Could not connect to APT Status Server For the best data quality, it is generally required to use all four FP-POS positions when observing at a given COS cenwave. See the COS Instrument Handbook for exceptions that may apply to observations with G130M/1291 or G160M. For the best data quality, it is generally required to use all four FP-POS positions when observing at a given COS cenwave. See the COS Instrument Handbook for exceptions that may apply to observations with G130M/1291 or G160M. For the best data quality, it is generally required to use all four FP-POS positions when observing at a given COS cenwave. See the COS Instrument Handbook for exceptions that may apply to observations with G130M/1291 or G160M. For the best data quality, it is generally required to use all four FP-POS positions when observing at a given COS cenwave. See the COS Instrument Handbook for exceptions that may apply to observations with G130M/1291 or G160M. For the best data quality, it is generally required to use all four FP-POS positions when observing at a given COS cenwave. See the COS Instrument Handbook for exceptions that may apply to observations with G130M/1291 or G160M. For the best data quality, it is generally required to use all four FP-POS positions when observing at a given COS cenwave. See the COS Instrument Handbook for exceptions that may apply to observations with G130M/1291 or G160M. For the best data quality, it is generally required to use all four FP-POS positions when observing at a given COS cenwave. See the COS Instrument Handbook for exceptions that may apply to observations with G130M/1291 or G160M. For the best data quality, it is generally required to use all four FP-POS positions when observing at a given COS cenwave. See the COS Instrument Handbook for exceptions that may apply to observations with G130M/1291 or G160M. For the best data quality, it is generally required to use all four FP-POS positions when observing at a given COS cenwave. See the COS Instrument Handbook for exceptions that may apply to observations with G130M/1291 or G160M. For the best data quality, it is generally required to use all four FP-POS positions when observing at a given COS cenwave. See the COS Instrument Handbook for exceptions that may apply to observations with G130M/1291 or G160M. For the best data quality, it is generally required to use all four FP-POS positions when observing at a given COS cenwave. See the COS Instrument Handbook for exceptions that may apply to observations with G130M/1291 or G160M. For the best data quality, it is generally required to use all four FP-POS positions when observing at a given COS cenwave. See the COS Instrument Handbook for exceptions that may apply to observations with G130M/1291 or G160M. Updates exptimes based on epoch 1 BETWEENs are shifted to match TESS Sector 59 and should be considered preliminary -1565214639 ----- Attempting Submission 1 (Thu Jul 29 17:13:45 GMT 2021) ----- ----- Attempting Submission 2 (Fri Jul 30 20:25:34 GMT 2021) ----- ----- Attempting Submission 3 (Sat Oct 30 00:56:51 GMT 2021) ----- ----- Attempting Submission 4 (Thu Jul 28 13:27:11 GMT 2022) ----- Warnings pertain to the use of FP-POS. This is intentional ULLYSES Monitoring Observations of the T Tauri Star BP Tau: Second Epoch 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 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 use COS NUV + FUV and all visits are single orbit with SCHED=100. This target will be observed by TESS in Sector 59, which runs from 2022-Nov-26 to 2022-Dec-23. For the purpose of coordinated observations, this version sets the BETWEEN for all visits to be from 2022-Nov-26 to 2023-Jan-31. The target should be scheduled as early in this window as possible. This window will be refined when more detailed information about the timing of TESS observations is available. The rotation period of the target is about 8.19 days =124 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. Therefore, the ideal visit spacing would be 31 orbits. If we allow windows that are multiples of 31.0 +/-5.1 orbits after visit 1C the required AFTER BY orbit values are as follows: Visit 1 D 1 E 1 F 1 G 1 H 1 I 1J 1 K 1 L 1M 1N Start 25.9 56.9 87.9 118.9 149.9 180.9 212.0 243.0 274.0 305.0 336.0 End 36.1 67.1 98.1 129.1 160.1 191.1 222.2 253.2 284.2 315.2 346.2 0 false SUPPORTED STAR EMISSION LINE STAR PRE-MAIN SEQUENCE STAR T TAURI STAR NO This object was generated by the targetselector and retrieved from the SIMBAD database. ------------------------------------------------------------------------------- tstatus; V-BP-TAU; P/COS approved for submission; S/ins not started; P/JRD 21/07/21; S/xx DD/MM/YY tcheck; APT/SIMBAD target names: ; V-BP-TAU 'V* BP Tau' tcheck; Target info verification status?; OK tcheck; Coordinates & P.M. verified, epoch checked?; Yes - Gaia coords - PM updated from Gaia tcheck; Adopted SED compared to Observations?; yes J2000 Timing link suitability includes constraints ([1D After 1C by 1.7 to 2.4 days] [1E After 1C by 3.8 to 4.4 days] [1F After 1C by 5.8 to 6.5 days] [1G After 1C by 7.9 to 8.5 days] [1H After 1C by 9.9 to 10.6 days] [1I After 1C by 12.0 to 12.6 days] [1J After 1C by 14.0 to 14.7 days] [1K After 1C by 16.1 to 16.7 days] [1L After 1C by 18.1 to 18.8 days] [1M After 1C by 20.2 to 20.8 days] [1N After 1C by 22.2 to 22.9 days]) The scheduling data was generated by CASM 30.3. CASM was run in Phase II mode. vstatus; 1C; V-BP-TAU; P/COS Approved for submission; P/JRD 21/07/21 ; intrev: complete ; P/WF 29/07/21 vcheck; Enter targ name & Inst. & Resp. Sci.; BP Tau ; COS ; DJS 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 vcheck; Selected ACQ strategy?; Double ACQ/IMAGE 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?; yes vcheck; BETWEENS for coordinated observations added?; yes vcheck; Is visit ready for int. review?; yes Allocated COS orbits = 12 1670901393000 110.08029514157721 (Tic-Visit :proposal-id 16589 :visit-id "1C" :proposal-version -1 :trans-version "20220516" :date "28-Jul-2022 09:14:55.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 122112 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16589 :visit-id "1C" :obset-id "1C" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16589 :visit-id "1C" :orbit-number 1 :pcs-time 393 :si-vis-utilization 2534 :al-overhead-at-end 0 :internal-dur-at-end 334 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2928 :pcs-gap 0 ) true 1 0 Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/IMAGE with BOA and MIRRORA takes 38 seconds for S/N=30 Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. ACQ/IMAGE with BOA and MIRRORA has peak pixel rate of 13.2 cps and global rate of 1380, so it is safe This is the first of two ACQ/IMAGES used in order to improve the likelihood of a successful acquisition. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/IMAGE with BOA and MIRRORA takes 38 seconds for S/N=30 Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. ACQ/IMAGE with BOA and MIRRORA has peak pixel rate of 13.2 cps and global rate of 1380, so it is safe This is the second of two ACQ/IMAGES used in order to improve the likelihood of a successful acquisition. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. 189 second exposure required to get S/N=20 at 2825 A. Exposure time expanded to fill orbit. Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. Peak local rate of 10.9 cps and global rate of 4409, so it is safe. Buffer fill time = 535 and 2/3 of this is 357. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. 190 second exposure required to get S/N=20 at 2825 A. Exposure time expanded to fill orbit. Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. Peak local rate of 10.8 cps and global rate of 5266, so it is safe. Buffer fill time = 447 and 2/3 of this is 298. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. 195 second exposure required to get S/N=30 at 1548.4 A, the peak of the C IV line. But this can be divided between the FP-POSs. Exposure time expanded to fill orbit. Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. Peak local rate of 0.5 cps and global rate of 908, so it is safe. Buffer Fill Time = 2597, so BUFFER-TIME set to 2/3 of this value. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. 195 second exposure required to get S/N=30 at 1548.4 A, the peak of the C IV line. But this can be divided between the FP-POSs. Exposure time expanded to fill orbit. Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. Peak local rate of 0.5 cps and global rate of 908, so it is safe. Buffer Fill Time = 2597, so BUFFER-TIME set to 2/3 of this value. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. 197 second exposure required to get S/N=30 at 1548.4 A, the peak of the C IV line. But this can be divided between the FP-POSs. Exposure time expanded to fill orbit. Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. Peak local rate of 0.5 cps and global rate of 832, so it is safe. Buffer Fill Time = 2835, so BUFFER-TIME set to 2/3 of this value. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. 197 second exposure required to get S/N=30 at 1548.4 A, the peak of the C IV line. But this can be divided between the FP-POSs. Exposure time expanded to fill orbit. Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. Peak local rate of 0.5 cps and global rate of 832, so it is safe. Buffer Fill Time = 2835, so BUFFER-TIME set to 2/3 of this value. Timing link suitability includes constraints ([1D After 1C by 1.7 to 2.4 days]) The scheduling data was generated by CASM 30.3. CASM was run in Phase II mode. vstatus; 1C; V-BP-TAU; P/COS ready for internal review; P/JRD 21/07/21 ; intrev: in progress ; P/WF 29/07/21 vcheck; Enter targ name & Inst. & Resp. Sci.; BP Tau ; COS ; DJS 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 vcheck; Selected ACQ strategy?; Double ACQ/IMAGE 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?; yes vcheck; BETWEENS for coordinated observations added?; yes vcheck; Is visit ready for int. review?; yes Allocated COS orbits = 12 1671101284000 105.93815751663578 (Tic-Visit :proposal-id 16589 :visit-id "1D" :proposal-version -1 :trans-version "20220516" :date "28-Jul-2022 09:14:56.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 122112 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16589 :visit-id "1D" :obset-id "1D" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16589 :visit-id "1D" :orbit-number 1 :pcs-time 393 :si-vis-utilization 2534 :al-overhead-at-end 0 :internal-dur-at-end 334 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2928 :pcs-gap 0 ) true 1 0 Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/IMAGE with BOA and MIRRORA takes 38 seconds for S/N=30 Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. ACQ/IMAGE with BOA and MIRRORA has peak pixel rate of 13.2 cps and global rate of 1380, so it is safe This is the first of two ACQ/IMAGES used in order to improve the likelihood of a successful acquisition. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/IMAGE with BOA and MIRRORA takes 38 seconds for S/N=30 Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. ACQ/IMAGE with BOA and MIRRORA has peak pixel rate of 13.2 cps and global rate of 1380, so it is safe This is the second of two ACQ/IMAGES used in order to improve the likelihood of a successful acquisition. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. 189 second exposure required to get S/N=20 at 2825 A. Exposure time expanded to fill orbit. Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. Peak local rate of 10.9 cps and global rate of 4409, so it is safe. Buffer fill time = 535 and 2/3 of this is 357. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. 190 second exposure required to get S/N=20 at 2825 A. Exposure time expanded to fill orbit. Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. Peak local rate of 10.8 cps and global rate of 5266, so it is safe. Buffer fill time = 447 and 2/3 of this is 298. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. 195 second exposure required to get S/N=30 at 1548.4 A, the peak of the C IV line. But this can be divided between the FP-POSs. Exposure time expanded to fill orbit. Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. Peak local rate of 0.5 cps and global rate of 908, so it is safe. Buffer Fill Time = 2597, so BUFFER-TIME set to 2/3 of this value. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. 195 second exposure required to get S/N=30 at 1548.4 A, the peak of the C IV line. But this can be divided between the FP-POSs. Exposure time expanded to fill orbit. Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. Peak local rate of 0.5 cps and global rate of 908, so it is safe. Buffer Fill Time = 2597, so BUFFER-TIME set to 2/3 of this value. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. 197 second exposure required to get S/N=30 at 1548.4 A, the peak of the C IV line. But this can be divided between the FP-POSs. Exposure time expanded to fill orbit. Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. Peak local rate of 0.5 cps and global rate of 832, so it is safe. Buffer Fill Time = 2835, so BUFFER-TIME set to 2/3 of this value. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. 197 second exposure required to get S/N=30 at 1548.4 A, the peak of the C IV line. But this can be divided between the FP-POSs. Exposure time expanded to fill orbit. Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. Peak local rate of 0.5 cps and global rate of 832, so it is safe. Buffer Fill Time = 2835, so BUFFER-TIME set to 2/3 of this value. Timing link suitability includes constraints ([1E After 1C by 3.8 to 4.4 days]) The scheduling data was generated by CASM 30.3. CASM was run in Phase II mode. vstatus; 1C; V-BP-TAU; P/COS Approved for submission; P/JRD 21/07/21 ; intrev: complete ; P/WF 29/07/21 vcheck; Enter targ name & Inst. & Resp. Sci.; BP Tau ; COS ; DJS 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 vcheck; Selected ACQ strategy?; Double ACQ/IMAGE 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?; yes vcheck; BETWEENS for coordinated observations added?; yes vcheck; Is visit ready for int. review?; yes Allocated COS orbits = 12 1671238350000 104.0 (Tic-Visit :proposal-id 16589 :visit-id "1E" :proposal-version -1 :trans-version "20220516" :date "28-Jul-2022 09:14:57.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 122112 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16589 :visit-id "1E" :obset-id "1E" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16589 :visit-id "1E" :orbit-number 1 :pcs-time 393 :si-vis-utilization 2534 :al-overhead-at-end 0 :internal-dur-at-end 334 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2928 :pcs-gap 0 ) true 1 0 Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/IMAGE with BOA and MIRRORA takes 38 seconds for S/N=30 Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. ACQ/IMAGE with BOA and MIRRORA has peak pixel rate of 13.2 cps and global rate of 1380, so it is safe This is the first of two ACQ/IMAGES used in order to improve the likelihood of a successful acquisition. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/IMAGE with BOA and MIRRORA takes 38 seconds for S/N=30 Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. ACQ/IMAGE with BOA and MIRRORA has peak pixel rate of 13.2 cps and global rate of 1380, so it is safe This is the second of two ACQ/IMAGES used in order to improve the likelihood of a successful acquisition. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. 189 second exposure required to get S/N=20 at 2825 A. Exposure time expanded to fill orbit. Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. Peak local rate of 10.9 cps and global rate of 4409, so it is safe. Buffer fill time = 535 and 2/3 of this is 357. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. 190 second exposure required to get S/N=20 at 2825 A. Exposure time expanded to fill orbit. Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. Peak local rate of 10.8 cps and global rate of 5266, so it is safe. Buffer fill time = 447 and 2/3 of this is 298. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. 195 second exposure required to get S/N=30 at 1548.4 A, the peak of the C IV line. But this can be divided between the FP-POSs. Exposure time expanded to fill orbit. Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. Peak local rate of 0.5 cps and global rate of 908, so it is safe. Buffer Fill Time = 2597, so BUFFER-TIME set to 2/3 of this value. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. 195 second exposure required to get S/N=30 at 1548.4 A, the peak of the C IV line. But this can be divided between the FP-POSs. Exposure time expanded to fill orbit. Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. Peak local rate of 0.5 cps and global rate of 908, so it is safe. Buffer Fill Time = 2597, so BUFFER-TIME set to 2/3 of this value. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. 197 second exposure required to get S/N=30 at 1548.4 A, the peak of the C IV line. But this can be divided between the FP-POSs. Exposure time expanded to fill orbit. Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. Peak local rate of 0.5 cps and global rate of 832, so it is safe. Buffer Fill Time = 2835, so BUFFER-TIME set to 2/3 of this value. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. 197 second exposure required to get S/N=30 at 1548.4 A, the peak of the C IV line. But this can be divided between the FP-POSs. Exposure time expanded to fill orbit. Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. Peak local rate of 0.5 cps and global rate of 832, so it is safe. Buffer Fill Time = 2835, so BUFFER-TIME set to 2/3 of this value. Timing link suitability includes constraints ([1F After 1C by 5.8 to 6.5 days]) The scheduling data was generated by CASM 30.3. CASM was run in Phase II mode. vstatus; 1C; V-BP-TAU; P/COS Approved for submission; P/JRD 21/07/21 ; intrev: complete ; P/WF 29/07/21 vcheck; Enter targ name & Inst. & Resp. Sci.; BP Tau ; COS ; DJS 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 vcheck; Selected ACQ strategy?; Double ACQ/IMAGE 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?; yes vcheck; BETWEENS for coordinated observations added?; yes vcheck; Is visit ready for int. review?; yes Allocated COS orbits = 12 1671455357000 100.61958368821593 (Tic-Visit :proposal-id 16589 :visit-id "1F" :proposal-version -1 :trans-version "20220516" :date "28-Jul-2022 09:14:58.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 122112 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16589 :visit-id "1F" :obset-id "1F" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16589 :visit-id "1F" :orbit-number 1 :pcs-time 393 :si-vis-utilization 2534 :al-overhead-at-end 0 :internal-dur-at-end 334 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2928 :pcs-gap 0 ) true 1 0 Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/IMAGE with BOA and MIRRORA takes 38 seconds for S/N=30 Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. ACQ/IMAGE with BOA and MIRRORA has peak pixel rate of 13.2 cps and global rate of 1380, so it is safe This is the first of two ACQ/IMAGES used in order to improve the likelihood of a successful acquisition. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/IMAGE with BOA and MIRRORA takes 38 seconds for S/N=30 Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. ACQ/IMAGE with BOA and MIRRORA has peak pixel rate of 13.2 cps and global rate of 1380, so it is safe This is the second of two ACQ/IMAGES used in order to improve the likelihood of a successful acquisition. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. 189 second exposure required to get S/N=20 at 2825 A. Exposure time expanded to fill orbit. Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. Peak local rate of 10.9 cps and global rate of 4409, so it is safe. Buffer fill time = 535 and 2/3 of this is 357. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. 190 second exposure required to get S/N=20 at 2825 A. Exposure time expanded to fill orbit. Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. Peak local rate of 10.8 cps and global rate of 5266, so it is safe. Buffer fill time = 447 and 2/3 of this is 298. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. 195 second exposure required to get S/N=30 at 1548.4 A, the peak of the C IV line. But this can be divided between the FP-POSs. Exposure time expanded to fill orbit. Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. Peak local rate of 0.5 cps and global rate of 908, so it is safe. Buffer Fill Time = 2597, so BUFFER-TIME set to 2/3 of this value. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. 195 second exposure required to get S/N=30 at 1548.4 A, the peak of the C IV line. But this can be divided between the FP-POSs. Exposure time expanded to fill orbit. Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. Peak local rate of 0.5 cps and global rate of 908, so it is safe. Buffer Fill Time = 2597, so BUFFER-TIME set to 2/3 of this value. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. 197 second exposure required to get S/N=30 at 1548.4 A, the peak of the C IV line. But this can be divided between the FP-POSs. Exposure time expanded to fill orbit. Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. Peak local rate of 0.5 cps and global rate of 832, so it is safe. Buffer Fill Time = 2835, so BUFFER-TIME set to 2/3 of this value. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. 197 second exposure required to get S/N=30 at 1548.4 A, the peak of the C IV line. But this can be divided between the FP-POSs. Exposure time expanded to fill orbit. Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. Peak local rate of 0.5 cps and global rate of 832, so it is safe. Buffer Fill Time = 2835, so BUFFER-TIME set to 2/3 of this value. Timing link suitability includes constraints ([1G After 1C by 7.9 to 8.5 days]) The scheduling data was generated by CASM 30.3. CASM was run in Phase II mode. vstatus; 1C; V-BP-TAU; P/COS Approved for submission; P/JRD 21/07/21 ; intrev: complete ; P/WF 29/07/21 vcheck; Enter targ name & Inst. & Resp. Sci.; BP Tau ; COS ; DJS 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 vcheck; Selected ACQ strategy?; Double ACQ/IMAGE 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?; yes vcheck; BETWEENS for coordinated observations added?; yes vcheck; Is visit ready for int. review?; yes Allocated COS orbits = 12 1671626700000 98.67191885323967 (Tic-Visit :proposal-id 16589 :visit-id "1G" :proposal-version -1 :trans-version "20220516" :date "28-Jul-2022 09:14:58.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 122112 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16589 :visit-id "1G" :obset-id "1G" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16589 :visit-id "1G" :orbit-number 1 :pcs-time 393 :si-vis-utilization 2534 :al-overhead-at-end 0 :internal-dur-at-end 334 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2928 :pcs-gap 0 ) true 1 0 Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/IMAGE with BOA and MIRRORA takes 38 seconds for S/N=30 Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. ACQ/IMAGE with BOA and MIRRORA has peak pixel rate of 13.2 cps and global rate of 1380, so it is safe This is the first of two ACQ/IMAGES used in order to improve the likelihood of a successful acquisition. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/IMAGE with BOA and MIRRORA takes 38 seconds for S/N=30 Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. ACQ/IMAGE with BOA and MIRRORA has peak pixel rate of 13.2 cps and global rate of 1380, so it is safe This is the second of two ACQ/IMAGES used in order to improve the likelihood of a successful acquisition. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. 189 second exposure required to get S/N=20 at 2825 A. Exposure time expanded to fill orbit. Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. Peak local rate of 10.9 cps and global rate of 4409, so it is safe. Buffer fill time = 535 and 2/3 of this is 357. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. 190 second exposure required to get S/N=20 at 2825 A. Exposure time expanded to fill orbit. Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. Peak local rate of 10.8 cps and global rate of 5266, so it is safe. Buffer fill time = 447 and 2/3 of this is 298. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. 195 second exposure required to get S/N=30 at 1548.4 A, the peak of the C IV line. But this can be divided between the FP-POSs. Exposure time expanded to fill orbit. Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. Peak local rate of 0.5 cps and global rate of 908, so it is safe. Buffer Fill Time = 2597, so BUFFER-TIME set to 2/3 of this value. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. 195 second exposure required to get S/N=30 at 1548.4 A, the peak of the C IV line. But this can be divided between the FP-POSs. Exposure time expanded to fill orbit. Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. Peak local rate of 0.5 cps and global rate of 908, so it is safe. Buffer Fill Time = 2597, so BUFFER-TIME set to 2/3 of this value. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. 197 second exposure required to get S/N=30 at 1548.4 A, the peak of the C IV line. But this can be divided between the FP-POSs. Exposure time expanded to fill orbit. Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. Peak local rate of 0.5 cps and global rate of 832, so it is safe. Buffer Fill Time = 2835, so BUFFER-TIME set to 2/3 of this value. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. 197 second exposure required to get S/N=30 at 1548.4 A, the peak of the C IV line. But this can be divided between the FP-POSs. Exposure time expanded to fill orbit. Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. Peak local rate of 0.5 cps and global rate of 832, so it is safe. Buffer Fill Time = 2835, so BUFFER-TIME set to 2/3 of this value. vstatus; 1C; V-BP-TAU; P/COS Approved for submission; P/JRD 21/07/21 ; intrev: complete ; P/WF 29/07/21 vcheck; Enter targ name & Inst. & Resp. Sci.; BP Tau ; COS ; DJS 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 vcheck; Selected ACQ strategy?; Double ACQ/IMAGE 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?; yes vcheck; BETWEENS for coordinated observations added?; yes vcheck; Is visit ready for int. review?; yes Allocated COS orbits = 12 HOPR repeat of visit 1G (Tic-Visit :proposal-id 16589 :visit-id "1G" :proposal-version -1 :trans-version "20220516" :date "28-Jul-2022 09:14:58.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 122112 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16589 :visit-id "1G" :obset-id "1G" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16589 :visit-id "1G" :orbit-number 1 :pcs-time 393 :si-vis-utilization 2534 :al-overhead-at-end 0 :internal-dur-at-end 334 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2928 :pcs-gap 0 ) false 1 0 Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/IMAGE with BOA and MIRRORA takes 38 seconds for S/N=30 Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. ACQ/IMAGE with BOA and MIRRORA has peak pixel rate of 13.2 cps and global rate of 1380, so it is safe This is the first of two ACQ/IMAGES used in order to improve the likelihood of a successful acquisition. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/IMAGE with BOA and MIRRORA takes 38 seconds for S/N=30 Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. ACQ/IMAGE with BOA and MIRRORA has peak pixel rate of 13.2 cps and global rate of 1380, so it is safe This is the second of two ACQ/IMAGES used in order to improve the likelihood of a successful acquisition. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. 189 second exposure required to get S/N=20 at 2825 A. Exposure time expanded to fill orbit. Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. Peak local rate of 10.9 cps and global rate of 4409, so it is safe. Buffer fill time = 535 and 2/3 of this is 357. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. 190 second exposure required to get S/N=20 at 2825 A. Exposure time expanded to fill orbit. Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. Peak local rate of 10.8 cps and global rate of 5266, so it is safe. Buffer fill time = 447 and 2/3 of this is 298. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. 195 second exposure required to get S/N=30 at 1548.4 A, the peak of the C IV line. But this can be divided between the FP-POSs. Exposure time expanded to fill orbit. Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. Peak local rate of 0.5 cps and global rate of 908, so it is safe. Buffer Fill Time = 2597, so BUFFER-TIME set to 2/3 of this value. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. 195 second exposure required to get S/N=30 at 1548.4 A, the peak of the C IV line. But this can be divided between the FP-POSs. Exposure time expanded to fill orbit. Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. Peak local rate of 0.5 cps and global rate of 908, so it is safe. Buffer Fill Time = 2597, so BUFFER-TIME set to 2/3 of this value. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. 197 second exposure required to get S/N=30 at 1548.4 A, the peak of the C IV line. But this can be divided between the FP-POSs. Exposure time expanded to fill orbit. Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. Peak local rate of 0.5 cps and global rate of 832, so it is safe. Buffer Fill Time = 2835, so BUFFER-TIME set to 2/3 of this value. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. 197 second exposure required to get S/N=30 at 1548.4 A, the peak of the C IV line. But this can be divided between the FP-POSs. Exposure time expanded to fill orbit. Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. Peak local rate of 0.5 cps and global rate of 832, so it is safe. Buffer Fill Time = 2835, so BUFFER-TIME set to 2/3 of this value. Timing link suitability includes constraints ([1H After 1C by 9.9 to 10.6 days]) The scheduling data was generated by CASM 30.3. CASM was run in Phase II mode. vstatus; 1C; V-BP-TAU; P/COS Approved for submission; P/JRD 21/07/21 ; intrev: complete ; P/WF 29/07/21 vcheck; Enter targ name & Inst. & Resp. Sci.; BP Tau ; COS ; DJS 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 vcheck; Selected ACQ strategy?; Double ACQ/IMAGE 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?; yes vcheck; BETWEENS for coordinated observations added?; yes vcheck; Is visit ready for int. review?; yes Allocated COS orbits = 12 1671798022000 97.01127926888762 (Tic-Visit :proposal-id 16589 :visit-id "1H" :proposal-version -1 :trans-version "20220516" :date "28-Jul-2022 09:14:59.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 122112 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16589 :visit-id "1H" :obset-id "1H" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16589 :visit-id "1H" :orbit-number 1 :pcs-time 393 :si-vis-utilization 2534 :al-overhead-at-end 0 :internal-dur-at-end 334 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2928 :pcs-gap 0 ) true 1 0 Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/IMAGE with BOA and MIRRORA takes 38 seconds for S/N=30 Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. ACQ/IMAGE with BOA and MIRRORA has peak pixel rate of 13.2 cps and global rate of 1380, so it is safe This is the first of two ACQ/IMAGES used in order to improve the likelihood of a successful acquisition. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/IMAGE with BOA and MIRRORA takes 38 seconds for S/N=30 Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. ACQ/IMAGE with BOA and MIRRORA has peak pixel rate of 13.2 cps and global rate of 1380, so it is safe This is the second of two ACQ/IMAGES used in order to improve the likelihood of a successful acquisition. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. 189 second exposure required to get S/N=20 at 2825 A. Exposure time expanded to fill orbit. Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. Peak local rate of 10.9 cps and global rate of 4409, so it is safe. Buffer fill time = 535 and 2/3 of this is 357. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. 190 second exposure required to get S/N=20 at 2825 A. Exposure time expanded to fill orbit. Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. Peak local rate of 10.8 cps and global rate of 5266, so it is safe. Buffer fill time = 447 and 2/3 of this is 298. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. 195 second exposure required to get S/N=30 at 1548.4 A, the peak of the C IV line. But this can be divided between the FP-POSs. Exposure time expanded to fill orbit. Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. Peak local rate of 0.5 cps and global rate of 908, so it is safe. Buffer Fill Time = 2597, so BUFFER-TIME set to 2/3 of this value. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. 195 second exposure required to get S/N=30 at 1548.4 A, the peak of the C IV line. But this can be divided between the FP-POSs. Exposure time expanded to fill orbit. Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. Peak local rate of 0.5 cps and global rate of 908, so it is safe. Buffer Fill Time = 2597, so BUFFER-TIME set to 2/3 of this value. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. 197 second exposure required to get S/N=30 at 1548.4 A, the peak of the C IV line. But this can be divided between the FP-POSs. Exposure time expanded to fill orbit. Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. Peak local rate of 0.5 cps and global rate of 832, so it is safe. Buffer Fill Time = 2835, so BUFFER-TIME set to 2/3 of this value. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. 197 second exposure required to get S/N=30 at 1548.4 A, the peak of the C IV line. But this can be divided between the FP-POSs. Exposure time expanded to fill orbit. Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. Peak local rate of 0.5 cps and global rate of 832, so it is safe. Buffer Fill Time = 2835, so BUFFER-TIME set to 2/3 of this value. Timing link suitability includes constraints ([1I After 1C by 12.0 to 12.6 days]) The scheduling data was generated by CASM 30.3. CASM was run in Phase II mode. vstatus; 1C; V-BP-TAU; P/COS Approved for submission; P/JRD 21/07/21 ; intrev: complete ; P/WF 29/07/21 vcheck; Enter targ name & Inst. & Resp. Sci.; BP Tau ; COS ; DJS 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 vcheck; Selected ACQ strategy?; Double ACQ/IMAGE 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?; yes vcheck; BETWEENS for coordinated observations added?; yes vcheck; Is visit ready for int. review?; yes Allocated COS orbits = 12 1671969356000 95.5775008326276 (Tic-Visit :proposal-id 16589 :visit-id "1I" :proposal-version -1 :trans-version "20220516" :date "28-Jul-2022 09:15:00.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 122112 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16589 :visit-id "1I" :obset-id "1I" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16589 :visit-id "1I" :orbit-number 1 :pcs-time 393 :si-vis-utilization 2534 :al-overhead-at-end 0 :internal-dur-at-end 334 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2928 :pcs-gap 0 ) true 1 0 Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/IMAGE with BOA and MIRRORA takes 38 seconds for S/N=30 Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. ACQ/IMAGE with BOA and MIRRORA has peak pixel rate of 13.2 cps and global rate of 1380, so it is safe This is the first of two ACQ/IMAGES used in order to improve the likelihood of a successful acquisition. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/IMAGE with BOA and MIRRORA takes 38 seconds for S/N=30 Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. ACQ/IMAGE with BOA and MIRRORA has peak pixel rate of 13.2 cps and global rate of 1380, so it is safe This is the second of two ACQ/IMAGES used in order to improve the likelihood of a successful acquisition. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. 189 second exposure required to get S/N=20 at 2825 A. Exposure time expanded to fill orbit. Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. Peak local rate of 10.9 cps and global rate of 4409, so it is safe. Buffer fill time = 535 and 2/3 of this is 357. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. 190 second exposure required to get S/N=20 at 2825 A. Exposure time expanded to fill orbit. Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. Peak local rate of 10.8 cps and global rate of 5266, so it is safe. Buffer fill time = 447 and 2/3 of this is 298. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. 195 second exposure required to get S/N=30 at 1548.4 A, the peak of the C IV line. But this can be divided between the FP-POSs. Exposure time expanded to fill orbit. Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. Peak local rate of 0.5 cps and global rate of 908, so it is safe. Buffer Fill Time = 2597, so BUFFER-TIME set to 2/3 of this value. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. 195 second exposure required to get S/N=30 at 1548.4 A, the peak of the C IV line. But this can be divided between the FP-POSs. Exposure time expanded to fill orbit. Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. Peak local rate of 0.5 cps and global rate of 908, so it is safe. Buffer Fill Time = 2597, so BUFFER-TIME set to 2/3 of this value. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. 197 second exposure required to get S/N=30 at 1548.4 A, the peak of the C IV line. But this can be divided between the FP-POSs. Exposure time expanded to fill orbit. Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. Peak local rate of 0.5 cps and global rate of 832, so it is safe. Buffer Fill Time = 2835, so BUFFER-TIME set to 2/3 of this value. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. 197 second exposure required to get S/N=30 at 1548.4 A, the peak of the C IV line. But this can be divided between the FP-POSs. Exposure time expanded to fill orbit. Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. Peak local rate of 0.5 cps and global rate of 832, so it is safe. Buffer Fill Time = 2835, so BUFFER-TIME set to 2/3 of this value. Timing link suitability includes constraints ([1J After 1C by 14.0 to 14.7 days]) The scheduling data was generated by CASM 30.3. CASM was run in Phase II mode. vstatus; 1C; V-BP-TAU; P/COS Approved for submission; P/JRD 21/07/21 ; intrev: complete ; P/WF 29/07/21 vcheck; Enter targ name & Inst. & Resp. Sci.; BP Tau ; COS ; DJS 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 vcheck; Selected ACQ strategy?; Double ACQ/IMAGE 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?; yes vcheck; BETWEENS for coordinated observations added?; yes vcheck; Is visit ready for int. review?; yes Allocated COS orbits = 12 1672157840000 94.20926857708417 (Tic-Visit :proposal-id 16589 :visit-id "1J" :proposal-version -1 :trans-version "20220516" :date "28-Jul-2022 09:15:01.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 122112 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16589 :visit-id "1J" :obset-id "1J" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16589 :visit-id "1J" :orbit-number 1 :pcs-time 393 :si-vis-utilization 2534 :al-overhead-at-end 0 :internal-dur-at-end 334 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2928 :pcs-gap 0 ) true 1 0 Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/IMAGE with BOA and MIRRORA takes 38 seconds for S/N=30 Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. ACQ/IMAGE with BOA and MIRRORA has peak pixel rate of 13.2 cps and global rate of 1380, so it is safe This is the first of two ACQ/IMAGES used in order to improve the likelihood of a successful acquisition. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/IMAGE with BOA and MIRRORA takes 38 seconds for S/N=30 Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. ACQ/IMAGE with BOA and MIRRORA has peak pixel rate of 13.2 cps and global rate of 1380, so it is safe This is the second of two ACQ/IMAGES used in order to improve the likelihood of a successful acquisition. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. 189 second exposure required to get S/N=20 at 2825 A. Exposure time expanded to fill orbit. Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. Peak local rate of 10.9 cps and global rate of 4409, so it is safe. Buffer fill time = 535 and 2/3 of this is 357. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. 190 second exposure required to get S/N=20 at 2825 A. Exposure time expanded to fill orbit. Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. Peak local rate of 10.8 cps and global rate of 5266, so it is safe. Buffer fill time = 447 and 2/3 of this is 298. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. 195 second exposure required to get S/N=30 at 1548.4 A, the peak of the C IV line. But this can be divided between the FP-POSs. Exposure time expanded to fill orbit. Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. Peak local rate of 0.5 cps and global rate of 908, so it is safe. Buffer Fill Time = 2597, so BUFFER-TIME set to 2/3 of this value. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. 195 second exposure required to get S/N=30 at 1548.4 A, the peak of the C IV line. But this can be divided between the FP-POSs. Exposure time expanded to fill orbit. Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. Peak local rate of 0.5 cps and global rate of 908, so it is safe. Buffer Fill Time = 2597, so BUFFER-TIME set to 2/3 of this value. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. 197 second exposure required to get S/N=30 at 1548.4 A, the peak of the C IV line. But this can be divided between the FP-POSs. Exposure time expanded to fill orbit. Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. Peak local rate of 0.5 cps and global rate of 832, so it is safe. Buffer Fill Time = 2835, so BUFFER-TIME set to 2/3 of this value. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. 197 second exposure required to get S/N=30 at 1548.4 A, the peak of the C IV line. But this can be divided between the FP-POSs. Exposure time expanded to fill orbit. Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. Peak local rate of 0.5 cps and global rate of 832, so it is safe. Buffer Fill Time = 2835, so BUFFER-TIME set to 2/3 of this value. Timing link suitability includes constraints ([1K After 1C by 16.1 to 16.7 days]) The scheduling data was generated by CASM 30.3. CASM was run in Phase II mode. vstatus; 1C; V-BP-TAU; P/COS Approved for submission; P/JRD 21/07/21 ; intrev: complete ;P/WF 29/07/21 vcheck; Enter targ name & Inst. & Resp. Sci.; BP Tau ; COS ; DJS 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 vcheck; Selected ACQ strategy?; Double ACQ/IMAGE 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?; yes vcheck; BETWEENS for coordinated observations added?; yes vcheck; Is visit ready for int. review?; yes Allocated COS orbits = 12 1672317708000 93.18799393932301 (Tic-Visit :proposal-id 16589 :visit-id "1K" :proposal-version -1 :trans-version "20220516" :date "28-Jul-2022 09:15:02.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 122112 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16589 :visit-id "1K" :obset-id "1K" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16589 :visit-id "1K" :orbit-number 1 :pcs-time 393 :si-vis-utilization 2534 :al-overhead-at-end 0 :internal-dur-at-end 334 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2928 :pcs-gap 0 ) true 1 0 Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/IMAGE with BOA and MIRRORA takes 38 seconds for S/N=30 Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. ACQ/IMAGE with BOA and MIRRORA has peak pixel rate of 13.2 cps and global rate of 1380, so it is safe This is the first of two ACQ/IMAGES used in order to improve the likelihood of a successful acquisition. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/IMAGE with BOA and MIRRORA takes 38 seconds for S/N=30 Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. ACQ/IMAGE with BOA and MIRRORA has peak pixel rate of 13.2 cps and global rate of 1380, so it is safe This is the second of two ACQ/IMAGES used in order to improve the likelihood of a successful acquisition. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. 189 second exposure required to get S/N=20 at 2825 A. Exposure time expanded to fill orbit. Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. Peak local rate of 10.9 cps and global rate of 4409, so it is safe. Buffer fill time = 535 and 2/3 of this is 357. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. 190 second exposure required to get S/N=20 at 2825 A. Exposure time expanded to fill orbit. Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. Peak local rate of 10.8 cps and global rate of 5266, so it is safe. Buffer fill time = 447 and 2/3 of this is 298. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. 195 second exposure required to get S/N=30 at 1548.4 A, the peak of the C IV line. But this can be divided between the FP-POSs. Exposure time expanded to fill orbit. Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. Peak local rate of 0.5 cps and global rate of 908, so it is safe. Buffer Fill Time = 2597, so BUFFER-TIME set to 2/3 of this value. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. 195 second exposure required to get S/N=30 at 1548.4 A, the peak of the C IV line. But this can be divided between the FP-POSs. Exposure time expanded to fill orbit. Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. Peak local rate of 0.5 cps and global rate of 908, so it is safe. Buffer Fill Time = 2597, so BUFFER-TIME set to 2/3 of this value. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. 197 second exposure required to get S/N=30 at 1548.4 A, the peak of the C IV line. But this can be divided between the FP-POSs. Exposure time expanded to fill orbit. Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. Peak local rate of 0.5 cps and global rate of 832, so it is safe. Buffer Fill Time = 2835, so BUFFER-TIME set to 2/3 of this value. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. 197 second exposure required to get S/N=30 at 1548.4 A, the peak of the C IV line. But this can be divided between the FP-POSs. Exposure time expanded to fill orbit. Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. Peak local rate of 0.5 cps and global rate of 832, so it is safe. Buffer Fill Time = 2835, so BUFFER-TIME set to 2/3 of this value. Timing link suitability includes constraints ([1L After 1C by 18.1 to 18.8 days]) The scheduling data was generated by CASM 30.3. CASM was run in Phase II mode. vstatus; 1C; V-BP-TAU; P/COS Approved for submission; P/JRD 21/07/21 ; intrev: complete ; P/WF 29/07/21 vcheck; Enter targ name & Inst. & Resp. Sci.; BP Tau ; COS ; DJS 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 vcheck; Selected ACQ strategy?; Double ACQ/IMAGE 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?; yes vcheck; BETWEENS for coordinated observations added?; yes vcheck; Is visit ready for int. review?; yes Allocated COS orbits = 12 1672500454000 92.14845723310282 (Tic-Visit :proposal-id 16589 :visit-id "1L" :proposal-version -1 :trans-version "20220516" :date "28-Jul-2022 09:15:03.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 122112 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16589 :visit-id "1L" :obset-id "1L" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16589 :visit-id "1L" :orbit-number 1 :pcs-time 393 :si-vis-utilization 2534 :al-overhead-at-end 0 :internal-dur-at-end 334 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2928 :pcs-gap 0 ) true 1 0 Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/IMAGE with BOA and MIRRORA takes 38 seconds for S/N=30 Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. ACQ/IMAGE with BOA and MIRRORA has peak pixel rate of 13.2 cps and global rate of 1380, so it is safe This is the first of two ACQ/IMAGES used in order to improve the likelihood of a successful acquisition. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/IMAGE with BOA and MIRRORA takes 38 seconds for S/N=30 Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. ACQ/IMAGE with BOA and MIRRORA has peak pixel rate of 13.2 cps and global rate of 1380, so it is safe This is the second of two ACQ/IMAGES used in order to improve the likelihood of a successful acquisition. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. 189 second exposure required to get S/N=20 at 2825 A. Exposure time expanded to fill orbit. Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. Peak local rate of 10.9 cps and global rate of 4409, so it is safe. Buffer fill time = 535 and 2/3 of this is 357. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. 190 second exposure required to get S/N=20 at 2825 A. Exposure time expanded to fill orbit. Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. Peak local rate of 10.8 cps and global rate of 5266, so it is safe. Buffer fill time = 447 and 2/3 of this is 298. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. 195 second exposure required to get S/N=30 at 1548.4 A, the peak of the C IV line. But this can be divided between the FP-POSs. Exposure time expanded to fill orbit. Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. Peak local rate of 0.5 cps and global rate of 908, so it is safe. Buffer Fill Time = 2597, so BUFFER-TIME set to 2/3 of this value. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. 195 second exposure required to get S/N=30 at 1548.4 A, the peak of the C IV line. But this can be divided between the FP-POSs. Exposure time expanded to fill orbit. Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. Peak local rate of 0.5 cps and global rate of 908, so it is safe. Buffer Fill Time = 2597, so BUFFER-TIME set to 2/3 of this value. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. 197 second exposure required to get S/N=30 at 1548.4 A, the peak of the C IV line. But this can be divided between the FP-POSs. Exposure time expanded to fill orbit. Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. Peak local rate of 0.5 cps and global rate of 832, so it is safe. Buffer Fill Time = 2835, so BUFFER-TIME set to 2/3 of this value. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. 197 second exposure required to get S/N=30 at 1548.4 A, the peak of the C IV line. But this can be divided between the FP-POSs. Exposure time expanded to fill orbit. Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. Peak local rate of 0.5 cps and global rate of 832, so it is safe. Buffer Fill Time = 2835, so BUFFER-TIME set to 2/3 of this value. Timing link suitability includes constraints ([1M After 1C by 20.2 to 20.8 days]) The scheduling data was generated by CASM 30.3. CASM was run in Phase II mode. vstatus; 1C; V-BP-TAU; P/COS Approved for submission; P/JRD 21/07/21 ; intrev: complete ; P/WF 29/07/21 vcheck; Enter targ name & Inst. & Resp. Sci.; BP Tau ; COS ; DJS 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 vcheck; Selected ACQ strategy?; Double ACQ/IMAGE 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?; yes vcheck; BETWEENS for coordinated observations added?; yes vcheck; Is visit ready for int. review?; yes Allocated COS orbits = 12 (Tic-Visit :proposal-id 16589 :visit-id "1M" :proposal-version -1 :trans-version "20220516" :date "28-Jul-2022 09:15:04.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 122112 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16589 :visit-id "1M" :obset-id "1M" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16589 :visit-id "1M" :orbit-number 1 :pcs-time 393 :si-vis-utilization 2534 :al-overhead-at-end 0 :internal-dur-at-end 334 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2928 :pcs-gap 0 ) true 1 0 Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/IMAGE with BOA and MIRRORA takes 38 seconds for S/N=30 Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. ACQ/IMAGE with BOA and MIRRORA has peak pixel rate of 13.2 cps and global rate of 1380, so it is safe This is the first of two ACQ/IMAGES used in order to improve the likelihood of a successful acquisition. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/IMAGE with BOA and MIRRORA takes 38 seconds for S/N=30 Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. ACQ/IMAGE with BOA and MIRRORA has peak pixel rate of 13.2 cps and global rate of 1380, so it is safe This is the second of two ACQ/IMAGES used in order to improve the likelihood of a successful acquisition. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. 189 second exposure required to get S/N=20 at 2825 A. Exposure time expanded to fill orbit. Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. Peak local rate of 10.9 cps and global rate of 4409, so it is safe. Buffer fill time = 535 and 2/3 of this is 357. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. 190 second exposure required to get S/N=20 at 2825 A. Exposure time expanded to fill orbit. Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. Peak local rate of 10.8 cps and global rate of 5266, so it is safe. Buffer fill time = 447 and 2/3 of this is 298. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. 195 second exposure required to get S/N=30 at 1548.4 A, the peak of the C IV line. But this can be divided between the FP-POSs. Exposure time expanded to fill orbit. Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. Peak local rate of 0.5 cps and global rate of 908, so it is safe. Buffer Fill Time = 2597, so BUFFER-TIME set to 2/3 of this value. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. 195 second exposure required to get S/N=30 at 1548.4 A, the peak of the C IV line. But this can be divided between the FP-POSs. Exposure time expanded to fill orbit. Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. Peak local rate of 0.5 cps and global rate of 908, so it is safe. Buffer Fill Time = 2597, so BUFFER-TIME set to 2/3 of this value. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. 197 second exposure required to get S/N=30 at 1548.4 A, the peak of the C IV line. But this can be divided between the FP-POSs. Exposure time expanded to fill orbit. Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. Peak local rate of 0.5 cps and global rate of 832, so it is safe. Buffer Fill Time = 2835, so BUFFER-TIME set to 2/3 of this value. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. 197 second exposure required to get S/N=30 at 1548.4 A, the peak of the C IV line. But this can be divided between the FP-POSs. Exposure time expanded to fill orbit. Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. Peak local rate of 0.5 cps and global rate of 832, so it is safe. Buffer Fill Time = 2835, so BUFFER-TIME set to 2/3 of this value. Timing link suitability includes constraints ([1N After 1C by 22.2 to 22.9 days]) The scheduling data was generated by CASM 30.3. CASM was run in Phase II mode. vstatus; 1C; V-BP-TAU; P/COS Approved for submission; P/JRD 21/07/21 ; intrev: complete ; P/WF 29/07/21 vcheck; Enter targ name & Inst. & Resp. Sci.; BP Tau ; COS ; DJS 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 vcheck; Selected ACQ strategy?; Double ACQ/IMAGE 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?; yes vcheck; BETWEENS for coordinated observations added?; yes vcheck; Is visit ready for int. review?; yes Allocated COS orbits = 12 (Tic-Visit :proposal-id 16589 :visit-id "1N" :proposal-version -1 :trans-version "20220516" :date "28-Jul-2022 09:15:05.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "31" :si-bright-earth-limb-angle 20.0 :data-volume 122112 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16589 :visit-id "1N" :obset-id "1N" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16589 :visit-id "1N" :orbit-number 1 :pcs-time 393 :si-vis-utilization 2534 :al-overhead-at-end 0 :internal-dur-at-end 334 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2928 :pcs-gap 0 ) true 1 0 Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/IMAGE with BOA and MIRRORA takes 38 seconds for S/N=30 Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. ACQ/IMAGE with BOA and MIRRORA has peak pixel rate of 13.2 cps and global rate of 1380, so it is safe This is the first of two ACQ/IMAGES used in order to improve the likelihood of a successful acquisition. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. ACQ/IMAGE with BOA and MIRRORA takes 38 seconds for S/N=30 Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. ACQ/IMAGE with BOA and MIRRORA has peak pixel rate of 13.2 cps and global rate of 1380, so it is safe This is the second of two ACQ/IMAGES used in order to improve the likelihood of a successful acquisition. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. 189 second exposure required to get S/N=20 at 2825 A. Exposure time expanded to fill orbit. Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. Peak local rate of 10.9 cps and global rate of 4409, so it is safe. Buffer fill time = 535 and 2/3 of this is 357. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. 190 second exposure required to get S/N=20 at 2825 A. Exposure time expanded to fill orbit. Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. Peak local rate of 10.8 cps and global rate of 5266, so it is safe. Buffer fill time = 447 and 2/3 of this is 298. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. 195 second exposure required to get S/N=30 at 1548.4 A, the peak of the C IV line. But this can be divided between the FP-POSs. Exposure time expanded to fill orbit. Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. Peak local rate of 0.5 cps and global rate of 908, so it is safe. Buffer Fill Time = 2597, so BUFFER-TIME set to 2/3 of this value. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. 195 second exposure required to get S/N=30 at 1548.4 A, the peak of the C IV line. But this can be divided between the FP-POSs. Exposure time expanded to fill orbit. Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. Peak local rate of 0.5 cps and global rate of 908, so it is safe. Buffer Fill Time = 2597, so BUFFER-TIME set to 2/3 of this value. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. 197 second exposure required to get S/N=30 at 1548.4 A, the peak of the C IV line. But this can be divided between the FP-POSs. Exposure time expanded to fill orbit. Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. Peak local rate of 0.5 cps and global rate of 832, so it is safe. Buffer Fill Time = 2835, so BUFFER-TIME set to 2/3 of this value. Used model spectrum bptau_lya2_etc.txt in the ETC in order to determine exposure times. This is the one listed as the ETC run for the exposure. 197 second exposure required to get S/N=30 at 1548.4 A, the peak of the C IV line. But this can be divided between the FP-POSs. Exposure time expanded to fill orbit. Used model spectrum bptau_lya2_x4.00_etc.txt in the ETC in order to determine bright object safety. Peak local rate of 0.5 cps and global rate of 832, so it is safe. Buffer Fill Time = 2835, so BUFFER-TIME set to 2/3 of this value.