2020 May 27: The ULLYSES CIT decided to use 15 orbits instead of 12 for this PID, so there is currently a mismatch between used and allocated.
2020 Oct 12: Resubmitting with a new visit AC to repeat failed 2nd orbit of 1C -- W. Fischer-137595498----- Attempting Submission 1 (Wed May 27 20:34:32 GMT 2020) -----
----- Attempting Submission 2 (Mon Oct 12 14:06:10 GMT 2020) -----ULLYSES LMC O9-B1 stars COSThe 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 includes a subset of the massive ULLYSES stars being observed in the Magellanic clouds.
Depending on target brightness, the main FUV spectral range will generally use either the STIS E140M setting or the combination of the COS c1291 + c1611 settings. Sufficiently bright stars without good FUSE data in the archive will also be observed with the COS c1096 setting to provide coverage at shorter wavelengths. Where time permits, stars of type O9 or later will also be observed with STIS E230M/1978, while for supergiants of spectral type B5 or later E230M/2707 may also be included. Where possible, targets of a given spectral type were selected to span both a range in extinction and in rotation rates to support a variety of stellar and ISM studies.
Signal-to-noise requirements used to determine the desired exposures times were defined as follows:
COS/G130M/c1096: 20 / nine-pixel resel at 1080 A
COS/G130M/c1291: 30 / six-pixel resel at 1150 A
COS/G160M/c1611: 30 / six-pixel resel at 1590 A
COS/G185M/c1953: 30 / three-pixel resel at 1860 A
COS/G185M/c1986: 30 / three-pixel resel at 1980 A
STIS/E140M/c1425: 20 / two-pixel resel at 1200 A
STIS/E230M/c1978: 20 / two-pixel resel at 1800 A
STIS/E230M/c2707: 20 / two-pixel resel at 2800 A
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.0falseSUPPORTEDEXT-STARB0-B2 V-IVNOHV5622 : MACHO79-4779, MACHO79_4779, MACHO 79.4779.34
Previous name : MACHO79-4779
Input file: LMC_2020Feb20/input/LMC_all_do1_fixed_wr_NewCoords_pids.csv
SIMBAD link (MACHO 79.4779.34): https://simbad.u-strasbg.fr/simbad/sim-id?Ident=MACHO+79.4779.34&submit=submit+id
SpT = B0V
COS/G130M/c1096 : rn-max(WM-Basic(B0 V, Z=0.008, Teff=30200, log_lum=4.80, log_g=4.00) (extinction lmcavg=0.060), flux1160 +- 30.0A flux=1.6e-13 Flam)
COS/G130M/c1291 : rn-max(WM-Basic(B0 V, Z=0.008, Teff=30200, log_lum=4.80, log_g=4.00) (extinction lmcavg=0.060), flux1360 +- 30.0A flux=1.5e-13 Flam)
COS/G160M/c1611 : rn-max(WM-Basic(B0 V, Z=0.008, Teff=30200, log_lum=4.80, log_g=4.00) (extinction lmcavg=0.060), flux1700 +- 5.0A flux=1e-13 Flam)
COS/G185M/c1921 : rn-max(WM-Basic(B0 V, Z=0.008, Teff=30200, log_lum=4.80, log_g=4.00) (extinction lmcavg=0.060), flux1700 +- 5.0A flux=1e-13 Flam)
COS/G185M/c1953 : rn-max(WM-Basic(B0 V, Z=0.008, Teff=30200, log_lum=4.80, log_g=4.00) (extinction lmcavg=0.060), flux1700 +- 5.0A flux=1e-13 Flam)
COS/G185M/c1986 : rn-max(WM-Basic(B0 V, Z=0.008, Teff=30200, log_lum=4.80, log_g=4.00) (extinction lmcavg=0.060), flux2200 +- 5.0A flux=5.4e-14 Flam)
STIS/E140M/c1425 : rn-max(WM-Basic(B0 V, Z=0.008, Teff=30200, log_lum=4.80, log_g=4.00) (extinction lmcavg=0.060), flux1360 +- 30.0A flux=1.5e-13 Flam)
STIS/E230M/c1978 : rn-max(WM-Basic(B0 V, Z=0.008, Teff=30200, log_lum=4.80, log_g=4.00) (extinction lmcavg=0.060), flux2200 +- 5.0A flux=5.4e-14 Flam)
STIS/E230M/c2707 : rn-max(WM-Basic(B0 V, Z=0.008, Teff=30200, log_lum=4.80, log_g=4.00) (extinction lmcavg=0.060), flux2200 +- 5.0A flux=5.4e-14 Flam)
Coordinate pedigree: Gaia
Calculation performed 2020-02-24T17:49:22, v0.4
-------------------------------------------------------------------------------
tstatus; HV5622; P/COS approved for submission; S/ins N/A; P/WF 27/02/20; S/xx DD/MM/YY
tcheck; APT/SIMBAD target names: ; HV5622 ...; WF 27/02/20
aka MACHO79-4779, MACHO79_4779, MACHO 79.4779.34
tcheck; Target info verification status?; complete ; WF 27/02/20
tcheck; Coordinates & P.M. updated?; yes - Gaia coords - PM set to zero; WF 27/02/20
tcheck; Adopted SED compared to Observations?; OK - good match at cenwaves to be observed; WF 27/02/20MACHO79-4779MACHO-79.4779.34J2000SpT=B0V; E(B-V)=0.06; U=14.1; B=14.6; V=14.8; F1160=1.64e-13; F1360=1.48e-13; F1700=1.01e-13; F2200=5.39e-14EXT-STARB0-B2 III-INOLH9-89 : N11-033, N11_33, [ELS2006] N11 033
Previous name : N11-033
Input file: LMC_2020Feb20/input/LMC_all_do1_fixed_wr_NewCoords_pids.csv
SIMBAD link ([ELS2006] N11 033): https://simbad.u-strasbg.fr/simbad/sim-id?Ident=[ELS2006]+N11+033&submit=submit+id
SpT = B0 IIIn
COS/G130M/c1096 : rn(WM-Basic(B0 III, Z=0.008, Teff=28184, log_lum=5.12, log_g=3.54) (extinction lmcavg=0.140), johnson B mag=13.520 vegamag)
COS/G130M/c1291 : rn(WM-Basic(B0 III, Z=0.008, Teff=28184, log_lum=5.12, log_g=3.54) (extinction lmcavg=0.140), johnson B mag=13.520 vegamag)
COS/G160M/c1611 : rn(WM-Basic(B0 III, Z=0.008, Teff=28184, log_lum=5.12, log_g=3.54) (extinction lmcavg=0.140), johnson B mag=13.520 vegamag)
COS/G185M/c1921 : rn(WM-Basic(B0 III, Z=0.008, Teff=28184, log_lum=5.12, log_g=3.54) (extinction lmcavg=0.140), johnson B mag=13.520 vegamag)
COS/G185M/c1953 : rn(WM-Basic(B0 III, Z=0.008, Teff=28184, log_lum=5.12, log_g=3.54) (extinction lmcavg=0.140), johnson B mag=13.520 vegamag)
COS/G185M/c1986 : rn(WM-Basic(B0 III, Z=0.008, Teff=28184, log_lum=5.12, log_g=3.54) (extinction lmcavg=0.140), johnson B mag=13.520 vegamag)
STIS/E140M/c1425 : rn(WM-Basic(B0 III, Z=0.008, Teff=28184, log_lum=5.12, log_g=3.54) (extinction lmcavg=0.140), johnson B mag=13.520 vegamag)
STIS/E230M/c1978 : rn(WM-Basic(B0 III, Z=0.008, Teff=28184, log_lum=5.12, log_g=3.54) (extinction lmcavg=0.140), johnson B mag=13.520 vegamag)
STIS/E230M/c2707 : rn(WM-Basic(B0 III, Z=0.008, Teff=28184, log_lum=5.12, log_g=3.54) (extinction lmcavg=0.140), johnson B mag=13.520 vegamag)
Coordinate pedigree: Gaia
v sin i = 256
Calculation performed 2020-02-24T17:48:57, v0.4
-------------------------------------------------------------------------------
tstatus; LH9-89; P/COS approved for submission; S/ins not started; P/WF 30/03/20; S/xx DD/MM/YY
tcheck; APT/SIMBAD target names: ; LH9-89 '[L72] LH 9-89' ...; WF 30/03/20
aka PGMW 1005, [ELS2006] N11 033, [HKN2006] OB 140
tcheck; Target info verification status?; complete ; WF 30/03/20
tcheck; Coordinates & P.M. updated?; yes - Gaia coords - PM set to zero ...; WF 30/03/20
Gaia coords differ from these by 0.06 arcsec, this was judged not to warrant updating
tcheck; Adopted SED compared to Observations?; OK - but only B and V phot exist; WF 30/03/20N11-033N11-33J2000SpT=B0 IIIn; E(B-V)=0.14; B=13.5; V=13.7; U=12.58; B=13.531; V=13.645EXT-STARB0-B2 V-IVNON206-FS-170 : [N206-FS]-170, [N206-FS]_170
Previous name : [N206-FS]-170
Input file: LMC_2020Feb20/input/LMC_all_do1_fixed_wr_NewCoords_pids.csv
SpT = B1 IV
COS/G130M/c1096 : rn(WM-Basic(B1 V, Z=0.008, Teff=26303, log_lum=4.45, log_g=4.00) (extinction lmcavg=0.090), johnson U mag=13.630 vegamag)
COS/G130M/c1291 : rn(WM-Basic(B1 V, Z=0.008, Teff=26303, log_lum=4.45, log_g=4.00) (extinction lmcavg=0.090), johnson U mag=13.630 vegamag)
COS/G160M/c1611 : rn(WM-Basic(B1 V, Z=0.008, Teff=26303, log_lum=4.45, log_g=4.00) (extinction lmcavg=0.090), johnson U mag=13.630 vegamag)
COS/G185M/c1921 : rn(WM-Basic(B1 V, Z=0.008, Teff=26303, log_lum=4.45, log_g=4.00) (extinction lmcavg=0.090), johnson U mag=13.630 vegamag)
COS/G185M/c1953 : rn(WM-Basic(B1 V, Z=0.008, Teff=26303, log_lum=4.45, log_g=4.00) (extinction lmcavg=0.090), johnson U mag=13.630 vegamag)
COS/G185M/c1986 : rn(WM-Basic(B1 V, Z=0.008, Teff=26303, log_lum=4.45, log_g=4.00) (extinction lmcavg=0.090), johnson U mag=13.630 vegamag)
STIS/E140M/c1425 : rn(WM-Basic(B1 V, Z=0.008, Teff=26303, log_lum=4.45, log_g=4.00) (extinction lmcavg=0.090), johnson U mag=13.630 vegamag)
STIS/E230M/c1978 : rn(WM-Basic(B1 V, Z=0.008, Teff=26303, log_lum=4.45, log_g=4.00) (extinction lmcavg=0.090), johnson U mag=13.630 vegamag)
STIS/E230M/c2707 : rn(WM-Basic(B1 V, Z=0.008, Teff=26303, log_lum=4.45, log_g=4.00) (extinction lmcavg=0.090), johnson U mag=13.630 vegamag)
Coordinate pedigree: InputCatalog
v sin i = 180
Calculation performed 2020-02-24T17:50:48, v0.4
-------------------------------------------------------------------------------
tstatus; N206-FS-170; P/COS approved for submission; S/ins not started; P/WF 13/04/20; S/xx DD/MM/YY
tcheck; APT/SIMBAD target names: ; N206-FS-170 '[RHH2018] 170'; WF 13/04/20
tcheck; Target info verification status?; complete ; WF 13/04/20
tcheck; Coordinates & P.M. updated?; yes - Gaia coords - PM set to zero ...; WF 13/04/20
Gaia RA differs from initial APT entry by 0.05 sec or 0.75 arcsec, so coordinates were corrected
tcheck; Adopted SED compared to Observations?; OK - only UBV phot exist; WF 13/04/20J2000SpT=B1 IV; E(B-V)=0.09; U=13.6; B=14.2; V=14.4EXT-STARB3-B5 III-INOSK-70D16 : [M2002]_22715, Sk -70 16, SK -70 16
Previous name : Sk -70 16
Input file: LMC_2020Feb20/input/LMC_all_do1_fixed_wr_NewCoords_pids.csv
SIMBAD link (SK -70 16): https://simbad.u-strasbg.fr/simbad/sim-id?Ident=SK+-70+16&submit=submit+id
SpT = B4 I
COS/G130M/c1291 : rn(ck04models(B4I,Teff=16080,metallicity=0.008,logG=2.52) (extinction lmcavg=0.070), johnson U mag=12.190 vegamag)
COS/G160M/c1611 : rn(ck04models(B4I,Teff=16080,metallicity=0.008,logG=2.52) (extinction lmcavg=0.070), johnson U mag=12.190 vegamag)
COS/G185M/c1921 : rn(ck04models(B4I,Teff=16080,metallicity=0.008,logG=2.52) (extinction lmcavg=0.070), johnson U mag=12.190 vegamag)
COS/G185M/c1953 : rn(ck04models(B4I,Teff=16080,metallicity=0.008,logG=2.52) (extinction lmcavg=0.070), johnson U mag=12.190 vegamag)
COS/G185M/c1986 : rn(ck04models(B4I,Teff=16080,metallicity=0.008,logG=2.52) (extinction lmcavg=0.070), johnson U mag=12.190 vegamag)
STIS/E140M/c1425 : rn(ck04models(B4I,Teff=16080,metallicity=0.008,logG=2.52) (extinction lmcavg=0.070), johnson U mag=12.190 vegamag)
STIS/E230M/c1978 : rn(ck04models(B4I,Teff=16080,metallicity=0.008,logG=2.52) (extinction lmcavg=0.070), johnson U mag=12.190 vegamag)
STIS/E230M/c2707 : rn(ck04models(B4I,Teff=16080,metallicity=0.008,logG=2.52) (extinction lmcavg=0.070), johnson U mag=12.190 vegamag)
Coordinate pedigree: Gaia
Calculation performed 2020-02-24T17:51:48, v0.4
-------------------------------------------------------------------------------
tstatus; SK-70D16; P/COS approved for submission; S/ins not started; P/WF 07/05/20; S/xx DD/MM/YY
tcheck; APT/SIMBAD target names: ; SK-70D16 'SK -70 16' ...; WF 07/05/20
aka GV 650, [FD82] 125, [M2002] LMC 22715
tcheck; Target info verification status?; complete ; WF 07/05/20
tcheck; Coordinates & P.M. updated?; yes - Gaia coords - PM set to zero; WF 07/05/20
tcheck; Adopted SED compared to Observations?; OK - only UBV phot exist; WF 07/05/20M2002-22715SK-70-16J2000SpT=B4 I; E(B-V)=0.07; U=12.2; B=13.0; V=13.1EXT-STARMAIN SEQUENCE ONOVFTS-66 : VFTS066, VFTS 66
Previous name : VFTS066
Input file: LMC_2020Feb20/input/LMC_all_do1_fixed_wr_NewCoords_pids.csv
SIMBAD link (VFTS 66): https://simbad.u-strasbg.fr/simbad/sim-id?Ident=VFTS+66&submit=submit+id
SpT = O9V + B0.2V
COS/G130M/c1096 : rn(WM-Basic(O9 V, Z=0.008, Teff=32359, log_lum=5.00, log_g=4.00), johnson B mag=15.640 vegamag)
COS/G130M/c1291 : rn(WM-Basic(O9 V, Z=0.008, Teff=32359, log_lum=5.00, log_g=4.00), johnson B mag=15.640 vegamag)
COS/G160M/c1611 : rn(WM-Basic(O9 V, Z=0.008, Teff=32359, log_lum=5.00, log_g=4.00), johnson B mag=15.640 vegamag)
COS/G185M/c1921 : rn(WM-Basic(O9 V, Z=0.008, Teff=32359, log_lum=5.00, log_g=4.00), johnson B mag=15.640 vegamag)
COS/G185M/c1953 : rn(WM-Basic(O9 V, Z=0.008, Teff=32359, log_lum=5.00, log_g=4.00), johnson B mag=15.640 vegamag)
COS/G185M/c1986 : rn(WM-Basic(O9 V, Z=0.008, Teff=32359, log_lum=5.00, log_g=4.00), johnson B mag=15.640 vegamag)
STIS/E140M/c1425 : rn(WM-Basic(O9 V, Z=0.008, Teff=32359, log_lum=5.00, log_g=4.00), johnson B mag=15.640 vegamag)
STIS/E230M/c1978 : rn(WM-Basic(O9 V, Z=0.008, Teff=32359, log_lum=5.00, log_g=4.00), johnson B mag=15.640 vegamag)
STIS/E230M/c2707 : rn(WM-Basic(O9 V, Z=0.008, Teff=32359, log_lum=5.00, log_g=4.00), johnson B mag=15.640 vegamag)
Coordinate pedigree: 2MASS
v sin i = >330
Calculation performed 2020-02-24T18:09:02, v0.4
-------------------------------------------------------------------------------
tstatus; VFTS-66; P/COS approved for submission; S/ins not started; P/WF 27/05/20; S/xx DD/MM/YY
tcheck; APT/SIMBAD target names:; VFTS-66 'VFTS 66' ...
aka 2MASS J05373309-6904343
tcheck; Target info verification status?; OK ...
E(B-V) was autopopulated to 0 but is best estimated as 0.37 (Mahy et al. 2020, A&A, 634, A118)
tcheck; Coordinates & P.M. updated?; yes - coords updated from 2MASS to Gaia - PM set to 0
tcheck; Adopted SED compared to Observations?; OK - only BV phot exist ...
Tarantula Survey Sabbi+2016 gives F275mag=14.39, F336mag=14.495, F555mag=15.607, F658mag=15.392
AAVSO Photometric All Sky Survey (APASS) DR9 (Henden+, 2016) gives V=15.516, B=15.673 so B-V=0.156
see See /1442515 for c12911611 normaized to F275W - S/N is perhaps a bit low in these? But E(B-V) probably low, so real FUV discrepancy probably much bigger?
ETC COS.sp.1442605 gives 3,865.3972s for c1291
or normalizing to F275W gives 7990s for c1291 COS.sp.1442606
or normalizing to F336W gives 5592 s COS.sp.1442609VFTS066J2000SpT=O9V + B0.2V; E(B-V)=0.37; B=15.6; V=15.5; F275MAG=14.39, F336MAG=14.495; F555mag=15.607; F658mag=15.392The scheduling data was generated by CASM 28.2.CASM was run in Phase II mode.vstatus; 1C; HV5622; P/COS approved for submission; P/WF 12/03/20 ; intrev: completed ; P/CP 14/05/20
vcheck; Enter targ name & Inst. & Resp. Sci.; HV5622 ; COS ; WF
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?; dispersed 1291
vcheck; Possible ACQ or Sci spoilers?; no
vcheck; Field BOT clear?; yes. BOT finds 2 safe stars, 0 unknown, 0 unsafe in GSC2 check
vcheck; Visual BOT check for stars not in catalog?; no objects of concern ...
The GSC2 doesn't include a lot of the stars in this field, but the brighest field object in the PSA macro aperture is well below any BOP limits as B/V = 19/17.1 in Zaritsky catalog and G=16.85 in Gaia.
vcheck; Orbit packing finalized?; yes ...
Exposure times for both cenwaves exceed request by 3%, FP-POS 1 of c1611 is split between orbits to keep times equal
vcheck; Buffer times optimized?; yes
vcheck; Verify visit grouping correct; n/a
vcheck; Is visit ready for int. review?; yes
Allocated COS orbits = 2, used = 21601492975000270.0(Tic-Visit
:proposal-id 16096
:visit-id "1C"
:proposal-version -1
:trans-version "20191203"
:date "15-May-2020 11:55:01.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 2
:saa-model "31"
:si-bright-earth-limb-angle 20.0
:data-volume 800352
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16096
:visit-id "1C"
:obset-id "1C"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16096
:visit-id "1C"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2577
: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 2970
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16096
:visit-id "1C"
:orbit-number 2
:pcs-time 302
:si-vis-utilization 2668
:al-overhead-at-end 0
:internal-dur-at-end 341
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2970
:pcs-gap 0
)true20rn-max(WM-Basic(B0 V, Z=0.008, Teff=30200, log_lum=4.80, log_g=4.00) (extinction lmcavg=0.060), flux1360 +- 30.0A flux=1.5e-13 Flam); cos,fuv,g130m,c1291,psa,mjd#59305; fp-pos=None, segment=None)
From file LMC_2020Feb20/input/LMC_all_do1_fixed_wr_NewCoords_pids.csv
Spectral type: B0V --> B0 V
SED = HV5622_COS_G130M_c1291_sed.fits
For exptime=1249.3 s, spectral region:
1150.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 3161.3 cts/s/segment
brightest pixel: 0.051 cts/s/pix at 1395.0 A
Calculation performed 2020-02-24T17:49:25, v0.4rn-max(WM-Basic(B0 V, Z=0.008, Teff=30200, log_lum=4.80, log_g=4.00) (extinction lmcavg=0.060), flux1360 +- 30.0A flux=1.5e-13 Flam); cos,fuv,g130m,c1291,psa,mjd#59305; fp-pos=None, segment=None)
From file LMC_2020Feb20/input/LMC_all_do1_fixed_wr_NewCoords_pids.csv
Spectral type: B0V --> B0 V
SED = HV5622_COS_G130M_c1291_sed.fits
For exptime=1249.3 s, spectral region:
1150.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 3161.3 cts/s/segment
brightest pixel: 0.051 cts/s/pix at 1395.0 A
Calculation performed 2020-02-24T17:49:25, v0.4rn-max(WM-Basic(B0 V, Z=0.008, Teff=30200, log_lum=4.80, log_g=4.00) (extinction lmcavg=0.060), flux1700 +- 5.0A flux=1e-13 Flam); cos,fuv,g160m,c1611,psa,mjd#59305; fp-pos=None, segment=None)
From file LMC_2020Feb20/input/LMC_all_do1_fixed_wr_NewCoords_pids.csv
Spectral type: B0V --> B0 V
SED = HV5622_COS_G160M_c1611_sed.fits
For exptime=2693.0 s, spectral region:
1590.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 1668.5 cts/s/segment
brightest pixel: 0.028 cts/s/pix at 1442.0 A
Calculation performed 2020-02-24T17:49:28, v0.4rn-max(WM-Basic(B0 V, Z=0.008, Teff=30200, log_lum=4.80, log_g=4.00) (extinction lmcavg=0.060), flux1700 +- 5.0A flux=1e-13 Flam); cos,fuv,g160m,c1611,psa,mjd#59305; fp-pos=None, segment=None)
From file LMC_2020Feb20/input/LMC_all_do1_fixed_wr_NewCoords_pids.csv
Spectral type: B0V --> B0 V
SED = HV5622_COS_G160M_c1611_sed.fits
For exptime=2693.0 s, spectral region:
1590.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 1668.5 cts/s/segment
brightest pixel: 0.028 cts/s/pix at 1442.0 A
Calculation performed 2020-02-24T17:49:28, v0.4rn-max(WM-Basic(B0 V, Z=0.008, Teff=30200, log_lum=4.80, log_g=4.00) (extinction lmcavg=0.060), flux1700 +- 5.0A flux=1e-13 Flam); cos,fuv,g160m,c1611,psa,mjd#59305; fp-pos=None, segment=None)
From file LMC_2020Feb20/input/LMC_all_do1_fixed_wr_NewCoords_pids.csv
Spectral type: B0V --> B0 V
SED = HV5622_COS_G160M_c1611_sed.fits
For exptime=2693.0 s, spectral region:
1590.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 1668.5 cts/s/segment
brightest pixel: 0.028 cts/s/pix at 1442.0 A
Calculation performed 2020-02-24T17:49:28, v0.4rn-max(WM-Basic(B0 V, Z=0.008, Teff=30200, log_lum=4.80, log_g=4.00) (extinction lmcavg=0.060), flux1700 +- 5.0A flux=1e-13 Flam); cos,fuv,g160m,c1611,psa,mjd#59305; fp-pos=None, segment=None)
From file LMC_2020Feb20/input/LMC_all_do1_fixed_wr_NewCoords_pids.csv
Spectral type: B0V --> B0 V
SED = HV5622_COS_G160M_c1611_sed.fits
For exptime=2693.0 s, spectral region:
1590.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 1668.5 cts/s/segment
brightest pixel: 0.028 cts/s/pix at 1442.0 A
Calculation performed 2020-02-24T17:49:28, v0.4rn-max(WM-Basic(B0 V, Z=0.008, Teff=30200, log_lum=4.80, log_g=4.00) (extinction lmcavg=0.060), flux1700 +- 5.0A flux=1e-13 Flam); cos,fuv,g160m,c1611,psa,mjd#59305; fp-pos=None, segment=None)
From file LMC_2020Feb20/input/LMC_all_do1_fixed_wr_NewCoords_pids.csv
Spectral type: B0V --> B0 V
SED = HV5622_COS_G160M_c1611_sed.fits
For exptime=2693.0 s, spectral region:
1590.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 1668.5 cts/s/segment
brightest pixel: 0.028 cts/s/pix at 1442.0 A
Calculation performed 2020-02-24T17:49:28, v0.4The scheduling data was generated by CASM 28.2.CASM was run in Phase II mode./private/var/folders/mk/5ss11qnx2hq98tz1y17xc5080001ws/T/OPVisit4953494738476339625.xmlvstatus; AC; HV5622; P/COS approved for submission; P/WF 12/03/20 ; intrev: completed ; P/CP 14/05/20
vcheck; Enter targ name & Inst. & Resp. Sci.; HV5622 ; COS ; WF
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?; dispersed 1291
vcheck; Possible ACQ or Sci spoilers?; no
vcheck; Field BOT clear?; yes. BOT finds 2 safe stars, 0 unknown, 0 unsafe in GSC2 check
vcheck; Visual BOT check for stars not in catalog?; no objects of concern ...
The GSC2 doesn't include a lot of the stars in this field, but the brighest field object in the PSA macro aperture is well below any BOP limits as B/V = 19/17.1 in Zaritsky catalog and G=16.85 in Gaia.
vcheck; Orbit packing finalized?; yes ...
Exposure times for both cenwaves exceed request by 3%, FP-POS 1 of c1611 is split between orbits to keep times equal
This is a repeat of the second orbit of visit 1C. See notes in the target's Box folder for details about how the orbit was set up.
vcheck; Buffer times optimized?; yes
vcheck; Verify visit grouping correct; n/a
vcheck; Is visit ready for int. review?; yes
Allocated COS orbits = 2, used = 2(Tic-Visit
:proposal-id 16096
:visit-id "AC"
:proposal-version -1
:trans-version "20200619"
:date "12-Oct-2020 09:56:03.0"
: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 287136
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16096
:visit-id "AC"
:obset-id "AC"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16096
:visit-id "AC"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2576
:al-overhead-at-end 0
:internal-dur-at-end 341
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2970
:pcs-gap 0
)true10rn-max(WM-Basic(B0 V, Z=0.008, Teff=30200, log_lum=4.80, log_g=4.00) (extinction lmcavg=0.060), flux1700 +- 5.0A flux=1e-13 Flam); cos,fuv,g160m,c1611,psa,mjd#59305; fp-pos=None, segment=None)
From file LMC_2020Feb20/input/LMC_all_do1_fixed_wr_NewCoords_pids.csv
Spectral type: B0V --> B0 V
SED = HV5622_COS_G160M_c1611_sed.fits
For exptime=2693.0 s, spectral region:
1590.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 1668.5 cts/s/segment
brightest pixel: 0.028 cts/s/pix at 1442.0 A
Calculation performed 2020-02-24T17:49:28, v0.4rn-max(WM-Basic(B0 V, Z=0.008, Teff=30200, log_lum=4.80, log_g=4.00) (extinction lmcavg=0.060), flux1700 +- 5.0A flux=1e-13 Flam); cos,fuv,g160m,c1611,psa,mjd#59305; fp-pos=None, segment=None)
From file LMC_2020Feb20/input/LMC_all_do1_fixed_wr_NewCoords_pids.csv
Spectral type: B0V --> B0 V
SED = HV5622_COS_G160M_c1611_sed.fits
For exptime=2693.0 s, spectral region:
1590.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 1668.5 cts/s/segment
brightest pixel: 0.028 cts/s/pix at 1442.0 A
Calculation performed 2020-02-24T17:49:28, v0.4rn-max(WM-Basic(B0 V, Z=0.008, Teff=30200, log_lum=4.80, log_g=4.00) (extinction lmcavg=0.060), flux1700 +- 5.0A flux=1e-13 Flam); cos,fuv,g160m,c1611,psa,mjd#59305; fp-pos=None, segment=None)
From file LMC_2020Feb20/input/LMC_all_do1_fixed_wr_NewCoords_pids.csv
Spectral type: B0V --> B0 V
SED = HV5622_COS_G160M_c1611_sed.fits
For exptime=2693.0 s, spectral region:
1590.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 1668.5 cts/s/segment
brightest pixel: 0.028 cts/s/pix at 1442.0 A
Calculation performed 2020-02-24T17:49:28, v0.4The scheduling data was generated by CASM 28.2.CASM was run in Phase II mode.vstatus; 2C; LH9-89; P/COS approved for submission; P/WF 09/04/20 ; intrev: completed ; P/CP 14/05/20
vcheck; Enter targ name & Inst. & Resp. Sci.; LH9-89 ; COS ; WF
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?; dispersed 1291
vcheck; Possible ACQ or Sci spoilers?; no
vcheck; Field BOT clear?; yes. BOT finds 6 safe stars, 2 unknown, 0 unsafe in GSC2 check ...
One unknown is the target, cleared with ETC. The other is in the BOA radius and 19th mag in Gaia, so safe.
vcheck; Visual BOT check for stars not in catalog?; no objects of concern
vcheck; Orbit packing finalized?; yes ...
Exposure times for both cenwaves exceed request by 99%, FP-POS 1 of c1611 is split between orbits to keep times equal
would need to cut exp times by about 30% to fit in one orbit
vcheck; Buffer times optimized?; yes
vcheck; Verify visit grouping correct; n/a
vcheck; Is visit ready for int. review?; yes
Allocated COS orbits = 2, used = 21595887185000229.50012518673282(Tic-Visit
:proposal-id 16096
:visit-id "2C"
:proposal-version -1
:trans-version "20191203"
:date "14-May-2020 15:49:18.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 2
:saa-model "31"
:si-bright-earth-limb-angle 20.0
:data-volume 1513440
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16096
:visit-id "2C"
:obset-id "2C"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16096
:visit-id "2C"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2577
:al-overhead-at-end 0
:internal-dur-at-end 86
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2970
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16096
:visit-id "2C"
:orbit-number 2
:pcs-time 302
:si-vis-utilization 2668
:al-overhead-at-end 0
:internal-dur-at-end 369
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2970
:pcs-gap 0
)true20rn(WM-Basic(B0 III, Z=0.008, Teff=28184, log_lum=5.12, log_g=3.54) (extinction lmcavg=0.140), johnson B mag=13.520 vegamag); cos,fuv,g130m,c1291,psa,mjd#59305; fp-pos=None, segment=None)
From file LMC_2020Feb20/input/LMC_all_do1_fixed_wr_NewCoords_pids.csv
Spectral type: B0 IIIn --> B0 III
SED = LH9-89_COS_G130M_c1291_sed.fits
For exptime=767.3 s, spectral region:
1150.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 5138.6 cts/s/segment
brightest pixel: 0.086 cts/s/pix at 1266.0 A
Calculation performed 2020-02-24T17:49:00, v0.4rn(WM-Basic(B0 III, Z=0.008, Teff=28184, log_lum=5.12, log_g=3.54) (extinction lmcavg=0.140), johnson B mag=13.520 vegamag); cos,fuv,g130m,c1291,psa,mjd#59305; fp-pos=None, segment=None)
From file LMC_2020Feb20/input/LMC_all_do1_fixed_wr_NewCoords_pids.csv
Spectral type: B0 IIIn --> B0 III
SED = LH9-89_COS_G130M_c1291_sed.fits
For exptime=767.3 s, spectral region:
1150.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 5138.6 cts/s/segment
brightest pixel: 0.086 cts/s/pix at 1266.0 A
Calculation performed 2020-02-24T17:49:00, v0.4rn(WM-Basic(B0 III, Z=0.008, Teff=28184, log_lum=5.12, log_g=3.54) (extinction lmcavg=0.140), johnson B mag=13.520 vegamag); cos,fuv,g160m,c1611,psa,mjd#59305; fp-pos=None, segment=None)
From file LMC_2020Feb20/input/LMC_all_do1_fixed_wr_NewCoords_pids.csv
Spectral type: B0 IIIn --> B0 III
SED = LH9-89_COS_G160M_c1611_sed.fits
For exptime=1211.6 s, spectral region:
1590.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 3363.0 cts/s/segment
brightest pixel: 0.055 cts/s/pix at 1442.0 A
Calculation performed 2020-02-24T17:49:02, v0.4rn(WM-Basic(B0 III, Z=0.008, Teff=28184, log_lum=5.12, log_g=3.54) (extinction lmcavg=0.140), johnson B mag=13.520 vegamag); cos,fuv,g160m,c1611,psa,mjd#59305; fp-pos=None, segment=None)
From file LMC_2020Feb20/input/LMC_all_do1_fixed_wr_NewCoords_pids.csv
Spectral type: B0 IIIn --> B0 III
SED = LH9-89_COS_G160M_c1611_sed.fits
For exptime=1211.6 s, spectral region:
1590.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 3363.0 cts/s/segment
brightest pixel: 0.055 cts/s/pix at 1442.0 A
Calculation performed 2020-02-24T17:49:02, v0.4rn(WM-Basic(B0 III, Z=0.008, Teff=28184, log_lum=5.12, log_g=3.54) (extinction lmcavg=0.140), johnson B mag=13.520 vegamag); cos,fuv,g160m,c1611,psa,mjd#59305; fp-pos=None, segment=None)
From file LMC_2020Feb20/input/LMC_all_do1_fixed_wr_NewCoords_pids.csv
Spectral type: B0 IIIn --> B0 III
SED = LH9-89_COS_G160M_c1611_sed.fits
For exptime=1211.6 s, spectral region:
1590.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 3363.0 cts/s/segment
brightest pixel: 0.055 cts/s/pix at 1442.0 A
Calculation performed 2020-02-24T17:49:02, v0.4rn(WM-Basic(B0 III, Z=0.008, Teff=28184, log_lum=5.12, log_g=3.54) (extinction lmcavg=0.140), johnson B mag=13.520 vegamag); cos,fuv,g160m,c1611,psa,mjd#59305; fp-pos=None, segment=None)
From file LMC_2020Feb20/input/LMC_all_do1_fixed_wr_NewCoords_pids.csv
Spectral type: B0 IIIn --> B0 III
SED = LH9-89_COS_G160M_c1611_sed.fits
For exptime=1211.6 s, spectral region:
1590.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 3363.0 cts/s/segment
brightest pixel: 0.055 cts/s/pix at 1442.0 A
Calculation performed 2020-02-24T17:49:02, v0.4rn(WM-Basic(B0 III, Z=0.008, Teff=28184, log_lum=5.12, log_g=3.54) (extinction lmcavg=0.140), johnson B mag=13.520 vegamag); cos,fuv,g160m,c1611,psa,mjd#59305; fp-pos=None, segment=None)
From file LMC_2020Feb20/input/LMC_all_do1_fixed_wr_NewCoords_pids.csv
Spectral type: B0 IIIn --> B0 III
SED = LH9-89_COS_G160M_c1611_sed.fits
For exptime=1211.6 s, spectral region:
1590.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 3363.0 cts/s/segment
brightest pixel: 0.055 cts/s/pix at 1442.0 A
Calculation performed 2020-02-24T17:49:02, v0.4The scheduling data was generated by CASM 28.2.CASM was run in Phase II mode.vstatus; 3C; N206-FS-170; P/COS approved for submission; P/WF 16/04/20 ; intrev: completed ; P/CP 14/05/20
vcheck; Enter targ name & Inst. & Resp. Sci.; N206-FS-170 ; COS ; WF
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?; dispersed 1291
vcheck; Possible ACQ or Sci spoilers?; no
vcheck; Field BOT clear?; yes. BOT finds 15-16 safe stars depending on config and 1 unsafe for 1291 in GSC2 check ...
The unsafe is the target (assumed O5V), but it was cleared with the ETC (actually B1V).
vcheck; Visual BOT check for stars not in catalog?; no objects of concern
vcheck; Orbit packing finalized?; yes ...
Exposure times for both cenwaves fall 3% short of request, FP-POS 1 of c1611 is split between orbits to keep times equal
vcheck; Buffer times optimized?; yes
vcheck; Verify visit grouping correct; n/a
vcheck; Is visit ready for int. review?; yes
Allocated COS orbits = 2, used = 21601504615000284.7446088183438(Tic-Visit
:proposal-id 16096
:visit-id "3C"
:proposal-version -1
:trans-version "20191203"
:date "14-May-2020 16:39:44.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 2
:saa-model "31"
:si-bright-earth-limb-angle 20.0
:data-volume 661136
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16096
:visit-id "3C"
:obset-id "3C"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16096
:visit-id "3C"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2596
: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 2989
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16096
:visit-id "3C"
:orbit-number 2
:pcs-time 302
:si-vis-utilization 2687
:al-overhead-at-end 0
:internal-dur-at-end 398
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2989
:pcs-gap 0
)true20rn(WM-Basic(B1 V, Z=0.008, Teff=26303, log_lum=4.45, log_g=4.00) (extinction lmcavg=0.090), johnson U mag=13.630 vegamag); cos,fuv,g130m,c1291,psa,mjd#59305; fp-pos=None, segment=None)
From file LMC_2020Feb20/input/LMC_all_do1_fixed_wr_NewCoords_pids.csv
Spectral type: B1 IV --> B1 V
SED = N206-FS-170_COS_G130M_c1291_sed.fits
For exptime=1448.0 s, spectral region:
1150.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 2849.2 cts/s/segment
brightest pixel: 0.044 cts/s/pix at 1265.0 A
Calculation performed 2020-02-24T17:50:52, v0.4rn(WM-Basic(B1 V, Z=0.008, Teff=26303, log_lum=4.45, log_g=4.00) (extinction lmcavg=0.090), johnson U mag=13.630 vegamag); cos,fuv,g130m,c1291,psa,mjd#59305; fp-pos=None, segment=None)
From file LMC_2020Feb20/input/LMC_all_do1_fixed_wr_NewCoords_pids.csv
Spectral type: B1 IV --> B1 V
SED = N206-FS-170_COS_G130M_c1291_sed.fits
For exptime=1448.0 s, spectral region:
1150.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 2849.2 cts/s/segment
brightest pixel: 0.044 cts/s/pix at 1265.0 A
Calculation performed 2020-02-24T17:50:52, v0.4rn(WM-Basic(B1 V, Z=0.008, Teff=26303, log_lum=4.45, log_g=4.00) (extinction lmcavg=0.090), johnson U mag=13.630 vegamag); cos,fuv,g160m,c1611,psa,mjd#59305; fp-pos=None, segment=None)
From file LMC_2020Feb20/input/LMC_all_do1_fixed_wr_NewCoords_pids.csv
Spectral type: B1 IV --> B1 V
SED = N206-FS-170_COS_G160M_c1611_sed.fits
For exptime=2657.7 s, spectral region:
1590.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 1490.2 cts/s/segment
brightest pixel: 0.026 cts/s/pix at 1435.0 A
Calculation performed 2020-02-24T17:50:55, v0.4rn(WM-Basic(B1 V, Z=0.008, Teff=26303, log_lum=4.45, log_g=4.00) (extinction lmcavg=0.090), johnson U mag=13.630 vegamag); cos,fuv,g160m,c1611,psa,mjd#59305; fp-pos=None, segment=None)
From file LMC_2020Feb20/input/LMC_all_do1_fixed_wr_NewCoords_pids.csv
Spectral type: B1 IV --> B1 V
SED = N206-FS-170_COS_G160M_c1611_sed.fits
For exptime=2657.7 s, spectral region:
1590.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 1490.2 cts/s/segment
brightest pixel: 0.026 cts/s/pix at 1435.0 A
Calculation performed 2020-02-24T17:50:55, v0.4rn(WM-Basic(B1 V, Z=0.008, Teff=26303, log_lum=4.45, log_g=4.00) (extinction lmcavg=0.090), johnson U mag=13.630 vegamag); cos,fuv,g160m,c1611,psa,mjd#59305; fp-pos=None, segment=None)
From file LMC_2020Feb20/input/LMC_all_do1_fixed_wr_NewCoords_pids.csv
Spectral type: B1 IV --> B1 V
SED = N206-FS-170_COS_G160M_c1611_sed.fits
For exptime=2657.7 s, spectral region:
1590.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 1490.2 cts/s/segment
brightest pixel: 0.026 cts/s/pix at 1435.0 A
Calculation performed 2020-02-24T17:50:55, v0.4rn(WM-Basic(B1 V, Z=0.008, Teff=26303, log_lum=4.45, log_g=4.00) (extinction lmcavg=0.090), johnson U mag=13.630 vegamag); cos,fuv,g160m,c1611,psa,mjd#59305; fp-pos=None, segment=None)
From file LMC_2020Feb20/input/LMC_all_do1_fixed_wr_NewCoords_pids.csv
Spectral type: B1 IV --> B1 V
SED = N206-FS-170_COS_G160M_c1611_sed.fits
For exptime=2657.7 s, spectral region:
1590.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 1490.2 cts/s/segment
brightest pixel: 0.026 cts/s/pix at 1435.0 A
Calculation performed 2020-02-24T17:50:55, v0.4rn(WM-Basic(B1 V, Z=0.008, Teff=26303, log_lum=4.45, log_g=4.00) (extinction lmcavg=0.090), johnson U mag=13.630 vegamag); cos,fuv,g160m,c1611,psa,mjd#59305; fp-pos=None, segment=None)
From file LMC_2020Feb20/input/LMC_all_do1_fixed_wr_NewCoords_pids.csv
Spectral type: B1 IV --> B1 V
SED = N206-FS-170_COS_G160M_c1611_sed.fits
For exptime=2657.7 s, spectral region:
1590.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 1490.2 cts/s/segment
brightest pixel: 0.026 cts/s/pix at 1435.0 A
Calculation performed 2020-02-24T17:50:55, v0.4The scheduling data was generated by CASM 28.2.CASM was run in Phase II mode.vstatus; 4C; SK-70D16; P/COS approved for submission; P/WF 11/05/20 ; intrev: completed ; P/CP 14/05/20
vcheck; Enter targ name & Inst. & Resp. Sci.; SK-70D16 ; COS ; WF
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?; dispersed 1291
vcheck; Possible ACQ or Sci spoilers?; no
vcheck; Field BOT clear?; yes. BOT finds 13-15 safe stars depending on config and 1 unsafe for FUV in GSC2 check ...
The unsafe is the target (assumed O5V), but it was cleared with the ETC (actually B4I).
vcheck; Visual BOT check for stars not in catalog?; no objects of concern
vcheck; Orbit packing finalized?; yes ...
Exposure times per cenwave exceed request by 6 to 23%
vcheck; Buffer times optimized?; yes
vcheck; Verify visit grouping correct; n/a
vcheck; Is visit ready for int. review?; yes
Allocated COS orbits = 3, used = 31603558021000316.7201669485503(Tic-Visit
:proposal-id 16096
:visit-id "4C"
:proposal-version -1
:trans-version "20191203"
:date "14-May-2020 15:50:35.0"
: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 1078800
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16096
:visit-id "4C"
:obset-id "4C"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16096
:visit-id "4C"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2596
:al-overhead-at-end 0
:internal-dur-at-end 95
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2989
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16096
:visit-id "4C"
:orbit-number 2
:pcs-time 302
:si-vis-utilization 2686
: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 2989
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16096
:visit-id "4C"
:orbit-number 3
:pcs-time 302
:si-vis-utilization 2684
:al-overhead-at-end 0
:internal-dur-at-end 360
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2989
:pcs-gap 0
)true30rn(ck04models(B4I,Teff=16080,metallicity=0.008,logG=2.52) (extinction lmcavg=0.070), johnson U mag=12.190 vegamag); cos,fuv,g130m,c1291,psa,mjd#59305; fp-pos=None, segment=None)
From file LMC_2020Feb20/input/LMC_all_do1_fixed_wr_NewCoords_pids.csv
Spectral type: B4 I --> B4 I
SED = SK-70D16_COS_G130M_c1291_sed.fits
For exptime=1182.9 s, spectral region:
1150.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 2871.7 cts/s/segment
brightest pixel: 0.054 cts/s/pix at 1277.0 A
Calculation performed 2020-02-24T17:51:53, v0.4rn(ck04models(B4I,Teff=16080,metallicity=0.008,logG=2.52) (extinction lmcavg=0.070), johnson U mag=12.190 vegamag); cos,fuv,g130m,c1291,psa,mjd#59305; fp-pos=None, segment=None)
From file LMC_2020Feb20/input/LMC_all_do1_fixed_wr_NewCoords_pids.csv
Spectral type: B4 I --> B4 I
SED = SK-70D16_COS_G130M_c1291_sed.fits
For exptime=1182.9 s, spectral region:
1150.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 2871.7 cts/s/segment
brightest pixel: 0.054 cts/s/pix at 1277.0 A
Calculation performed 2020-02-24T17:51:53, v0.4rn(ck04models(B4I,Teff=16080,metallicity=0.008,logG=2.52) (extinction lmcavg=0.070), johnson U mag=12.190 vegamag); cos,fuv,g160m,c1611,psa,mjd#59305; fp-pos=None, segment=None)
From file LMC_2020Feb20/input/LMC_all_do1_fixed_wr_NewCoords_pids.csv
Spectral type: B4 I --> B4 I
SED = SK-70D16_COS_G160M_c1611_sed.fits
For exptime=1326.7 s, spectral region:
1590.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 2508.3 cts/s/segment
brightest pixel: 0.038 cts/s/pix at 1442.0 A
Calculation performed 2020-02-24T17:51:55, v0.4rn(ck04models(B4I,Teff=16080,metallicity=0.008,logG=2.52) (extinction lmcavg=0.070), johnson U mag=12.190 vegamag); cos,nuv,g185m,c1953,psa,mjd#59305
From file LMC_2020Feb20/input/LMC_all_do1_fixed_wr_NewCoords_pids.csv
Spectral type: B4 I --> B4 I
SED = SK-70D16_COS_G185M_c1953_sed.fits
For exptime=1229.6 s, spectral region:
1860.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 1681.0 cts/s/segment
brightest pixel: 0.139 cts/s/pix at 1872.0 A
Calculation performed 2020-02-24T17:51:56, v0.4rn(ck04models(B4I,Teff=16080,metallicity=0.008,logG=2.52) (extinction lmcavg=0.070), johnson U mag=12.190 vegamag); cos,nuv,g185m,c1986,psa,mjd#59305
From file LMC_2020Feb20/input/LMC_all_do1_fixed_wr_NewCoords_pids.csv
Spectral type: B4 I --> B4 I
SED = SK-70D16_COS_G185M_c1986_sed.fits
For exptime=1192.7 s, spectral region:
1980.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 1680.5 cts/s/segment
brightest pixel: 0.145 cts/s/pix at 1875.0 A
Calculation performed 2020-02-24T17:51:56, v0.4The scheduling data was generated by CASM 28.2.CASM was run in Phase II mode.vstatus; 5C; VFTS-66; P/COS approved for submission; P/WF 27/05/20 ; intrev: needs to be redone ; P/CP 14/05/20
vcheck; Enter targ name & Inst. & Resp. Sci.; VFTS-66; COS; WF
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?; dispersed 1291
vcheck; Possible ACQ or Sci spoilers?; no ...
The GSC2 entry that is very close to the target is 4 magnitudes fainter at V
vcheck; Field BOT clear?; yes. BOT/GSC2 finds 11-12 safe stars depending on config and 1 unknown ...
The unknown is a pair of stars in Gaia, both with G fainter than 19th mag, so it is fine
vcheck; Visual BOT check for stars not in catalog?; no concerns
vcheck; Orbit packing finalized?; yes ...
Exposure time is only 32% of ETC as agreed upon by CIT
vcheck; Buffer times optimized?; yes
vcheck; Verify visit grouping correct; none needed
vcheck; Is visit ready for int. review?; yes
Allocated COS orbits = 3, used = 31603632412000307.5182834557381(Tic-Visit
:proposal-id 16096
:visit-id "5C"
:proposal-version -1
:trans-version "20191203"
:date "27-May-2020 14:31:10.0"
: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 304528
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16096
:visit-id "5C"
:obset-id "5C"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16096
:visit-id "5C"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2577
:al-overhead-at-end 0
:internal-dur-at-end 114
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2970
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16096
:visit-id "5C"
:orbit-number 2
:pcs-time 302
:si-vis-utilization 2668
: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 2970
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16096
:visit-id "5C"
:orbit-number 3
:pcs-time 302
:si-vis-utilization 2668
:al-overhead-at-end 0
:internal-dur-at-end 341
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2970
:pcs-gap 0
)true30rn(WM-Basic(O9 V, Z=0.008, Teff=32359, log_lum=5.00, log_g=4.00), johnson B mag=15.640 vegamag); cos,fuv,g130m,c1291,psa,mjd#59305; fp-pos=None, segment=None)
From file LMC_2020Feb20/input/LMC_all_do1_fixed_wr_NewCoords_pids.csv
Spectral type: O9V + B0.2V --> O9 V
SED = VFTS-66_COS_G130M_c1291_sed.fits
For exptime=1126.3 s, spectral region:
1150.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 3060.8 cts/s/segment
brightest pixel: 0.042 cts/s/pix at 1265.0 A
Calculation performed 2020-02-24T18:09:05, v0.4rn(WM-Basic(O9 V, Z=0.008, Teff=32359, log_lum=5.00, log_g=4.00), johnson B mag=15.640 vegamag); cos,fuv,g130m,c1291,psa,mjd#59305; fp-pos=None, segment=None)
From file LMC_2020Feb20/input/LMC_all_do1_fixed_wr_NewCoords_pids.csv
Spectral type: O9V + B0.2V --> O9 V
SED = VFTS-66_COS_G130M_c1291_sed.fits
For exptime=1126.3 s, spectral region:
1150.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 3060.8 cts/s/segment
brightest pixel: 0.042 cts/s/pix at 1265.0 A
Calculation performed 2020-02-24T18:09:05, v0.4rn(WM-Basic(O9 V, Z=0.008, Teff=32359, log_lum=5.00, log_g=4.00), johnson B mag=15.640 vegamag); cos,fuv,g130m,c1291,psa,mjd#59305; fp-pos=None, segment=None)
From file LMC_2020Feb20/input/LMC_all_do1_fixed_wr_NewCoords_pids.csv
Spectral type: O9V + B0.2V --> O9 V
SED = VFTS-66_COS_G130M_c1291_sed.fits
For exptime=1126.3 s, spectral region:
1150.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 3060.8 cts/s/segment
brightest pixel: 0.042 cts/s/pix at 1265.0 A
Calculation performed 2020-02-24T18:09:05, v0.4rn(WM-Basic(O9 V, Z=0.008, Teff=32359, log_lum=5.00, log_g=4.00), johnson B mag=15.640 vegamag); cos,fuv,g130m,c1291,psa,mjd#59305; fp-pos=None, segment=None)
From file LMC_2020Feb20/input/LMC_all_do1_fixed_wr_NewCoords_pids.csv
Spectral type: O9V + B0.2V --> O9 V
SED = VFTS-66_COS_G130M_c1291_sed.fits
For exptime=1126.3 s, spectral region:
1150.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 3060.8 cts/s/segment
brightest pixel: 0.042 cts/s/pix at 1265.0 A
Calculation performed 2020-02-24T18:09:05, v0.4The scheduling data was generated by CASM 28.2.CASM was run in Phase II mode.vstatus; 5C; VFTS-66; P/COS approved for submission; P/WF 27/05/20 ; intrev: needs to be redone ; P/CP 14/05/27
vcheck; Enter targ name & Inst. & Resp. Sci.; VFTS-66; COS; WF
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?; dispersed 1611
vcheck; Possible ACQ or Sci spoilers?; no ...
The GSC2 entry that is very close to the target is 4 magnitudes fainter at V
vcheck; Field BOT clear?; yes. BOT/GSC2 finds 11-12 safe stars depending on config and 1 unknown ...
The unknown is a pair of stars in Gaia, both with G fainter than 19th mag, so it is fine
vcheck; Visual BOT check for stars not in catalog?; no concerns
vcheck; Orbit packing finalized?; yes ...
Exposure time is only 38% of ETC as agreed upon by CIT
vcheck; Buffer times optimized?; yes
vcheck; Verify visit grouping correct; none needed
vcheck; Is visit ready for int. review?; yes
Allocated COS orbits = 3, used = 31603649559000307.714523094016(Tic-Visit
:proposal-id 16096
:visit-id "5D"
:proposal-version -1
:trans-version "20191203"
:date "27-May-2020 14:28:42.0"
: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 252464
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16096
:visit-id "5D"
:obset-id "5D"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16096
:visit-id "5D"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2577
:al-overhead-at-end 0
:internal-dur-at-end 38
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2970
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16096
:visit-id "5D"
:orbit-number 2
:pcs-time 302
:si-vis-utilization 2668
: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 2970
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16096
:visit-id "5D"
:orbit-number 3
:pcs-time 302
:si-vis-utilization 2668
:al-overhead-at-end 0
:internal-dur-at-end 360
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2970
:pcs-gap 0
)true30rn(WM-Basic(O9 V, Z=0.008, Teff=32359, log_lum=5.00, log_g=4.00), johnson B mag=15.640 vegamag); cos,fuv,g160m,c1611,psa,mjd#59305; fp-pos=None, segment=None)
From file LMC_2020Feb20/input/LMC_all_do1_fixed_wr_NewCoords_pids.csv
Spectral type: O9V + B0.2V --> O9 V
SED = VFTS-66_COS_G160M_c1611_sed.fits
For exptime=3862.6 s, spectral region:
1590.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 1230.6 cts/s/segment
brightest pixel: 0.020 cts/s/pix at 1442.0 A
Calculation performed 2020-02-24T18:09:07, v0.4rn(WM-Basic(O9 V, Z=0.008, Teff=32359, log_lum=5.00, log_g=4.00), johnson B mag=15.640 vegamag); cos,fuv,g160m,c1611,psa,mjd#59305; fp-pos=None, segment=None)
From file LMC_2020Feb20/input/LMC_all_do1_fixed_wr_NewCoords_pids.csv
Spectral type: O9V + B0.2V --> O9 V
SED = VFTS-66_COS_G160M_c1611_sed.fits
For exptime=3862.6 s, spectral region:
1590.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 1230.6 cts/s/segment
brightest pixel: 0.020 cts/s/pix at 1442.0 A
Calculation performed 2020-02-24T18:09:07, v0.4rn(WM-Basic(O9 V, Z=0.008, Teff=32359, log_lum=5.00, log_g=4.00), johnson B mag=15.640 vegamag); cos,fuv,g160m,c1611,psa,mjd#59305; fp-pos=None, segment=None)
From file LMC_2020Feb20/input/LMC_all_do1_fixed_wr_NewCoords_pids.csv
Spectral type: O9V + B0.2V --> O9 V
SED = VFTS-66_COS_G160M_c1611_sed.fits
For exptime=3862.6 s, spectral region:
1590.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 1230.6 cts/s/segment
brightest pixel: 0.020 cts/s/pix at 1442.0 A
Calculation performed 2020-02-24T18:09:07, v0.4rn(WM-Basic(O9 V, Z=0.008, Teff=32359, log_lum=5.00, log_g=4.00), johnson B mag=15.640 vegamag); cos,fuv,g160m,c1611,psa,mjd#59305; fp-pos=None, segment=None)
From file LMC_2020Feb20/input/LMC_all_do1_fixed_wr_NewCoords_pids.csv
Spectral type: O9V + B0.2V --> O9 V
SED = VFTS-66_COS_G160M_c1611_sed.fits
For exptime=3862.6 s, spectral region:
1590.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 1230.6 cts/s/segment
brightest pixel: 0.020 cts/s/pix at 1442.0 A
Calculation performed 2020-02-24T18:09:07, v0.4rn(WM-Basic(O9 V, Z=0.008, Teff=32359, log_lum=5.00, log_g=4.00), johnson B mag=15.640 vegamag); cos,fuv,g160m,c1611,psa,mjd#59305; fp-pos=None, segment=None)
From file LMC_2020Feb20/input/LMC_all_do1_fixed_wr_NewCoords_pids.csv
Spectral type: O9V + B0.2V --> O9 V
SED = VFTS-66_COS_G160M_c1611_sed.fits
For exptime=3862.6 s, spectral region:
1590.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 1230.6 cts/s/segment
brightest pixel: 0.020 cts/s/pix at 1442.0 A
Calculation performed 2020-02-24T18:09:07, v0.4rn(WM-Basic(O9 V, Z=0.008, Teff=32359, log_lum=5.00, log_g=4.00), johnson B mag=15.640 vegamag); cos,fuv,g160m,c1611,psa,mjd#59305; fp-pos=None, segment=None)
From file LMC_2020Feb20/input/LMC_all_do1_fixed_wr_NewCoords_pids.csv
Spectral type: O9V + B0.2V --> O9 V
SED = VFTS-66_COS_G160M_c1611_sed.fits
For exptime=3862.6 s, spectral region:
1590.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 1230.6 cts/s/segment
brightest pixel: 0.020 cts/s/pix at 1442.0 A
Calculation performed 2020-02-24T18:09:07, v0.4