0INEFFICIENT ORDERING OF FP-POS POSITIONS
INEFFICIENT ORDERING OF FP-POS POSITIONSVisit 2C is currently at 5 orbits. If this is turning out to be an issue, we can work to split this visit into two.
The science exposures in visit 2C had the wrong target selected! This submission corrects that.1997273094----- Attempting Submission 1 (Mon Mar 28 17:54:10 GMT 2022) -----
----- Attempting Submission 2 (Fri Apr 08 19:42:22 GMT 2022) -----Already ran all tools. The warnings are for inefficient FP-POS ordering, but that is from orbit to the next adn the overhead is during occultationULLYSES Sextans A COS SpectroscopyThe 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 over ~150 OB stars in the Magellanic Clouds and lower metallicity galaxies in the Local Group, and ~40 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.This proposal includes3 massive stars in Sextans A, to be observed with G140L/800, so as to maximize the wavelength coverage of these faint targets.
For all targets, exposure times were computed to reach S/N = 15 at 1130 A.
Model spectra for each target were obtained from fitting the WFC3 F225W, F275W, F336W, F475W, and F814W SED from program 16104 with CMFGEN and Castelli & Kurucz (2004) stellar models with LMC Average dust extinction.
The actual implemented exposure times may be adjusted to efficiently use HST orbits, but should always provide at least 80% of the desired time as defined by the above requirements.
Additional details about the scientific motivation and technical implementation strategy of the ULLYSES observations can be found at http://www.stsci.edu/stsci-research/research-topics-and-programs/ullyses. The ULLYSES program is based on the recommendations of a working group led by Sally Oey; the full text of that group's report can be found at http://www.stsci.edu/files/live/sites/www/files/home/stsci-research/research-topics-and-programs/ullyses/_documents/HSTUV-report-ULLYSES.pdf.6falsefalsefalsefalsefalsefalsefalseSUPPORTEDEXT-STARMAIN SEQUENCE ONOPhotometry from program 16104
Spt and E(B-V) originally from Garcia+2019: O3-5Vz; E(B-V) =0.22
Revised/adjusted using WFC3 photometry to O5V with E(B-V) = 0.13
tstatus; SEXTANS-A-GHN-S2; P/COS approved for submission; S/ins N/A; P/JRD 02/08/2022; S/?? 0MM/DD/YYYY)
tcheck; APT/SIMBAD target names: [VPW98] 1670 ; Gaia DR2 3779987321206922624; JRD 2/08/22
tcheck; Target info verification status?; complete ; JRD 2/08/22
tcheck; Coordinates & P.M. updated?; yes - Gaia coords - PM set to zero; JRD 2/08/22
tcheck; Adopted SED compared to Observations?; OK ; JRD 2/08/22J2000F225W Vega=18.606; F275W Vega=18.828; F336W Vega=19.28; F475W Vega=20.88; F814W Vega=20.854EXT-STARMAIN SEQUENCE ONOPhotometry from program 16104
Spt and E(B-V) originally from Garcia+2019: O6Vz; E(B-V) =0.05
Revised/adjusted using WFC3 photometry to O6V with E(B-V) = 0.045
tstatus; SEXTANS-A-GHN-S4; P/COS approved for submission; S/ins N/A; P/JRD 02/08/2022; S/?? 0MM/DD/YYYY)
tcheck; APT/SIMBAD target names: ; ; JRD 2/08/22
tcheck; Target info verification status?; complete ; JRD 2/08/22
tcheck; Coordinates & P.M. updated?; yes - Coordinates from 2007AJ....133.2393M reported in 2019MNRAS.484..422G - PM set to zero; JRD 2/08/22
tcheck; Adopted SED compared to Observations?; OK ; JRD 2/08/22J2000F225W Vega=18.132; F275W Vega=18.453; F336W Vega=19.039; F475W Vega=20.784; F814W Vega=21.141EXT-STARB0-B2 III-INOPhotometry from program 16104
Spt and E(B-V) originally from Garcia+2019: B0 I; E(B-V) =0.05
Revised/adjusted using WFC3 photometry to B0 I with E(B-V) = 0.077
tstatus; SEXTANS-A-GHN-S8; P/COS approved for submission; S/ins N/A; P/JRD 02/08/2022; S/?? 0MM/DD/YYYY)
tcheck; APT/SIMBAD target names: [VPW98] 412 ; Gaia DR2 3779987733523729280; JRD 2/08/22
tcheck; Target info verification status?; complete ; JRD 2/08/22
tcheck; Coordinates & P.M. updated?; yes - Gaia coords - PM set to zero; JRD 2/08/22
tcheck; Adopted SED compared to Observations?; OK ; JRD 2/08/22J2000F225W Vega=17.526; F275W Vega=17.739; F336W Vega=18.191; F475W Vega=19.721; F814W Vega=19.937/private/var/folders/xp/1hn1qjsn1b55pcrmzptg2_cc0004pj/T/OPVisit1383104812288261953.xmlThe scheduling data was generated by CASM 30.1.CASM was run in Phase II mode.vstatus; 1C; SEXTANS-A-GHN-S2; P/COS approved for submission; P/JRD 08/02/22 ; intrev: complete ; P/AF 26/03/22
vcheck; Enter targ name & Inst. & Resp. Sci.; SEXTANS-A-GHN-S2 ; COS ; JRD
vcheck; ETC numbers entered in APT?; Yes
vcheck; Any screening violations?; No
vcheck; S/N ETC calcs done & documented?; Yes
vcheck; Field images checked & saved?; Yes
vcheck; Selected ACQ strategy?; Yes
vcheck; Possible ACQ or Sci spoilers?; no
vcheck; Field BOT clear?; Yes
vcheck; Visual BOT check for stars not in catalog?; Yes
vcheck; Orbit packing finalized?; Yes
vcheck; Buffer times optimized?; Yes
vcheck; Verify visit grouping correct; N/A
vcheck; Is visit ready for int. review?; Yes
Allocated COS orbits = 9(Tic-Visit
:proposal-id 16930
:visit-id "1C"
:proposal-version -1
:trans-version "20211222"
:date "08-Apr-2022 15:36:51.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 3
:saa-model "31"
:si-bright-earth-limb-angle 20.0
:data-volume 139296
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16930
:visit-id "1C"
:obset-id "1C"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16930
:visit-id "1C"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2525
:al-overhead-at-end 0
:internal-dur-at-end 67
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2918
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16930
:visit-id "1C"
:orbit-number 2
:pcs-time 392
:si-vis-utilization 2524
:al-overhead-at-end 0
:internal-dur-at-end 76
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2918
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16930
:visit-id "1C"
:orbit-number 3
:pcs-time 392
:si-vis-utilization 2524
:al-overhead-at-end 0
:internal-dur-at-end 372
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2918
:pcs-gap 0
)true302 unknown field stars are in the PSA macro-aperture. Those stars are fainter than the target. Since the target is safe for PSA/MIRRORA, so are the unknown field stars.
Exptime computed from model SED that includes stellar emission and dust extinction. Two stellar models examined: WM-Basic and C&K04. Files for SED models are sed_WM-B_SEXTANS-A-GHF-S2.fits and sed_CK_SEXTANS-A-GHF-S2.fitsWM-Basic gives 22ks, CK04 gives 23ks
All field stars clearWM-Basic gives 22ks, CK04 gives 23ks
All field stars clearWM-Basic gives 22ks, CK04 gives 23ks
All field stars clear/private/var/folders/xp/1hn1qjsn1b55pcrmzptg2_cc0004pj/T/OPVisit15092966844354595526.xmlThe scheduling data was generated by CASM 30.1.CASM was run in Phase II mode.vstatus; 1D; SEXTANS-A-GHN-S2; P/COS approved for submission ; P/JRD 08/02/22 ;intrev: complete; P/AF 26/03/22
vcheck; Enter targ name & Inst. & Resp. Sci.; SEXTANS-A-GHN-S2 ; COS ; JRD
vcheck; ETC numbers entered in APT?; Yes
vcheck; Any screening violations?; No
vcheck; S/N ETC calcs done & documented?; Yes
vcheck; Field images checked & saved?; Yes
vcheck; Selected ACQ strategy?; Yes
vcheck; Possible ACQ or Sci spoilers?; no
vcheck; Field BOT clear?; Yes
vcheck; Visual BOT check for stars not in catalog?; Yes
vcheck; Orbit packing finalized?; Yes
vcheck; Buffer times optimized?; Yes
vcheck; Verify visit grouping correct; N/A
vcheck; Is visit ready for int. review?; Yes
Allocated COS orbits = 9(Tic-Visit
:proposal-id 16930
:visit-id "1D"
:proposal-version -1
:trans-version "20211222"
:date "08-Apr-2022 15:36:51.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 3
:saa-model "31"
:si-bright-earth-limb-angle 20.0
:data-volume 139296
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16930
:visit-id "1D"
:obset-id "1D"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16930
:visit-id "1D"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2525
:al-overhead-at-end 0
:internal-dur-at-end 67
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2918
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16930
:visit-id "1D"
:orbit-number 2
:pcs-time 392
:si-vis-utilization 2524
:al-overhead-at-end 0
:internal-dur-at-end 76
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2918
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16930
:visit-id "1D"
:orbit-number 3
:pcs-time 392
:si-vis-utilization 2524
:al-overhead-at-end 0
:internal-dur-at-end 372
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2918
:pcs-gap 0
)true302 unknown field stars are in the PSA macro-aperture. Those stars are fainter than the target. Since the target is safe for PSA/MIRRORA, so are the unknown field stars.
Exptime computed from model SED that includes stellar emission and dust extinction. Two stellar models examined: WM-Basic and C&K04. Files for SED models are sed_WM-B_SEXTANS-A-GHF-S2.fits and sed_CK_SEXTANS-A-GHF-S2.fitsWM-Basic gives 22ks, CK04 gives 23ks
All field stars clearWM-Basic gives 22ks, CK04 gives 23ks
All field stars clearWM-Basic gives 22ks, CK04 gives 23ks
All field stars clear/private/var/folders/xp/1hn1qjsn1b55pcrmzptg2_cc0004pj/T/OPVisit7442808010752085452.xmlThe scheduling data was generated by CASM 30.1.CASM was run in Phase II mode.vstatus; 1E; SEXTANS-A-GHN-S2; P/COS approved for submission ; P/JRD 08/02/22 ; intrev: complete ; P/AF 26/03/22
vcheck; Enter targ name & Inst. & Resp. Sci.; SEXTANS-A-GHN-S2 ; COS ; JRD
vcheck; ETC numbers entered in APT?; Yes
vcheck; Any screening violations?; No
vcheck; S/N ETC calcs done & documented?; Yes
vcheck; Field images checked & saved?; Yes
vcheck; Selected ACQ strategy?; Yes
vcheck; Possible ACQ or Sci spoilers?; no
vcheck; Field BOT clear?; Yes
vcheck; Visual BOT check for stars not in catalog?; Yes
vcheck; Orbit packing finalized?; Yes
vcheck; Buffer times optimized?; Yes
vcheck; Verify visit grouping correct; N/A
vcheck; Is visit ready for int. review?; Yes
Allocated COS orbits = 9(Tic-Visit
:proposal-id 16930
:visit-id "1E"
:proposal-version -1
:trans-version "20211222"
:date "08-Apr-2022 15:36:52.0"
:trans-errors '(:WARNINGS 1 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 3
:saa-model "31"
:si-bright-earth-limb-angle 20.0
:data-volume 130736
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16930
:visit-id "1E"
:obset-id "1E"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16930
:visit-id "1E"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2525
:al-overhead-at-end 0
:internal-dur-at-end 67
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2918
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16930
:visit-id "1E"
:orbit-number 2
:pcs-time 392
:si-vis-utilization 2524
:al-overhead-at-end 0
:internal-dur-at-end 76
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2918
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16930
:visit-id "1E"
:orbit-number 3
:pcs-time 392
:si-vis-utilization 2519
:al-overhead-at-end 0
:internal-dur-at-end 334
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2918
:pcs-gap 0
)true302 unknown field stars are in the PSA macro-aperture. Those stars are fainter than the target. Since the target is safe for PSA/MIRRORA, so are the unknown field stars.
Exptime computed from model SED that includes stellar emission and dust extinction. Two stellar models examined: WM-Basic and C&K04. Files for SED models are sed_WM-B_SEXTANS-A-GHF-S2.fits and sed_CK_SEXTANS-A-GHF-S2.fitsWM-Basic gives 22ks, CK04 gives 23ks
All field stars clearWM-Basic gives 22ks, CK04 gives 23ks
All field stars clearWM-Basic gives 22ks, CK04 gives 23ks
All field stars clear/private/var/folders/xp/1hn1qjsn1b55pcrmzptg2_cc0004pj/T/OPVisit14106525931729542346.xmlThe scheduling data was generated by CASM 30.1.CASM was run in Phase II mode.vstatus; 2C; SEXTANS-A-GHN-S4; P/COS approved for submission ; P/JRD 08/02/22 ; intrev: complete ; P/AF 26/03/22
vcheck; Enter targ name & Inst. & Resp. Sci.; SEXTANS-A-GHN-S4 ; COS ; JRD
vcheck; ETC numbers entered in APT?; Yes
vcheck; Any screening violations?; No
vcheck; S/N ETC calcs done & documented?; Yes
vcheck; Field images checked & saved?; Yes
vcheck; Selected ACQ strategy?; Yes
vcheck; Possible ACQ or Sci spoilers?; no
vcheck; Field BOT clear?; Yes
vcheck; Visual BOT check for stars not in catalog?; Yes
vcheck; Orbit packing finalized?; Yes
vcheck; Buffer times optimized?; Yes
vcheck; Verify visit grouping correct; N/A
vcheck; Is visit ready for int. review?; Yes
Allocated COS orbits = 5(Tic-Visit
:proposal-id 16930
:visit-id "2C"
:proposal-version -1
:trans-version "20211222"
:date "08-Apr-2022 15:36:10.0"
:trans-errors '(:WARNINGS 1 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 5
:saa-model "31"
:si-bright-earth-limb-angle 20.0
:data-volume 217760
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16930
:visit-id "2C"
:obset-id "2C"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16930
:visit-id "2C"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2525
:al-overhead-at-end 0
:internal-dur-at-end 67
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2918
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16930
:visit-id "2C"
:orbit-number 2
:pcs-time 392
:si-vis-utilization 2524
:al-overhead-at-end 0
:internal-dur-at-end 76
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2918
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16930
:visit-id "2C"
:orbit-number 3
:pcs-time 392
:si-vis-utilization 2524
:al-overhead-at-end 0
:internal-dur-at-end 76
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2918
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16930
:visit-id "2C"
:orbit-number 4
:pcs-time 392
:si-vis-utilization 2524
:al-overhead-at-end 0
:internal-dur-at-end 76
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2918
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16930
:visit-id "2C"
:orbit-number 5
:pcs-time 392
:si-vis-utilization 2519
:al-overhead-at-end 0
:internal-dur-at-end 334
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2918
:pcs-gap 0
)true50All field stars clear
Exptime computed from model SED that includes stellar emission and dust extinction. Two stellar models examined: WM-Basic and C&K04. Files for SED models are sed_WM-B_SEXTANS-A-GHF-S4.fits and sed_CK_SEXTANS-A-GHF-S4.fitsAll field stars clear
Exptime computed from model SED that includes stellar emission and dust extinction. Two stellar models examined: WM-Basic and C&K04. Files for SED models are sed_WM-B_SEXTANS-A-GHF-S4.fits and sed_CK_SEXTANS-A-GHF-S4.fitsWM-Basic gives 10ks, CK04 gives 11ks
All field stars clearWM-Basic gives 10ks, CK04 gives 11ks
All field stars clearWM-Basic gives 10ks, CK04 gives 11ks
All field stars clearWM-Basic gives 10ks, CWM-Basic gives 10ks, CK04 gives 11ks
All field stars clearK04 gives 11ksWM-Basic gives 10ks, CK04 gives 11ks
All field stars clear/private/var/folders/xp/1hn1qjsn1b55pcrmzptg2_cc0004pj/T/OPVisit6700909238081731345.xmlThe scheduling data was generated by CASM 30.1.CASM was run in Phase II mode.vstatus; 3C; SEXTANS-A-GHN-S8; P/COS approved for submission ; P/JRD 08/02/22 ; intrev: complete ; P/AF 26/03/22
vcheck; Enter targ name & Inst. & Resp. Sci.; SEXTANS-A-GHN-S8 ; COS ; JRD
vcheck; ETC numbers entered in APT?; Yes
vcheck; Any screening violations?; No
vcheck; S/N ETC calcs done & documented?; Yes
vcheck; Field images checked & saved?; Yes
vcheck; Selected ACQ strategy?; Yes
vcheck; Possible ACQ or Sci spoilers?; no
vcheck; Field BOT clear?; Yes
vcheck; Visual BOT check for stars not in catalog?; Yes
vcheck; Orbit packing finalized?; Yes
vcheck; Buffer times optimized?; Yes
vcheck; Verify visit grouping correct; N/A
vcheck; Is visit ready for int. review?; Yes
Allocated COS orbits = 6(Tic-Visit
:proposal-id 16930
:visit-id "3C"
:proposal-version -1
:trans-version "20211222"
:date "08-Apr-2022 15:36:53.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 3
:saa-model "31"
:si-bright-earth-limb-angle 20.0
:data-volume 139296
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16930
:visit-id "3C"
:obset-id "3C"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16930
:visit-id "3C"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2522
:al-overhead-at-end 0
:internal-dur-at-end 67
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2918
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16930
:visit-id "3C"
:orbit-number 2
:pcs-time 392
:si-vis-utilization 2524
:al-overhead-at-end 0
:internal-dur-at-end 76
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2918
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16930
:visit-id "3C"
:orbit-number 3
:pcs-time 392
:si-vis-utilization 2524
:al-overhead-at-end 0
:internal-dur-at-end 372
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2918
:pcs-gap 0
)true30Unsafe object reported by GALEX corresponds to 3 massive stars listed in Camacho+2016: OB121, OB523, OB524. The brightest of those is OB523, which was observed as part of GO-14245 (G140L) and GO-15880 (G130M). This is a O9 I star with V = 19.49. This star clears with the ETC under the PSA/MIRRORA configuation, and a Kurucz O9V input model normalized to V = 19.49 without extinction (see COS.ta.1689686). In the FUV, the input spectrum plotted in the ETC in this case is a factor of 2 brighter than the observed G140L spectrum. Therefore, OB121, OB 523 and OB524 are safe to observe with PSA/MIRRORA
Exptime computed from model SED that includes stellar emission and dust extinction. Two stellar models examined: WM-Basic and C&K04. Files for SED models are sed_WM-B_SEXTANS-A-GHF-S8.fits and sed_CK_SEXTANS-A-GHF-S8.fitsWM-Basic gives 15ks, CK04 gives 14ks
All stars (target and fields) clearWM-Basic gives 15ks, CK04 gives 14ks
All stars (target and fields) clearWM-Basic gives 15ks, CK04 gives 14ks
All stars (target and fields) clear/private/var/folders/xp/1hn1qjsn1b55pcrmzptg2_cc0004pj/T/OPVisit5260755736843269910.xmlThe scheduling data was generated by CASM 30.1.CASM was run in Phase II mode.vstatus; 3D; SEXTANS-A-GHN-S8; P/COS approved for submission ; P/JRD 08/02/22 ; intrev: complete ; P/AF 26/03/22
vcheck; Enter targ name & Inst. & Resp. Sci.; SEXTANS-A-GHN-S8 ; COS ; JRD
vcheck; ETC numbers entered in APT?; Yes
vcheck; Any screening violations?; No
vcheck; S/N ETC calcs done & documented?; Yes
vcheck; Field images checked & saved?; Yes
vcheck; Selected ACQ strategy?; Yes
vcheck; Possible ACQ or Sci spoilers?; no
vcheck; Field BOT clear?; Yes
vcheck; Visual BOT check for stars not in catalog?; Yes
vcheck; Orbit packing finalized?; Yes
vcheck; Buffer times optimized?; Yes
vcheck; Verify visit grouping correct; N/A
vcheck; Is visit ready for int. review?; Yes
Allocated COS orbits = 6(Tic-Visit
:proposal-id 16930
:visit-id "3D"
:proposal-version -1
:trans-version "20211222"
:date "08-Apr-2022 15:36:53.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 3
:saa-model "31"
:si-bright-earth-limb-angle 20.0
:data-volume 148048
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16930
:visit-id "3D"
:obset-id "3D"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16930
:visit-id "3D"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2525
:al-overhead-at-end 0
:internal-dur-at-end 48
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2918
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16930
:visit-id "3D"
:orbit-number 2
:pcs-time 392
:si-vis-utilization 2526
:al-overhead-at-end 0
:internal-dur-at-end 57
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2918
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16930
:visit-id "3D"
:orbit-number 3
:pcs-time 392
:si-vis-utilization 2524
:al-overhead-at-end 0
:internal-dur-at-end 372
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2918
:pcs-gap 0
)true30Unsafe object reported by GALEX corresponds to 3 massive stars listed in Camacho+2016: OB121, OB523, OB524. The brightest of those is OB523, which was observed as part of GO-14245 (G140L) and GO-15880 (G130M). This is a O9 I star with V = 19.49. This star clears with the ETC under the PSA/MIRRORA configuation, and a Kurucz O9V input model normalized to V = 19.49 without extinction (see COS.ta.1689686). In the FUV, the input spectrum plotted in the ETC in this case is a factor of 2 brighter than the observed G140L spectrum. Therefore, OB121, OB 523 and OB524 are safe to observe with PSA/MIRRORA
Exptime computed from model SED that includes stellar emission and dust extinction. Two stellar models examined: WM-Basic and C&K04. Files for SED models are sed_WM-B_SEXTANS-A-GHF-S8.fits and sed_CK_SEXTANS-A-GHF-S8.fitsWM-Basic gives 15ks, CK04 gives 14ks
All stars (target and fields) clearWM-Basic gives 15ks, CK04 gives 14ks
All stars (target and fields) clearWM-Basic gives 15ks, CK04 gives 14ks
All stars (target and fields) clearWM-Basic gives 15ks, CK04 gives 14ks
All stars (target and fields) clearWM-Basic gives 15ks, CK04 gives 14ks
All stars (target and fields) clear