The list of Investigators does not match the STScI records for this program.Needed only 16 orbits, 1 under the original estimate of 17
Resubmitting to fix non-ascii characters in comment fields.-1821517242----- Attempting Submission 1 (Sat May 16 02:16:46 GMT 2020) -----
----- Attempting Submission 2 (Wed May 20 19:27:50 GMT 2020) -----Proposer list reflects current membership of CIT team
Removed Andrew Fox from CoI list at his request.
Only needed 16 orbits instead of the 17 allocated.ULLYSES SMC B2 to B4 Supergiants COS/STISThe 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-STARB3-B5 III-INOAV187 : AV_187, AzV 187
Previous name : AV187
Input file: SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
SIMBAD link (AzV 187): https://simbad.u-strasbg.fr/simbad/sim-id?Ident=AzV+187&submit=submit+id
SpT = B3Ia
COS/G130M/c1096 : rn-max(ck04models(B3I,Teff=18560,metallicity=0.004,logG=2.6) (extinction smcbar=0.030), flux1160 +- 30.0A flux=5.1e-13 Flam)
COS/G130M/c1291 : rn-max(ck04models(B3I,Teff=18560,metallicity=0.004,logG=2.6) (extinction smcbar=0.030), flux1360 +- 30.0A flux=5.3e-13 Flam)
COS/G160M/c1611 : rn-max(ck04models(B3I,Teff=18560,metallicity=0.004,logG=2.6) (extinction smcbar=0.030), flux1700 +- 5.0A flux=4.7e-13 Flam)
COS/G185M/c1921 : rn-max(ck04models(B3I,Teff=18560,metallicity=0.004,logG=2.6) (extinction smcbar=0.030), flux1700 +- 5.0A flux=4.7e-13 Flam)
COS/G185M/c1953 : rn-max(ck04models(B3I,Teff=18560,metallicity=0.004,logG=2.6) (extinction smcbar=0.030), flux1700 +- 5.0A flux=4.7e-13 Flam)
COS/G185M/c1986 : rn-max(ck04models(B3I,Teff=18560,metallicity=0.004,logG=2.6) (extinction smcbar=0.030), flux1700 +- 5.0A flux=4.7e-13 Flam)
STIS/E140M/c1425 : rn-max(ck04models(B3I,Teff=18560,metallicity=0.004,logG=2.6) (extinction smcbar=0.030), flux1360 +- 30.0A flux=5.3e-13 Flam)
STIS/E230M/c1978 : rn-max(ck04models(B3I,Teff=18560,metallicity=0.004,logG=2.6) (extinction smcbar=0.030), flux1700 +- 5.0A flux=4.7e-13 Flam)
STIS/E230M/c2707 : rn-max(ck04models(B3I,Teff=18560,metallicity=0.004,logG=2.6) (extinction smcbar=0.030), flux1700 +- 5.0A flux=4.7e-13 Flam)
Coordinate pedigree: Gaia
Calculation performed 2020-02-24T17:53:41, v0.4
-------------------------------------------------------------------------------
tstatus; AV187; P/COS Approved for submission; S/STIS ready for internal review; P/CP 25/02/20; S/CP DD/MM/YY
tcheck; APT/SIMBAD target names: ; aka SK 68
tcheck; Target info verification status?; complete ...
SIMBAD gives SpT=B2.5Ia, SIMBAD photometry close to our results.
tcheck; Coordinates & P.M. updated?; Yes ...
coordinates from Gaia agree with SIMBAD - proper motion corrections not needed
tcheck; Adopted SED compared to Observations?; Yes ...
suggests slightly steeper spectrum - perhaps E(B-V)=0.06 rather than 0.03
c160040100000nvo4ttagfcal_vo.fits lwp12385mxlo_vo.fits swp32626mxlo_vo.fitsSK682MASS-J00573171-7119592J2000SpT=B3Ia; E(B-V)=0.03; U=11.2; B=12.0; V=12.1; F1160=5.08e-13; F1360=5.30e-13; F1700=4.70e-13EXT-STARB3-B5 III-INOAV234 : [M2002]_47028, AV 234, AzV 234
Previous name : AV 234
Input file: SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
SIMBAD link (AzV 234): https://simbad.u-strasbg.fr/simbad/sim-id?Ident=AzV+234&submit=submit+id
SpT = B3Iab
COS/G130M/c1096 : rn-max(ck04models(B3I,Teff=18560,metallicity=0.004,logG=2.6) (extinction smcbar=0.030), flux1160 +- 30.0A flux=5.4e-13 Flam)
COS/G130M/c1291 : rn-max(ck04models(B3I,Teff=18560,metallicity=0.004,logG=2.6) (extinction smcbar=0.030), flux1360 +- 30.0A flux=2.1e-13 Flam)
COS/G160M/c1611 : rn-max(ck04models(B3I,Teff=18560,metallicity=0.004,logG=2.6) (extinction smcbar=0.030), flux1700 +- 5.0A flux=1.8e-13 Flam)
COS/G185M/c1921 : rn-max(ck04models(B3I,Teff=18560,metallicity=0.004,logG=2.6) (extinction smcbar=0.030), flux1700 +- 5.0A flux=1.8e-13 Flam)
COS/G185M/c1953 : rn-max(ck04models(B3I,Teff=18560,metallicity=0.004,logG=2.6) (extinction smcbar=0.030), flux1700 +- 5.0A flux=1.8e-13 Flam)
COS/G185M/c1986 : rn-max(ck04models(B3I,Teff=18560,metallicity=0.004,logG=2.6) (extinction smcbar=0.030), flux2200 +- 5.0A flux=1.2e-13 Flam)
STIS/E140M/c1425 : rn-max(ck04models(B3I,Teff=18560,metallicity=0.004,logG=2.6) (extinction smcbar=0.030), flux1360 +- 30.0A flux=2.1e-13 Flam)
STIS/E230M/c1978 : rn-max(ck04models(B3I,Teff=18560,metallicity=0.004,logG=2.6) (extinction smcbar=0.030), flux2200 +- 5.0A flux=1.2e-13 Flam)
STIS/E230M/c2707 : rn-max(ck04models(B3I,Teff=18560,metallicity=0.004,logG=2.6) (extinction smcbar=0.030), flux2200 +- 5.0A flux=1.2e-13 Flam)
Coordinate pedigree: Gaia
Calculation performed 2020-02-24T17:53:26, v0.4
-------------------------------------------------------------------------------
tstatus; AV234; P/COS Approved for submission; S/STIS ready for internal review; P/CP 21/04/20; S/CP 21/04/20
tcheck; APT/SIMBAD target names: ; AzV 234, SK 81
tcheck; Target info verification status?; Good
tcheck; Coordinates & P.M. updated?; good
tcheck; Adopted SED compared to Observations?; OK? ...
Overall shape isn't quite right, and UBV photometry is a factor of two too bright - however, LWP spectrum does show a upturn at the red end, consistent with the U band flux, so this looks to be a funny shape to the SED rather than a flux underestimate by the IUE/SWP spectra. Emission line at 1212 in IUE spectrum is geo-coronal lyman alpha so not in stellar spectrum. No other backup to FUV/NUV flux so may want to be extra cautious on buffer times and BOP checks. Will adopt as best overall fit to SED the default c1611 spectrum which is normalize at 1700 angstroms and use this for S/N check, but will also do BOP and buffer time checks normalized to V band in case there is something odd about the IUE throughput for this one.SK81M2002-47028J2000SpT=B3Iab; E(B-V)=0.03; U=12.0; B=12.8; V=12.9; I=12.44; F1160=5.35e-13; F1360=2.13e-13; F1700=1.85e-13; F2200=1.25e-13EXT-STARB3-B5 III-INOAV324 : AV_324, AzV324, AzV 324
Previous name : AzV324
Input file: SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
SIMBAD link (AzV 324): https://simbad.u-strasbg.fr/simbad/sim-id?Ident=AzV+324&submit=submit+id
SpT = B4Iab
COS/G130M/c1291 : rn-max(ck04models(B4I,Teff=16080,metallicity=0.004,logG=2.52) (extinction smcbar=0.080), flux1360 +- 30.0A flux=1.9e-13 Flam)
COS/G160M/c1611 : rn-max(ck04models(B4I,Teff=16080,metallicity=0.004,logG=2.52) (extinction smcbar=0.080), flux1700 +- 5.0A flux=1.4e-13 Flam)
COS/G185M/c1921 : rn-max(ck04models(B4I,Teff=16080,metallicity=0.004,logG=2.52) (extinction smcbar=0.080), flux1700 +- 5.0A flux=1.4e-13 Flam)
COS/G185M/c1953 : rn-max(ck04models(B4I,Teff=16080,metallicity=0.004,logG=2.52) (extinction smcbar=0.080), flux1700 +- 5.0A flux=1.4e-13 Flam)
COS/G185M/c1986 : rn-max(ck04models(B4I,Teff=16080,metallicity=0.004,logG=2.52) (extinction smcbar=0.080), flux2200 +- 5.0A flux=7.9e-14 Flam)
STIS/E140M/c1425 : rn-max(ck04models(B4I,Teff=16080,metallicity=0.004,logG=2.52) (extinction smcbar=0.080), flux1360 +- 30.0A flux=1.9e-13 Flam)
STIS/E230M/c1978 : rn-max(ck04models(B4I,Teff=16080,metallicity=0.004,logG=2.52) (extinction smcbar=0.080), flux2200 +- 5.0A flux=7.9e-14 Flam)
STIS/E230M/c2707 : rn-max(ck04models(B4I,Teff=16080,metallicity=0.004,logG=2.52) (extinction smcbar=0.080), flux2200 +- 5.0A flux=7.9e-14 Flam)
Coordinate pedigree: Gaia
Calculation performed 2020-02-24T17:53:56, v0.4
-------------------------------------------------------------------------------
tstatus; AV324; P/COS Approved for submission; S/STIS ready for internal review; P/CP 21/04/20; S/CP 21/04/20
tcheck; APT/SIMBAD target names: ; Verified
tcheck; Target info verification status?; Good
tcheck; Coordinates & P.M. updated?; Verified
tcheck; Adopted SED compared to Observations?; agreement between any plausible SED, IUE spectra and optical photometry is poor. Will use smaller of model and IUE to estimate exposure time, larger to estimate BOP and buffer timesDACHS-SMC-2-8M2002-SMC-55226J2000SpT=B4Iab; E(B-V)=0.08; U=12.1; B=12.8; V=12.8; F1160=2.18e-13; F1360=1.94e-13; F1700=1.41e-13; F2200=7.93e-14EXT-STARB0-B2 III-INOAV393 : AzV-393, Sk-124, SK 124
Previous name : Sk-124
Input file: SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
SIMBAD link (SK 124): https://simbad.u-strasbg.fr/simbad/sim-id?Ident=SK+124&submit=submit+id
SpT = B2 Ia
COS/G130M/c1096 : rn-max(ck04models(B2I,Teff=21040,metallicity=0.004,logG=3) (extinction smcbar=0.140), flux1160 +- 30.0A flux=6e-13 Flam)
COS/G130M/c1291 : rn-max(ck04models(B2I,Teff=21040,metallicity=0.004,logG=3) (extinction smcbar=0.140), flux1360 +- 30.0A flux=7e-13 Flam)
COS/G160M/c1611 : rn-max(ck04models(B2I,Teff=21040,metallicity=0.004,logG=3) (extinction smcbar=0.140), flux1700 +- 5.0A flux=6e-13 Flam)
COS/G185M/c1921 : rn-max(ck04models(B2I,Teff=21040,metallicity=0.004,logG=3) (extinction smcbar=0.140), flux1700 +- 5.0A flux=6e-13 Flam)
COS/G185M/c1953 : rn-max(ck04models(B2I,Teff=21040,metallicity=0.004,logG=3) (extinction smcbar=0.140), flux1700 +- 5.0A flux=6e-13 Flam)
COS/G185M/c1986 : rn-max(ck04models(B2I,Teff=21040,metallicity=0.004,logG=3) (extinction smcbar=0.140), flux2200 +- 5.0A flux=5e-13 Flam)
STIS/E140M/c1425 : rn-max(ck04models(B2I,Teff=21040,metallicity=0.004,logG=3) (extinction smcbar=0.140), flux1360 +- 30.0A flux=7e-13 Flam)
STIS/E230M/c1978 : rn-max(ck04models(B2I,Teff=21040,metallicity=0.004,logG=3) (extinction smcbar=0.140), flux2200 +- 5.0A flux=5e-13 Flam)
STIS/E230M/c2707 : rn-max(ck04models(B2I,Teff=21040,metallicity=0.004,logG=3) (extinction smcbar=0.140), flux2200 +- 5.0A flux=5e-13 Flam)
Coordinate pedigree: Gaia
Calculation performed 2020-02-24T17:52:42, v0.4
-------------------------------------------------------------------------------
tstatus; AV393; P/COS Approved for submission; S/STIS ready for internal review; P/CP 21/04/25; S/CP 21/04/25
tcheck; APT/SIMBAD target names: ; SK 124 ; LHA 115-S 45
tcheck; Target info verification status?; Good
tcheck; Coordinates & P.M. updated?; OK
tcheck; Adopted SED compared to Observations?; Good enough. IUE flux in short FUV range consistent with FUSE, but ~30% higher than GHRS G140L. None of the models fit very well, so we have adopted a pasted together version of the observed FUSE+IUE spectra for BOP and instrument safety estimates. See AV393_c1291_default_sed.png in proposal directorySK1242MASS-J01055631-7219448J2000SpT=B2 Ia; E(B-V)=0.14; U=10.6; B=11.4; V=11.5; F1160=6.00e-13; F1360=7.00e-13; F1700=6.00e-13; F2200=5.00e-13The scheduling data was generated by CASM 28.0.CASM was run in Phase II mode.vstatus; 1C; AV187; P/COS Approved for submission; P/CP 12/03/20; intrev: complete; P/WF 12/05/20
vcheck; Enter targ name & Inst. & Resp. Sci.; AV 187 ; COS ; Charles Proffitt
vcheck; ETC numbers entered in APT?; Done
vcheck; Any screening violations?; No ...
Adopted E(B-V)=0.06 with normalization in the U band for baseline calculations (see av187_adopted_vs_iue_fuse.png)
Some warning that irregulary variable limit exceeded, but have IUE and FUSE data so flux secure.
Also checked IUE spectrum directly against c1291 observation to verify safety of broad emission line, see COS.sp.1431878
vcheck; S/N ETC calcs done & documented?; Yes
vcheck; Field images checked & saved?; yes av187_gsc2_field_cos.png
vcheck; Selected ACQ strategy?; Dispersed ...
One bright star at edge of field prevents BOA MIRRORA imaging ACQ, so falling back to dispersed light acq
vcheck; Possible ACQ or Sci spoilers?; none
vcheck; Field BOT clear?; yes ...
Only GSC2 BOT violation is for the target, which defaults to an unreddened O star, but our detailed SED and spectral type (B3 I) supercede this
vcheck; Visual BOT check for stars not in catalog?; OK all bright stars in image have GSC2 entries
vcheck; Orbit packing finalized?; Yes ...
c1291 expo time increased by 30% above request, c1611 by 55%
vcheck; Buffer times optimized?; Yes ...
due to relatively high count rates, c1291 buffer time set to about 71% of ETC estimate
vcheck; Verify visit grouping correct; NA
vcheck; Is visit ready for int. review?; Yes
Allocated COS orbits = 1, used=11595418794000280.0545225061686(Tic-Visit
:proposal-id 16102
:visit-id "1C"
:proposal-version -1
:trans-version "20191203"
:date "22-Apr-2020 12:06:22.0"
: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 591472
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16102
:visit-id "1C"
:obset-id "1C"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16102
:visit-id "1C"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2594
: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
)true10Updated SED to better fit the overall shape - updated E(B-V) to 0.06 and normalized to U Band
rn-max(ck04models(B3I,Teff=18560,metallicity=0.004,logG=2.6) (extinction smcbar=0.030), flux1360 +- 30.0A flux=5.3e-13 Flam); cos,fuv,g130m,c1291,psa,mjd#59305; fp-pos=None, segment=None)
From file SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
Spectral type: B3Ia --> B3 I
SED = AV187_COS_G130M_c1291_sed.fits
For exptime=351.9 s, spectral region:
1150.0 Angstroms +/-0.5 Angstroms achieves SNR=30.0/resel
global countrate (brightest segment): 8546.6 cts/s/segment
brightest pixel: 0.153 cts/s/pix at 1275.0 Angstroms
Calculation performed 2020-02-24T17:53:46, v0.4rn-max(ck04models(B3I,Teff=18560,metallicity=0.004,logG=2.6) (extinction smcbar=0.030), flux1360 +- 30.0A flux=5.3e-13 Flam); cos,fuv,g130m,c1291,psa,mjd#59305; fp-pos=None, segment=None)
From file SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
Spectral type: B3Ia --> B3 I
SED = AV187_COS_G130M_c1291_sed.fits
For exptime=351.9 s, spectral region:
1150.0 +/- 0.5 Angstroms achieves SNR=30.0/resel
global countrate (brightest segment): 8546.6 cts/s/segment
brightest pixel: 0.153 cts/s/pix at 1275.0 angstroms
Calculation performed 2020-02-24T17:53:46, v0.4Updated SED to better fit the overall shape - updated E(B-V) to 0.06 and normalized to U Band
rn-max(ck04models(B3I,Teff=18560,metallicity=0.004,logG=2.6) (extinction smcbar=0.030), flux1700 +- 5.0A flux=4.7e-13 Flam); cos,fuv,g160m,c1611,psa,mjd#59305; fp-pos=None, segment=None)
From file SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
Spectral type: B3Ia --> B3 I
SED = AV187_COS_G160M_c1611_sed.fits
For exptime=493.7 s, spectral region:
1590.0 +/- 0.5 Angstroms achieves SNR=30.0/resel
global countrate (brightest segment): 6915.7 cts/s/segment
brightest pixel: 0.110 cts/s/pix at 1442.0 Angstroms
Calculation performed 2020-02-24T17:53:48, v0.4The scheduling data was generated by CASM 28.0.CASM was run in Phase II mode.vstatus; 1S; AV187; S/STIS Approved for submission; P/CP 12/03/20 ; intrev: complete; P/TS 15/05/20
vcheck; Enter targ name & Inst. & Resp. Sci.; AV 187 ; STIS ; Charles Proffitt
vcheck; ETC numbers entered in APT?; Yes
vcheck; Any screening violations?; No
vcheck; S/N ETC calcs done & documented?; Yes
for adopted SED see av187_adopted_vs_iue_fuse.png
vcheck; Field images checked & saved?; Yes av187_gsc2_field_cos.png
vcheck; Selected ACQ strategy?; F28X50LP, S/N=120
vcheck; Possible ACQ or Sci spoilers?; None
vcheck; Field BOT clear?; Yes
vcheck; Visual BOT check for stars not in catalog?; Yes - all stars have GSC2 values, so field BOT clear
vcheck; Orbit packing finalized?; Yes - 1 orbit would give only 68% of requested time; 2 orbits gives 152% so used 2 orbits
vcheck; Buffer times optimized?; Yes
vcheck; Verify visit grouping correct; NA
vcheck; Is visit ready for int. review?; Yes
Allocated STIS orbits = 2, used = 21595257648000278.1741199204673(Tic-Visit
:proposal-id 16102
:visit-id "1S"
:proposal-version -1
:trans-version "20191203"
:date "22-Apr-2020 13:28:46.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 2
:saa-model "24"
:si-bright-earth-limb-angle 20.0
:data-volume 1426864
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16102
:visit-id "1S"
:obset-id "1S"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16102
:visit-id "1S"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2596.0
:al-overhead-at-end 0
:internal-dur-at-end 316.0
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2989
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16102
:visit-id "1S"
:orbit-number 2
:pcs-time 302
:si-vis-utilization 2687
:al-overhead-at-end 0
:internal-dur-at-end 578
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2989
:pcs-gap 0
)true20S/N = 120rn-max(ck04models(B3I,Teff=18560,metallicity=0.004,logG=2.6) (extinction smcbar=0.030), flux1700 +- 5.0A flux=4.7e-13 Flam); stis,nuvmama,e230m,c1978,0.2x0.2,mjd#59305
From file SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
Spectral type: B3Ia --> B3 I
SED = AV187_STIS_E230M_c1978_sed.fits
For exptime=3159.6 s, spectral region:
1800.0+/-0.5 A achieves SNR=20.0/resel
global countrate (brightest segment): 6080.0 cts/s/segment
brightest pixel: 0.120 cts/s/pix at 2267.5 A
Calculation performed 2020-02-24T17:53:55, v0.4rn-max(ck04models(B3I,Teff=18560,metallicity=0.004,logG=2.6) (extinction smcbar=0.030), flux1700 +- 5.0A flux=4.7e-13 Flam); stis,nuvmama,e230m,c1978,0.2x0.2,mjd#59305
From file SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
Spectral type: B3Ia --> B3 I
SED = AV187_STIS_E230M_c1978_sed.fits
For exptime=3159.6 s, spectral region:
1800.0+/-0.5 A achieves SNR=20.0/resel
global countrate (brightest segment): 6080.0 cts/s/segment
brightest pixel: 0.120 cts/s/pix at 2267.5 A
Calculation performed 2020-02-24T17:53:55, v0.4The scheduling data was generated by CASM 28.0.CASM was run in Phase II mode.vstatus; 2C; AV234; P/COS Approved for submission; P/CP 16/04/20; intrev: complete; P/WF 12/05/20
vcheck; Enter targ name & Inst. & Resp. Sci.; AV234 ; COS ; CP
vcheck; ETC numbers entered in APT?; yes ...
adopted default SEDs in av234/seds AV234_COS_G130M_c1291_sed.fits, AV234_COS_G160M_c1611_sed.fits
each is appropriate for its needed wavelength range, even though the fit of any one to the overall SED is mediocre.
vcheck; Any screening violations?; no, all calculations well under BOP limits
vcheck; S/N ETC calcs done & documented?; Yes, default calcs meet specs ...
since UBV mags signficantly brighter that consistent with observed UV spectra, will do extra checks using best overall fit to FUV shape be renormalized to observed V in case its the IUE spectra rather than the SED shape that's funny
c1291 renormalizing default c1611 spectrum to observed Vmag=12.9 reduces buffer time to 2/3*212s, but still safe COS.sp.1438513
c1611 renormalizing default c1611 spectrum to observed Vmag=12.9 reduces buffer time to 2/3*418s, but still safe COS.sp.1438508
vcheck; Field images checked & saved?; yes, see azv234_gsc2.png
vcheck; Selected ACQ strategy?; dispersed
vcheck; Possible ACQ or Sci spoilers?; none
vcheck; Field BOT clear?; Yes, GSC2 BOT only flags the target as unsafe - 26 others safe, no unknowns
vcheck; Visual BOT check for stars not in catalog?; OK, all bright stars have GSC2 entries, but note that GSC2 finds a star ~1.5 mags fainter at about 1" from target, but neither 2MASS nor Gaia include any such star and 2MASS and Gaia agree well on target coordinates
vcheck; Orbit packing finalized?; Yes ...
this one can't quite squeeze into one orbit even at 80%, but fits very easily into 2. Get 235% and 175% of requested c1291/c1611 times
vcheck; Buffer times optimized?; yes, was more conservative than ETC suggests due to higher visual fluxes than consistent with models + UV obs
vcheck; Verify visit grouping correct; N/A
vcheck; Is visit ready for int. review?; Yes
Allocated COS orbits = 21595543698000281.3637415422734(Tic-Visit
:proposal-id 16102
:visit-id "2C"
:proposal-version -1
:trans-version "20191203"
:date "22-Apr-2020 12:12:30.0"
: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 1861296
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16102
:visit-id "2C"
:obset-id "2C"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16102
:visit-id "2C"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2595
: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 16102
:visit-id "2C"
:orbit-number 2
:pcs-time 302
:si-vis-utilization 2687
: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 2989
:pcs-gap 0
)true20rn-max(ck04models(B3I,Teff=18560,metallicity=0.004,logG=2.6) (extinction smcbar=0.030), flux1360 +- 30.0A flux=2.1e-13 Flam); cos,fuv,g130m,c1291,psa,mjd#59305; fp-pos=None, segment=None)
From file SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
Spectral type: B3Iab --> B3 I
SED = AV234_COS_G130M_c1291_sed.fits
For exptime=875.8 s, spectral region:
1150.0+/-0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 3574.1 cts/s/segment
brightest pixel: 0.062 cts/s/pix at 1275.0 A
Calculation performed 2020-02-24T17:53:31, v0.4rn-max(ck04models(B3I,Teff=18560,metallicity=0.004,logG=2.6) (extinction smcbar=0.030), flux1360 +- 30.0A flux=2.1e-13 Flam); cos,fuv,g130m,c1291,psa,mjd#59305; fp-pos=None, segment=None)
From file SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
Spectral type: B3Iab --> B3 I
SED = AV234_COS_G130M_c1291_sed.fits
For exptime=875.8 s, spectral region:
1150.0+/-0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 3574.1 cts/s/segment
brightest pixel: 0.062 cts/s/pix at 1275.0 A
Calculation performed 2020-02-24T17:53:31, v0.4rn-max(ck04models(B3I,Teff=18560,metallicity=0.004,logG=2.6) (extinction smcbar=0.030), flux1700 +- 5.0A flux=1.8e-13 Flam); cos,fuv,g160m,c1611,psa,mjd#59305; fp-pos=None, segment=None)
From file SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
Spectral type: B3Iab --> B3 I
SED = AV234_COS_G160M_c1611_sed.fits
For exptime=1254.8 s, spectral region:
1590.0+/-0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 2741.8 cts/s/segment
brightest pixel: 0.043 cts/s/pix at 1442.0 A
Calculation performed 2020-02-24T17:53:33, v0.4The scheduling data was generated by CASM 28.0.CASM was run in Phase II mode.vstatus; 2S; AV234; S/STIS Approved for submission; P/CP 16/04/20 ; intrev: complete; P/TS 15/05/20
vcheck; Enter targ name & Inst. & Resp. Sci.; AV234 ; STIS ;CP
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: azv234_gsc2_STIS.png
vcheck; Selected ACQ strategy?; OII filter
Something is funny about this star's UV vs visual SED and in case there is a red companion of comparable brightness we'll do the acq with the OII filter even though it takes a little more time
vcheck; Possible ACQ or Sci spoilers?; Stellar iamge looks a bit extended, but nothing of comparable brightness close enough to affect the ACQ - but will use OII UV acq to avoid confusion if cool companion exists
vcheck; Field BOT clear?; Yes
vcheck; Visual BOT check for stars not in catalog?; GSC2 finds a star ~1.5 mags fainter at about 1" from target, but neither 2MASS nor Gaia include any such star and 2MASS and Gaia agree well on target coordinates
vcheck; Orbit packing finalized?; Yes two 2-orbit visits give 85% of reqeusted time
vcheck; Buffer times optimized?; Yes, but for buffer times normalized to V band instead of observed UV flux to allow for possible mis-centering of IUE spectra
vcheck; Verify visit grouping correct; yes
vcheck; Is visit ready for int. review?; yes
Allocated STIS orbits = 5 ; 2+2 will get 84.5% of requested exposure time; 2+3 would get 108% of requested time. Will go with 2+21598136000000313.0730883082507(Tic-Visit
:proposal-id 16102
:visit-id "2S"
:proposal-version -1
:trans-version "20191203"
:date "22-Apr-2020 12:06:49.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 2
:saa-model "24"
:si-bright-earth-limb-angle 20.0
:data-volume 1009360
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16102
:visit-id "2S"
:obset-id "2S"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16102
:visit-id "2S"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2596
:al-overhead-at-end 0
:internal-dur-at-end 316
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2989
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16102
:visit-id "2S"
:orbit-number 2
:pcs-time 302
:si-vis-utilization 2687
:al-overhead-at-end 0
:internal-dur-at-end 578
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2989
:pcs-gap 0
)true20Something is funny about this star's UV vs visual SED and in case there is a red companion of comparable brightness we'll do the acq with the OII filter even though it takes a little more timern-max(ck04models(B3I,Teff=18560,metallicity=0.004,logG=2.6) (extinction smcbar=0.030), flux2200 +- 5.0A flux=1.2e-13 Flam); stis,nuvmama,e230m,c1978,0.2x0.2,mjd#59305
Desire total of 11271.3 s
From file SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
Spectral type: B3Iab --> B3 I
SED = AV234_STIS_E230M_c1978_sed.fits
For exptime=11271.3 s, spectral region:
1800.0 0.5achieves SNR=20.0/resel
global countrate (brightest segment): 3676.8 cts/s/segment
brightest pixel: 0.045 cts/s/pix at 2267.5
Calculation performed 2020-02-24T17:53:41, v0.4rn-max(ck04models(B3I,Teff=18560,metallicity=0.004,logG=2.6) (extinction smcbar=0.030), flux2200 +- 5.0A flux=1.2e-13 Flam); stis,nuvmama,e230m,c1978,0.2x0.2,mjd#59305
From file SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
Spectral type: B3Iab --> B3 I
SED = AV234_STIS_E230M_c1978_sed.fits
For exptime=11271.3 s, spectral region:
1800.0+/-0.5 A achieves SNR=20.0/resel
global countrate (brightest segment): 3676.8 cts/s/segment
brightest pixel: 0.045 cts/s/pix at 2267.5 A
Calculation performed 2020-02-24T17:53:41, v0.4The scheduling data was generated by CASM 28.0.CASM was run in Phase II mode.vstatus; 2S; AV234; S/STIS Approved for submission; P/CP 16/04/20 ; intrev: complete; P/TS 15/05/20
vcheck; Enter targ name & Inst. & Resp. Sci.; AV234 ; STIS ;CP
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?; ------
vcheck; Selected ACQ strategy?; OII filter
Something is funny about this star's UV vs visual SED and in case there is a red companion of comparable brightness we'll do the acq with the OII filter even though it takes a little more time
vcheck; Possible ACQ or Sci spoilers?; Stellar iamge looks a bit extended, but nothing of comparable brightness close enough to affect the ACQ - but will use OII UV acq to avoid confusion if cool companion exists
vcheck; Field BOT clear?; Yes
vcheck; Visual BOT check for stars not in catalog?; GSC2 finds a star ~1.5 mags fainter at about 1" from target, but neither 2MASS nor Gaia include any such star and 2MASS and Gaia agree well on target coordinates
vcheck; Orbit packing finalized?; Yes
vcheck; Buffer times optimized?; Yes, but for buffer times normalized to V band instead of observed UV flux to allow for possible mis-centering of IUE spectra
vcheck; Verify visit grouping correct; N/A
vcheck; Is visit ready for int. review?; ------
Allocated STIS orbits = 5 ; 2+2 will get 84.5% of requested exposure time calculated normalizing to IUE spectra, while 2+3 would get 108% of requested time. Will go for 2+2 and save the orbit1597814473000315.0(Tic-Visit
:proposal-id 16102
:visit-id "2T"
:proposal-version -1
:trans-version "20191203"
:date "07-May-2020 10:59:05.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 2
:saa-model "24"
:si-bright-earth-limb-angle 20.0
:data-volume 1009360
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16102
:visit-id "2T"
:obset-id "2T"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16102
:visit-id "2T"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2596
:al-overhead-at-end 0
:internal-dur-at-end 316
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2989
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16102
:visit-id "2T"
:orbit-number 2
:pcs-time 302
:si-vis-utilization 2687
:al-overhead-at-end 0
:internal-dur-at-end 578
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2989
:pcs-gap 0
)true20Something is funny about this star's UV vs visual SED and in case there is a red companion of comparable brightness we'll do the acq with the OII filter even though it takes a little more timern-max(ck04models(B3I,Teff=18560,metallicity=0.004,logG=2.6) (extinction smcbar=0.030), flux2200 +- 5.0A flux=1.2e-13 Flam); stis,nuvmama,e230m,c1978,0.2x0.2,mjd#59305
Desire total of 11271.3 s
From file SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
Spectral type: B3Iab --> B3 I
SED = AV234_STIS_E230M_c1978_sed.fits
For exptime=11271.3 s, spectral region:
1800.0 0.5achieves SNR=20.0/resel
global countrate (brightest segment): 3676.8 cts/s/segment
brightest pixel: 0.045 cts/s/pix at 2267.5
Calculation performed 2020-02-24T17:53:41, v0.4rn-max(ck04models(B3I,Teff=18560,metallicity=0.004,logG=2.6) (extinction smcbar=0.030), flux2200 +- 5.0A flux=1.2e-13 Flam); stis,nuvmama,e230m,c1978,0.2x0.2,mjd#59305
From file SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
Spectral type: B3Iab --> B3 I
SED = AV234_STIS_E230M_c1978_sed.fits
For exptime=11271.3 s, spectral region:
1800.0+/-0.5 A achieves SNR=20.0/resel
global countrate (brightest segment): 3676.8 cts/s/segment
brightest pixel: 0.045 cts/s/pix at 2267.5 A
Calculation performed 2020-02-24T17:53:41, v0.4The scheduling data was generated by CASM 28.0.CASM was run in Phase II mode.vstatus; 3C; AV324; P/COS Approved for submission; P/CP 22/04/20; intrev: complete; P/WF 12/05/20
vcheck; Enter targ name & Inst. & Resp. Sci.; AzV324 ; COS ; CP
vcheck; ETC numbers entered in APT?; Yes
vcheck; Any screening violations?; NO
vcheck; S/N ETC calcs done & documented?; yes ...
used default SEDs for S/N and expo time, but conservative upper limit for BOP and buffer times that matchs FUV+optical
see file av324-bop-conservative-sed.png
vcheck; Field images checked & saved?; Yes av324_gsc2.png
vcheck; Selected ACQ strategy?; Dispersed G130M/1291. Up ACQ time from 0.37s to 1.0s to allow for any SED uncertainty
vcheck; Possible ACQ or Sci spoilers?; none
vcheck; Field BOT clear?; yes ...
Yes, GSC2 has adequate coverage for selected modes.
vcheck; Visual BOT check for stars not in catalog?; OK ...
Blue star 2.2 mags fainter and 4" W of target not in GSC2 is cleared by IUE spectrum as that will include both components
vcheck; Orbit packing finalized?; Yes get 145% of requestd c1291 time and 141% of requested c1611.
vcheck; Buffer times optimized?; Yes
vcheck; Verify visit grouping correct; N/A
vcheck; Is visit ready for int. review?; yes
Allocated COS orbits = 4 ; implement as 2+2 (FUV and NUV visits)1595362318000278.4142570793797(Tic-Visit
:proposal-id 16102
:visit-id "3C"
:proposal-version -1
:trans-version "20191203"
:date "22-Apr-2020 12:07:00.0"
: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 1130768
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16102
:visit-id "3C"
:obset-id "3C"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16102
:visit-id "3C"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2595
: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 16102
:visit-id "3C"
:orbit-number 2
:pcs-time 302
:si-vis-utilization 2686
:al-overhead-at-end 0
:internal-dur-at-end 350
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2989
:pcs-gap 0
)true20rn-max(ck04models(B4I,Teff=16080,metallicity=0.004,logG=2.52) (extinction smcbar=0.080), flux1360 +- 30.0A flux=1.9e-13 Flam); cos,fuv,g130m,c1291,psa,mjd#59305; fp-pos=None, segment=None)
From file SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
Spectral type: B4Iab --> B4 I
SED = AV324_COS_G130M_c1291_sed.fits
For exptime=1420.6 s, spectral region:
1150.0+/-0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 2700.1 cts/s/segment
brightest pixel: 0.050 cts/s/pix at 1277.0 A
Calculation performed 2020-02-24T17:54:00, v0.4rn-max(ck04models(B4I,Teff=16080,metallicity=0.004,logG=2.52) (extinction smcbar=0.080), flux1360 +- 30.0A flux=1.9e-13 Flam); cos,fuv,g130m,c1291,psa,mjd#59305; fp-pos=None, segment=None)
From file SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
Spectral type: B4Iab --> B4 I
SED = AV324_COS_G130M_c1291_sed.fits
For exptime=1420.6 s, spectral region:
1150.0+/-0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 2700.1 cts/s/segment
brightest pixel: 0.050 cts/s/pix at 1277.0 A
Calculation performed 2020-02-24T17:54:00, v0.4rn-max(ck04models(B4I,Teff=16080,metallicity=0.004,logG=2.52) (extinction smcbar=0.080), flux1700 +- 5.0A flux=1.4e-13 Flam); cos,fuv,g160m,c1611,psa,mjd#59305; fp-pos=None, segment=None)
From file SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
Spectral type: B4Iab --> B4 I
SED = AV324_COS_G160M_c1611_sed.fits
For exptime=1661.5 s, spectral region:
1590.0+/-0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 1914.1 cts/s/segment
brightest pixel: 0.028 cts/s/pix at 1442.0 A
Calculation performed 2020-02-24T17:54:03, v0.4The scheduling data was generated by CASM 28.0.CASM was run in Phase II mode.vstatus; 3D; AV324; P/COS Approved for submission; P/CP 22/04/20; intrev: complete; P/WF 12/05/20
vcheck; Enter targ name & Inst. & Resp. Sci.; AzV 324 ; COS ; CP
vcheck; ETC numbers entered in APT?; Yes
vcheck; Any screening violations?; No
vcheck; S/N ETC calcs done & documented?; Yes, used default SEDS for S/N
vcheck; Field images checked & saved?; Yes
vcheck; Selected ACQ strategy?; Dispersed G230L 2950
vcheck; Possible ACQ or Sci spoilers?; none
vcheck; Field BOT clear?; yes ...
Yes, GSC2 has adequate coverage for selected modes.
vcheck; Visual BOT check for stars not in catalog?; OK ...
Blue star 2.2 mags fainter and 4" W of target not in GSC2 is cleared by IUE spectrum
vcheck; Orbit packing finalized?; Yes get 136% of G185M and 127% of G185M goals
vcheck; Buffer times optimized?; YES
vcheck; Verify visit grouping correct; N/A
vcheck; Is visit ready for int. review?; Yes
Allocated COS orbits = 41595206211000276.5417718549524(Tic-Visit
:proposal-id 16102
:visit-id "3D"
:proposal-version -1
:trans-version "20191203"
:date "22-Apr-2020 12:07:05.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 2
:saa-model "32"
:si-bright-earth-limb-angle 20.0
:data-volume 835136
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16102
:visit-id "3D"
:obset-id "3D"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16102
:visit-id "3D"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2595
: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 2989
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16102
:visit-id "3D"
:orbit-number 2
:pcs-time 302
:si-vis-utilization 2684
:al-overhead-at-end 0
:internal-dur-at-end 350
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2989
:pcs-gap 0
)true20rn-max(ck04models(B4I,Teff=16080,metallicity=0.004,logG=2.52) (extinction smcbar=0.080), flux1700 +- 5.0A flux=1.4e-13 Flam); cos,nuv,g185m,c1953,psa,mjd#59305
From file SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
Spectral type: B4Iab --> B4 I
SED = AV324_COS_G185M_c1953_sed.fits
For exptime=1359.2 s, spectral region:
1860.0 +/- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 1650.4 cts/s/segment
brightest pixel: 0.127 cts/s/pix at 1872.0 A
Calculation performed 2020-02-24T17:54:03, v0.4rn-max(ck04models(B4I,Teff=16080,metallicity=0.004,logG=2.52) (extinction smcbar=0.080), flux2200 +- 5.0A flux=7.9e-14 Flam); cos,nuv,g185m,c1986,psa,mjd#59305
From file SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
Spectral type: B4Iab --> B4 I
SED = AV324_COS_G185M_c1986_sed.fits
For exptime=1886.2 s, spectral region:
1980.0+/-0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 1409.7 cts/s/segment
brightest pixel: 0.088 cts/s/pix at 1875.0 A
Calculation performed 2020-02-24T17:54:04, v0.4The scheduling data was generated by CASM 28.0.CASM was run in Phase II mode.vstatus; 3S; AV324; S/STIS Approved for submission; P/CP 21/04/20 ; intrev: complete; P/TS 15/05/20
vcheck; Enter targ name & Inst. & Resp. Sci.; AzV324 ; STIS ; CP
vcheck; ETC numbers entered in APT?; Yes
vcheck; Any screening violations?; No
vcheck; S/N ETC calcs done & documented?; Yes, used original calcs for S/N, conservative upper limit for BOP
vcheck; Field images checked & saved?; ------
vcheck; Selected ACQ strategy?; OII filter
vcheck; Possible ACQ or Sci spoilers?; No
vcheck; Field BOT clear?; Yes, default GSC2 BOT covers necessary stars
vcheck; Visual BOT check for stars not in catalog?; OK,
vcheck; Orbit packing finalized?; Yes got 80% of optimal exposure time in one orbit
vcheck; Buffer times optimized?; yes
vcheck; Verify visit grouping correct; N/A
vcheck; Is visit ready for int. review?; yes
Allocated STIS orbits = 11595966664000285.7755938994066(Tic-Visit
:proposal-id 16102
:visit-id "3S"
:proposal-version -1
:trans-version "20191203"
:date "22-Apr-2020 12:07:09.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 1
:saa-model "24"
:si-bright-earth-limb-angle 20.0
:data-volume 504896
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16102
:visit-id "3S"
:obset-id "3S"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16102
:visit-id "3S"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2596
:al-overhead-at-end 0
:internal-dur-at-end 578
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2989
:pcs-gap 0
)true10rn-max(ck04models(B4I,Teff=16080,metallicity=0.004,logG=2.52) (extinction smcbar=0.080), flux2200 +- 5.0A flux=7.9e-14 Flam); stis,nuvmama,e230m,c2707,0.2x0.2,mjd#59305
From file SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
Spectral type: B4Iab --> B4 I
SED = AV324_STIS_E230M_c2707_sed.fits
For exptime=2648.0 s, spectral region:
2800.0+/-0.5 A achieves SNR=20.0/resel
global countrate (brightest segment): 3921.4 cts/s/segment
brightest pixel: 0.041 cts/s/pix at 2648.5 A
Calculation performed 2020-02-24T17:54:08, v0.4The scheduling data was generated by CASM 28.0.CASM was run in Phase II mode.vstatus; 4C; AV393; P/COS Approved for submission; P/CP 07/05M/20; intrev: complete; P/WF 12/05/20
vcheck; Enter targ name & Inst. & Resp. Sci.; AV393 ; AzV 393 ; CP
vcheck; ETC numbers entered in APT?; Yes, used pasted together FUSE+IUE spectra in file av393_fue_iue_paste.dat
vcheck; Any screening violations?; no
vcheck; S/N ETC calcs done & documented?; yes OK to use defaults for S/N despite poor overall fit
IUE flux in short FUV range consistent with FUSE, but ~30% higher than GHRS G140L. None of the models fit very well, so we have adopted a pasted together version of the observed FUSE+IUE spectra for BOP and instrument safety estimates. See file av393_fue_iue_paste.dat
vcheck; Field images checked & saved?; Yes AV393-gsc2-COS-image.png
vcheck; Selected ACQ strategy?; dispersed 1291
vcheck; Possible ACQ or Sci spoilers?; None
vcheck; Field BOT clear?; yes ...
BOT only flags the target itself as unsafe, but also has 2 unknowns. One, a supposed star of mag=8 in the J plate at about 20" distance and a PA of 120 degrees is clearly spurious as there is clearly no such bright star in the GSC2 image and the only stars visible in the image near that location have mag ~ 19. The other has an F plate mag of 14 at ~ 1.2" and a PA near 135. There is no evidence for such a star in the Gaia DR2 catalog which has a nominal resolution of 0.4" and it is difficult to see how the GSC2 could have resolved it from the main source. Perhaps this is an artifact from the bright central source? Note that the relatively bright star in the upper right (R ~ 18", PA~ 220) is about mag 15 and is easily safe in the BOA for all optical elements.
vcheck; Visual BOT check for stars not in catalog?; None, but as noted above, the BOT finds apparently spurious stars that aren't visible in the image.
vcheck; Orbit packing finalized?; Yes got 125% of c1291 and 143% of 1611 request - this should compensate for S/N even if lower GHRS fluxes are correct
vcheck; Buffer times optimized?; Yes
vcheck; Verify visit grouping correct; N/A
vcheck; Is visit ready for int. review?; Yes
Allocated COS orbits = 11597831637000313.59756645043217(Tic-Visit
:proposal-id 16102
:visit-id "4C"
:proposal-version -1
:trans-version "20191203"
:date "22-Apr-2020 12:07:14.0"
: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 730576
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16102
:visit-id "4C"
:obset-id "4C"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16102
:visit-id "4C"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2592
:al-overhead-at-end 0
:internal-dur-at-end 426
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2989
:pcs-gap 0
)true10rn-max(ck04models(B2I,Teff=21040,metallicity=0.004,logG=3) (extinction smcbar=0.140), flux1360 +- 30.0A flux=7e-13 Flam); cos,fuv,g130m,c1291,psa,mjd#59305; fp-pos=None, segment=None)
From file SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
Spectral type: B2 Ia --> B2 I
SED = AV393_COS_G130M_c1291_sed.fits
For exptime=395.0 s, spectral region:
1150.0+/-0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 9490.3 cts/s/segment
brightest pixel: 0.175 cts/s/pix at 1277.0 A
Calculation performed 2020-02-24T17:52:46, v0.4rn-max(ck04models(B2I,Teff=21040,metallicity=0.004,logG=3) (extinction smcbar=0.140), flux1360 +- 30.0A flux=7e-13 Flam); cos,fuv,g130m,c1291,psa,mjd#59305; fp-pos=None, segment=None)
From file SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
Spectral type: B2 Ia --> B2 I
SED = AV393_COS_G130M_c1291_sed.fits
For exptime=395.0 s, spectral region:
1150.0+/-0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 9490.3 cts/s/segment
brightest pixel: 0.175 cts/s/pix at 1277.0 A
Calculation performed 2020-02-24T17:52:46, v0.4rn-max(ck04models(B2I,Teff=21040,metallicity=0.004,logG=3) (extinction smcbar=0.140), flux1700 +- 5.0A flux=6e-13 Flam); cos,fuv,g160m,c1611,psa,mjd#59305; fp-pos=None, segment=None)
From file SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
Spectral type: B2 Ia --> B2 I
SED = AV393_COS_G160M_c1611_sed.fits
For exptime=424.5 s, spectral region:
1590.0+/-0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 7444.5 cts/s/segment
brightest pixel: 0.113 cts/s/pix at 1442.0 A
Calculation performed 2020-02-24T17:52:49, v0.4The scheduling data was generated by CASM 28.0.CASM was run in Phase II mode.vstatus; 4S; AV393; S/STIS Approved for submission; S/CP 07/05/20 ; intrev: complete; P/TS 15/05/20
vcheck; Enter targ name & Inst. & Resp. Sci.; AzV 393; STIS ; CP
vcheck; ETC numbers entered in APT?; Yes
vcheck; Any screening violations?; no
vcheck; S/N ETC calcs done & documented?; Yes
Reduced from initial 2436.8 to 2146s to fit into 1 orbit, but IUE flux slightly higher than planning model.
see STIS.sp.1439510 for calc using observed IUE spectrum
vcheck; Field images checked & saved?; Yes AV393-gsc2-COS-image.png
vcheck; Selected ACQ strategy?; OII filter ACQ
vcheck; Possible ACQ or Sci spoilers?; None
vcheck; Field BOT clear?; Yes, 2 safe stars only found
vcheck; Visual BOT check for stars not in catalog?; OK, no stars not included in GSC2 nearby
vcheck; Orbit packing finalized?; Yes, get 88% of requested time in 1 orbit
vcheck; Buffer times optimized?; yes
vcheck; Verify visit grouping correct; N/A
vcheck; Is visit ready for int. review?; Yes
Allocated STIS orbits = 11597877768000300.0(Tic-Visit
:proposal-id 16102
:visit-id "4S"
:proposal-version -1
:trans-version "20191203"
:date "22-Apr-2020 12:07:23.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 1
:saa-model "24"
:si-bright-earth-limb-angle 20.0
:data-volume 783232
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16102
:visit-id "4S"
:obset-id "4S"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16102
:visit-id "4S"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2596.0
:al-overhead-at-end 0
:internal-dur-at-end 578.0
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2989
:pcs-gap 0
)true10Reduced from initial 2436.8 to 2146s to fit into 1 orbit, but IUE flux slightly higher than planning model.
rn-max(ck04models(B2I,Teff=21040,metallicity=0.004,logG=3) (extinction smcbar=0.140), flux2200 +- 5.0A flux=5e-13 Flam); stis,nuvmama,e230m,c1978,0.2x0.2,mjd#59305
From file SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
Spectral type: B2 Ia --> B2 I
SED = AV393_STIS_E230M_c1978_sed.fits
For exptime=2436.8 s, spectral region:
1800.0 A 0.5 A achieves SNR=20.0/resel
global countrate (brightest segment): 7672.5 cts/s/segment
brightest pixel: 0.178 cts/s/pix at 2267.5 A
Calculation performed 2020-02-24T17:52:56, v0.4