For the best data quality, it is strongly recommended that all four FP-POS positions be used when observing at a given COS CENWAVE setting. Unschedulable Visit For the best data quality, it is strongly recommended that all four FP-POS positions be used when observing at a given COS CENWAVE setting. Unschedulable Visit For the best data quality, it is strongly recommended that all four FP-POS positions be used when observing at a given COS CENWAVE setting. Unschedulable Visit For the best data quality, it is strongly recommended that all four FP-POS positions be used when observing at a given COS CENWAVE setting. Unschedulable Visit For the best data quality, it is strongly recommended that all four FP-POS positions be used when observing at a given COS CENWAVE setting. Unschedulable Visit For the best data quality, it is strongly recommended that all four FP-POS positions be used when observing at a given COS CENWAVE setting. Unschedulable Visit For the best data quality, it is strongly recommended that all four FP-POS positions be used when observing at a given COS CENWAVE setting. Unschedulable Visit For the best data quality, it is strongly recommended that all four FP-POS positions be used when observing at a given COS CENWAVE setting. Unschedulable Visit For the best data quality, it is strongly recommended that all four FP-POS positions be used when observing at a given COS CENWAVE setting. Unschedulable Visit For the best data quality, it is strongly recommended that all four FP-POS positions be used when observing at a given COS CENWAVE setting. Unschedulable Visit For the best data quality, it is strongly recommended that all four FP-POS positions be used when observing at a given COS CENWAVE setting. Unschedulable Visit For the best data quality, it is strongly recommended that all four FP-POS positions be used when observing at a given COS CENWAVE setting. Unschedulable Visit For the best data quality, it is strongly recommended that all four FP-POS positions be used when observing at a given COS CENWAVE setting. 8/16/2021: This update contains visit AD, a repeat of visit 1D under HOPR 92062 5/25/2021: This update contains the fully implemented and internally reviewed visits. It is ready for CS review. 12/18/2020: This is a placeholder for ULLYSES observations of RU Lup intended to allow tests of scheduling. While the exposure details given in this version are plausible, they may change significantly in the final executed version. Full details needed for bright object screening have yet to be provided, so this isn't ready for a final CS review. -1868929186 ----- Attempting Submission 1 (Fri Dec 18 20:28:10 GMT 2020) ----- ----- Attempting Submission 2 (Tue May 25 20:44:26 GMT 2021) ----- ----- Attempting Submission 3 (Mon Aug 16 20:31:07 GMT 2021) ----- The list of investigators has been updated to reflect current ULLYSES staffing. In the NUV, FP-POS requirements do not apply. In the FUV, this combination of FP-POS and cenwaves effectively satisfies the FP-POS rules. Visits reported as "Unscheduleable" have already run or been scheduled. 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 in the XMM field of view and for the purpose of coordinated observations this version sets the BETWEEN for all visits to be from 2021-Aug-10 to 2021-Sep-18. The rotation period of the target is about 3.71 days = 56.1 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 14.03 orbits. If we allow windows that are multiples of 14.0 +/- 3.1 orbits after visit 1 the required AFTER BY orbit values are as follows Visit 2.0 3.0 4.0 5.0 6.0 7.0 8.0 9.0 10.0 11.0 12.0 Start 10.9 25.0 39.0 53.0 67.1 81.1 95.1 109.1 123.2 137.2 151.2 End 17.1 31.2 45.2 59.2 73.3 87.3 101.3 115.3 129.4 143.4 157.4 If we allow windows that are multiples of 14.0 +/- 4.1 orbits after visit 1 the required AFTER BY orbit values are as follows Visit 2.0 3.0 4.0 5.0 6.0 7.0 8.0 9.0 10.0 11.0 12.0 Start 9.9 24.0 38.0 52.0 66.1 80.1 94.1 108.1 122.2 136.2 150.2 End 18.1 32.2 46.2 60.2 74.3 88.3 102.3 116.3 130.4 144.4 158.4 If we allow windows that are multiples of 14.0 +/- 5.1 orbits after visit 1 the required AFTER BY orbit values are as follows Visit 2.0 3.0 4.0 5.0 6.0 7.0 8.0 9.0 10.0 11.0 12.0 Start 8.9 23.0 37.0 51.0 65.1 79.1 93.1 107.1 121.2 135.2 149.2 End 19.1 33.2 47.2 61.2 75.3 89.3 103.3 117.3 131.4 145.4 159.4 Much more than this and the adjacent phase bins will start running into each other. This version uses the rather narrow +/-3.1 orbit windows. Individual windows will likely need to be shifted or widened when detailed scheduling is done. 0 false SUPPORTED STAR PRE-MAIN SEQUENCE STAR T TAURI STAR NO This object was generated by the targetselector and retrieved from the SIMBAD database.Note that while SIMBAD classifies this as K7/M0, only one of many authors assigns this as a M star. K7 is the most commonly adopted designation, and some early authors even classfy this as a G star. Alcala et al. (2014, A&A, 561, A2) properly account for the accretion excess emission from 0.3-2.5 microns and assign a spectral type of K7; this can be considered authoritative. ------------------------------------------------------------------------------- tstatus; V-RU-LUP ; P/COS approved for submission; S/ins not started; P/WF 20/05/21; S/xx DD/MM/YY tcheck; APT/SIMBAD target names: ; HD 142560, HBC 251, 2MASS J15564230-3749154, Sz 83 tcheck; Target info verification status?; OK tcheck; Coordinates & P.M. verified, epoch checked?; yes tcheck; Adopted SED compared to Observations?; yes ... use BVRI photometry from AAVSO averaged from 26 Apr 2021 to 19 May 2021 and mean U-B color from Herbst et al. (1994) ... results lie between 92% and 134% of model, consistent with normal variability 2MASS-J15564230-3749154 HD142560 J2000 SpT=K7, U=9.27, B=10.07, V=9.60, G=10.7107, J=8.732, H=7.824, K=7.138 1621952161008 Timing link suitability includes constraints ([1D After 1C by 0.7 to 1.1 days] [1E After 1C by 1.7 to 2.1 days] [1F After 1C by 2.6 to 3.0 days] [1G After 1C by 3.5 to 3.9 days] [1H After 1C by 4.4 to 4.8 days] [1I After 1C by 5.4 to 5.8 days] [1J After 1C by 6.3 to 6.7 days] [1K After 1C by 7.2 to 7.6 days] [1L After 1C by 8.1 to 8.6 days] [1M After 1C by 9.1 to 9.5 days] [1N After 1C by 10.0 to 10.4 days]) The scheduling data was generated by CASM 29.2. CASM was run in Phase II mode. /Users/wfischer/Box/ullyses_tech/ullyses_proposals/monitor/16110/OP-cache/ULLYSES_16110-v1C.xml vstatus; 1C; V-RU-LUP; P/COS approved for submission; P/WF 20/05/21 ; intrev: complete ; P/JRD 24/05/2021 vcheck; Enter targ name & Inst. & Resp. Sci.; RU Lup ; COS ; WF 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?; G230L/2950, repeated to guard against late GS acq vcheck; Possible ACQ or Sci spoilers?; No vcheck; Field BOT clear?; Yes. BOT complains about the target under the assumption it is an O5 star. vcheck; Visual BOT check for stars not in catalog?; nothing visible in DSS 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 (for XMM) vcheck; Is visit ready for int. review?; yes Allocated COS orbits = 12 1628627594000 97.22682382052881 (Tic-Visit :proposal-id 16110 :visit-id "1C" :proposal-version -1 :trans-version "20200619" :date "25-May-2021 10:16:00.0" :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 695920 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16110 :visit-id "1C" :obset-id "1C" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16110 :visit-id "1C" :orbit-number 1 :pcs-time 393 :si-vis-utilization 2534 :al-overhead-at-end 0 :internal-dur-at-end 407 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2927 :pcs-gap 0 ) true 1 0 ETC 1517209 with model spectrum rulup_lya2_etc.txt gives 0.3 sec, round up to 1 sec For BOP check, ETC 1517210 with 4x model spectrum rulup_lya2_x4.00_etc.txt gives 47 cts/sec in brightest pixel and 22,010 cts/sec in brightest stripe. This exceeds the per-stripe count rate limit for irregularly variable sources, but the 4x case is designed to account for variability. It is below the per-stripe count rate limit of 30,000 cts/sec for nonvariable sources. ETC 1517211 with model spectrum rulup_lya2_etc.txt gives 0.2 sec, round up to 1 sec For BOP check, ETC 1517212 with 4x model spectrum rulup_lya2_x4.00_etc.txt gives 47 cts/sec in brightest pixel and 22,010 cts/sec in brightest stripe. This exceeds the per-stripe count rate limit for irregularly variable sources, but the 4x case is designed to account for variability. It is below the per-stripe count rate limit of 30,000 cts/sec for nonvariable sources. ETC 1517209 with model spectrum rulup_lya2_etc.txt gives 0.3 sec, round up to 1 sec For BOP check, ETC 1517210 with 4x model spectrum rulup_lya2_x4.00_etc.txt gives 47 cts/sec in brightest pixel and 22,010 cts/sec in brightest stripe. This exceeds the per-stripe count rate limit for irregularly variable sources, but the 4x case is designed to account for variability. It is below the per-stripe count rate limit of 30,000 cts/sec for nonvariable sources. ETC 1517211 with model spectrum rulup_lya2_etc.txt gives 0.2 sec, round up to 1 sec For BOP check, ETC 1517212 with 4x model spectrum rulup_lya2_x4.00_etc.txt gives 47 cts/sec in brightest pixel and 22,010 cts/sec in brightest stripe. This exceeds the per-stripe count rate limit for irregularly variable sources, but the 4x case is designed to account for variability. It is below the per-stripe count rate limit of 30,000 cts/sec for nonvariable sources. ETC 1517213 with model spectrum rulup_lya2_etc.txt gives 19 sec to reach S/N = 20 at 2820 A, in the continuum near Mg II 2800. Round up to 30 sec. For BOP check, ETC 1517214 with 4x model spectrum rulup_lya2_x4.00_etc.txt gives 47 cts/sec in brightest pixel and 22,010 cts/sec in brightest stripe. This exceeds the per-stripe count rate limit for irregularly variable sources, but the 4x case is designed to account for variability. It is below the per-stripe count rate limit of 30,000 cts/sec for nonvariable sources. BUFFER-TIME set to 80 sec following COS IHB recommendation when exposure time < 80 sec and ETC buffer time > 80 sec. ETC 1517215 with model spectrum rulup_lya2_etc.txt gives 19 sec to reach S/N = 20 at 2820 A, in the continuum near Mg II 2800. Round up to 30 sec. For BOP check, ETC 1517216 with 4x model spectrum rulup_lya2_x4.00_etc.txt gives 47 cts/sec in brightest pixel and 24,480 cts/sec in brightest stripe. This exceeds the per-stripe count rate limit for irregularly variable sources, but the 4x case is designed to account for variability. It is below the per-stripe count rate limit of 30,000 cts/sec for nonvariable sources. BUFFER-TIME set to 80 sec following COS IHB recommendation when exposure time < 80 sec and ETC buffer time > 80 sec. ETC 1517218 with archival spectrum lbgj530b0_etc.txt, a cenwave 1623 spectrum of this star, gives 550 sec to reach S/N = 30 at 1548 A, the peak of C IV. This is 138 sec per G160M exposure; expand to 219 sec to fill the orbit and account for the possibility of a faint state. For BOP check, ETC 1517219 with 4x archival spectrum lbgj530b0_x4.00_etc.txt gives 0.18 cts/sec in brightest pixel and 1279 cts/sec in entire detector. BUFFER-TIME set to 110 sec to guard against a bright state and reduce overheads. ETC 1517218 with archival spectrum lbgj530b0_etc.txt, a cenwave 1623 spectrum of this star, gives 550 sec to reach S/N = 30 at 1548 A, the peak of C IV. This is 138 sec per G160M exposure; expand to 220 sec to fill the orbit and account for the possibility of a faint state. For BOP check, ETC 1517219 with 4x archival spectrum lbgj530b0_x4.00_etc.txt gives 0.18 cts/sec in brightest pixel and 1279 cts/sec in entire detector. BUFFER-TIME set to 110 sec to guard against a bright state and reduce overheads. ETC 1517220 with archival spectrum lbgj530b0_etc.txt, a cenwave 1623 spectrum of this star, gives 549 sec to reach S/N = 30 at 1548 A, the peak of C IV. This is 138 sec per G160M exposure; expand to 220 sec to fill the orbit and account for the possibility of a faint state. For BOP check, ETC 1517221 with 4x archival spectrum lbgj530b0_x4.00_etc.txt gives 0.18 cts/sec in brightest pixel and 1458 cts/sec in entire detector. BUFFER-TIME set to 110 sec to guard against a bright state and reduce overheads. ETC 1517220 with archival spectrum lbgj530b0_etc.txt, a cenwave 1623 spectrum of this star, gives 549 sec to reach S/N = 30 at 1548 A, the peak of C IV. This is 138 sec per G160M exposure; expand to 220 sec to fill the orbit and account for the possibility of a faint state. For BOP check, ETC 1517221 with 4x archival spectrum lbgj530b0_x4.00_etc.txt gives 0.18 cts/sec in brightest pixel and 1458 cts/sec in entire detector. BUFFER-TIME set to 110 sec to guard against a bright state and reduce overheads. 1621952163371 Timing link suitability includes constraints ([1D After 1C by 0.7 to 1.1 days]) The scheduling data was generated by CASM 29.2. CASM was run in Phase II mode. /Users/wfischer/Box/ullyses_tech/ullyses_proposals/monitor/16110/OP-cache/ULLYSES_16110-v1D.xml vstatus; 1C; V-RU-LUP; P/COS approved for submission; P/WF 20/05/21 ; intrev: complete ; P/JRD 24/05/2021 vcheck; Enter targ name & Inst. & Resp. Sci.; RU Lup ; COS ; WF 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?; G230L/2950, repeated to guard against late GS acq vcheck; Possible ACQ or Sci spoilers?; No vcheck; Field BOT clear?; Yes. BOT complains about the target under the assumption it is an O5 star. vcheck; Visual BOT check for stars not in catalog?; nothing visible in DSS 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 (for XMM) vcheck; Is visit ready for int. review?; yes Allocated COS orbits = 12 1628690487000 97.44843127045277 (Tic-Visit :proposal-id 16110 :visit-id "1D" :proposal-version -1 :trans-version "20200619" :date "25-May-2021 10:16:03.0" :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 695920 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16110 :visit-id "1D" :obset-id "1D" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16110 :visit-id "1D" :orbit-number 1 :pcs-time 393 :si-vis-utilization 2534 :al-overhead-at-end 0 :internal-dur-at-end 407 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2927 :pcs-gap 0 ) true 1 0 ETC 1517209 with model spectrum rulup_lya2_etc.txt gives 0.3 sec, round up to 1 sec For BOP check, ETC 1517210 with 4x model spectrum rulup_lya2_x4.00_etc.txt gives 47 cts/sec in brightest pixel and 22,010 cts/sec in brightest stripe. This exceeds the per-stripe count rate limit for irregularly variable sources, but the 4x case is designed to account for variability. It is below the per-stripe count rate limit of 30,000 cts/sec for nonvariable sources. ETC 1517211 with model spectrum rulup_lya2_etc.txt gives 0.2 sec, round up to 1 sec For BOP check, ETC 1517212 with 4x model spectrum rulup_lya2_x4.00_etc.txt gives 47 cts/sec in brightest pixel and 22,010 cts/sec in brightest stripe. This exceeds the per-stripe count rate limit for irregularly variable sources, but the 4x case is designed to account for variability. It is below the per-stripe count rate limit of 30,000 cts/sec for nonvariable sources. ETC 1517209 with model spectrum rulup_lya2_etc.txt gives 0.3 sec, round up to 1 sec For BOP check, ETC 1517210 with 4x model spectrum rulup_lya2_x4.00_etc.txt gives 47 cts/sec in brightest pixel and 22,010 cts/sec in brightest stripe. This exceeds the per-stripe count rate limit for irregularly variable sources, but the 4x case is designed to account for variability. It is below the per-stripe count rate limit of 30,000 cts/sec for nonvariable sources. ETC 1517211 with model spectrum rulup_lya2_etc.txt gives 0.2 sec, round up to 1 sec For BOP check, ETC 1517212 with 4x model spectrum rulup_lya2_x4.00_etc.txt gives 47 cts/sec in brightest pixel and 22,010 cts/sec in brightest stripe. This exceeds the per-stripe count rate limit for irregularly variable sources, but the 4x case is designed to account for variability. It is below the per-stripe count rate limit of 30,000 cts/sec for nonvariable sources. ETC 1517213 with model spectrum rulup_lya2_etc.txt gives 19 sec to reach S/N = 20 at 2820 A, in the continuum near Mg II 2800. Round up to 30 sec. For BOP check, ETC 1517214 with 4x model spectrum rulup_lya2_x4.00_etc.txt gives 47 cts/sec in brightest pixel and 22,010 cts/sec in brightest stripe. This exceeds the per-stripe count rate limit for irregularly variable sources, but the 4x case is designed to account for variability. It is below the per-stripe count rate limit of 30,000 cts/sec for nonvariable sources. BUFFER-TIME set to 80 sec following COS IHB recommendation when exposure time < 80 sec and ETC buffer time > 80 sec. ETC 1517215 with model spectrum rulup_lya2_etc.txt gives 19 sec to reach S/N = 20 at 2820 A, in the continuum near Mg II 2800. Round up to 30 sec. For BOP check, ETC 1517216 with 4x model spectrum rulup_lya2_x4.00_etc.txt gives 47 cts/sec in brightest pixel and 24,480 cts/sec in brightest stripe. This exceeds the per-stripe count rate limit for irregularly variable sources, but the 4x case is designed to account for variability. It is below the per-stripe count rate limit of 30,000 cts/sec for nonvariable sources. BUFFER-TIME set to 80 sec following COS IHB recommendation when exposure time < 80 sec and ETC buffer time > 80 sec. ETC 1517218 with archival spectrum lbgj530b0_etc.txt, a cenwave 1623 spectrum of this star, gives 550 sec to reach S/N = 30 at 1548 A, the peak of C IV. This is 138 sec per G160M exposure; expand to 219 sec to fill the orbit and account for the possibility of a faint state. For BOP check, ETC 1517219 with 4x archival spectrum lbgj530b0_x4.00_etc.txt gives 0.18 cts/sec in brightest pixel and 1279 cts/sec in entire detector. BUFFER-TIME set to 110 sec to guard against a bright state and reduce overheads. ETC 1517218 with archival spectrum lbgj530b0_etc.txt, a cenwave 1623 spectrum of this star, gives 550 sec to reach S/N = 30 at 1548 A, the peak of C IV. This is 138 sec per G160M exposure; expand to 220 sec to fill the orbit and account for the possibility of a faint state. For BOP check, ETC 1517219 with 4x archival spectrum lbgj530b0_x4.00_etc.txt gives 0.18 cts/sec in brightest pixel and 1279 cts/sec in entire detector. BUFFER-TIME set to 110 sec to guard against a bright state and reduce overheads. ETC 1517220 with archival spectrum lbgj530b0_etc.txt, a cenwave 1623 spectrum of this star, gives 549 sec to reach S/N = 30 at 1548 A, the peak of C IV. This is 138 sec per G160M exposure; expand to 220 sec to fill the orbit and account for the possibility of a faint state. For BOP check, ETC 1517221 with 4x archival spectrum lbgj530b0_x4.00_etc.txt gives 0.18 cts/sec in brightest pixel and 1458 cts/sec in entire detector. BUFFER-TIME set to 110 sec to guard against a bright state and reduce overheads. ETC 1517220 with archival spectrum lbgj530b0_etc.txt, a cenwave 1623 spectrum of this star, gives 549 sec to reach S/N = 30 at 1548 A, the peak of C IV. This is 138 sec per G160M exposure; expand to 220 sec to fill the orbit and account for the possibility of a faint state. For BOP check, ETC 1517221 with 4x archival spectrum lbgj530b0_x4.00_etc.txt gives 0.18 cts/sec in brightest pixel and 1458 cts/sec in entire detector. BUFFER-TIME set to 110 sec to guard against a bright state and reduce overheads. 1621952164611 Timing link suitability includes constraints ([1E After 1C by 1.7 to 2.1 days]) The scheduling data was generated by CASM 29.2. CASM was run in Phase II mode. /Users/wfischer/Box/ullyses_tech/ullyses_proposals/monitor/16110/OP-cache/ULLYSES_16110-v1E.xml vstatus; 1C; V-RU-LUP; P/COS approved for submission; P/WF 20/05/21 ;intrev: complete ; P/JRD 24/05/2021 vcheck; Enter targ name & Inst. & Resp. Sci.; RU Lup ; COS ; WF 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?; G230L/2950, repeated to guard against late GS acq vcheck; Possible ACQ or Sci spoilers?; No vcheck; Field BOT clear?; Yes. BOT complains about the target under the assumption it is an O5 star. vcheck; Visual BOT check for stars not in catalog?; nothing visible in DSS 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 (for XMM) vcheck; Is visit ready for int. review?; yes Allocated COS orbits = 12 1628793399000 97.80811802901371 (Tic-Visit :proposal-id 16110 :visit-id "1E" :proposal-version -1 :trans-version "20200619" :date "25-May-2021 10:16:04.0" :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 695920 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16110 :visit-id "1E" :obset-id "1E" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16110 :visit-id "1E" :orbit-number 1 :pcs-time 393 :si-vis-utilization 2534 :al-overhead-at-end 0 :internal-dur-at-end 407 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2927 :pcs-gap 0 ) true 1 0 ETC 1517209 with model spectrum rulup_lya2_etc.txt gives 0.3 sec, round up to 1 sec For BOP check, ETC 1517210 with 4x model spectrum rulup_lya2_x4.00_etc.txt gives 47 cts/sec in brightest pixel and 22,010 cts/sec in brightest stripe. This exceeds the per-stripe count rate limit for irregularly variable sources, but the 4x case is designed to account for variability. It is below the per-stripe count rate limit of 30,000 cts/sec for nonvariable sources. ETC 1517211 with model spectrum rulup_lya2_etc.txt gives 0.2 sec, round up to 1 sec For BOP check, ETC 1517212 with 4x model spectrum rulup_lya2_x4.00_etc.txt gives 47 cts/sec in brightest pixel and 22,010 cts/sec in brightest stripe. This exceeds the per-stripe count rate limit for irregularly variable sources, but the 4x case is designed to account for variability. It is below the per-stripe count rate limit of 30,000 cts/sec for nonvariable sources. ETC 1517209 with model spectrum rulup_lya2_etc.txt gives 0.3 sec, round up to 1 sec For BOP check, ETC 1517210 with 4x model spectrum rulup_lya2_x4.00_etc.txt gives 47 cts/sec in brightest pixel and 22,010 cts/sec in brightest stripe. This exceeds the per-stripe count rate limit for irregularly variable sources, but the 4x case is designed to account for variability. It is below the per-stripe count rate limit of 30,000 cts/sec for nonvariable sources. ETC 1517211 with model spectrum rulup_lya2_etc.txt gives 0.2 sec, round up to 1 sec For BOP check, ETC 1517212 with 4x model spectrum rulup_lya2_x4.00_etc.txt gives 47 cts/sec in brightest pixel and 22,010 cts/sec in brightest stripe. This exceeds the per-stripe count rate limit for irregularly variable sources, but the 4x case is designed to account for variability. It is below the per-stripe count rate limit of 30,000 cts/sec for nonvariable sources. ETC 1517213 with model spectrum rulup_lya2_etc.txt gives 19 sec to reach S/N = 20 at 2820 A, in the continuum near Mg II 2800. Round up to 30 sec. For BOP check, ETC 1517214 with 4x model spectrum rulup_lya2_x4.00_etc.txt gives 47 cts/sec in brightest pixel and 22,010 cts/sec in brightest stripe. This exceeds the per-stripe count rate limit for irregularly variable sources, but the 4x case is designed to account for variability. It is below the per-stripe count rate limit of 30,000 cts/sec for nonvariable sources. BUFFER-TIME set to 80 sec following COS IHB recommendation when exposure time < 80 sec and ETC buffer time > 80 sec. ETC 1517215 with model spectrum rulup_lya2_etc.txt gives 19 sec to reach S/N = 20 at 2820 A, in the continuum near Mg II 2800. Round up to 30 sec. For BOP check, ETC 1517216 with 4x model spectrum rulup_lya2_x4.00_etc.txt gives 47 cts/sec in brightest pixel and 24,480 cts/sec in brightest stripe. This exceeds the per-stripe count rate limit for irregularly variable sources, but the 4x case is designed to account for variability. It is below the per-stripe count rate limit of 30,000 cts/sec for nonvariable sources. BUFFER-TIME set to 80 sec following COS IHB recommendation when exposure time < 80 sec and ETC buffer time > 80 sec. ETC 1517218 with archival spectrum lbgj530b0_etc.txt, a cenwave 1623 spectrum of this star, gives 550 sec to reach S/N = 30 at 1548 A, the peak of C IV. This is 138 sec per G160M exposure; expand to 219 sec to fill the orbit and account for the possibility of a faint state. For BOP check, ETC 1517219 with 4x archival spectrum lbgj530b0_x4.00_etc.txt gives 0.18 cts/sec in brightest pixel and 1279 cts/sec in entire detector. BUFFER-TIME set to 110 sec to guard against a bright state and reduce overheads. ETC 1517218 with archival spectrum lbgj530b0_etc.txt, a cenwave 1623 spectrum of this star, gives 550 sec to reach S/N = 30 at 1548 A, the peak of C IV. This is 138 sec per G160M exposure; expand to 220 sec to fill the orbit and account for the possibility of a faint state. For BOP check, ETC 1517219 with 4x archival spectrum lbgj530b0_x4.00_etc.txt gives 0.18 cts/sec in brightest pixel and 1279 cts/sec in entire detector. BUFFER-TIME set to 110 sec to guard against a bright state and reduce overheads. ETC 1517220 with archival spectrum lbgj530b0_etc.txt, a cenwave 1623 spectrum of this star, gives 549 sec to reach S/N = 30 at 1548 A, the peak of C IV. This is 138 sec per G160M exposure; expand to 220 sec to fill the orbit and account for the possibility of a faint state. For BOP check, ETC 1517221 with 4x archival spectrum lbgj530b0_x4.00_etc.txt gives 0.18 cts/sec in brightest pixel and 1458 cts/sec in entire detector. BUFFER-TIME set to 110 sec to guard against a bright state and reduce overheads. ETC 1517220 with archival spectrum lbgj530b0_etc.txt, a cenwave 1623 spectrum of this star, gives 549 sec to reach S/N = 30 at 1548 A, the peak of C IV. This is 138 sec per G160M exposure; expand to 220 sec to fill the orbit and account for the possibility of a faint state. For BOP check, ETC 1517221 with 4x archival spectrum lbgj530b0_x4.00_etc.txt gives 0.18 cts/sec in brightest pixel and 1458 cts/sec in entire detector. BUFFER-TIME set to 110 sec to guard against a bright state and reduce overheads. 1621952165846 Timing link suitability includes constraints ([1F After 1C by 2.6 to 3.0 days]) The scheduling data was generated by CASM 29.2. CASM was run in Phase II mode. /Users/wfischer/Box/ullyses_tech/ullyses_proposals/monitor/16110/OP-cache/ULLYSES_16110-v1F.xml vstatus; 1C; V-RU-LUP; P/COS approved for submission; P/WF 20/05/21 ; intrev: complete ; P/JRD 24/05/2021 vcheck; Enter targ name & Inst. & Resp. Sci.; RU Lup ; COS ; WF 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?; G230L/2950, repeated to guard against late GS acq vcheck; Possible ACQ or Sci spoilers?; No vcheck; Field BOT clear?; Yes. BOT complains about the target under the assumption it is an O5 star. vcheck; Visual BOT check for stars not in catalog?; nothing visible in DSS 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 (for XMM) vcheck; Is visit ready for int. review?; yes Allocated COS orbits = 12 1628850571000 98.00646372798252 (Tic-Visit :proposal-id 16110 :visit-id "1F" :proposal-version -1 :trans-version "20200619" :date "25-May-2021 10:16:05.0" :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 695920 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16110 :visit-id "1F" :obset-id "1F" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16110 :visit-id "1F" :orbit-number 1 :pcs-time 393 :si-vis-utilization 2534 :al-overhead-at-end 0 :internal-dur-at-end 407 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2927 :pcs-gap 0 ) true 1 0 ETC 1517209 with model spectrum rulup_lya2_etc.txt gives 0.3 sec, round up to 1 sec For BOP check, ETC 1517210 with 4x model spectrum rulup_lya2_x4.00_etc.txt gives 47 cts/sec in brightest pixel and 22,010 cts/sec in brightest stripe. This exceeds the per-stripe count rate limit for irregularly variable sources, but the 4x case is designed to account for variability. It is below the per-stripe count rate limit of 30,000 cts/sec for nonvariable sources. ETC 1517211 with model spectrum rulup_lya2_etc.txt gives 0.2 sec, round up to 1 sec For BOP check, ETC 1517212 with 4x model spectrum rulup_lya2_x4.00_etc.txt gives 47 cts/sec in brightest pixel and 22,010 cts/sec in brightest stripe. This exceeds the per-stripe count rate limit for irregularly variable sources, but the 4x case is designed to account for variability. It is below the per-stripe count rate limit of 30,000 cts/sec for nonvariable sources. ETC 1517209 with model spectrum rulup_lya2_etc.txt gives 0.3 sec, round up to 1 sec For BOP check, ETC 1517210 with 4x model spectrum rulup_lya2_x4.00_etc.txt gives 47 cts/sec in brightest pixel and 22,010 cts/sec in brightest stripe. This exceeds the per-stripe count rate limit for irregularly variable sources, but the 4x case is designed to account for variability. It is below the per-stripe count rate limit of 30,000 cts/sec for nonvariable sources. ETC 1517211 with model spectrum rulup_lya2_etc.txt gives 0.2 sec, round up to 1 sec For BOP check, ETC 1517212 with 4x model spectrum rulup_lya2_x4.00_etc.txt gives 47 cts/sec in brightest pixel and 22,010 cts/sec in brightest stripe. This exceeds the per-stripe count rate limit for irregularly variable sources, but the 4x case is designed to account for variability. It is below the per-stripe count rate limit of 30,000 cts/sec for nonvariable sources. ETC 1517213 with model spectrum rulup_lya2_etc.txt gives 19 sec to reach S/N = 20 at 2820 A, in the continuum near Mg II 2800. Round up to 30 sec. For BOP check, ETC 1517214 with 4x model spectrum rulup_lya2_x4.00_etc.txt gives 47 cts/sec in brightest pixel and 22,010 cts/sec in brightest stripe. This exceeds the per-stripe count rate limit for irregularly variable sources, but the 4x case is designed to account for variability. It is below the per-stripe count rate limit of 30,000 cts/sec for nonvariable sources. BUFFER-TIME set to 80 sec following COS IHB recommendation when exposure time < 80 sec and ETC buffer time > 80 sec. ETC 1517215 with model spectrum rulup_lya2_etc.txt gives 19 sec to reach S/N = 20 at 2820 A, in the continuum near Mg II 2800. Round up to 30 sec. For BOP check, ETC 1517216 with 4x model spectrum rulup_lya2_x4.00_etc.txt gives 47 cts/sec in brightest pixel and 24,480 cts/sec in brightest stripe. This exceeds the per-stripe count rate limit for irregularly variable sources, but the 4x case is designed to account for variability. It is below the per-stripe count rate limit of 30,000 cts/sec for nonvariable sources. BUFFER-TIME set to 80 sec following COS IHB recommendation when exposure time < 80 sec and ETC buffer time > 80 sec. ETC 1517218 with archival spectrum lbgj530b0_etc.txt, a cenwave 1623 spectrum of this star, gives 550 sec to reach S/N = 30 at 1548 A, the peak of C IV. This is 138 sec per G160M exposure; expand to 219 sec to fill the orbit and account for the possibility of a faint state. For BOP check, ETC 1517219 with 4x archival spectrum lbgj530b0_x4.00_etc.txt gives 0.18 cts/sec in brightest pixel and 1279 cts/sec in entire detector. BUFFER-TIME set to 110 sec to guard against a bright state and reduce overheads. ETC 1517218 with archival spectrum lbgj530b0_etc.txt, a cenwave 1623 spectrum of this star, gives 550 sec to reach S/N = 30 at 1548 A, the peak of C IV. This is 138 sec per G160M exposure; expand to 220 sec to fill the orbit and account for the possibility of a faint state. For BOP check, ETC 1517219 with 4x archival spectrum lbgj530b0_x4.00_etc.txt gives 0.18 cts/sec in brightest pixel and 1279 cts/sec in entire detector. BUFFER-TIME set to 110 sec to guard against a bright state and reduce overheads. ETC 1517220 with archival spectrum lbgj530b0_etc.txt, a cenwave 1623 spectrum of this star, gives 549 sec to reach S/N = 30 at 1548 A, the peak of C IV. This is 138 sec per G160M exposure; expand to 220 sec to fill the orbit and account for the possibility of a faint state. For BOP check, ETC 1517221 with 4x archival spectrum lbgj530b0_x4.00_etc.txt gives 0.18 cts/sec in brightest pixel and 1458 cts/sec in entire detector. BUFFER-TIME set to 110 sec to guard against a bright state and reduce overheads. ETC 1517220 with archival spectrum lbgj530b0_etc.txt, a cenwave 1623 spectrum of this star, gives 549 sec to reach S/N = 30 at 1548 A, the peak of C IV. This is 138 sec per G160M exposure; expand to 220 sec to fill the orbit and account for the possibility of a faint state. For BOP check, ETC 1517221 with 4x archival spectrum lbgj530b0_x4.00_etc.txt gives 0.18 cts/sec in brightest pixel and 1458 cts/sec in entire detector. BUFFER-TIME set to 110 sec to guard against a bright state and reduce overheads. 1621952167029 Timing link suitability includes constraints ([1G After 1C by 3.5 to 3.9 days]) The scheduling data was generated by CASM 29.2. CASM was run in Phase II mode. /Users/wfischer/Box/ullyses_tech/ullyses_proposals/monitor/16110/OP-cache/ULLYSES_16110-v1G.xml vstatus; 1C; V-RU-LUP; P/COS approved for submission; P/WF 20/05/21 ; intrev: complete ; P/JRD 24/05/2021 vcheck; Enter targ name & Inst. & Resp. Sci.; RU Lup ; COS ; WF 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?; G230L/2950, repeated to guard against late GS acq vcheck; Possible ACQ or Sci spoilers?; No vcheck; Field BOT clear?; Yes. BOT complains about the target under the assumption it is an O5 star. vcheck; Visual BOT check for stars not in catalog?; nothing visible in DSS 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 (for XMM) vcheck; Is visit ready for int. review?; yes Allocated COS orbits = 12 1628930611000 98.2824961489755 (Tic-Visit :proposal-id 16110 :visit-id "1G" :proposal-version -1 :trans-version "20200619" :date "25-May-2021 10:16:06.0" :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 695920 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16110 :visit-id "1G" :obset-id "1G" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16110 :visit-id "1G" :orbit-number 1 :pcs-time 393 :si-vis-utilization 2534 :al-overhead-at-end 0 :internal-dur-at-end 407 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2927 :pcs-gap 0 ) true 1 0 ETC 1517209 with model spectrum rulup_lya2_etc.txt gives 0.3 sec, round up to 1 sec For BOP check, ETC 1517210 with 4x model spectrum rulup_lya2_x4.00_etc.txt gives 47 cts/sec in brightest pixel and 22,010 cts/sec in brightest stripe. This exceeds the per-stripe count rate limit for irregularly variable sources, but the 4x case is designed to account for variability. It is below the per-stripe count rate limit of 30,000 cts/sec for nonvariable sources. ETC 1517211 with model spectrum rulup_lya2_etc.txt gives 0.2 sec, round up to 1 sec For BOP check, ETC 1517212 with 4x model spectrum rulup_lya2_x4.00_etc.txt gives 47 cts/sec in brightest pixel and 22,010 cts/sec in brightest stripe. This exceeds the per-stripe count rate limit for irregularly variable sources, but the 4x case is designed to account for variability. It is below the per-stripe count rate limit of 30,000 cts/sec for nonvariable sources. ETC 1517209 with model spectrum rulup_lya2_etc.txt gives 0.3 sec, round up to 1 sec For BOP check, ETC 1517210 with 4x model spectrum rulup_lya2_x4.00_etc.txt gives 47 cts/sec in brightest pixel and 22,010 cts/sec in brightest stripe. This exceeds the per-stripe count rate limit for irregularly variable sources, but the 4x case is designed to account for variability. It is below the per-stripe count rate limit of 30,000 cts/sec for nonvariable sources. ETC 1517211 with model spectrum rulup_lya2_etc.txt gives 0.2 sec, round up to 1 sec For BOP check, ETC 1517212 with 4x model spectrum rulup_lya2_x4.00_etc.txt gives 47 cts/sec in brightest pixel and 22,010 cts/sec in brightest stripe. This exceeds the per-stripe count rate limit for irregularly variable sources, but the 4x case is designed to account for variability. It is below the per-stripe count rate limit of 30,000 cts/sec for nonvariable sources. ETC 1517213 with model spectrum rulup_lya2_etc.txt gives 19 sec to reach S/N = 20 at 2820 A, in the continuum near Mg II 2800. Round up to 30 sec. For BOP check, ETC 1517214 with 4x model spectrum rulup_lya2_x4.00_etc.txt gives 47 cts/sec in brightest pixel and 22,010 cts/sec in brightest stripe. This exceeds the per-stripe count rate limit for irregularly variable sources, but the 4x case is designed to account for variability. It is below the per-stripe count rate limit of 30,000 cts/sec for nonvariable sources. BUFFER-TIME set to 80 sec following COS IHB recommendation when exposure time < 80 sec and ETC buffer time > 80 sec. ETC 1517215 with model spectrum rulup_lya2_etc.txt gives 19 sec to reach S/N = 20 at 2820 A, in the continuum near Mg II 2800. Round up to 30 sec. For BOP check, ETC 1517216 with 4x model spectrum rulup_lya2_x4.00_etc.txt gives 47 cts/sec in brightest pixel and 24,480 cts/sec in brightest stripe. This exceeds the per-stripe count rate limit for irregularly variable sources, but the 4x case is designed to account for variability. It is below the per-stripe count rate limit of 30,000 cts/sec for nonvariable sources. BUFFER-TIME set to 80 sec following COS IHB recommendation when exposure time < 80 sec and ETC buffer time > 80 sec. ETC 1517218 with archival spectrum lbgj530b0_etc.txt, a cenwave 1623 spectrum of this star, gives 550 sec to reach S/N = 30 at 1548 A, the peak of C IV. This is 138 sec per G160M exposure; expand to 219 sec to fill the orbit and account for the possibility of a faint state. For BOP check, ETC 1517219 with 4x archival spectrum lbgj530b0_x4.00_etc.txt gives 0.18 cts/sec in brightest pixel and 1279 cts/sec in entire detector. BUFFER-TIME set to 110 sec to guard against a bright state and reduce overheads. ETC 1517218 with archival spectrum lbgj530b0_etc.txt, a cenwave 1623 spectrum of this star, gives 550 sec to reach S/N = 30 at 1548 A, the peak of C IV. This is 138 sec per G160M exposure; expand to 220 sec to fill the orbit and account for the possibility of a faint state. For BOP check, ETC 1517219 with 4x archival spectrum lbgj530b0_x4.00_etc.txt gives 0.18 cts/sec in brightest pixel and 1279 cts/sec in entire detector. BUFFER-TIME set to 110 sec to guard against a bright state and reduce overheads. ETC 1517220 with archival spectrum lbgj530b0_etc.txt, a cenwave 1623 spectrum of this star, gives 549 sec to reach S/N = 30 at 1548 A, the peak of C IV. This is 138 sec per G160M exposure; expand to 220 sec to fill the orbit and account for the possibility of a faint state. For BOP check, ETC 1517221 with 4x archival spectrum lbgj530b0_x4.00_etc.txt gives 0.18 cts/sec in brightest pixel and 1458 cts/sec in entire detector. BUFFER-TIME set to 110 sec to guard against a bright state and reduce overheads. ETC 1517220 with archival spectrum lbgj530b0_etc.txt, a cenwave 1623 spectrum of this star, gives 549 sec to reach S/N = 30 at 1548 A, the peak of C IV. This is 138 sec per G160M exposure; expand to 220 sec to fill the orbit and account for the possibility of a faint state. For BOP check, ETC 1517221 with 4x archival spectrum lbgj530b0_x4.00_etc.txt gives 0.18 cts/sec in brightest pixel and 1458 cts/sec in entire detector. BUFFER-TIME set to 110 sec to guard against a bright state and reduce overheads. 1621952168244 Timing link suitability includes constraints ([1H After 1C by 4.4 to 4.8 days]) The scheduling data was generated by CASM 29.2. CASM was run in Phase II mode. /Users/wfischer/Box/ullyses_tech/ullyses_proposals/monitor/16110/OP-cache/ULLYSES_16110-v1H.xml vstatus; 1C; V-RU-LUP; P/COS approved for submissionw; P/WF 20/05/21 ;intrev: complete ; P/JRD 24/05/2021 vcheck; Enter targ name & Inst. & Resp. Sci.; RU Lup ; COS ; WF 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?; G230L/2950, repeated to guard against late GS acq vcheck; Possible ACQ or Sci spoilers?; No vcheck; Field BOT clear?; Yes. BOT complains about the target under the assumption it is an O5 star. vcheck; Visual BOT check for stars not in catalog?; nothing visible in DSS 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 (for XMM) vcheck; Is visit ready for int. review?; yes Allocated COS orbits = 12 1629016368000 98.57625424737131 (Tic-Visit :proposal-id 16110 :visit-id "1H" :proposal-version -1 :trans-version "20200619" :date "25-May-2021 10:16:08.0" :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 695920 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16110 :visit-id "1H" :obset-id "1H" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16110 :visit-id "1H" :orbit-number 1 :pcs-time 393 :si-vis-utilization 2534 :al-overhead-at-end 0 :internal-dur-at-end 407 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2927 :pcs-gap 0 ) true 1 0 ETC 1517209 with model spectrum rulup_lya2_etc.txt gives 0.3 sec, round up to 1 sec For BOP check, ETC 1517210 with 4x model spectrum rulup_lya2_x4.00_etc.txt gives 47 cts/sec in brightest pixel and 22,010 cts/sec in brightest stripe. This exceeds the per-stripe count rate limit for irregularly variable sources, but the 4x case is designed to account for variability. It is below the per-stripe count rate limit of 30,000 cts/sec for nonvariable sources. ETC 1517211 with model spectrum rulup_lya2_etc.txt gives 0.2 sec, round up to 1 sec For BOP check, ETC 1517212 with 4x model spectrum rulup_lya2_x4.00_etc.txt gives 47 cts/sec in brightest pixel and 22,010 cts/sec in brightest stripe. This exceeds the per-stripe count rate limit for irregularly variable sources, but the 4x case is designed to account for variability. It is below the per-stripe count rate limit of 30,000 cts/sec for nonvariable sources. ETC 1517209 with model spectrum rulup_lya2_etc.txt gives 0.3 sec, round up to 1 sec For BOP check, ETC 1517210 with 4x model spectrum rulup_lya2_x4.00_etc.txt gives 47 cts/sec in brightest pixel and 22,010 cts/sec in brightest stripe. This exceeds the per-stripe count rate limit for irregularly variable sources, but the 4x case is designed to account for variability. It is below the per-stripe count rate limit of 30,000 cts/sec for nonvariable sources. ETC 1517211 with model spectrum rulup_lya2_etc.txt gives 0.2 sec, round up to 1 sec For BOP check, ETC 1517212 with 4x model spectrum rulup_lya2_x4.00_etc.txt gives 47 cts/sec in brightest pixel and 22,010 cts/sec in brightest stripe. This exceeds the per-stripe count rate limit for irregularly variable sources, but the 4x case is designed to account for variability. It is below the per-stripe count rate limit of 30,000 cts/sec for nonvariable sources. ETC 1517213 with model spectrum rulup_lya2_etc.txt gives 19 sec to reach S/N = 20 at 2820 A, in the continuum near Mg II 2800. Round up to 30 sec. For BOP check, ETC 1517214 with 4x model spectrum rulup_lya2_x4.00_etc.txt gives 47 cts/sec in brightest pixel and 22,010 cts/sec in brightest stripe. This exceeds the per-stripe count rate limit for irregularly variable sources, but the 4x case is designed to account for variability. It is below the per-stripe count rate limit of 30,000 cts/sec for nonvariable sources. BUFFER-TIME set to 80 sec following COS IHB recommendation when exposure time < 80 sec and ETC buffer time > 80 sec. ETC 1517215 with model spectrum rulup_lya2_etc.txt gives 19 sec to reach S/N = 20 at 2820 A, in the continuum near Mg II 2800. Round up to 30 sec. For BOP check, ETC 1517216 with 4x model spectrum rulup_lya2_x4.00_etc.txt gives 47 cts/sec in brightest pixel and 24,480 cts/sec in brightest stripe. This exceeds the per-stripe count rate limit for irregularly variable sources, but the 4x case is designed to account for variability. It is below the per-stripe count rate limit of 30,000 cts/sec for nonvariable sources. BUFFER-TIME set to 80 sec following COS IHB recommendation when exposure time < 80 sec and ETC buffer time > 80 sec. ETC 1517218 with archival spectrum lbgj530b0_etc.txt, a cenwave 1623 spectrum of this star, gives 550 sec to reach S/N = 30 at 1548 A, the peak of C IV. This is 138 sec per G160M exposure; expand to 219 sec to fill the orbit and account for the possibility of a faint state. For BOP check, ETC 1517219 with 4x archival spectrum lbgj530b0_x4.00_etc.txt gives 0.18 cts/sec in brightest pixel and 1279 cts/sec in entire detector. BUFFER-TIME set to 110 sec to guard against a bright state and reduce overheads. ETC 1517218 with archival spectrum lbgj530b0_etc.txt, a cenwave 1623 spectrum of this star, gives 550 sec to reach S/N = 30 at 1548 A, the peak of C IV. This is 138 sec per G160M exposure; expand to 220 sec to fill the orbit and account for the possibility of a faint state. For BOP check, ETC 1517219 with 4x archival spectrum lbgj530b0_x4.00_etc.txt gives 0.18 cts/sec in brightest pixel and 1279 cts/sec in entire detector. BUFFER-TIME set to 110 sec to guard against a bright state and reduce overheads. ETC 1517220 with archival spectrum lbgj530b0_etc.txt, a cenwave 1623 spectrum of this star, gives 549 sec to reach S/N = 30 at 1548 A, the peak of C IV. This is 138 sec per G160M exposure; expand to 220 sec to fill the orbit and account for the possibility of a faint state. For BOP check, ETC 1517221 with 4x archival spectrum lbgj530b0_x4.00_etc.txt gives 0.18 cts/sec in brightest pixel and 1458 cts/sec in entire detector. BUFFER-TIME set to 110 sec to guard against a bright state and reduce overheads. ETC 1517220 with archival spectrum lbgj530b0_etc.txt, a cenwave 1623 spectrum of this star, gives 549 sec to reach S/N = 30 at 1548 A, the peak of C IV. This is 138 sec per G160M exposure; expand to 220 sec to fill the orbit and account for the possibility of a faint state. For BOP check, ETC 1517221 with 4x archival spectrum lbgj530b0_x4.00_etc.txt gives 0.18 cts/sec in brightest pixel and 1458 cts/sec in entire detector. BUFFER-TIME set to 110 sec to guard against a bright state and reduce overheads. 1621952170509 Timing link suitability includes constraints ([1I After 1C by 5.4 to 5.8 days]) The scheduling data was generated by CASM 29.2. CASM was run in Phase II mode. /Users/wfischer/Box/ullyses_tech/ullyses_proposals/monitor/16110/OP-cache/ULLYSES_16110-v1I.xml vstatus; 1C; V-RU-LUP; P/COS approved for submission; P/WF 20/05/21 ; intrev: complete ; P/JRD 24/05/2021 vcheck; Enter targ name & Inst. & Resp. Sci.; RU Lup ; COS ; WF 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?; G230L/2950, repeated to guard against late GS acq vcheck; Possible ACQ or Sci spoilers?; No vcheck; Field BOT clear?; Yes. BOT complains about the target under the assumption it is an O5 star. vcheck; Visual BOT check for stars not in catalog?; nothing visible in DSS 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 (for XMM) vcheck; Is visit ready for int. review?; yes Allocated COS orbits = 12 1629107842000 98.887513391418 (Tic-Visit :proposal-id 16110 :visit-id "1I" :proposal-version -1 :trans-version "20200619" :date "25-May-2021 10:16:10.0" :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 695920 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16110 :visit-id "1I" :obset-id "1I" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16110 :visit-id "1I" :orbit-number 1 :pcs-time 393 :si-vis-utilization 2534 :al-overhead-at-end 0 :internal-dur-at-end 407 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2927 :pcs-gap 0 ) true 1 0 ETC 1517209 with model spectrum rulup_lya2_etc.txt gives 0.3 sec, round up to 1 sec For BOP check, ETC 1517210 with 4x model spectrum rulup_lya2_x4.00_etc.txt gives 47 cts/sec in brightest pixel and 22,010 cts/sec in brightest stripe. This exceeds the per-stripe count rate limit for irregularly variable sources, but the 4x case is designed to account for variability. It is below the per-stripe count rate limit of 30,000 cts/sec for nonvariable sources. ETC 1517211 with model spectrum rulup_lya2_etc.txt gives 0.2 sec, round up to 1 sec For BOP check, ETC 1517212 with 4x model spectrum rulup_lya2_x4.00_etc.txt gives 47 cts/sec in brightest pixel and 22,010 cts/sec in brightest stripe. This exceeds the per-stripe count rate limit for irregularly variable sources, but the 4x case is designed to account for variability. It is below the per-stripe count rate limit of 30,000 cts/sec for nonvariable sources. ETC 1517209 with model spectrum rulup_lya2_etc.txt gives 0.3 sec, round up to 1 sec For BOP check, ETC 1517210 with 4x model spectrum rulup_lya2_x4.00_etc.txt gives 47 cts/sec in brightest pixel and 22,010 cts/sec in brightest stripe. This exceeds the per-stripe count rate limit for irregularly variable sources, but the 4x case is designed to account for variability. It is below the per-stripe count rate limit of 30,000 cts/sec for nonvariable sources. ETC 1517211 with model spectrum rulup_lya2_etc.txt gives 0.2 sec, round up to 1 sec For BOP check, ETC 1517212 with 4x model spectrum rulup_lya2_x4.00_etc.txt gives 47 cts/sec in brightest pixel and 22,010 cts/sec in brightest stripe. This exceeds the per-stripe count rate limit for irregularly variable sources, but the 4x case is designed to account for variability. It is below the per-stripe count rate limit of 30,000 cts/sec for nonvariable sources. ETC 1517213 with model spectrum rulup_lya2_etc.txt gives 19 sec to reach S/N = 20 at 2820 A, in the continuum near Mg II 2800. Round up to 30 sec. For BOP check, ETC 1517214 with 4x model spectrum rulup_lya2_x4.00_etc.txt gives 47 cts/sec in brightest pixel and 22,010 cts/sec in brightest stripe. This exceeds the per-stripe count rate limit for irregularly variable sources, but the 4x case is designed to account for variability. It is below the per-stripe count rate limit of 30,000 cts/sec for nonvariable sources. BUFFER-TIME set to 80 sec following COS IHB recommendation when exposure time < 80 sec and ETC buffer time > 80 sec. ETC 1517215 with model spectrum rulup_lya2_etc.txt gives 19 sec to reach S/N = 20 at 2820 A, in the continuum near Mg II 2800. Round up to 30 sec. For BOP check, ETC 1517216 with 4x model spectrum rulup_lya2_x4.00_etc.txt gives 47 cts/sec in brightest pixel and 24,480 cts/sec in brightest stripe. This exceeds the per-stripe count rate limit for irregularly variable sources, but the 4x case is designed to account for variability. It is below the per-stripe count rate limit of 30,000 cts/sec for nonvariable sources. BUFFER-TIME set to 80 sec following COS IHB recommendation when exposure time < 80 sec and ETC buffer time > 80 sec. ETC 1517218 with archival spectrum lbgj530b0_etc.txt, a cenwave 1623 spectrum of this star, gives 550 sec to reach S/N = 30 at 1548 A, the peak of C IV. This is 138 sec per G160M exposure; expand to 219 sec to fill the orbit and account for the possibility of a faint state. For BOP check, ETC 1517219 with 4x archival spectrum lbgj530b0_x4.00_etc.txt gives 0.18 cts/sec in brightest pixel and 1279 cts/sec in entire detector. BUFFER-TIME set to 110 sec to guard against a bright state and reduce overheads. ETC 1517218 with archival spectrum lbgj530b0_etc.txt, a cenwave 1623 spectrum of this star, gives 550 sec to reach S/N = 30 at 1548 A, the peak of C IV. This is 138 sec per G160M exposure; expand to 220 sec to fill the orbit and account for the possibility of a faint state. For BOP check, ETC 1517219 with 4x archival spectrum lbgj530b0_x4.00_etc.txt gives 0.18 cts/sec in brightest pixel and 1279 cts/sec in entire detector. BUFFER-TIME set to 110 sec to guard against a bright state and reduce overheads. ETC 1517220 with archival spectrum lbgj530b0_etc.txt, a cenwave 1623 spectrum of this star, gives 549 sec to reach S/N = 30 at 1548 A, the peak of C IV. This is 138 sec per G160M exposure; expand to 220 sec to fill the orbit and account for the possibility of a faint state. For BOP check, ETC 1517221 with 4x archival spectrum lbgj530b0_x4.00_etc.txt gives 0.18 cts/sec in brightest pixel and 1458 cts/sec in entire detector. BUFFER-TIME set to 110 sec to guard against a bright state and reduce overheads. ETC 1517220 with archival spectrum lbgj530b0_etc.txt, a cenwave 1623 spectrum of this star, gives 549 sec to reach S/N = 30 at 1548 A, the peak of C IV. This is 138 sec per G160M exposure; expand to 220 sec to fill the orbit and account for the possibility of a faint state. For BOP check, ETC 1517221 with 4x archival spectrum lbgj530b0_x4.00_etc.txt gives 0.18 cts/sec in brightest pixel and 1458 cts/sec in entire detector. BUFFER-TIME set to 110 sec to guard against a bright state and reduce overheads. 1621952172456 Timing link suitability includes constraints ([1J After 1C by 6.3 to 6.7 days]) The scheduling data was generated by CASM 29.2. CASM was run in Phase II mode. /Users/wfischer/Box/ullyses_tech/ullyses_proposals/monitor/16110/OP-cache/ULLYSES_16110-v1J.xml vstatus; 1C; V-RU-LUP; P/COS approved for submission; P/WF 20/05/21 ; intrev: complete ; P/JRD 24/05/2021 vcheck; Enter targ name & Inst. & Resp. Sci.; RU Lup ; COS ; WF 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?; G230L/2950, repeated to guard against late GS acq vcheck; Possible ACQ or Sci spoilers?; No vcheck; Field BOT clear?; Yes. BOT complains about the target under the assumption it is an O5 star. vcheck; Visual BOT check for stars not in catalog?; nothing visible in DSS 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 (for XMM) vcheck; Is visit ready for int. review?; yes Allocated COS orbits = 12 1629193598000 99.17754085604662 (Tic-Visit :proposal-id 16110 :visit-id "1J" :proposal-version -1 :trans-version "20200619" :date "25-May-2021 10:16:12.0" :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 695920 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16110 :visit-id "1J" :obset-id "1J" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16110 :visit-id "1J" :orbit-number 1 :pcs-time 393 :si-vis-utilization 2534 :al-overhead-at-end 0 :internal-dur-at-end 407 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2927 :pcs-gap 0 ) true 1 0 ETC 1517209 with model spectrum rulup_lya2_etc.txt gives 0.3 sec, round up to 1 sec For BOP check, ETC 1517210 with 4x model spectrum rulup_lya2_x4.00_etc.txt gives 47 cts/sec in brightest pixel and 22,010 cts/sec in brightest stripe. This exceeds the per-stripe count rate limit for irregularly variable sources, but the 4x case is designed to account for variability. It is below the per-stripe count rate limit of 30,000 cts/sec for nonvariable sources. ETC 1517211 with model spectrum rulup_lya2_etc.txt gives 0.2 sec, round up to 1 sec For BOP check, ETC 1517212 with 4x model spectrum rulup_lya2_x4.00_etc.txt gives 47 cts/sec in brightest pixel and 22,010 cts/sec in brightest stripe. This exceeds the per-stripe count rate limit for irregularly variable sources, but the 4x case is designed to account for variability. It is below the per-stripe count rate limit of 30,000 cts/sec for nonvariable sources. ETC 1517209 with model spectrum rulup_lya2_etc.txt gives 0.3 sec, round up to 1 sec For BOP check, ETC 1517210 with 4x model spectrum rulup_lya2_x4.00_etc.txt gives 47 cts/sec in brightest pixel and 22,010 cts/sec in brightest stripe. This exceeds the per-stripe count rate limit for irregularly variable sources, but the 4x case is designed to account for variability. It is below the per-stripe count rate limit of 30,000 cts/sec for nonvariable sources. ETC 1517211 with model spectrum rulup_lya2_etc.txt gives 0.2 sec, round up to 1 sec For BOP check, ETC 1517212 with 4x model spectrum rulup_lya2_x4.00_etc.txt gives 47 cts/sec in brightest pixel and 22,010 cts/sec in brightest stripe. This exceeds the per-stripe count rate limit for irregularly variable sources, but the 4x case is designed to account for variability. It is below the per-stripe count rate limit of 30,000 cts/sec for nonvariable sources. ETC 1517213 with model spectrum rulup_lya2_etc.txt gives 19 sec to reach S/N = 20 at 2820 A, in the continuum near Mg II 2800. Round up to 30 sec. For BOP check, ETC 1517214 with 4x model spectrum rulup_lya2_x4.00_etc.txt gives 47 cts/sec in brightest pixel and 22,010 cts/sec in brightest stripe. This exceeds the per-stripe count rate limit for irregularly variable sources, but the 4x case is designed to account for variability. It is below the per-stripe count rate limit of 30,000 cts/sec for nonvariable sources. BUFFER-TIME set to 80 sec following COS IHB recommendation when exposure time < 80 sec and ETC buffer time > 80 sec. ETC 1517215 with model spectrum rulup_lya2_etc.txt gives 19 sec to reach S/N = 20 at 2820 A, in the continuum near Mg II 2800. Round up to 30 sec. For BOP check, ETC 1517216 with 4x model spectrum rulup_lya2_x4.00_etc.txt gives 47 cts/sec in brightest pixel and 24,480 cts/sec in brightest stripe. This exceeds the per-stripe count rate limit for irregularly variable sources, but the 4x case is designed to account for variability. It is below the per-stripe count rate limit of 30,000 cts/sec for nonvariable sources. BUFFER-TIME set to 80 sec following COS IHB recommendation when exposure time < 80 sec and ETC buffer time > 80 sec. ETC 1517218 with archival spectrum lbgj530b0_etc.txt, a cenwave 1623 spectrum of this star, gives 550 sec to reach S/N = 30 at 1548 A, the peak of C IV. This is 138 sec per G160M exposure; expand to 219 sec to fill the orbit and account for the possibility of a faint state. For BOP check, ETC 1517219 with 4x archival spectrum lbgj530b0_x4.00_etc.txt gives 0.18 cts/sec in brightest pixel and 1279 cts/sec in entire detector. BUFFER-TIME set to 110 sec to guard against a bright state and reduce overheads. ETC 1517218 with archival spectrum lbgj530b0_etc.txt, a cenwave 1623 spectrum of this star, gives 550 sec to reach S/N = 30 at 1548 A, the peak of C IV. This is 138 sec per G160M exposure; expand to 220 sec to fill the orbit and account for the possibility of a faint state. For BOP check, ETC 1517219 with 4x archival spectrum lbgj530b0_x4.00_etc.txt gives 0.18 cts/sec in brightest pixel and 1279 cts/sec in entire detector. BUFFER-TIME set to 110 sec to guard against a bright state and reduce overheads. ETC 1517220 with archival spectrum lbgj530b0_etc.txt, a cenwave 1623 spectrum of this star, gives 549 sec to reach S/N = 30 at 1548 A, the peak of C IV. This is 138 sec per G160M exposure; expand to 220 sec to fill the orbit and account for the possibility of a faint state. For BOP check, ETC 1517221 with 4x archival spectrum lbgj530b0_x4.00_etc.txt gives 0.18 cts/sec in brightest pixel and 1458 cts/sec in entire detector. BUFFER-TIME set to 110 sec to guard against a bright state and reduce overheads. ETC 1517220 with archival spectrum lbgj530b0_etc.txt, a cenwave 1623 spectrum of this star, gives 549 sec to reach S/N = 30 at 1548 A, the peak of C IV. This is 138 sec per G160M exposure; expand to 220 sec to fill the orbit and account for the possibility of a faint state. For BOP check, ETC 1517221 with 4x archival spectrum lbgj530b0_x4.00_etc.txt gives 0.18 cts/sec in brightest pixel and 1458 cts/sec in entire detector. BUFFER-TIME set to 110 sec to guard against a bright state and reduce overheads. 1621952173647 Timing link suitability includes constraints ([1K After 1C by 7.2 to 7.6 days]) The scheduling data was generated by CASM 29.2. CASM was run in Phase II mode. /Users/wfischer/Box/ullyses_tech/ullyses_proposals/monitor/16110/OP-cache/ULLYSES_16110-v1K.xml vstatus; 1C; V-RU-LUP; P/COS approved for submission; P/WF 20/05/21 ; intrev: complete ; P/JRD 24/05/2021 vcheck; Enter targ name & Inst. & Resp. Sci.; RU Lup ; COS ; WF 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?; G230L/2950, repeated to guard against late GS acq vcheck; Possible ACQ or Sci spoilers?; No vcheck; Field BOT clear?; Yes. BOT complains about the target under the assumption it is an O5 star. vcheck; Visual BOT check for stars not in catalog?; nothing visible in DSS 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 (for XMM) vcheck; Is visit ready for int. review?; yes Allocated COS orbits = 12 1629267920000 99.42764054797868 (Tic-Visit :proposal-id 16110 :visit-id "1K" :proposal-version -1 :trans-version "20200619" :date "25-May-2021 10:16:13.0" :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 695920 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16110 :visit-id "1K" :obset-id "1K" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16110 :visit-id "1K" :orbit-number 1 :pcs-time 393 :si-vis-utilization 2534 :al-overhead-at-end 0 :internal-dur-at-end 407 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2927 :pcs-gap 0 ) true 1 0 ETC 1517209 with model spectrum rulup_lya2_etc.txt gives 0.3 sec, round up to 1 sec For BOP check, ETC 1517210 with 4x model spectrum rulup_lya2_x4.00_etc.txt gives 47 cts/sec in brightest pixel and 22,010 cts/sec in brightest stripe. This exceeds the per-stripe count rate limit for irregularly variable sources, but the 4x case is designed to account for variability. It is below the per-stripe count rate limit of 30,000 cts/sec for nonvariable sources. ETC 1517211 with model spectrum rulup_lya2_etc.txt gives 0.2 sec, round up to 1 sec For BOP check, ETC 1517212 with 4x model spectrum rulup_lya2_x4.00_etc.txt gives 47 cts/sec in brightest pixel and 22,010 cts/sec in brightest stripe. This exceeds the per-stripe count rate limit for irregularly variable sources, but the 4x case is designed to account for variability. It is below the per-stripe count rate limit of 30,000 cts/sec for nonvariable sources. ETC 1517209 with model spectrum rulup_lya2_etc.txt gives 0.3 sec, round up to 1 sec For BOP check, ETC 1517210 with 4x model spectrum rulup_lya2_x4.00_etc.txt gives 47 cts/sec in brightest pixel and 22,010 cts/sec in brightest stripe. This exceeds the per-stripe count rate limit for irregularly variable sources, but the 4x case is designed to account for variability. It is below the per-stripe count rate limit of 30,000 cts/sec for nonvariable sources. ETC 1517211 with model spectrum rulup_lya2_etc.txt gives 0.2 sec, round up to 1 sec For BOP check, ETC 1517212 with 4x model spectrum rulup_lya2_x4.00_etc.txt gives 47 cts/sec in brightest pixel and 22,010 cts/sec in brightest stripe. This exceeds the per-stripe count rate limit for irregularly variable sources, but the 4x case is designed to account for variability. It is below the per-stripe count rate limit of 30,000 cts/sec for nonvariable sources. ETC 1517213 with model spectrum rulup_lya2_etc.txt gives 19 sec to reach S/N = 20 at 2820 A, in the continuum near Mg II 2800. Round up to 30 sec. For BOP check, ETC 1517214 with 4x model spectrum rulup_lya2_x4.00_etc.txt gives 47 cts/sec in brightest pixel and 22,010 cts/sec in brightest stripe. This exceeds the per-stripe count rate limit for irregularly variable sources, but the 4x case is designed to account for variability. It is below the per-stripe count rate limit of 30,000 cts/sec for nonvariable sources. BUFFER-TIME set to 80 sec following COS IHB recommendation when exposure time < 80 sec and ETC buffer time > 80 sec. ETC 1517215 with model spectrum rulup_lya2_etc.txt gives 19 sec to reach S/N = 20 at 2820 A, in the continuum near Mg II 2800. Round up to 30 sec. For BOP check, ETC 1517216 with 4x model spectrum rulup_lya2_x4.00_etc.txt gives 47 cts/sec in brightest pixel and 24,480 cts/sec in brightest stripe. This exceeds the per-stripe count rate limit for irregularly variable sources, but the 4x case is designed to account for variability. It is below the per-stripe count rate limit of 30,000 cts/sec for nonvariable sources. BUFFER-TIME set to 80 sec following COS IHB recommendation when exposure time < 80 sec and ETC buffer time > 80 sec. ETC 1517218 with archival spectrum lbgj530b0_etc.txt, a cenwave 1623 spectrum of this star, gives 550 sec to reach S/N = 30 at 1548 A, the peak of C IV. This is 138 sec per G160M exposure; expand to 219 sec to fill the orbit and account for the possibility of a faint state. For BOP check, ETC 1517219 with 4x archival spectrum lbgj530b0_x4.00_etc.txt gives 0.18 cts/sec in brightest pixel and 1279 cts/sec in entire detector. BUFFER-TIME set to 110 sec to guard against a bright state and reduce overheads. ETC 1517218 with archival spectrum lbgj530b0_etc.txt, a cenwave 1623 spectrum of this star, gives 550 sec to reach S/N = 30 at 1548 A, the peak of C IV. This is 138 sec per G160M exposure; expand to 220 sec to fill the orbit and account for the possibility of a faint state. For BOP check, ETC 1517219 with 4x archival spectrum lbgj530b0_x4.00_etc.txt gives 0.18 cts/sec in brightest pixel and 1279 cts/sec in entire detector. BUFFER-TIME set to 110 sec to guard against a bright state and reduce overheads. ETC 1517220 with archival spectrum lbgj530b0_etc.txt, a cenwave 1623 spectrum of this star, gives 549 sec to reach S/N = 30 at 1548 A, the peak of C IV. This is 138 sec per G160M exposure; expand to 220 sec to fill the orbit and account for the possibility of a faint state. For BOP check, ETC 1517221 with 4x archival spectrum lbgj530b0_x4.00_etc.txt gives 0.18 cts/sec in brightest pixel and 1458 cts/sec in entire detector. BUFFER-TIME set to 110 sec to guard against a bright state and reduce overheads. ETC 1517220 with archival spectrum lbgj530b0_etc.txt, a cenwave 1623 spectrum of this star, gives 549 sec to reach S/N = 30 at 1548 A, the peak of C IV. This is 138 sec per G160M exposure; expand to 220 sec to fill the orbit and account for the possibility of a faint state. For BOP check, ETC 1517221 with 4x archival spectrum lbgj530b0_x4.00_etc.txt gives 0.18 cts/sec in brightest pixel and 1458 cts/sec in entire detector. BUFFER-TIME set to 110 sec to guard against a bright state and reduce overheads. 1621952175761 Timing link suitability includes constraints ([1L After 1C by 8.1 to 8.6 days]) The scheduling data was generated by CASM 29.2. CASM was run in Phase II mode. /Users/wfischer/Box/ullyses_tech/ullyses_proposals/monitor/16110/OP-cache/ULLYSES_16110-v1L.xml vstatus; 1C; V-RU-LUP; P/COS approved for submission; P/WF 20/05/21 ;intrev: complete ; P/JRD 24/05/2021 vcheck; Enter targ name & Inst. & Resp. Sci.; RU Lup ; COS ; WF 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?; G230L/2950, repeated to guard against late GS acq vcheck; Possible ACQ or Sci spoilers?; No vcheck; Field BOT clear?; Yes. BOT complains about the target under the assumption it is an O5 star. vcheck; Visual BOT check for stars not in catalog?; nothing visible in DSS 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 (for XMM) vcheck; Is visit ready for int. review?; yes Allocated COS orbits = 12 1629353676000 99.71491059831129 (Tic-Visit :proposal-id 16110 :visit-id "1L" :proposal-version -1 :trans-version "20200619" :date "25-May-2021 10:16:15.0" :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 695920 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16110 :visit-id "1L" :obset-id "1L" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16110 :visit-id "1L" :orbit-number 1 :pcs-time 393 :si-vis-utilization 2534 :al-overhead-at-end 0 :internal-dur-at-end 407 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2927 :pcs-gap 0 ) true 1 0 ETC 1517209 with model spectrum rulup_lya2_etc.txt gives 0.3 sec, round up to 1 sec For BOP check, ETC 1517210 with 4x model spectrum rulup_lya2_x4.00_etc.txt gives 47 cts/sec in brightest pixel and 22,010 cts/sec in brightest stripe. This exceeds the per-stripe count rate limit for irregularly variable sources, but the 4x case is designed to account for variability. It is below the per-stripe count rate limit of 30,000 cts/sec for nonvariable sources. ETC 1517211 with model spectrum rulup_lya2_etc.txt gives 0.2 sec, round up to 1 sec For BOP check, ETC 1517212 with 4x model spectrum rulup_lya2_x4.00_etc.txt gives 47 cts/sec in brightest pixel and 22,010 cts/sec in brightest stripe. This exceeds the per-stripe count rate limit for irregularly variable sources, but the 4x case is designed to account for variability. It is below the per-stripe count rate limit of 30,000 cts/sec for nonvariable sources. ETC 1517209 with model spectrum rulup_lya2_etc.txt gives 0.3 sec, round up to 1 sec For BOP check, ETC 1517210 with 4x model spectrum rulup_lya2_x4.00_etc.txt gives 47 cts/sec in brightest pixel and 22,010 cts/sec in brightest stripe. This exceeds the per-stripe count rate limit for irregularly variable sources, but the 4x case is designed to account for variability. It is below the per-stripe count rate limit of 30,000 cts/sec for nonvariable sources. ETC 1517211 with model spectrum rulup_lya2_etc.txt gives 0.2 sec, round up to 1 sec For BOP check, ETC 1517212 with 4x model spectrum rulup_lya2_x4.00_etc.txt gives 47 cts/sec in brightest pixel and 22,010 cts/sec in brightest stripe. This exceeds the per-stripe count rate limit for irregularly variable sources, but the 4x case is designed to account for variability. It is below the per-stripe count rate limit of 30,000 cts/sec for nonvariable sources. ETC 1517213 with model spectrum rulup_lya2_etc.txt gives 19 sec to reach S/N = 20 at 2820 A, in the continuum near Mg II 2800. Round up to 30 sec. For BOP check, ETC 1517214 with 4x model spectrum rulup_lya2_x4.00_etc.txt gives 47 cts/sec in brightest pixel and 22,010 cts/sec in brightest stripe. This exceeds the per-stripe count rate limit for irregularly variable sources, but the 4x case is designed to account for variability. It is below the per-stripe count rate limit of 30,000 cts/sec for nonvariable sources. BUFFER-TIME set to 80 sec following COS IHB recommendation when exposure time < 80 sec and ETC buffer time > 80 sec. ETC 1517215 with model spectrum rulup_lya2_etc.txt gives 19 sec to reach S/N = 20 at 2820 A, in the continuum near Mg II 2800. Round up to 30 sec. For BOP check, ETC 1517216 with 4x model spectrum rulup_lya2_x4.00_etc.txt gives 47 cts/sec in brightest pixel and 24,480 cts/sec in brightest stripe. This exceeds the per-stripe count rate limit for irregularly variable sources, but the 4x case is designed to account for variability. It is below the per-stripe count rate limit of 30,000 cts/sec for nonvariable sources. BUFFER-TIME set to 80 sec following COS IHB recommendation when exposure time < 80 sec and ETC buffer time > 80 sec. ETC 1517218 with archival spectrum lbgj530b0_etc.txt, a cenwave 1623 spectrum of this star, gives 550 sec to reach S/N = 30 at 1548 A, the peak of C IV. This is 138 sec per G160M exposure; expand to 219 sec to fill the orbit and account for the possibility of a faint state. For BOP check, ETC 1517219 with 4x archival spectrum lbgj530b0_x4.00_etc.txt gives 0.18 cts/sec in brightest pixel and 1279 cts/sec in entire detector. BUFFER-TIME set to 110 sec to guard against a bright state and reduce overheads. ETC 1517218 with archival spectrum lbgj530b0_etc.txt, a cenwave 1623 spectrum of this star, gives 550 sec to reach S/N = 30 at 1548 A, the peak of C IV. This is 138 sec per G160M exposure; expand to 220 sec to fill the orbit and account for the possibility of a faint state. For BOP check, ETC 1517219 with 4x archival spectrum lbgj530b0_x4.00_etc.txt gives 0.18 cts/sec in brightest pixel and 1279 cts/sec in entire detector. BUFFER-TIME set to 110 sec to guard against a bright state and reduce overheads. ETC 1517220 with archival spectrum lbgj530b0_etc.txt, a cenwave 1623 spectrum of this star, gives 549 sec to reach S/N = 30 at 1548 A, the peak of C IV. This is 138 sec per G160M exposure; expand to 220 sec to fill the orbit and account for the possibility of a faint state. For BOP check, ETC 1517221 with 4x archival spectrum lbgj530b0_x4.00_etc.txt gives 0.18 cts/sec in brightest pixel and 1458 cts/sec in entire detector. BUFFER-TIME set to 110 sec to guard against a bright state and reduce overheads. ETC 1517220 with archival spectrum lbgj530b0_etc.txt, a cenwave 1623 spectrum of this star, gives 549 sec to reach S/N = 30 at 1548 A, the peak of C IV. This is 138 sec per G160M exposure; expand to 220 sec to fill the orbit and account for the possibility of a faint state. For BOP check, ETC 1517221 with 4x archival spectrum lbgj530b0_x4.00_etc.txt gives 0.18 cts/sec in brightest pixel and 1458 cts/sec in entire detector. BUFFER-TIME set to 110 sec to guard against a bright state and reduce overheads. 1621952177823 Timing link suitability includes constraints ([1M After 1C by 9.1 to 9.5 days]) The scheduling data was generated by CASM 29.2. CASM was run in Phase II mode. /Users/wfischer/Box/ullyses_tech/ullyses_proposals/monitor/16110/OP-cache/ULLYSES_16110-v1M.xml vstatus; 1C; V-RU-LUP; P/COS approved for submission; P/WF 20/05/21 ; intrev: complete ; P/JRD 24/05/2021 vcheck; Enter targ name & Inst. & Resp. Sci.; RU Lup ; COS ; WF 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?; G230L/2950, repeated to guard against late GS acq vcheck; Possible ACQ or Sci spoilers?; No vcheck; Field BOT clear?; Yes. BOT complains about the target under the assumption it is an O5 star. vcheck; Visual BOT check for stars not in catalog?; nothing visible in DSS 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 (for XMM) vcheck; Is visit ready for int. review?; yes Allocated COS orbits = 12 1629439432000 100.00093685279279 (Tic-Visit :proposal-id 16110 :visit-id "1M" :proposal-version -1 :trans-version "20200619" :date "25-May-2021 10:16:17.0" :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 695920 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16110 :visit-id "1M" :obset-id "1M" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16110 :visit-id "1M" :orbit-number 1 :pcs-time 393 :si-vis-utilization 2534 :al-overhead-at-end 0 :internal-dur-at-end 407 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2927 :pcs-gap 0 ) true 1 0 ETC 1517209 with model spectrum rulup_lya2_etc.txt gives 0.3 sec, round up to 1 sec For BOP check, ETC 1517210 with 4x model spectrum rulup_lya2_x4.00_etc.txt gives 47 cts/sec in brightest pixel and 22,010 cts/sec in brightest stripe. This exceeds the per-stripe count rate limit for irregularly variable sources, but the 4x case is designed to account for variability. It is below the per-stripe count rate limit of 30,000 cts/sec for nonvariable sources. ETC 1517211 with model spectrum rulup_lya2_etc.txt gives 0.2 sec, round up to 1 sec For BOP check, ETC 1517212 with 4x model spectrum rulup_lya2_x4.00_etc.txt gives 47 cts/sec in brightest pixel and 22,010 cts/sec in brightest stripe. This exceeds the per-stripe count rate limit for irregularly variable sources, but the 4x case is designed to account for variability. It is below the per-stripe count rate limit of 30,000 cts/sec for nonvariable sources. ETC 1517209 with model spectrum rulup_lya2_etc.txt gives 0.3 sec, round up to 1 sec For BOP check, ETC 1517210 with 4x model spectrum rulup_lya2_x4.00_etc.txt gives 47 cts/sec in brightest pixel and 22,010 cts/sec in brightest stripe. This exceeds the per-stripe count rate limit for irregularly variable sources, but the 4x case is designed to account for variability. It is below the per-stripe count rate limit of 30,000 cts/sec for nonvariable sources. ETC 1517211 with model spectrum rulup_lya2_etc.txt gives 0.2 sec, round up to 1 sec For BOP check, ETC 1517212 with 4x model spectrum rulup_lya2_x4.00_etc.txt gives 47 cts/sec in brightest pixel and 22,010 cts/sec in brightest stripe. This exceeds the per-stripe count rate limit for irregularly variable sources, but the 4x case is designed to account for variability. It is below the per-stripe count rate limit of 30,000 cts/sec for nonvariable sources. ETC 1517213 with model spectrum rulup_lya2_etc.txt gives 19 sec to reach S/N = 20 at 2820 A, in the continuum near Mg II 2800. Round up to 30 sec. For BOP check, ETC 1517214 with 4x model spectrum rulup_lya2_x4.00_etc.txt gives 47 cts/sec in brightest pixel and 22,010 cts/sec in brightest stripe. This exceeds the per-stripe count rate limit for irregularly variable sources, but the 4x case is designed to account for variability. It is below the per-stripe count rate limit of 30,000 cts/sec for nonvariable sources. BUFFER-TIME set to 80 sec following COS IHB recommendation when exposure time < 80 sec and ETC buffer time > 80 sec. ETC 1517215 with model spectrum rulup_lya2_etc.txt gives 19 sec to reach S/N = 20 at 2820 A, in the continuum near Mg II 2800. Round up to 30 sec. For BOP check, ETC 1517216 with 4x model spectrum rulup_lya2_x4.00_etc.txt gives 47 cts/sec in brightest pixel and 24,480 cts/sec in brightest stripe. This exceeds the per-stripe count rate limit for irregularly variable sources, but the 4x case is designed to account for variability. It is below the per-stripe count rate limit of 30,000 cts/sec for nonvariable sources. BUFFER-TIME set to 80 sec following COS IHB recommendation when exposure time < 80 sec and ETC buffer time > 80 sec. ETC 1517218 with archival spectrum lbgj530b0_etc.txt, a cenwave 1623 spectrum of this star, gives 550 sec to reach S/N = 30 at 1548 A, the peak of C IV. This is 138 sec per G160M exposure; expand to 219 sec to fill the orbit and account for the possibility of a faint state. For BOP check, ETC 1517219 with 4x archival spectrum lbgj530b0_x4.00_etc.txt gives 0.18 cts/sec in brightest pixel and 1279 cts/sec in entire detector. BUFFER-TIME set to 110 sec to guard against a bright state and reduce overheads. ETC 1517218 with archival spectrum lbgj530b0_etc.txt, a cenwave 1623 spectrum of this star, gives 550 sec to reach S/N = 30 at 1548 A, the peak of C IV. This is 138 sec per G160M exposure; expand to 220 sec to fill the orbit and account for the possibility of a faint state. For BOP check, ETC 1517219 with 4x archival spectrum lbgj530b0_x4.00_etc.txt gives 0.18 cts/sec in brightest pixel and 1279 cts/sec in entire detector. BUFFER-TIME set to 110 sec to guard against a bright state and reduce overheads. ETC 1517220 with archival spectrum lbgj530b0_etc.txt, a cenwave 1623 spectrum of this star, gives 549 sec to reach S/N = 30 at 1548 A, the peak of C IV. This is 138 sec per G160M exposure; expand to 220 sec to fill the orbit and account for the possibility of a faint state. For BOP check, ETC 1517221 with 4x archival spectrum lbgj530b0_x4.00_etc.txt gives 0.18 cts/sec in brightest pixel and 1458 cts/sec in entire detector. BUFFER-TIME set to 110 sec to guard against a bright state and reduce overheads. ETC 1517220 with archival spectrum lbgj530b0_etc.txt, a cenwave 1623 spectrum of this star, gives 549 sec to reach S/N = 30 at 1548 A, the peak of C IV. This is 138 sec per G160M exposure; expand to 220 sec to fill the orbit and account for the possibility of a faint state. For BOP check, ETC 1517221 with 4x archival spectrum lbgj530b0_x4.00_etc.txt gives 0.18 cts/sec in brightest pixel and 1458 cts/sec in entire detector. BUFFER-TIME set to 110 sec to guard against a bright state and reduce overheads. 1621952178948 Timing link suitability includes constraints ([1N After 1C by 10.0 to 10.4 days]) The scheduling data was generated by CASM 29.2. CASM was run in Phase II mode. /Users/wfischer/Box/ullyses_tech/ullyses_proposals/monitor/16110/OP-cache/ULLYSES_16110-v1N.xml vstatus; 1C; V-RU-LUP; P/COS approved for submission; P/WF 20/05/21 ; intrev: complete ; P/JRD 24/05/2021 vcheck; Enter targ name & Inst. & Resp. Sci.; RU Lup ; COS ; WF 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?; G230L/2950, repeated to guard against late GS acq vcheck; Possible ACQ or Sci spoilers?; No vcheck; Field BOT clear?; Yes. BOT complains about the target under the assumption it is an O5 star. vcheck; Visual BOT check for stars not in catalog?; nothing visible in DSS 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 (for XMM) vcheck; Is visit ready for int. review?; yes Allocated COS orbits = 12 1629525189000 100.28588285989542 (Tic-Visit :proposal-id 16110 :visit-id "1N" :proposal-version -1 :trans-version "20200619" :date "25-May-2021 10:16:18.0" :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 695920 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16110 :visit-id "1N" :obset-id "1N" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16110 :visit-id "1N" :orbit-number 1 :pcs-time 393 :si-vis-utilization 2534 :al-overhead-at-end 0 :internal-dur-at-end 407 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2927 :pcs-gap 0 ) true 1 0 ETC 1517209 with model spectrum rulup_lya2_etc.txt gives 0.3 sec, round up to 1 sec For BOP check, ETC 1517210 with 4x model spectrum rulup_lya2_x4.00_etc.txt gives 47 cts/sec in brightest pixel and 22,010 cts/sec in brightest stripe. This exceeds the per-stripe count rate limit for irregularly variable sources, but the 4x case is designed to account for variability. It is below the per-stripe count rate limit of 30,000 cts/sec for nonvariable sources. ETC 1517211 with model spectrum rulup_lya2_etc.txt gives 0.2 sec, round up to 1 sec For BOP check, ETC 1517212 with 4x model spectrum rulup_lya2_x4.00_etc.txt gives 47 cts/sec in brightest pixel and 22,010 cts/sec in brightest stripe. This exceeds the per-stripe count rate limit for irregularly variable sources, but the 4x case is designed to account for variability. It is below the per-stripe count rate limit of 30,000 cts/sec for nonvariable sources. ETC 1517209 with model spectrum rulup_lya2_etc.txt gives 0.3 sec, round up to 1 sec For BOP check, ETC 1517210 with 4x model spectrum rulup_lya2_x4.00_etc.txt gives 47 cts/sec in brightest pixel and 22,010 cts/sec in brightest stripe. This exceeds the per-stripe count rate limit for irregularly variable sources, but the 4x case is designed to account for variability. It is below the per-stripe count rate limit of 30,000 cts/sec for nonvariable sources. ETC 1517211 with model spectrum rulup_lya2_etc.txt gives 0.2 sec, round up to 1 sec For BOP check, ETC 1517212 with 4x model spectrum rulup_lya2_x4.00_etc.txt gives 47 cts/sec in brightest pixel and 22,010 cts/sec in brightest stripe. This exceeds the per-stripe count rate limit for irregularly variable sources, but the 4x case is designed to account for variability. It is below the per-stripe count rate limit of 30,000 cts/sec for nonvariable sources. ETC 1517213 with model spectrum rulup_lya2_etc.txt gives 19 sec to reach S/N = 20 at 2820 A, in the continuum near Mg II 2800. Round up to 30 sec. For BOP check, ETC 1517214 with 4x model spectrum rulup_lya2_x4.00_etc.txt gives 47 cts/sec in brightest pixel and 22,010 cts/sec in brightest stripe. This exceeds the per-stripe count rate limit for irregularly variable sources, but the 4x case is designed to account for variability. It is below the per-stripe count rate limit of 30,000 cts/sec for nonvariable sources. BUFFER-TIME set to 80 sec following COS IHB recommendation when exposure time < 80 sec and ETC buffer time > 80 sec. ETC 1517215 with model spectrum rulup_lya2_etc.txt gives 19 sec to reach S/N = 20 at 2820 A, in the continuum near Mg II 2800. Round up to 30 sec. For BOP check, ETC 1517216 with 4x model spectrum rulup_lya2_x4.00_etc.txt gives 47 cts/sec in brightest pixel and 24,480 cts/sec in brightest stripe. This exceeds the per-stripe count rate limit for irregularly variable sources, but the 4x case is designed to account for variability. It is below the per-stripe count rate limit of 30,000 cts/sec for nonvariable sources. BUFFER-TIME set to 80 sec following COS IHB recommendation when exposure time < 80 sec and ETC buffer time > 80 sec. ETC 1517218 with archival spectrum lbgj530b0_etc.txt, a cenwave 1623 spectrum of this star, gives 550 sec to reach S/N = 30 at 1548 A, the peak of C IV. This is 138 sec per G160M exposure; expand to 219 sec to fill the orbit and account for the possibility of a faint state. For BOP check, ETC 1517219 with 4x archival spectrum lbgj530b0_x4.00_etc.txt gives 0.18 cts/sec in brightest pixel and 1279 cts/sec in entire detector. BUFFER-TIME set to 110 sec to guard against a bright state and reduce overheads. ETC 1517218 with archival spectrum lbgj530b0_etc.txt, a cenwave 1623 spectrum of this star, gives 550 sec to reach S/N = 30 at 1548 A, the peak of C IV. This is 138 sec per G160M exposure; expand to 220 sec to fill the orbit and account for the possibility of a faint state. For BOP check, ETC 1517219 with 4x archival spectrum lbgj530b0_x4.00_etc.txt gives 0.18 cts/sec in brightest pixel and 1279 cts/sec in entire detector. BUFFER-TIME set to 110 sec to guard against a bright state and reduce overheads. ETC 1517220 with archival spectrum lbgj530b0_etc.txt, a cenwave 1623 spectrum of this star, gives 549 sec to reach S/N = 30 at 1548 A, the peak of C IV. This is 138 sec per G160M exposure; expand to 220 sec to fill the orbit and account for the possibility of a faint state. For BOP check, ETC 1517221 with 4x archival spectrum lbgj530b0_x4.00_etc.txt gives 0.18 cts/sec in brightest pixel and 1458 cts/sec in entire detector. BUFFER-TIME set to 110 sec to guard against a bright state and reduce overheads. ETC 1517220 with archival spectrum lbgj530b0_etc.txt, a cenwave 1623 spectrum of this star, gives 549 sec to reach S/N = 30 at 1548 A, the peak of C IV. This is 138 sec per G160M exposure; expand to 220 sec to fill the orbit and account for the possibility of a faint state. For BOP check, ETC 1517221 with 4x archival spectrum lbgj530b0_x4.00_etc.txt gives 0.18 cts/sec in brightest pixel and 1458 cts/sec in entire detector. BUFFER-TIME set to 110 sec to guard against a bright state and reduce overheads. 1629145609158 The scheduling data was generated by CASM 29.2. CASM was run in Phase II mode. /private/var/folders/mk/5ss11qnx2hq98tz1y17xc5080001ws/T/OPVisit6343284745935732265.xml vstatus; AD; V-RU-LUP; P/COS approved for submission; P/WF 16/08/21 ; intrev: complete ; P/JRD 24/05/2021 vcheck; Enter targ name & Inst. & Resp. Sci.; RU Lup ; COS ; WF ... This is a repeat of visit 1D under HOPR 92062 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?; G230L/2950, repeated to guard against late GS acq vcheck; Possible ACQ or Sci spoilers?; No vcheck; Field BOT clear?; Yes. BOT complains about the target under the assumption it is an O5 star. vcheck; Visual BOT check for stars not in catalog?; nothing visible in DSS 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?; N/A ... As advised by the PC, all timing constraints were removed for this repeat visit vcheck; Is visit ready for int. review?; yes Allocated COS orbits = 12 (Tic-Visit :proposal-id 16110 :visit-id "AD" :proposal-version -1 :trans-version "20210514" :date "16-Aug-2021 16:26:48.0" :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 695920 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16110 :visit-id "AD" :obset-id "AD" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16110 :visit-id "AD" :orbit-number 1 :pcs-time 393 :si-vis-utilization 2534 :al-overhead-at-end 0 :internal-dur-at-end 410 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2927 :pcs-gap 0 ) true 1 0 ETC 1517209 with model spectrum rulup_lya2_etc.txt gives 0.3 sec, round up to 1 sec For BOP check, ETC 1517210 with 4x model spectrum rulup_lya2_x4.00_etc.txt gives 47 cts/sec in brightest pixel and 22,010 cts/sec in brightest stripe. This exceeds the per-stripe count rate limit for irregularly variable sources, but the 4x case is designed to account for variability. It is below the per-stripe count rate limit of 30,000 cts/sec for nonvariable sources. ETC 1517211 with model spectrum rulup_lya2_etc.txt gives 0.2 sec, round up to 1 sec For BOP check, ETC 1517212 with 4x model spectrum rulup_lya2_x4.00_etc.txt gives 47 cts/sec in brightest pixel and 22,010 cts/sec in brightest stripe. This exceeds the per-stripe count rate limit for irregularly variable sources, but the 4x case is designed to account for variability. It is below the per-stripe count rate limit of 30,000 cts/sec for nonvariable sources. ETC 1517209 with model spectrum rulup_lya2_etc.txt gives 0.3 sec, round up to 1 sec For BOP check, ETC 1517210 with 4x model spectrum rulup_lya2_x4.00_etc.txt gives 47 cts/sec in brightest pixel and 22,010 cts/sec in brightest stripe. This exceeds the per-stripe count rate limit for irregularly variable sources, but the 4x case is designed to account for variability. It is below the per-stripe count rate limit of 30,000 cts/sec for nonvariable sources. ETC 1517211 with model spectrum rulup_lya2_etc.txt gives 0.2 sec, round up to 1 sec For BOP check, ETC 1517212 with 4x model spectrum rulup_lya2_x4.00_etc.txt gives 47 cts/sec in brightest pixel and 22,010 cts/sec in brightest stripe. This exceeds the per-stripe count rate limit for irregularly variable sources, but the 4x case is designed to account for variability. It is below the per-stripe count rate limit of 30,000 cts/sec for nonvariable sources. ETC 1517213 with model spectrum rulup_lya2_etc.txt gives 19 sec to reach S/N = 20 at 2820 A, in the continuum near Mg II 2800. Round up to 30 sec. For BOP check, ETC 1517214 with 4x model spectrum rulup_lya2_x4.00_etc.txt gives 47 cts/sec in brightest pixel and 22,010 cts/sec in brightest stripe. This exceeds the per-stripe count rate limit for irregularly variable sources, but the 4x case is designed to account for variability. It is below the per-stripe count rate limit of 30,000 cts/sec for nonvariable sources. BUFFER-TIME set to 80 sec following COS IHB recommendation when exposure time < 80 sec and ETC buffer time > 80 sec. ETC 1517215 with model spectrum rulup_lya2_etc.txt gives 19 sec to reach S/N = 20 at 2820 A, in the continuum near Mg II 2800. Round up to 30 sec. For BOP check, ETC 1517216 with 4x model spectrum rulup_lya2_x4.00_etc.txt gives 47 cts/sec in brightest pixel and 24,480 cts/sec in brightest stripe. This exceeds the per-stripe count rate limit for irregularly variable sources, but the 4x case is designed to account for variability. It is below the per-stripe count rate limit of 30,000 cts/sec for nonvariable sources. BUFFER-TIME set to 80 sec following COS IHB recommendation when exposure time < 80 sec and ETC buffer time > 80 sec. ETC 1517218 with archival spectrum lbgj530b0_etc.txt, a cenwave 1623 spectrum of this star, gives 550 sec to reach S/N = 30 at 1548 A, the peak of C IV. This is 138 sec per G160M exposure; expand to 219 sec to fill the orbit and account for the possibility of a faint state. For BOP check, ETC 1517219 with 4x archival spectrum lbgj530b0_x4.00_etc.txt gives 0.18 cts/sec in brightest pixel and 1279 cts/sec in entire detector. BUFFER-TIME set to 110 sec to guard against a bright state and reduce overheads. ETC 1517218 with archival spectrum lbgj530b0_etc.txt, a cenwave 1623 spectrum of this star, gives 550 sec to reach S/N = 30 at 1548 A, the peak of C IV. This is 138 sec per G160M exposure; expand to 220 sec to fill the orbit and account for the possibility of a faint state. For BOP check, ETC 1517219 with 4x archival spectrum lbgj530b0_x4.00_etc.txt gives 0.18 cts/sec in brightest pixel and 1279 cts/sec in entire detector. BUFFER-TIME set to 110 sec to guard against a bright state and reduce overheads. ETC 1517220 with archival spectrum lbgj530b0_etc.txt, a cenwave 1623 spectrum of this star, gives 549 sec to reach S/N = 30 at 1548 A, the peak of C IV. This is 138 sec per G160M exposure; expand to 220 sec to fill the orbit and account for the possibility of a faint state. For BOP check, ETC 1517221 with 4x archival spectrum lbgj530b0_x4.00_etc.txt gives 0.18 cts/sec in brightest pixel and 1458 cts/sec in entire detector. BUFFER-TIME set to 110 sec to guard against a bright state and reduce overheads. ETC 1517220 with archival spectrum lbgj530b0_etc.txt, a cenwave 1623 spectrum of this star, gives 549 sec to reach S/N = 30 at 1548 A, the peak of C IV. This is 138 sec per G160M exposure; expand to 220 sec to fill the orbit and account for the possibility of a faint state. For BOP check, ETC 1517221 with 4x archival spectrum lbgj530b0_x4.00_etc.txt gives 0.18 cts/sec in brightest pixel and 1458 cts/sec in entire detector. BUFFER-TIME set to 110 sec to guard against a bright state and reduce overheads.