nov-2021 13:03:24 - [ 94] Visit: 1M (V-GM-AUR-COS-11) Visit Requirements: SCHED 100%; AFTER 1C BY 226.6 Orbits TO 234.8 Orbits; BETWEEN 01-OCT-2021:00:00:00 AND 11-OCT-2021:08:10:00; BETWEEN 12-OCT-2021:17:00:00 AND 24-OCT-2021:04:15:00; BETWEEN 25-OCT-2021:17:20:00 AND 05-NOV-2021:21:10:00 On Hold Comments: Additional Comments: vstatus; 1M; V-GM-AUR; P/COS approved for submission; P/AH 19/07/21 ; intrev: complete ; P/WF 19/07/21 vcheck; Enter targ name & Inst. & Resp. Sci.; GM Aur ; COS ; AH vcheck; ETC numbers entered in APT?; Yes vcheck; Any screening violations?; No vcheck; M-dwarf check complete and added to box folder?; N/A vcheck; S/N ETC calcs done & documented?; Yes vcheck; Field images checked & saved?; Yes ... located at: box/ullyses_tech/ullyses_proposals/monitor/16018/images/ vcheck; Selected ACQ strategy?; Double ACQ/PeakXD+ACQ/PeakD, G230L, S/N = 40 vcheck; Possible ACQ or Sci spoilers?; No vcheck; Field BOT clear?; Yes vcheck; Visual BOT check for stars not in catalog?; Yes vcheck; Orbit packing finalized?; Yes vcheck; Buffer times optimized?; Yes vcheck; Verify visit grouping correct; Yes vcheck; phase constraint for ground based observations added?; N/A vcheck; BETWEENS for coordinated observations added?; Yes ... 01 OCT 2021 00:00 to 11 OCT 2021 08:10 and 12 OCT 2021 17:00 to 24 OCT 2021 04:15 and 25 OCT 2021 17:20 to 05 NOV 2021 21:10 vcheck; Is visit ready for int. review?; Yes Allocated COS orbits = 12 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 V-GM-AUR COS/NUV ACQ/PEA PSA G230L 2950 STRIPE=DEF 1 5.8 S (5.8 KXD S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC (COS.sa.1522537) in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/PEAKXD with PSA takes 5.8 seconds for S/N=40. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sa.1522540) in order to determine bright object safety. ACQ/PEAKXD with PSA has peak pixel rate of 5.943 counts per second and global rate of 2997.808, so it is safe. This is the first of two ACQ/PEAKXD+ACQ/PEAKD used in order to improve the likelihood of a successful acquisition. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [ 95] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 2 V-GM-AUR COS/NUV ACQ/PEA PSA G230L 2950 CENTER=FLUX-WT-FLR, NUM-POS=5, 1 5.3 S (5.3 KD STEP-SIZE=0.9 S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC (COS.sa.1522538) in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/PEAKD with PSA takes 5.3 seconds for S/N=40. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sa.1522541) in order to determine bright object safety. ACQ/PEAKD with PSA has peak pixel rate of 5.943 counts per second and global rate of 2997.808, so it is safe. This is the first of two ACQ/PEAKXD+ACQ/PEAKD used in order to improve the likelihood of a successful acquisition. ------------------------------------------------------------------------------------------------------------------------------------ 3 V-GM-AUR COS/NUV ACQ/PEA PSA G230L 2950 STRIPE=DEF 1 5.8 S (5.8 KXD S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC (COS.sa.1522537) in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/PEAKXD with PSA takes 5.8 seconds for S/N=40. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sa.1522540) in order to determine bright object safety. ACQ/PEAKXD with PSA has peak pixel rate of 5.943 counts per second and global rate of 2997.808, so it is safe. This is the second of two ACQ/PEAKXD+ACQ/PEAKD used in order to improve the likelihood of a successful acquisition. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [ 96] 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 V-GM-AUR COS/NUV ACQ/PEA PSA G230L 2950 CENTER=FLUX-WT-FLR, NUM-POS=5, 1 5.3 S (5.3 KD STEP-SIZE=0.9 S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC (COS.sa.1522538) in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/PEAKD with PSA takes 5.3 seconds for S/N=40. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sa.1522541) in order to determine bright object safety. ACQ/PEAKD with PSA has peak pixel rate of 5.943 counts per second and global rate of 2997.808, so it is safe. This is the second of two ACQ/PEAKXD+ACQ/PEAKD used in order to improve the likelihood of a successful acquisition. ------------------------------------------------------------------------------------------------------------------------------------ 5 V-GM-AUR COS/NUV TIME-TA PSA G230L 2950 FP-POS=4, BUFFER-TIME=524 1 184 S (184 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522552). 362.4388 seconds to achieve S/N = 20 at 2825 A. This time is halved (= 181.2194 seconds) to account for the other G230L cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522735) uses the expanded exposure time to fill the orbit (184 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is minimal. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522691) in order to determine bright object safety. Peak local rate of 5.943 counts per second and global rate of 2997.808, so it is safe. Buffer fill time = 786 seconds, and 2/3 of this is 524 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [ 97] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 6 V-GM-AUR COS/NUV TIME-TA PSA G230L 2635 FP-POS=1, BUFFER-TIME=448 1 184 S (184 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522553). 364.1707 seconds to achieve S/N = 20 at 2825 A. This time is halved (= 182.08535 seconds) to account for the other G230L cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522737) uses the expanded exposure time to fill the orbit (184 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is minimal. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522690) in order to determine bright object safety. Peak local rate of 5.927 counts per second and global rate of 2199.263, so it is safe. Buffer fill time = 672 seconds, and 2/3 of this is 448 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [ 98] 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 V-GM-AUR COS/FUV TIME-TA PSA G160M 1589 FP-POS=3, BUFFER-TIME=2865 1 186 S (186 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522544). 376.7304 seconds to achieve S/N = 30 at 1548.5 A. This time is quartered (= 94.1826 seconds) to account for both the other G160M cenwave and the two FP-POS settings per cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522739) uses the expanded exposure time to fill the orbit (186 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is significant compared to the G230L exposures. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522682) in order to determine bright object safety. Peak local rate of 0.315 counts per second and global rate of 548.875, so it is safe. Buffer fill time = 4297 seconds, and 2/3 of this is 2864.667 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [ 99] 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 V-GM-AUR COS/FUV TIME-TA PSA G160M 1589 FP-POS=4, BUFFER-TIME=2865 1 186 S (186 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522544). 376.7304 seconds to achieve S/N = 30 at 1548.5 A. This time is quartered (= 94.1826 seconds) to account for both the other G160M cenwave and the two FP-POS settings per cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522739) uses the expanded exposure time to fill the orbit (186 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is significant compared to the G230L exposures. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522682) in order to determine bright object safety. Peak local rate of 0.315 counts per second and global rate of 548.875, so it is safe. Buffer fill time = 4297 seconds, and 2/3 of this is 2864.667 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [100] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 9 V-GM-AUR COS/FUV TIME-TA PSA G160M 1623 FP-POS=1, BUFFER-TIME=3154 1 186 S (186 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522545). 393.2034 seconds to achieve S/N = 30 at 1548.5 A. This time is quartered (= 98.30085 seconds) to account for both the other G160M cenwave and the two FP-POS settings per cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522741) uses the expanded exposure time to fill the orbit (186 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is significant compared to the G230L exposures. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522683) in order to determine bright object safety. Peak local rate of 0.317 counts per second and global rate of 498.525, so it is safe. Buffer fill time = 4731 seconds, and 2/3 of this is 3154 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [101] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 10 V-GM-AUR COS/FUV TIME-TA PSA G160M 1623 FP-POS=2, BUFFER-TIME=3154 1 186 S (186 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522545). 393.2034 seconds to achieve S/N = 30 at 1548.5 A. This time is quartered (= 98.30085 seconds) to account for both the other G160M cenwave and the two FP-POS settings per cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522741) uses the expanded exposure time to fill the orbit (186 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is significant compared to the G230L exposures. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522683) in order to determine bright object safety. Peak local rate of 0.317 counts per second and global rate of 498.525, so it is safe. Buffer fill time = 4731 seconds, and 2/3 of this is 3154 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 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 | ------------------------------------------------------------------------------------------------------------------------------------ V-GM-AUR 1 COS/NUV ACQ/PEA PSA G230L 2950 none none none none 1 N/A KXD V-GM-AUR 2 COS/NUV ACQ/PEA PSA G230L 2950 none none none none 1 N/A KD V-GM-AUR 3 COS/NUV ACQ/PEA PSA G230L 2950 none none none none 1 N/A KXD V-GM-AUR 4 COS/NUV ACQ/PEA PSA G230L 2950 none none none none 1 N/A KD V-GM-AUR 5 COS/NUV TIME-TA PSA G230L 2950 none none none none 1 N/A G V-GM-AUR 6 COS/NUV TIME-TA PSA G230L 2635 none none none none 1 N/A G V-GM-AUR 7 COS/FUV TIME-TA PSA G160M 1589 none none none none 1 N/A G 16108( 6) - 02-Nov-2021 13:03:24 - [102] 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 | ------------------------------------------------------------------------------------------------------------------------------------ V-GM-AUR 8 COS/FUV TIME-TA PSA G160M 1589 none none none none 1 N/A G V-GM-AUR 9 COS/FUV TIME-TA PSA G160M 1623 none none none none 1 N/A G V-GM-AUR 10 COS/FUV TIME-TA PSA G160M 1623 none none none none 1 N/A G 16108( 6) - 02-Nov-2021 13:03:24 - [103] Visit: 1N (V-GM-AUR-COS-12) Visit Requirements: SCHED 100%; AFTER 1C BY 249.6 Orbits TO 257.8 Orbits; BETWEEN 01-OCT-2021:00:00:00 AND 11-OCT-2021:08:10:00; BETWEEN 12-OCT-2021:17:00:00 AND 24-OCT-2021:04:15:00; BETWEEN 25-OCT-2021:17:20:00 AND 05-NOV-2021:21:10:00 On Hold Comments: Additional Comments: vstatus; 1N; V-GM-AUR; P/COS approved for submission; P/AH 19/07/21 ; intrev: complete ; P/WF 19/07/21 vcheck; Enter targ name & Inst. & Resp. Sci.; GM Aur ; COS ; AH vcheck; ETC numbers entered in APT?; Yes vcheck; Any screening violations?; No vcheck; M-dwarf check complete and added to box folder?; N/A vcheck; S/N ETC calcs done & documented?; Yes vcheck; Field images checked & saved?; Yes ... located at: box/ullyses_tech/ullyses_proposals/monitor/16018/images/ vcheck; Selected ACQ strategy?; Double ACQ/PeakXD+ACQ/PeakD, G230L, S/N = 40 vcheck; Possible ACQ or Sci spoilers?; No vcheck; Field BOT clear?; Yes vcheck; Visual BOT check for stars not in catalog?; Yes vcheck; Orbit packing finalized?; Yes vcheck; Buffer times optimized?; Yes vcheck; Verify visit grouping correct; Yes vcheck; phase constraint for ground based observations added?; N/A vcheck; BETWEENS for coordinated observations added?; Yes ... 01 OCT 2021 00:00 to 11 OCT 2021 08:10 and 12 OCT 2021 17:00 to 24 OCT 2021 04:15 and 25 OCT 2021 17:20 to 05 NOV 2021 21:10 vcheck; Is visit ready for int. review?; Yes Allocated COS orbits = 12 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 V-GM-AUR COS/NUV ACQ/PEA PSA G230L 2950 STRIPE=DEF 1 5.8 S (5.8 KXD S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC (COS.sa.1522537) in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/PEAKXD with PSA takes 5.8 seconds for S/N=40. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sa.1522540) in order to determine bright object safety. ACQ/PEAKXD with PSA has peak pixel rate of 5.943 counts per second and global rate of 2997.808, so it is safe. This is the first of two ACQ/PEAKXD+ACQ/PEAKD used in order to improve the likelihood of a successful acquisition. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [104] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 2 V-GM-AUR COS/NUV ACQ/PEA PSA G230L 2950 CENTER=FLUX-WT-FLR, NUM-POS=5, 1 5.3 S (5.3 KD STEP-SIZE=0.9 S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC (COS.sa.1522538) in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/PEAKD with PSA takes 5.3 seconds for S/N=40. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sa.1522541) in order to determine bright object safety. ACQ/PEAKD with PSA has peak pixel rate of 5.943 counts per second and global rate of 2997.808, so it is safe. This is the first of two ACQ/PEAKXD+ACQ/PEAKD used in order to improve the likelihood of a successful acquisition. ------------------------------------------------------------------------------------------------------------------------------------ 3 V-GM-AUR COS/NUV ACQ/PEA PSA G230L 2950 STRIPE=DEF 1 5.8 S (5.8 KXD S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC (COS.sa.1522537) in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/PEAKXD with PSA takes 5.8 seconds for S/N=40. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sa.1522540) in order to determine bright object safety. ACQ/PEAKXD with PSA has peak pixel rate of 5.943 counts per second and global rate of 2997.808, so it is safe. This is the second of two ACQ/PEAKXD+ACQ/PEAKD used in order to improve the likelihood of a successful acquisition. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [105] 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 V-GM-AUR COS/NUV ACQ/PEA PSA G230L 2950 CENTER=FLUX-WT-FLR, NUM-POS=5, 1 5.3 S (5.3 KD STEP-SIZE=0.9 S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC (COS.sa.1522538) in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/PEAKD with PSA takes 5.3 seconds for S/N=40. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sa.1522541) in order to determine bright object safety. ACQ/PEAKD with PSA has peak pixel rate of 5.943 counts per second and global rate of 2997.808, so it is safe. This is the second of two ACQ/PEAKXD+ACQ/PEAKD used in order to improve the likelihood of a successful acquisition. ------------------------------------------------------------------------------------------------------------------------------------ 5 V-GM-AUR COS/NUV TIME-TA PSA G230L 2950 FP-POS=4, BUFFER-TIME=524 1 184 S (184 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522552). 362.4388 seconds to achieve S/N = 20 at 2825 A. This time is halved (= 181.2194 seconds) to account for the other G230L cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522735) uses the expanded exposure time to fill the orbit (184 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is minimal. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522691) in order to determine bright object safety. Peak local rate of 5.943 counts per second and global rate of 2997.808, so it is safe. Buffer fill time = 786 seconds, and 2/3 of this is 524 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [106] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 6 V-GM-AUR COS/NUV TIME-TA PSA G230L 2635 FP-POS=1, BUFFER-TIME=448 1 184 S (184 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522553). 364.1707 seconds to achieve S/N = 20 at 2825 A. This time is halved (= 182.08535 seconds) to account for the other G230L cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522737) uses the expanded exposure time to fill the orbit (184 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is minimal. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522690) in order to determine bright object safety. Peak local rate of 5.927 counts per second and global rate of 2199.263, so it is safe. Buffer fill time = 672 seconds, and 2/3 of this is 448 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [107] 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 V-GM-AUR COS/FUV TIME-TA PSA G160M 1589 FP-POS=3, BUFFER-TIME=2865 1 186 S (186 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522544). 376.7304 seconds to achieve S/N = 30 at 1548.5 A. This time is quartered (= 94.1826 seconds) to account for both the other G160M cenwave and the two FP-POS settings per cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522739) uses the expanded exposure time to fill the orbit (186 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is significant compared to the G230L exposures. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522682) in order to determine bright object safety. Peak local rate of 0.315 counts per second and global rate of 548.875, so it is safe. Buffer fill time = 4297 seconds, and 2/3 of this is 2864.667 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [108] 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 V-GM-AUR COS/FUV TIME-TA PSA G160M 1589 FP-POS=4, BUFFER-TIME=2865 1 186 S (186 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522544). 376.7304 seconds to achieve S/N = 30 at 1548.5 A. This time is quartered (= 94.1826 seconds) to account for both the other G160M cenwave and the two FP-POS settings per cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522739) uses the expanded exposure time to fill the orbit (186 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is significant compared to the G230L exposures. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522682) in order to determine bright object safety. Peak local rate of 0.315 counts per second and global rate of 548.875, so it is safe. Buffer fill time = 4297 seconds, and 2/3 of this is 2864.667 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [109] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 9 V-GM-AUR COS/FUV TIME-TA PSA G160M 1623 FP-POS=1, BUFFER-TIME=3154 1 186 S (186 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522545). 393.2034 seconds to achieve S/N = 30 at 1548.5 A. This time is quartered (= 98.30085 seconds) to account for both the other G160M cenwave and the two FP-POS settings per cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522741) uses the expanded exposure time to fill the orbit (186 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is significant compared to the G230L exposures. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522683) in order to determine bright object safety. Peak local rate of 0.317 counts per second and global rate of 498.525, so it is safe. Buffer fill time = 4731 seconds, and 2/3 of this is 3154 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [110] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 10 V-GM-AUR COS/FUV TIME-TA PSA G160M 1623 FP-POS=2, BUFFER-TIME=3154 1 186 S (186 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522545). 393.2034 seconds to achieve S/N = 30 at 1548.5 A. This time is quartered (= 98.30085 seconds) to account for both the other G160M cenwave and the two FP-POS settings per cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522741) uses the expanded exposure time to fill the orbit (186 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is significant compared to the G230L exposures. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522683) in order to determine bright object safety. Peak local rate of 0.317 counts per second and global rate of 498.525, so it is safe. Buffer fill time = 4731 seconds, and 2/3 of this is 3154 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 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 | ------------------------------------------------------------------------------------------------------------------------------------ V-GM-AUR 1 COS/NUV ACQ/PEA PSA G230L 2950 none none none none 1 N/A KXD V-GM-AUR 2 COS/NUV ACQ/PEA PSA G230L 2950 none none none none 1 N/A KD V-GM-AUR 3 COS/NUV ACQ/PEA PSA G230L 2950 none none none none 1 N/A KXD V-GM-AUR 4 COS/NUV ACQ/PEA PSA G230L 2950 none none none none 1 N/A KD V-GM-AUR 5 COS/NUV TIME-TA PSA G230L 2950 none none none none 1 N/A G V-GM-AUR 6 COS/NUV TIME-TA PSA G230L 2635 none none none none 1 N/A G V-GM-AUR 7 COS/FUV TIME-TA PSA G160M 1589 none none none none 1 N/A G 16108( 6) - 02-Nov-2021 13:03:24 - [111] 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 | ------------------------------------------------------------------------------------------------------------------------------------ V-GM-AUR 8 COS/FUV TIME-TA PSA G160M 1589 none none none none 1 N/A G V-GM-AUR 9 COS/FUV TIME-TA PSA G160M 1623 none none none none 1 N/A G V-GM-AUR 10 COS/FUV TIME-TA PSA G160M 1623 none none none none 1 N/A G 16108( 6) - 02-Nov-2021 13:03:24 - [112] Visit: AJ (V-GM-AUR-COS-8) Visit Requirements: SCHED 100%; BETWEEN 25-OCT-2021:17:20:00 AND 15-DEC-2021:21:10:00 On Hold Comments: Additional Comments: vstatus; 1J; V-GM-AUR; P/COS approved for submission; P/AH 19/07/21 ; intrev: complete ; P/WF 19/07/21 vcheck; Enter targ name & Inst. & Resp. Sci.; GM Aur ; COS ; AH vcheck; ETC numbers entered in APT?; Yes vcheck; Any screening violations?; No vcheck; M-dwarf check complete and added to box folder?; N/A vcheck; S/N ETC calcs done & documented?; Yes vcheck; Field images checked & saved?; Yes ... located at: box/ullyses_tech/ullyses_proposals/monitor/16018/images/ vcheck; Selected ACQ strategy?; Double ACQ/PeakXD+ACQ/PeakD, G230L, S/N = 40 vcheck; Possible ACQ or Sci spoilers?; No vcheck; Field BOT clear?; Yes vcheck; Visual BOT check for stars not in catalog?; Yes vcheck; Orbit packing finalized?; Yes vcheck; Buffer times optimized?; Yes vcheck; Verify visit grouping correct; Yes vcheck; phase constraint for ground based observations added?; N/A vcheck; BETWEENS for coordinated observations added?; Yes ... 01 OCT 2021 00:00 to 11 OCT 2021 08:10 and 12 OCT 2021 17:00 to 24 OCT 2021 04:15 and 25 OCT 2021 17:20 to 05 NOV 2021 21:10 vcheck; Is visit ready for int. review?; Yes Allocated COS orbits = 12 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 V-GM-AUR COS/NUV ACQ/PEA PSA G230L 2950 STRIPE=DEF 1 5.8 S (5.8 KXD S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC (COS.sa.1522537) in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/PEAKXD with PSA takes 5.8 seconds for S/N=40. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sa.1522540) in order to determine bright object safety. ACQ/PEAKXD with PSA has peak pixel rate of 5.943 counts per second and global rate of 2997.808, so it is safe. This is the first of two ACQ/PEAKXD+ACQ/PEAKD used in order to improve the likelihood of a successful acquisition. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [113] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 2 V-GM-AUR COS/NUV ACQ/PEA PSA G230L 2950 CENTER=FLUX-WT-FLR, NUM-POS=5, 1 5.3 S (5.3 KD STEP-SIZE=0.9 S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC (COS.sa.1522538) in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/PEAKD with PSA takes 5.3 seconds for S/N=40. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sa.1522541) in order to determine bright object safety. ACQ/PEAKD with PSA has peak pixel rate of 5.943 counts per second and global rate of 2997.808, so it is safe. This is the first of two ACQ/PEAKXD+ACQ/PEAKD used in order to improve the likelihood of a successful acquisition. ------------------------------------------------------------------------------------------------------------------------------------ 3 V-GM-AUR COS/NUV ACQ/PEA PSA G230L 2950 STRIPE=DEF 1 5.8 S (5.8 KXD S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC (COS.sa.1522537) in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/PEAKXD with PSA takes 5.8 seconds for S/N=40. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sa.1522540) in order to determine bright object safety. ACQ/PEAKXD with PSA has peak pixel rate of 5.943 counts per second and global rate of 2997.808, so it is safe. This is the second of two ACQ/PEAKXD+ACQ/PEAKD used in order to improve the likelihood of a successful acquisition. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [114] 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 V-GM-AUR COS/NUV ACQ/PEA PSA G230L 2950 CENTER=FLUX-WT-FLR, NUM-POS=5, 1 5.3 S (5.3 KD STEP-SIZE=0.9 S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC (COS.sa.1522538) in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/PEAKD with PSA takes 5.3 seconds for S/N=40. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sa.1522541) in order to determine bright object safety. ACQ/PEAKD with PSA has peak pixel rate of 5.943 counts per second and global rate of 2997.808, so it is safe. This is the second of two ACQ/PEAKXD+ACQ/PEAKD used in order to improve the likelihood of a successful acquisition. ------------------------------------------------------------------------------------------------------------------------------------ 5 V-GM-AUR COS/NUV TIME-TA PSA G230L 2950 FP-POS=4, BUFFER-TIME=524 1 50 S (50 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522552). 362.4388 seconds to achieve S/N = 20 at 2825 A. This time is halved (= 181.2194 seconds) to account for the other G230L cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522735) uses the expanded exposure time to fill the orbit (184 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is minimal. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522691) in order to determine bright object safety. Peak local rate of 5.943 counts per second and global rate of 2997.808, so it is safe. Buffer fill time = 786 seconds, and 2/3 of this is 524 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [115] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 6 V-GM-AUR COS/NUV TIME-TA PSA G230L 2635 FP-POS=1, BUFFER-TIME=448 1 50 S (50 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522553). 364.1707 seconds to achieve S/N = 20 at 2825 A. This time is halved (= 182.08535 seconds) to account for the other G230L cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522737) uses the expanded exposure time to fill the orbit (184 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is minimal. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522690) in order to determine bright object safety. Peak local rate of 5.927 counts per second and global rate of 2199.263, so it is safe. Buffer fill time = 672 seconds, and 2/3 of this is 448 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [116] 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 V-GM-AUR COS/FUV TIME-TA PSA G160M 1589 FP-POS=3, BUFFER-TIME=2865 1 265 S (265 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522544). 376.7304 seconds to achieve S/N = 30 at 1548.5 A. This time is quartered (= 94.1826 seconds) to account for both the other G160M cenwave and the two FP-POS settings per cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522739) uses the expanded exposure time to fill the orbit (186 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is significant compared to the G230L exposures. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522682) in order to determine bright object safety. Peak local rate of 0.315 counts per second and global rate of 548.875, so it is safe. Buffer fill time = 4297 seconds, and 2/3 of this is 2864.667 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [117] 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 V-GM-AUR COS/FUV TIME-TA PSA G160M 1589 FP-POS=4, BUFFER-TIME=2865 1 265 S (265 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522544). 376.7304 seconds to achieve S/N = 30 at 1548.5 A. This time is quartered (= 94.1826 seconds) to account for both the other G160M cenwave and the two FP-POS settings per cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522739) uses the expanded exposure time to fill the orbit (186 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is significant compared to the G230L exposures. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522682) in order to determine bright object safety. Peak local rate of 0.315 counts per second and global rate of 548.875, so it is safe. Buffer fill time = 4297 seconds, and 2/3 of this is 2864.667 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [118] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 9 V-GM-AUR COS/FUV TIME-TA PSA G160M 1623 FP-POS=1, BUFFER-TIME=3154 1 265 S (265 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522545). 393.2034 seconds to achieve S/N = 30 at 1548.5 A. This time is quartered (= 98.30085 seconds) to account for both the other G160M cenwave and the two FP-POS settings per cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522741) uses the expanded exposure time to fill the orbit (186 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is significant compared to the G230L exposures. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522683) in order to determine bright object safety. Peak local rate of 0.317 counts per second and global rate of 498.525, so it is safe. Buffer fill time = 4731 seconds, and 2/3 of this is 3154 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [119] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 10 V-GM-AUR COS/FUV TIME-TA PSA G160M 1623 FP-POS=2, BUFFER-TIME=3154 1 265 S (265 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522545). 393.2034 seconds to achieve S/N = 30 at 1548.5 A. This time is quartered (= 98.30085 seconds) to account for both the other G160M cenwave and the two FP-POS settings per cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522741) uses the expanded exposure time to fill the orbit (186 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is significant compared to the G230L exposures. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522683) in order to determine bright object safety. Peak local rate of 0.317 counts per second and global rate of 498.525, so it is safe. Buffer fill time = 4731 seconds, and 2/3 of this is 3154 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 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 | ------------------------------------------------------------------------------------------------------------------------------------ V-GM-AUR 1 COS/NUV ACQ/PEA PSA G230L 2950 none none none none 1 N/A KXD V-GM-AUR 2 COS/NUV ACQ/PEA PSA G230L 2950 none none none none 1 N/A KD V-GM-AUR 3 COS/NUV ACQ/PEA PSA G230L 2950 none none none none 1 N/A KXD V-GM-AUR 4 COS/NUV ACQ/PEA PSA G230L 2950 none none none none 1 N/A KD V-GM-AUR 5 COS/NUV TIME-TA PSA G230L 2950 none none none none 1 N/A G V-GM-AUR 6 COS/NUV TIME-TA PSA G230L 2635 none none none none 1 N/A G V-GM-AUR 7 COS/FUV TIME-TA PSA G160M 1589 none none none none 1 N/A G 16108( 6) - 02-Nov-2021 13:03:24 - [120] 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 | ------------------------------------------------------------------------------------------------------------------------------------ V-GM-AUR 8 COS/FUV TIME-TA PSA G160M 1589 none none none none 1 N/A G V-GM-AUR 9 COS/FUV TIME-TA PSA G160M 1623 none none none none 1 N/A G V-GM-AUR 10 COS/FUV TIME-TA PSA G160M 1623 none none none none 1 N/A G 16108( 6) - 02-Nov-2021 13:03:24 - [121] Visit: AK (V-GM-AUR-COS-9) Visit Requirements: SCHED 100%; AFTER AJ BY 19 Orbits TO 27.2 Orbits; BETWEEN 25-OCT-2021:17:20:00 AND 15-DEC-2021:21:10:00 On Hold Comments: Additional Comments: vstatus; 1K; V-GM-AUR; P/COS approved for submission; P/AH 19/07/21 ; intrev: complete ; P/WF 19/07/21 vcheck; Enter targ name & Inst. & Resp. Sci.; GM Aur ; COS ; AH vcheck; ETC numbers entered in APT?; Yes vcheck; Any screening violations?; No vcheck; M-dwarf check complete and added to box folder?; N/A vcheck; S/N ETC calcs done & documented?; Yes vcheck; Field images checked & saved?; Yes ... located at: box/ullyses_tech/ullyses_proposals/monitor/16018/images/ vcheck; Selected ACQ strategy?; Double ACQ/PeakXD+ACQ/PeakD, G230L, S/N = 40 vcheck; Possible ACQ or Sci spoilers?; No vcheck; Field BOT clear?; Yes vcheck; Visual BOT check for stars not in catalog?; Yes vcheck; Orbit packing finalized?; Yes vcheck; Buffer times optimized?; Yes vcheck; Verify visit grouping correct; Yes vcheck; phase constraint for ground based observations added?; N/A vcheck; BETWEENS for coordinated observations added?; Yes ... 01 OCT 2021 00:00 to 11 OCT 2021 08:10 and 12 OCT 2021 17:00 to 24 OCT 2021 04:15 and 25 OCT 2021 17:20 to 05 NOV 2021 21:10 vcheck; Is visit ready for int. review?; Yes Allocated COS orbits = 12 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 V-GM-AUR COS/NUV ACQ/PEA PSA G230L 2950 STRIPE=DEF 1 5.8 S (5.8 KXD S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC (COS.sa.1522537) in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/PEAKXD with PSA takes 5.8 seconds for S/N=40. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sa.1522540) in order to determine bright object safety. ACQ/PEAKXD with PSA has peak pixel rate of 5.943 counts per second and global rate of 2997.808, so it is safe. This is the first of two ACQ/PEAKXD+ACQ/PEAKD used in order to improve the likelihood of a successful acquisition. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [122] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 2 V-GM-AUR COS/NUV ACQ/PEA PSA G230L 2950 CENTER=FLUX-WT-FLR, NUM-POS=5, 1 5.3 S (5.3 KD STEP-SIZE=0.9 S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC (COS.sa.1522538) in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/PEAKD with PSA takes 5.3 seconds for S/N=40. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sa.1522541) in order to determine bright object safety. ACQ/PEAKD with PSA has peak pixel rate of 5.943 counts per second and global rate of 2997.808, so it is safe. This is the first of two ACQ/PEAKXD+ACQ/PEAKD used in order to improve the likelihood of a successful acquisition. ------------------------------------------------------------------------------------------------------------------------------------ 3 V-GM-AUR COS/NUV ACQ/PEA PSA G230L 2950 STRIPE=DEF 1 5.8 S (5.8 KXD S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC (COS.sa.1522537) in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/PEAKXD with PSA takes 5.8 seconds for S/N=40. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sa.1522540) in order to determine bright object safety. ACQ/PEAKXD with PSA has peak pixel rate of 5.943 counts per second and global rate of 2997.808, so it is safe. This is the second of two ACQ/PEAKXD+ACQ/PEAKD used in order to improve the likelihood of a successful acquisition. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [123] 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 V-GM-AUR COS/NUV ACQ/PEA PSA G230L 2950 CENTER=FLUX-WT-FLR, NUM-POS=5, 1 5.3 S (5.3 KD STEP-SIZE=0.9 S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC (COS.sa.1522538) in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/PEAKD with PSA takes 5.3 seconds for S/N=40. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sa.1522541) in order to determine bright object safety. ACQ/PEAKD with PSA has peak pixel rate of 5.943 counts per second and global rate of 2997.808, so it is safe. This is the second of two ACQ/PEAKXD+ACQ/PEAKD used in order to improve the likelihood of a successful acquisition. ------------------------------------------------------------------------------------------------------------------------------------ 5 V-GM-AUR COS/NUV TIME-TA PSA G230L 2950 FP-POS=4, BUFFER-TIME=524 1 50 S (50 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522552). 362.4388 seconds to achieve S/N = 20 at 2825 A. This time is halved (= 181.2194 seconds) to account for the other G230L cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522735) uses the expanded exposure time to fill the orbit (184 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is minimal. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522691) in order to determine bright object safety. Peak local rate of 5.943 counts per second and global rate of 2997.808, so it is safe. Buffer fill time = 786 seconds, and 2/3 of this is 524 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [124] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 6 V-GM-AUR COS/NUV TIME-TA PSA G230L 2635 FP-POS=1, BUFFER-TIME=448 1 50 S (50 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522553). 364.1707 seconds to achieve S/N = 20 at 2825 A. This time is halved (= 182.08535 seconds) to account for the other G230L cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522737) uses the expanded exposure time to fill the orbit (184 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is minimal. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522690) in order to determine bright object safety. Peak local rate of 5.927 counts per second and global rate of 2199.263, so it is safe. Buffer fill time = 672 seconds, and 2/3 of this is 448 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [125] 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 V-GM-AUR COS/FUV TIME-TA PSA G160M 1589 FP-POS=3, BUFFER-TIME=2865 1 265 S (265 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522544). 376.7304 seconds to achieve S/N = 30 at 1548.5 A. This time is quartered (= 94.1826 seconds) to account for both the other G160M cenwave and the two FP-POS settings per cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522739) uses the expanded exposure time to fill the orbit (186 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is significant compared to the G230L exposures. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522682) in order to determine bright object safety. Peak local rate of 0.315 counts per second and global rate of 548.875, so it is safe. Buffer fill time = 4297 seconds, and 2/3 of this is 2864.667 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [126] 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 V-GM-AUR COS/FUV TIME-TA PSA G160M 1589 FP-POS=4, BUFFER-TIME=2865 1 265 S (265 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522544). 376.7304 seconds to achieve S/N = 30 at 1548.5 A. This time is quartered (= 94.1826 seconds) to account for both the other G160M cenwave and the two FP-POS settings per cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522739) uses the expanded exposure time to fill the orbit (186 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is significant compared to the G230L exposures. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522682) in order to determine bright object safety. Peak local rate of 0.315 counts per second and global rate of 548.875, so it is safe. Buffer fill time = 4297 seconds, and 2/3 of this is 2864.667 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [127] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 9 V-GM-AUR COS/FUV TIME-TA PSA G160M 1623 FP-POS=1, BUFFER-TIME=3154 1 265 S (265 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522545). 393.2034 seconds to achieve S/N = 30 at 1548.5 A. This time is quartered (= 98.30085 seconds) to account for both the other G160M cenwave and the two FP-POS settings per cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522741) uses the expanded exposure time to fill the orbit (186 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is significant compared to the G230L exposures. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522683) in order to determine bright object safety. Peak local rate of 0.317 counts per second and global rate of 498.525, so it is safe. Buffer fill time = 4731 seconds, and 2/3 of this is 3154 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [128] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 10 V-GM-AUR COS/FUV TIME-TA PSA G160M 1623 FP-POS=2, BUFFER-TIME=3154 1 265 S (265 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522545). 393.2034 seconds to achieve S/N = 30 at 1548.5 A. This time is quartered (= 98.30085 seconds) to account for both the other G160M cenwave and the two FP-POS settings per cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522741) uses the expanded exposure time to fill the orbit (186 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is significant compared to the G230L exposures. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522683) in order to determine bright object safety. Peak local rate of 0.317 counts per second and global rate of 498.525, so it is safe. Buffer fill time = 4731 seconds, and 2/3 of this is 3154 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 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 | ------------------------------------------------------------------------------------------------------------------------------------ V-GM-AUR 1 COS/NUV ACQ/PEA PSA G230L 2950 none none none none 1 N/A KXD V-GM-AUR 2 COS/NUV ACQ/PEA PSA G230L 2950 none none none none 1 N/A KD V-GM-AUR 3 COS/NUV ACQ/PEA PSA G230L 2950 none none none none 1 N/A KXD V-GM-AUR 4 COS/NUV ACQ/PEA PSA G230L 2950 none none none none 1 N/A KD V-GM-AUR 5 COS/NUV TIME-TA PSA G230L 2950 none none none none 1 N/A G V-GM-AUR 6 COS/NUV TIME-TA PSA G230L 2635 none none none none 1 N/A G V-GM-AUR 7 COS/FUV TIME-TA PSA G160M 1589 none none none none 1 N/A G 16108( 6) - 02-Nov-2021 13:03:24 - [129] 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 | ------------------------------------------------------------------------------------------------------------------------------------ V-GM-AUR 8 COS/FUV TIME-TA PSA G160M 1589 none none none none 1 N/A G V-GM-AUR 9 COS/FUV TIME-TA PSA G160M 1623 none none none none 1 N/A G V-GM-AUR 10 COS/FUV TIME-TA PSA G160M 1623 none none none none 1 N/A G 16108( 6) - 02-Nov-2021 13:03:24 - [130] Visit: AL (V-GM-AUR-COS-10) Visit Requirements: SCHED 100%; AFTER AJ BY 42 Orbits TO 50.2 Orbits; BETWEEN 25-OCT-2021:17:20:00 AND 15-DEC-2021:21:10:00 On Hold Comments: Additional Comments: vstatus; 1L; V-GM-AUR; P/COS approved for submission; P/AH 19/07/21 ; intrev: complete ; P/WF 19/07/21 vcheck; Enter targ name & Inst. & Resp. Sci.; GM Aur ; COS ; AH vcheck; ETC numbers entered in APT?; Yes vcheck; Any screening violations?; No vcheck; M-dwarf check complete and added to box folder?; N/A vcheck; S/N ETC calcs done & documented?; Yes vcheck; Field images checked & saved?; Yes ... located at: box/ullyses_tech/ullyses_proposals/monitor/16018/images/ vcheck; Selected ACQ strategy?; Double ACQ/PeakXD+ACQ/PeakD, G230L, S/N = 40 vcheck; Possible ACQ or Sci spoilers?; No vcheck; Field BOT clear?; Yes vcheck; Visual BOT check for stars not in catalog?; Yes vcheck; Orbit packing finalized?; Yes vcheck; Buffer times optimized?; Yes vcheck; Verify visit grouping correct; Yes vcheck; phase constraint for ground based observations added?; N/A vcheck; BETWEENS for coordinated observations added?; Yes ... 01 OCT 2021 00:00 to 11 OCT 2021 08:10 and 12 OCT 2021 17:00 to 24 OCT 2021 04:15 and 25 OCT 2021 17:20 to 05 NOV 2021 21:10 vcheck; Is visit ready for int. review?; Yes Allocated COS orbits = 12 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 V-GM-AUR COS/NUV ACQ/PEA PSA G230L 2950 STRIPE=DEF 1 5.8 S (5.8 KXD S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC (COS.sa.1522537) in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/PEAKXD with PSA takes 5.8 seconds for S/N=40. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sa.1522540) in order to determine bright object safety. ACQ/PEAKXD with PSA has peak pixel rate of 5.943 counts per second and global rate of 2997.808, so it is safe. This is the first of two ACQ/PEAKXD+ACQ/PEAKD used in order to improve the likelihood of a successful acquisition. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [131] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 2 V-GM-AUR COS/NUV ACQ/PEA PSA G230L 2950 CENTER=FLUX-WT-FLR, NUM-POS=5, 1 5.3 S (5.3 KD STEP-SIZE=0.9 S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC (COS.sa.1522538) in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/PEAKD with PSA takes 5.3 seconds for S/N=40. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sa.1522541) in order to determine bright object safety. ACQ/PEAKD with PSA has peak pixel rate of 5.943 counts per second and global rate of 2997.808, so it is safe. This is the first of two ACQ/PEAKXD+ACQ/PEAKD used in order to improve the likelihood of a successful acquisition. ------------------------------------------------------------------------------------------------------------------------------------ 3 V-GM-AUR COS/NUV ACQ/PEA PSA G230L 2950 STRIPE=DEF 1 5.8 S (5.8 KXD S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC (COS.sa.1522537) in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/PEAKXD with PSA takes 5.8 seconds for S/N=40. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sa.1522540) in order to determine bright object safety. ACQ/PEAKXD with PSA has peak pixel rate of 5.943 counts per second and global rate of 2997.808, so it is safe. This is the second of two ACQ/PEAKXD+ACQ/PEAKD used in order to improve the likelihood of a successful acquisition. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [132] 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 V-GM-AUR COS/NUV ACQ/PEA PSA G230L 2950 CENTER=FLUX-WT-FLR, NUM-POS=5, 1 5.3 S (5.3 KD STEP-SIZE=0.9 S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC (COS.sa.1522538) in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/PEAKD with PSA takes 5.3 seconds for S/N=40. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sa.1522541) in order to determine bright object safety. ACQ/PEAKD with PSA has peak pixel rate of 5.943 counts per second and global rate of 2997.808, so it is safe. This is the second of two ACQ/PEAKXD+ACQ/PEAKD used in order to improve the likelihood of a successful acquisition. ------------------------------------------------------------------------------------------------------------------------------------ 5 V-GM-AUR COS/NUV TIME-TA PSA G230L 2950 FP-POS=4, BUFFER-TIME=524 1 50 S (50 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522552). 362.4388 seconds to achieve S/N = 20 at 2825 A. This time is halved (= 181.2194 seconds) to account for the other G230L cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522735) uses the expanded exposure time to fill the orbit (184 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is minimal. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522691) in order to determine bright object safety. Peak local rate of 5.943 counts per second and global rate of 2997.808, so it is safe. Buffer fill time = 786 seconds, and 2/3 of this is 524 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [133] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 6 V-GM-AUR COS/NUV TIME-TA PSA G230L 2635 FP-POS=1, BUFFER-TIME=448 1 50 S (50 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522553). 364.1707 seconds to achieve S/N = 20 at 2825 A. This time is halved (= 182.08535 seconds) to account for the other G230L cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522737) uses the expanded exposure time to fill the orbit (184 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is minimal. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522690) in order to determine bright object safety. Peak local rate of 5.927 counts per second and global rate of 2199.263, so it is safe. Buffer fill time = 672 seconds, and 2/3 of this is 448 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [134] 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 V-GM-AUR COS/FUV TIME-TA PSA G160M 1589 FP-POS=3, BUFFER-TIME=2865 1 265 S (265 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522544). 376.7304 seconds to achieve S/N = 30 at 1548.5 A. This time is quartered (= 94.1826 seconds) to account for both the other G160M cenwave and the two FP-POS settings per cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522739) uses the expanded exposure time to fill the orbit (186 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is significant compared to the G230L exposures. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522682) in order to determine bright object safety. Peak local rate of 0.315 counts per second and global rate of 548.875, so it is safe. Buffer fill time = 4297 seconds, and 2/3 of this is 2864.667 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [135] 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 V-GM-AUR COS/FUV TIME-TA PSA G160M 1589 FP-POS=4, BUFFER-TIME=2865 1 265 S (265 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522544). 376.7304 seconds to achieve S/N = 30 at 1548.5 A. This time is quartered (= 94.1826 seconds) to account for both the other G160M cenwave and the two FP-POS settings per cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522739) uses the expanded exposure time to fill the orbit (186 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is significant compared to the G230L exposures. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522682) in order to determine bright object safety. Peak local rate of 0.315 counts per second and global rate of 548.875, so it is safe. Buffer fill time = 4297 seconds, and 2/3 of this is 2864.667 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [136] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 9 V-GM-AUR COS/FUV TIME-TA PSA G160M 1623 FP-POS=1, BUFFER-TIME=3154 1 265 S (265 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522545). 393.2034 seconds to achieve S/N = 30 at 1548.5 A. This time is quartered (= 98.30085 seconds) to account for both the other G160M cenwave and the two FP-POS settings per cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522741) uses the expanded exposure time to fill the orbit (186 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is significant compared to the G230L exposures. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522683) in order to determine bright object safety. Peak local rate of 0.317 counts per second and global rate of 498.525, so it is safe. Buffer fill time = 4731 seconds, and 2/3 of this is 3154 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [137] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 10 V-GM-AUR COS/FUV TIME-TA PSA G160M 1623 FP-POS=2, BUFFER-TIME=3154 1 265 S (265 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522545). 393.2034 seconds to achieve S/N = 30 at 1548.5 A. This time is quartered (= 98.30085 seconds) to account for both the other G160M cenwave and the two FP-POS settings per cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522741) uses the expanded exposure time to fill the orbit (186 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is significant compared to the G230L exposures. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522683) in order to determine bright object safety. Peak local rate of 0.317 counts per second and global rate of 498.525, so it is safe. Buffer fill time = 4731 seconds, and 2/3 of this is 3154 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 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 | ------------------------------------------------------------------------------------------------------------------------------------ V-GM-AUR 1 COS/NUV ACQ/PEA PSA G230L 2950 none none none none 1 N/A KXD V-GM-AUR 2 COS/NUV ACQ/PEA PSA G230L 2950 none none none none 1 N/A KD V-GM-AUR 3 COS/NUV ACQ/PEA PSA G230L 2950 none none none none 1 N/A KXD V-GM-AUR 4 COS/NUV ACQ/PEA PSA G230L 2950 none none none none 1 N/A KD V-GM-AUR 5 COS/NUV TIME-TA PSA G230L 2950 none none none none 1 N/A G V-GM-AUR 6 COS/NUV TIME-TA PSA G230L 2635 none none none none 1 N/A G V-GM-AUR 7 COS/FUV TIME-TA PSA G160M 1589 none none none none 1 N/A G 16108( 6) - 02-Nov-2021 13:03:24 - [138] 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 | ------------------------------------------------------------------------------------------------------------------------------------ V-GM-AUR 8 COS/FUV TIME-TA PSA G160M 1589 none none none none 1 N/A G V-GM-AUR 9 COS/FUV TIME-TA PSA G160M 1623 none none none none 1 N/A G V-GM-AUR 10 COS/FUV TIME-TA PSA G160M 1623 none none none none 1 N/A G 16108( 6) - 02-Nov-2021 13:03:24 - [139] Visit: AM (V-GM-AUR-COS-11) Visit Requirements: SCHED 100%; AFTER AJ BY 65.1 Orbits TO 73.3 Orbits; BETWEEN 25-OCT-2021:17:20:00 AND 15-DEC-2021:21:10:00 On Hold Comments: Additional Comments: vstatus; 1M; V-GM-AUR; P/COS approved for submission; P/AH 19/07/21 ; intrev: complete ; P/WF 19/07/21 vcheck; Enter targ name & Inst. & Resp. Sci.; GM Aur ; COS ; AH vcheck; ETC numbers entered in APT?; Yes vcheck; Any screening violations?; No vcheck; M-dwarf check complete and added to box folder?; N/A vcheck; S/N ETC calcs done & documented?; Yes vcheck; Field images checked & saved?; Yes ... located at: box/ullyses_tech/ullyses_proposals/monitor/16018/images/ vcheck; Selected ACQ strategy?; Double ACQ/PeakXD+ACQ/PeakD, G230L, S/N = 40 vcheck; Possible ACQ or Sci spoilers?; No vcheck; Field BOT clear?; Yes vcheck; Visual BOT check for stars not in catalog?; Yes vcheck; Orbit packing finalized?; Yes vcheck; Buffer times optimized?; Yes vcheck; Verify visit grouping correct; Yes vcheck; phase constraint for ground based observations added?; N/A vcheck; BETWEENS for coordinated observations added?; Yes ... 01 OCT 2021 00:00 to 11 OCT 2021 08:10 and 12 OCT 2021 17:00 to 24 OCT 2021 04:15 and 25 OCT 2021 17:20 to 05 NOV 2021 21:10 vcheck; Is visit ready for int. review?; Yes Allocated COS orbits = 12 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 V-GM-AUR COS/NUV ACQ/PEA PSA G230L 2950 STRIPE=DEF 1 5.8 S (5.8 KXD S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC (COS.sa.1522537) in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/PEAKXD with PSA takes 5.8 seconds for S/N=40. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sa.1522540) in order to determine bright object safety. ACQ/PEAKXD with PSA has peak pixel rate of 5.943 counts per second and global rate of 2997.808, so it is safe. This is the first of two ACQ/PEAKXD+ACQ/PEAKD used in order to improve the likelihood of a successful acquisition. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [140] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 2 V-GM-AUR COS/NUV ACQ/PEA PSA G230L 2950 CENTER=FLUX-WT-FLR, NUM-POS=5, 1 5.3 S (5.3 KD STEP-SIZE=0.9 S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC (COS.sa.1522538) in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/PEAKD with PSA takes 5.3 seconds for S/N=40. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sa.1522541) in order to determine bright object safety. ACQ/PEAKD with PSA has peak pixel rate of 5.943 counts per second and global rate of 2997.808, so it is safe. This is the first of two ACQ/PEAKXD+ACQ/PEAKD used in order to improve the likelihood of a successful acquisition. ------------------------------------------------------------------------------------------------------------------------------------ 3 V-GM-AUR COS/NUV ACQ/PEA PSA G230L 2950 STRIPE=DEF 1 5.8 S (5.8 KXD S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC (COS.sa.1522537) in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/PEAKXD with PSA takes 5.8 seconds for S/N=40. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sa.1522540) in order to determine bright object safety. ACQ/PEAKXD with PSA has peak pixel rate of 5.943 counts per second and global rate of 2997.808, so it is safe. This is the second of two ACQ/PEAKXD+ACQ/PEAKD used in order to improve the likelihood of a successful acquisition. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [141] 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 V-GM-AUR COS/NUV ACQ/PEA PSA G230L 2950 CENTER=FLUX-WT-FLR, NUM-POS=5, 1 5.3 S (5.3 KD STEP-SIZE=0.9 S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC (COS.sa.1522538) in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/PEAKD with PSA takes 5.3 seconds for S/N=40. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sa.1522541) in order to determine bright object safety. ACQ/PEAKD with PSA has peak pixel rate of 5.943 counts per second and global rate of 2997.808, so it is safe. This is the second of two ACQ/PEAKXD+ACQ/PEAKD used in order to improve the likelihood of a successful acquisition. ------------------------------------------------------------------------------------------------------------------------------------ 5 V-GM-AUR COS/NUV TIME-TA PSA G230L 2950 FP-POS=4, BUFFER-TIME=524 1 50 S (50 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522552). 362.4388 seconds to achieve S/N = 20 at 2825 A. This time is halved (= 181.2194 seconds) to account for the other G230L cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522735) uses the expanded exposure time to fill the orbit (184 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is minimal. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522691) in order to determine bright object safety. Peak local rate of 5.943 counts per second and global rate of 2997.808, so it is safe. Buffer fill time = 786 seconds, and 2/3 of this is 524 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [142] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 6 V-GM-AUR COS/NUV TIME-TA PSA G230L 2635 FP-POS=1, BUFFER-TIME=448 1 50 S (50 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522553). 364.1707 seconds to achieve S/N = 20 at 2825 A. This time is halved (= 182.08535 seconds) to account for the other G230L cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522737) uses the expanded exposure time to fill the orbit (184 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is minimal. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522690) in order to determine bright object safety. Peak local rate of 5.927 counts per second and global rate of 2199.263, so it is safe. Buffer fill time = 672 seconds, and 2/3 of this is 448 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [143] 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 V-GM-AUR COS/FUV TIME-TA PSA G160M 1589 FP-POS=3, BUFFER-TIME=2865 1 265 S (265 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522544). 376.7304 seconds to achieve S/N = 30 at 1548.5 A. This time is quartered (= 94.1826 seconds) to account for both the other G160M cenwave and the two FP-POS settings per cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522739) uses the expanded exposure time to fill the orbit (186 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is significant compared to the G230L exposures. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522682) in order to determine bright object safety. Peak local rate of 0.315 counts per second and global rate of 548.875, so it is safe. Buffer fill time = 4297 seconds, and 2/3 of this is 2864.667 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [144] 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 V-GM-AUR COS/FUV TIME-TA PSA G160M 1589 FP-POS=4, BUFFER-TIME=2865 1 265 S (265 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522544). 376.7304 seconds to achieve S/N = 30 at 1548.5 A. This time is quartered (= 94.1826 seconds) to account for both the other G160M cenwave and the two FP-POS settings per cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522739) uses the expanded exposure time to fill the orbit (186 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is significant compared to the G230L exposures. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522682) in order to determine bright object safety. Peak local rate of 0.315 counts per second and global rate of 548.875, so it is safe. Buffer fill time = 4297 seconds, and 2/3 of this is 2864.667 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [145] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 9 V-GM-AUR COS/FUV TIME-TA PSA G160M 1623 FP-POS=1, BUFFER-TIME=3154 1 265 S (265 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522545). 393.2034 seconds to achieve S/N = 30 at 1548.5 A. This time is quartered (= 98.30085 seconds) to account for both the other G160M cenwave and the two FP-POS settings per cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522741) uses the expanded exposure time to fill the orbit (186 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is significant compared to the G230L exposures. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522683) in order to determine bright object safety. Peak local rate of 0.317 counts per second and global rate of 498.525, so it is safe. Buffer fill time = 4731 seconds, and 2/3 of this is 3154 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [146] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 10 V-GM-AUR COS/FUV TIME-TA PSA G160M 1623 FP-POS=2, BUFFER-TIME=3154 1 265 S (265 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522545). 393.2034 seconds to achieve S/N = 30 at 1548.5 A. This time is quartered (= 98.30085 seconds) to account for both the other G160M cenwave and the two FP-POS settings per cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522741) uses the expanded exposure time to fill the orbit (186 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is significant compared to the G230L exposures. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522683) in order to determine bright object safety. Peak local rate of 0.317 counts per second and global rate of 498.525, so it is safe. Buffer fill time = 4731 seconds, and 2/3 of this is 3154 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 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 | ------------------------------------------------------------------------------------------------------------------------------------ V-GM-AUR 1 COS/NUV ACQ/PEA PSA G230L 2950 none none none none 1 N/A KXD V-GM-AUR 2 COS/NUV ACQ/PEA PSA G230L 2950 none none none none 1 N/A KD V-GM-AUR 3 COS/NUV ACQ/PEA PSA G230L 2950 none none none none 1 N/A KXD V-GM-AUR 4 COS/NUV ACQ/PEA PSA G230L 2950 none none none none 1 N/A KD V-GM-AUR 5 COS/NUV TIME-TA PSA G230L 2950 none none none none 1 N/A G V-GM-AUR 6 COS/NUV TIME-TA PSA G230L 2635 none none none none 1 N/A G V-GM-AUR 7 COS/FUV TIME-TA PSA G160M 1589 none none none none 1 N/A G 16108( 6) - 02-Nov-2021 13:03:24 - [147] 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 | ------------------------------------------------------------------------------------------------------------------------------------ V-GM-AUR 8 COS/FUV TIME-TA PSA G160M 1589 none none none none 1 N/A G V-GM-AUR 9 COS/FUV TIME-TA PSA G160M 1623 none none none none 1 N/A G V-GM-AUR 10 COS/FUV TIME-TA PSA G160M 1623 none none none none 1 N/A G 16108( 6) - 02-Nov-2021 13:03:24 - [148] Visit: AN (V-GM-AUR-COS-12) Visit Requirements: SCHED 100%; AFTER AJ BY 88.2 Orbits TO 96.4 Orbits; BETWEEN 25-OCT-2021:17:20:00 AND 15-DEC-2021:21:10:00 On Hold Comments: Additional Comments: vstatus; 1N; V-GM-AUR; P/COS approved for submission; P/AH 19/07/21 ; intrev: complete ; P/WF 19/07/21 vcheck; Enter targ name & Inst. & Resp. Sci.; GM Aur ; COS ; AH vcheck; ETC numbers entered in APT?; Yes vcheck; Any screening violations?; No vcheck; M-dwarf check complete and added to box folder?; N/A vcheck; S/N ETC calcs done & documented?; Yes vcheck; Field images checked & saved?; Yes ... located at: box/ullyses_tech/ullyses_proposals/monitor/16018/images/ vcheck; Selected ACQ strategy?; Double ACQ/PeakXD+ACQ/PeakD, G230L, S/N = 40 vcheck; Possible ACQ or Sci spoilers?; No vcheck; Field BOT clear?; Yes vcheck; Visual BOT check for stars not in catalog?; Yes vcheck; Orbit packing finalized?; Yes vcheck; Buffer times optimized?; Yes vcheck; Verify visit grouping correct; Yes vcheck; phase constraint for ground based observations added?; N/A vcheck; BETWEENS for coordinated observations added?; Yes ... 01 OCT 2021 00:00 to 11 OCT 2021 08:10 and 12 OCT 2021 17:00 to 24 OCT 2021 04:15 and 25 OCT 2021 17:20 to 05 NOV 2021 21:10 vcheck; Is visit ready for int. review?; Yes Allocated COS orbits = 12 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 V-GM-AUR COS/NUV ACQ/PEA PSA G230L 2950 STRIPE=DEF 1 5.8 S (5.8 KXD S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC (COS.sa.1522537) in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/PEAKXD with PSA takes 5.8 seconds for S/N=40. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sa.1522540) in order to determine bright object safety. ACQ/PEAKXD with PSA has peak pixel rate of 5.943 counts per second and global rate of 2997.808, so it is safe. This is the first of two ACQ/PEAKXD+ACQ/PEAKD used in order to improve the likelihood of a successful acquisition. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [149] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 2 V-GM-AUR COS/NUV ACQ/PEA PSA G230L 2950 CENTER=FLUX-WT-FLR, NUM-POS=5, 1 5.3 S (5.3 KD STEP-SIZE=0.9 S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC (COS.sa.1522538) in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/PEAKD with PSA takes 5.3 seconds for S/N=40. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sa.1522541) in order to determine bright object safety. ACQ/PEAKD with PSA has peak pixel rate of 5.943 counts per second and global rate of 2997.808, so it is safe. This is the first of two ACQ/PEAKXD+ACQ/PEAKD used in order to improve the likelihood of a successful acquisition. ------------------------------------------------------------------------------------------------------------------------------------ 3 V-GM-AUR COS/NUV ACQ/PEA PSA G230L 2950 STRIPE=DEF 1 5.8 S (5.8 KXD S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC (COS.sa.1522537) in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/PEAKXD with PSA takes 5.8 seconds for S/N=40. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sa.1522540) in order to determine bright object safety. ACQ/PEAKXD with PSA has peak pixel rate of 5.943 counts per second and global rate of 2997.808, so it is safe. This is the second of two ACQ/PEAKXD+ACQ/PEAKD used in order to improve the likelihood of a successful acquisition. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [150] 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 V-GM-AUR COS/NUV ACQ/PEA PSA G230L 2950 CENTER=FLUX-WT-FLR, NUM-POS=5, 1 5.3 S (5.3 KD STEP-SIZE=0.9 S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC (COS.sa.1522538) in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/PEAKD with PSA takes 5.3 seconds for S/N=40. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sa.1522541) in order to determine bright object safety. ACQ/PEAKD with PSA has peak pixel rate of 5.943 counts per second and global rate of 2997.808, so it is safe. This is the second of two ACQ/PEAKXD+ACQ/PEAKD used in order to improve the likelihood of a successful acquisition. ------------------------------------------------------------------------------------------------------------------------------------ 5 V-GM-AUR COS/NUV TIME-TA PSA G230L 2950 FP-POS=4, BUFFER-TIME=524 1 50 S (50 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522552). 362.4388 seconds to achieve S/N = 20 at 2825 A. This time is halved (= 181.2194 seconds) to account for the other G230L cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522735) uses the expanded exposure time to fill the orbit (184 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is minimal. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522691) in order to determine bright object safety. Peak local rate of 5.943 counts per second and global rate of 2997.808, so it is safe. Buffer fill time = 786 seconds, and 2/3 of this is 524 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [151] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 6 V-GM-AUR COS/NUV TIME-TA PSA G230L 2635 FP-POS=1, BUFFER-TIME=448 1 50 S (50 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522553). 364.1707 seconds to achieve S/N = 20 at 2825 A. This time is halved (= 182.08535 seconds) to account for the other G230L cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522737) uses the expanded exposure time to fill the orbit (184 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is minimal. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522690) in order to determine bright object safety. Peak local rate of 5.927 counts per second and global rate of 2199.263, so it is safe. Buffer fill time = 672 seconds, and 2/3 of this is 448 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [152] 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 V-GM-AUR COS/FUV TIME-TA PSA G160M 1589 FP-POS=3, BUFFER-TIME=2865 1 265 S (265 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522544). 376.7304 seconds to achieve S/N = 30 at 1548.5 A. This time is quartered (= 94.1826 seconds) to account for both the other G160M cenwave and the two FP-POS settings per cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522739) uses the expanded exposure time to fill the orbit (186 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is significant compared to the G230L exposures. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522682) in order to determine bright object safety. Peak local rate of 0.315 counts per second and global rate of 548.875, so it is safe. Buffer fill time = 4297 seconds, and 2/3 of this is 2864.667 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [153] 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 V-GM-AUR COS/FUV TIME-TA PSA G160M 1589 FP-POS=4, BUFFER-TIME=2865 1 265 S (265 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522544). 376.7304 seconds to achieve S/N = 30 at 1548.5 A. This time is quartered (= 94.1826 seconds) to account for both the other G160M cenwave and the two FP-POS settings per cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522739) uses the expanded exposure time to fill the orbit (186 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is significant compared to the G230L exposures. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522682) in order to determine bright object safety. Peak local rate of 0.315 counts per second and global rate of 548.875, so it is safe. Buffer fill time = 4297 seconds, and 2/3 of this is 2864.667 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [154] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 9 V-GM-AUR COS/FUV TIME-TA PSA G160M 1623 FP-POS=1, BUFFER-TIME=3154 1 265 S (265 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522545). 393.2034 seconds to achieve S/N = 30 at 1548.5 A. This time is quartered (= 98.30085 seconds) to account for both the other G160M cenwave and the two FP-POS settings per cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522741) uses the expanded exposure time to fill the orbit (186 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is significant compared to the G230L exposures. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522683) in order to determine bright object safety. Peak local rate of 0.317 counts per second and global rate of 498.525, so it is safe. Buffer fill time = 4731 seconds, and 2/3 of this is 3154 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 16108( 6) - 02-Nov-2021 13:03:24 - [155] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 10 V-GM-AUR COS/FUV TIME-TA PSA G160M 1623 FP-POS=2, BUFFER-TIME=3154 1 265 S (265 G S) Comments: Used model spectrum gmaur_lya2_etc.txt in the ETC in order to determine exposure times (COS.sp.1522545). 393.2034 seconds to achieve S/N = 30 at 1548.5 A. This time is quartered (= 98.30085 seconds) to account for both the other G160M cenwave and the two FP-POS settings per cenwave also observing this spectral feature. The listed ETC Run # for this exposure (COS.sp.1522741) uses the expanded exposure time to fill the orbit (186 seconds). The G160M exposures received priority for Unused Orbital Visibility, so the increased exposure time here is significant compared to the G230L exposures. Used model spectrum gmaur_lya2_x4.00_etc.txt in the ETC (COS.sp.1522683) in order to determine bright object safety. Peak local rate of 0.317 counts per second and global rate of 498.525, so it is safe. Buffer fill time = 4731 seconds, and 2/3 of this is 3154 seconds. ------------------------------------------------------------------------------------------------------------------------------------ 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 | ------------------------------------------------------------------------------------------------------------------------------------ V-GM-AUR 1 COS/NUV ACQ/PEA PSA G230L 2950 none none none none 1 N/A KXD V-GM-AUR 2 COS/NUV ACQ/PEA PSA G230L 2950 none none none none 1 N/A KD V-GM-AUR 3 COS/NUV ACQ/PEA PSA G230L 2950 none none none none 1 N/A KXD V-GM-AUR 4 COS/NUV ACQ/PEA PSA G230L 2950 none none none none 1 N/A KD V-GM-AUR 5 COS/NUV TIME-TA PSA G230L 2950 none none none none 1 N/A G V-GM-AUR 6 COS/NUV TIME-TA PSA G230L 2635 none none none none 1 N/A G V-GM-AUR 7 COS/FUV TIME-TA PSA G160M 1589 none none none none 1 N/A G 16108( 6) - 02-Nov-2021 13:03:24 - [156] 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 | ------------------------------------------------------------------------------------------------------------------------------------ V-GM-AUR 8 COS/FUV TIME-TA PSA G160M 1589 none none none none 1 N/A G V-GM-AUR 9 COS/FUV TIME-TA PSA G160M 1623 none none none none 1 N/A G V-GM-AUR 10 COS/FUV TIME-TA PSA G160M 1623 none none none none 1 N/A G 16108( 6) - 02-Nov-2021 13:03:24 - [157] Summary Form for Proposal 16108 Item Used in this proposal ------------------------------------------------------------------------------------------------------------------------------------ Apertures PSA ------------------------------------------------------------------------------------------------------------------------------------ Configurations COS/FUV, COS/NUV ------------------------------------------------------------------------------------------------------------------------------------ Opmodes ACQ/PEAKD, ACQ/PEAKXD, TIME-TAG ------------------------------------------------------------------------------------------------------------------------------------ Optional Parameters BUFFER-TIME=2865, BUFFER-TIME=3154, BUFFER-TIME=448, BUFFER-TIME=524, CENTER=FLUX-WT-FLR, FP-POS=1, FP-POS=2, FP-POS=3, FP-POS=4, NUM-POS=5, STEP-SIZE=0.9, STRIPE=DEF ------------------------------------------------------------------------------------------------------------------------------------ Special Requirements AFTER 1C BY 111.2 Orbits TO 119.4 Orbits, AFTER 1C BY 134.3 Orbits TO 142.5 Orbits, AFTER 1C BY 157.4 Orbits TO 165.6 Orbits, AFTER 1C BY 180.4 Orbits TO 188.6 Orbits, AFTER 1C BY 19.0 Orbits TO 27.2 Orbits, AFTER 1C BY 203.5 Orbits TO 213.2 Orbits, AFTER 1C BY 226.6 Orbits TO 234.8 Orbits, AFTER 1C BY 249.6 Orbits TO 257.8 Orbits, AFTER 1C BY 42.0 Orbits TO 50.2 Orbits, AFTER 1C BY 65.1 Orbits TO 73.3 Orbits, AFTER 1C BY 88.2 Orbits TO 96.4 Orbits, AFTER AJ BY 19 Orbits TO 27.2 Orbits, AFTER AJ BY 42 Orbits TO 50.2 Orbits, AFTER AJ BY 65.1 Orbits TO 73.3 Orbits, AFTER AJ BY 88.2 Orbits TO 96.4 Orbits, BETWEEN 01-OCT-2021:00:00:00 AND 11-OCT-2021:08:10:00, BETWEEN 12-OCT-2021:17:00:00 AND 24-OCT-2021:04:15:00, BETWEEN 25-OCT-2021:17:20:00 AND 05-NOV-2021:21:10:00, BETWEEN 25-OCT-2021:17:20:00 AND 15-DEC-2021:21:10:00, SCHED 100% ------------------------------------------------------------------------------------------------------------------------------------ Spectral Elements G160M, G230L ------------------------------------------------------------------------------------------------------------------------------------ Target Names V-GM-AUR ------------------------------------------------------------------------------------------------------------------------------------