For the best data quality, it is strongly recommended that all four FP-POS positions be used when observing at a given COS CENWAVE setting.Visit BC has been added as a repeat of partially failed visit 2C, to obtain the NUV exposures using G185M/1953 and 1986.
Visits BS and CS have been added to replace the failed visits 2S and 3S -- NUV-MAMA/G230M/2707 spectra for AV314 and AV343-1225384840----- Attempting Submission 1 (Sun Jul 18 19:41:48 GMT 2021) -----
----- Attempting Submission 2 (Tue Nov 02 15:53:26 GMT 2021) -----
----- Attempting Submission 3 (Thu Dec 23 21:52:41 GMT 2021) -----The Warning concerning the list of investigators is benign and can be fixed by the PI if desires.
The Warning concerning the use of only 2 FP-POS for the G185M/1953 and G185M/1986 configurations of visit 3C has been discussed internally.
For the modest exposure times, the overheads required to implement 4 FP-POS are considered to be too costly, particularly considering that
pixel-to-pixel flat-field errors are not as significant for NUV configurations of COS as for FUV configurations. Dividing the available time into
exposures at 2 FP-POS of longer duration is expected to provide higher quality data than exposures of shorter duration at 4 FP-POS.
The visit and orbit planners have been run for the new/replacement visits BS and CS.ULLYSES SMC Late B Stars COS and 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-STARB6-B9.5 III-INOAV200 : AV_200, AzV200, AzV 200
Previous name : AzV200
Input file: SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
SIMBAD link (AzV 200): https://simbad.u-strasbg.fr/simbad/sim-id?Ident=AzV+200&submit=submit+id
SpT = B8Ia
COS/G130M/c1291 : rn-max(ck04models(B8I,Teff=11278,metallicity=0.004,logG=2.26) (extinction smcbar=0.080), flux1360 +- 30.0A flux=8.1e-14 Flam)
COS/G160M/c1611 : rn-max(ck04models(B8I,Teff=11278,metallicity=0.004,logG=2.26) (extinction smcbar=0.080), flux1700 +- 5.0A flux=1e-13 Flam)
COS/G185M/c1921 : rn-max(ck04models(B8I,Teff=11278,metallicity=0.004,logG=2.26) (extinction smcbar=0.080), flux1700 +- 5.0A flux=1e-13 Flam)
COS/G185M/c1953 : rn-max(ck04models(B8I,Teff=11278,metallicity=0.004,logG=2.26) (extinction smcbar=0.080), flux1700 +- 5.0A flux=1e-13 Flam)
COS/G185M/c1986 : rn-max(ck04models(B8I,Teff=11278,metallicity=0.004,logG=2.26) (extinction smcbar=0.080), flux2200 +- 5.0A flux=9.2e-14 Flam)
STIS/E140M/c1425 : rn-max(ck04models(B8I,Teff=11278,metallicity=0.004,logG=2.26) (extinction smcbar=0.080), flux1360 +- 30.0A flux=8.1e-14 Flam)
STIS/E230M/c1978 : rn-max(ck04models(B8I,Teff=11278,metallicity=0.004,logG=2.26) (extinction smcbar=0.080), flux2200 +- 5.0A flux=9.2e-14 Flam)
STIS/E230M/c2707 : rn-max(ck04models(B8I,Teff=11278,metallicity=0.004,logG=2.26) (extinction smcbar=0.080), flux2200 +- 5.0A flux=9.2e-14 Flam)
Coordinate pedigree: Gaia
Calculation performed 2020-02-24T17:54:58, v0.4
-------------------------------------------------------------------------------
tstatus; AV200; P/COS approved for submission; S/STIS approved for submission; P/CP 02/11/20; S/CP 02/11/20
tcheck; APT/SIMBAD target names: ; AV200 'AV 200' ...
aka Sk 69
tcheck; Target info verification status?; Done
tcheck; Coordinates & P.M. updated?; Verified as good enough (not bothering with proper motions)
tcheck; Adopted SED compared to Observations?; OK, ...
New STIS G430L spectrum from Massa taken in October 2020 shows a significantly smaller Balmer jump than our adopted model, but original model mostly good enough fit to IUE if locally normalized in wavelength, but E230M c2707 needs to be normalized at a longer wavelength than 2200.. No easy way to manipulate SED to get great overall fit, although a somewhat warmer Teff with a high E(B-V) helps. But if we trust IUE, not really a problem. Note that STIS TA image shows only 1 obvious star in FOVAZV-200SK-69J2000SpT=B8Ia; E(B-V)=0.08; U=11.7; B=12.2; V=12.2; F1160=1.34e-13; F1360=8.09e-14; F1700=1.02e-13; F2200=9.20e-14EXT-STARB3-B5 III-INOAV314 : AV_314, AzV314, AzV 314
Previous name : AzV314
Input file: SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
SIMBAD link (AzV 314): https://simbad.u-strasbg.fr/simbad/sim-id?Ident=AzV+314&submit=submit+id
SpT = B5Iab
COS/G130M/c1291 : rn-max(ck04models(B5I,Teff=13600,metallicity=0.004,logG=2.5), flux1360 +- 30.0A flux=1.8e-13 Flam)
COS/G160M/c1611 : rn-max(ck04models(B5I,Teff=13600,metallicity=0.004,logG=2.5), flux1700 +- 5.0A flux=1.5e-13 Flam)
COS/G185M/c1921 : rn-max(ck04models(B5I,Teff=13600,metallicity=0.004,logG=2.5), flux1700 +- 5.0A flux=1.5e-13 Flam)
COS/G185M/c1953 : rn-max(ck04models(B5I,Teff=13600,metallicity=0.004,logG=2.5), flux1700 +- 5.0A flux=1.5e-13 Flam)
COS/G185M/c1986 : rn-max(ck04models(B5I,Teff=13600,metallicity=0.004,logG=2.5), flux2200 +- 5.0A flux=1e-13 Flam)
STIS/E140M/c1425 : rn-max(ck04models(B5I,Teff=13600,metallicity=0.004,logG=2.5), flux1360 +- 30.0A flux=1.8e-13 Flam)
STIS/E230M/c1978 : rn-max(ck04models(B5I,Teff=13600,metallicity=0.004,logG=2.5), flux2200 +- 5.0A flux=1e-13 Flam)
STIS/E230M/c2707 : rn-max(ck04models(B5I,Teff=13600,metallicity=0.004,logG=2.5), flux2200 +- 5.0A flux=1e-13 Flam)
Coordinate pedigree: Gaia
Calculation performed 2020-02-24T17:54:08, v0.4
-------------------------------------------------------------------------------
tstatus; AV314; P/COS approved for submission; S/STIS approved for submission; P/CP 02/11/20; S/DW 22/05/21
tcheck; APT/SIMBAD target names: ; AV314 'AV 314'
tcheck; Target info verification status?; good
tcheck; Coordinates & P.M. updated?; Verified (not including proper motions)
tcheck; Adopted SED compared to Observations?; yes ...
For STIS/E230M, new G430L spectrum agrees well with IUE, B, V (but U seems too bright) -- model slightly overestimates Balmer jump -- SED2707 agrees reasonably well with IUE over most of E230H/2707 range -- G430L acq has only target in acq boxAZV314M2002-SMC-54568J2000SpT=B5Iab; E(B-V)=0.00; U=11.98 B=12.82; V=12.93; I=13.05; F1160=1.85e-13; F1360=1.78e-13; F1700=1.48e-13; F2200=1.03e-13EXT-STARB6-B9.5 III-INOAV343 : AV_343, AzV343, AzV 343
Previous name : AzV343
Input file: SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
SIMBAD link (AzV 343): https://simbad.u-strasbg.fr/simbad/sim-id?Ident=AzV+343&submit=submit+id
SpT = B6Iab
COS/G130M/c1291 : rn(ck04models(B6I,Teff=12826,metallicity=0.004,logG=2.5) (extinction smcbar=0.020), johnson U mag=12.320 vegamag)
COS/G160M/c1611 : rn(ck04models(B6I,Teff=12826,metallicity=0.004,logG=2.5) (extinction smcbar=0.020), johnson U mag=12.320 vegamag)
COS/G185M/c1921 : rn(ck04models(B6I,Teff=12826,metallicity=0.004,logG=2.5) (extinction smcbar=0.020), johnson U mag=12.320 vegamag)
COS/G185M/c1953 : rn(ck04models(B6I,Teff=12826,metallicity=0.004,logG=2.5) (extinction smcbar=0.020), johnson U mag=12.320 vegamag)
COS/G185M/c1986 : rn(ck04models(B6I,Teff=12826,metallicity=0.004,logG=2.5) (extinction smcbar=0.020), johnson U mag=12.320 vegamag)
STIS/E140M/c1425 : rn(ck04models(B6I,Teff=12826,metallicity=0.004,logG=2.5) (extinction smcbar=0.020), johnson U mag=12.320 vegamag)
STIS/E230M/c1978 : rn(ck04models(B6I,Teff=12826,metallicity=0.004,logG=2.5) (extinction smcbar=0.020), johnson U mag=12.320 vegamag)
STIS/E230M/c2707 : rn(ck04models(B6I,Teff=12826,metallicity=0.004,logG=2.5) (extinction smcbar=0.020), johnson U mag=12.320 vegamag)
Coordinate pedigree: Gaia
Calculation performed 2020-02-24T17:54:33, v0.4
-------------------------------------------------------------------------------
tstatus; AV343; P/COS approved for submission ; S/STIS approved for submission; P/RS 24/06/21; S/DW 22/05/21
tcheck; APT/SIMBAD target names: ; AV343 'AzV 343' ...
aka Sk 111
tcheck; Target info verification status?; Good
tcheck; Coordinates & P.M. updated?; Good
tcheck; Adopted SED compared to Observations?; yes ...
Shape of adopted spectrum matches IUE obs, but observed IUE fluxes only ~ 80% of that found from default model U band normalization. Instead normalize to F1360=8.3e-14 with E(B-V)=0.029 smcbar to optimize fit over UV range. In box folder this is in the file AV343_revised_sed.fits which should be used for all FUV ETC calculations. Note that two sets of IUE spectra were taken a number of years apart (swp09317 & lwp02614 vs swp22006 & lwr08078) and show excellent agreement so unlikely that target was just poorly centered.
For STIS/E230M, new G430L spectrum agrees well with IUE, B, V (but U seems too bright) -- model ok at Balmer jump -- SED2707 agrees reasonably well with IUE over most of E230H/2707 range -- mwavg extinction used (MW foreground should dominate, for this low E(B-V)) -- G430L acq has only target in acq boxAZV-343SK-111J2000SpT=B6Iab; E(B-V)=0.02; U=12.3; B=13.0; V=13.1; R=12.99; G=13.06; F1360=8.3e-14EXT-STARB3-B5 III-INOAV445 : [2dFS]_2538, AV 445, AzV 445
Previous name : AV 445
Input file: SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
SIMBAD link (AzV 445): https://simbad.u-strasbg.fr/simbad/sim-id?Ident=AzV+445&submit=submit+id
SpT = B5 (Iab)
COS/G130M/c1291 : rn-max(ck04models(B5I,Teff=13600,metallicity=0.004,logG=2.5) (extinction smcbar=0.030), flux1360 +- 30.0A flux=1.9e-13 Flam)
COS/G160M/c1611 : rn-max(ck04models(B5I,Teff=13600,metallicity=0.004,logG=2.5) (extinction smcbar=0.030), flux1700 +- 5.0A flux=1.8e-13 Flam)
COS/G185M/c1921 : rn-max(ck04models(B5I,Teff=13600,metallicity=0.004,logG=2.5) (extinction smcbar=0.030), flux1700 +- 5.0A flux=1.8e-13 Flam)
COS/G185M/c1953 : rn-max(ck04models(B5I,Teff=13600,metallicity=0.004,logG=2.5) (extinction smcbar=0.030), flux1700 +- 5.0A flux=1.8e-13 Flam)
COS/G185M/c1986 : rn-max(ck04models(B5I,Teff=13600,metallicity=0.004,logG=2.5) (extinction smcbar=0.030), flux2200 +- 5.0A flux=1.3e-13 Flam)
STIS/E140M/c1425 : rn-max(ck04models(B5I,Teff=13600,metallicity=0.004,logG=2.5) (extinction smcbar=0.030), flux1360 +- 30.0A flux=1.9e-13 Flam)
STIS/E230M/c1978 : rn-max(ck04models(B5I,Teff=13600,metallicity=0.004,logG=2.5) (extinction smcbar=0.030), flux2200 +- 5.0A flux=1.3e-13 Flam)
STIS/E230M/c2707 : rn-max(ck04models(B5I,Teff=13600,metallicity=0.004,logG=2.5) (extinction smcbar=0.030), flux2200 +- 5.0A flux=1.3e-13 Flam)
Coordinate pedigree: Gaia
Calculation performed 2020-02-24T17:54:20, v0.4
-------------------------------------------------------------------------------
tstatus; AV445; P/COS approved for submission; S/STIS approved for submission; P/CP 03/06/21; S/DW 22/05/21
tcheck; APT/SIMBAD target names: ; AV445 'AV 445' ...
aka Sk 138
tcheck; Target info verification status?; Good. SIMBAD gives B5 Iab
tcheck; Coordinates & P.M. updated?; confirmed
tcheck; Adopted SED compared to Observations?; yes ...
Default model underestimates mid and NUV fluxes by ~ 10%. Model AV445_revised_sed.fits F1700=1.7e-13, E(B-V)=0.02 does a better overall job of fitting the data, although this might slighly overestimate flux at 1150, so use original model for c1291. sed comparisons in AV445_c1291_sed.png and AV445_revised_sed.png
for STIS/E230M, SED2707 agrees reasonably well with IUE over most of E230H/2707 range, also UBV -- mwavg extinction used (MW foreground should dominate, for this small E(B-V))AZV-445SK-138J2000SpT=B5 (Iab); E(B-V)=0.03; U=11.90; B=12.68; V=12.78; F1160=1.48e-13; I=12.78; F1360=1.90e-13; F1700=1.76e-13; F2200=1.27e-13EXT-STARB6-B9.5 III-INOSK179 : [M2002]_82928, Sk 179, SK 179
Previous name : Sk 179
Input file: SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
SIMBAD link (SK 179): https://simbad.u-strasbg.fr/simbad/sim-id?Ident=SK+179&submit=submit+id
SpT = B6 I
COS/G130M/c1291 : rn(ck04models(B6I,Teff=12826,metallicity=0.004,logG=2.5), johnson U mag=12.240 vegamag)
COS/G160M/c1611 : rn(ck04models(B6I,Teff=12826,metallicity=0.004,logG=2.5), johnson U mag=12.240 vegamag)
COS/G185M/c1921 : rn(ck04models(B6I,Teff=12826,metallicity=0.004,logG=2.5), johnson U mag=12.240 vegamag)
COS/G185M/c1953 : rn(ck04models(B6I,Teff=12826,metallicity=0.004,logG=2.5), johnson U mag=12.240 vegamag)
COS/G185M/c1986 : rn(ck04models(B6I,Teff=12826,metallicity=0.004,logG=2.5), johnson U mag=12.240 vegamag)
STIS/E140M/c1425 : rn(ck04models(B6I,Teff=12826,metallicity=0.004,logG=2.5), johnson U mag=12.240 vegamag)
STIS/E230M/c1978 : rn(ck04models(B6I,Teff=12826,metallicity=0.004,logG=2.5), johnson U mag=12.240 vegamag)
STIS/E230M/c2707 : rn(ck04models(B6I,Teff=12826,metallicity=0.004,logG=2.5), johnson U mag=12.240 vegamag)
Coordinate pedigree: Gaia
Calculation performed 2020-02-24T17:54:45, v0.4
-------------------------------------------------------------------------------
tstatus; SK179; P/COS approved for submission; S/STIS approved for submission; P/CP 26/06/21; S/DW 22/05/21
tcheck; APT/SIMBAD target names: ; SK179 'Sk 179'
tcheck; Target info verification status?; Good
tcheck; Coordinates & P.M. updated?; Verfied (PM not included)
tcheck; Adopted SED compared to Observations?; Yes - photometry is poor for this object, nothing from Zaritsky for this field, negative E(B-V) is suspicious, and source of U mag is unclear, but adding dust makes fit to photometry worse.
for STIS/E230M, new G430L spectrum agrees well with UBV -- model slightly overestimates Balmer jump -- SED2707 agrees reasonably well with G430L below Balmer jump -- G430L acq has only target in acq boxM2002-SMC-82928J2000SpT=B6 I; E(B-V)=-0.03; U=12.2; B=12.97; V=13.09; R=13.32; I=13.31The scheduling data was generated by CASM 29.2.CASM was run in Phase II mode.vstatus; 1C; AV200;P/COS approved for submission; P/CP 02/11/20 ; intrev: complete ; P/AF 14/07/21
vcheck; Enter targ name & Inst. & Resp. Sci.; AV200 ; COS ; 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
vcheck; Selected ACQ strategy?; G130M/c1291 dispersed
vcheck; Possible ACQ or Sci spoilers?; None
vcheck; Field BOT clear?; Yes, with explanation ...
GSC 2 "unknowns" lack GSC color info, but can be easily shown to be safe using Zaritsky catalog.
Brightest U band Zaritsky objects near target:
In PSA macro-aperture:
UBVI = 18.191, 17.199, 16.061, 14.651
UBVI = 18.134, 18.721, 18.685, 18.570 at 9.17" from target PA=205.7D > BOP limiting star
But unreddened O star llimit for all COS modes is much brighter than this: see ETC 1417065, 1417089, 1431784, and 1431798
anything fainter than V=14.5 is safe in PSA
In BOA brightest U band measure in Zaritsky is
UVBI = 14.995, 16.003, 16.069, 16.209 at 18" from target
But anything fainter than V=9.25 is safe for BOA
All Zaritsky stars without U mags are fainter than V=18.2
vcheck; Visual BOT check for stars not in catalog?; non-found; see figure av200_gsc2_zaritsky.png in box folder
vcheck; Orbit packing finalized?; ...
can fit about 85% of requested c1291 exposure time into a single 3 orbit visit; remaining exposures fit into a second 3 orbit visit with a bit of time to spare. (113% of requested c1611, 104% of c1953, 109% of c1986)
vcheck; Buffer times optimized?; yes
vcheck; Verify visit grouping correct; N/A
vcheck; Is visit ready for int. review?; Yes
Allocated COS orbits = 6 do as 3+3(Tic-Visit
:proposal-id 16375
:visit-id "1C"
:proposal-version -1
:trans-version "20210514"
:date "02-Nov-2021 11:52:23.0"
: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 939424
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16375
:visit-id "1C"
:obset-id "1C"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16375
:visit-id "1C"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2596
: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 2989
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16375
:visit-id "1C"
:orbit-number 2
:pcs-time 392
:si-vis-utilization 2597
: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 16375
:visit-id "1C"
:orbit-number 3
:pcs-time 392
:si-vis-utilization 2597
:al-overhead-at-end 0
:internal-dur-at-end 344
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2989
:pcs-gap 0
)true30rn-max(ck04models(B8I,Teff=11278,metallicity=0.004,logG=2.26) (extinction smcbar=0.080), flux1360 +- 30.0A flux=8.1e-14 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: B8Ia --> B8 I
SED = AV200_COS_G130M_c1291_sed.fits
For exptime=8424.8 s, spectral region:
1150.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 1155.2 cts/s/segment
brightest pixel: 0.016 cts/s/pix at 1277.0 A
Calculation performed 2020-02-24T17:55:02, v0.4rn-max(ck04models(B8I,Teff=11278,metallicity=0.004,logG=2.26) (extinction smcbar=0.080), flux1360 +- 30.0A flux=8.1e-14 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: B8Ia --> B8 I
SED = AV200_COS_G130M_c1291_sed.fits
For exptime=8424.8 s, spectral region:
1150.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 1155.2 cts/s/segment
brightest pixel: 0.016 cts/s/pix at 1277.0 A
Calculation performed 2020-02-24T17:55:02, v0.4rn-max(ck04models(B8I,Teff=11278,metallicity=0.004,logG=2.26) (extinction smcbar=0.080), flux1360 +- 30.0A flux=8.1e-14 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: B8Ia --> B8 I
SED = AV200_COS_G130M_c1291_sed.fits
For exptime=8424.8 s, spectral region:
1150.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 1155.2 cts/s/segment
brightest pixel: 0.016 cts/s/pix at 1277.0 A
Calculation performed 2020-02-24T17:55:02, v0.4rn-max(ck04models(B8I,Teff=11278,metallicity=0.004,logG=2.26) (extinction smcbar=0.080), flux1360 +- 30.0A flux=8.1e-14 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: B8Ia --> B8 I
SED = AV200_COS_G130M_c1291_sed.fits
For exptime=8424.8 s, spectral region:
1150.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 1155.2 cts/s/segment
brightest pixel: 0.016 cts/s/pix at 1277.0 A
Calculation performed 2020-02-24T17:55:02, v0.4The scheduling data was generated by CASM 29.2.CASM was run in Phase II mode.vstatus; 1D; AV200;P/COS approved for submission; P/CP 02/11/20 ; intrev: complete ; P/AF 14/07/21
vcheck; Enter targ name & Inst. & Resp. Sci.; AV200 ; COS ; 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
vcheck; Selected ACQ strategy?; G130M/c1291 dispersed
vcheck; Possible ACQ or Sci spoilers?; None
vcheck; Field BOT clear?; Yes, with explanation ...
GSC 2 "unknowns" lack GSC color info, but can be easily shown to be safe using Zaritsky catalog.
Brightest U band Zaritsky objects near target:
In PSA macro-aperture:
UBVI = 18.191, 17.199, 16.061, 14.651
UBVI = 18.134, 18.721, 18.685, 18.570 at 9.17" from target PA=205.7D > BOP limiting star
But unreddened O star llimit for all COS modes is much brighter than this: see ETC 1417065, 1417089, 1431784, and 1431798
anything fainter than V=14.5 is safe in PSA
In BOA brightest U band measure in Zaritsky is
UVBI = 14.995, 16.003, 16.069, 16.209 at 18" from target
But anything fainter than V=9.25 is safe for BOA
All Zaritsky stars without U mags are fainter than V=18.2
vcheck; Visual BOT check for stars not in catalog?; non-found; see figure av200_gsc2_zaritsky.png in box folder
vcheck; Orbit packing finalized?; ...
can fit about 85% of requested c1291 into a single 3 orbit visit; remaining exposures fit into a second 3 orbit visit with a bit of time to spare. (113% of requested c1611, 104% of c1953, 109% of c1986)
vcheck; Buffer times optimized?; yes
vcheck; Verify visit grouping correct; N/A
vcheck; Is visit ready for int. review?; Yes
Allocated COS orbits = 6 do as 3+3163556113000025.69999999999999(Tic-Visit
:proposal-id 16375
:visit-id "1D"
:proposal-version -1
:trans-version "20210514"
:date "02-Nov-2021 11:52:24.0"
: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 1287536
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16375
:visit-id "1D"
:obset-id "1D"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16375
:visit-id "1D"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2594
: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 2989
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16375
:visit-id "1D"
:orbit-number 2
:pcs-time 392
:si-vis-utilization 2593
: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 16375
:visit-id "1D"
:orbit-number 3
:pcs-time 392
:si-vis-utilization 2597
:al-overhead-at-end 0
:internal-dur-at-end 363
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2989
:pcs-gap 0
)true30rn-max(ck04models(B8I,Teff=11278,metallicity=0.004,logG=2.26) (extinction smcbar=0.080), flux1700 +- 5.0A flux=1e-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: B8Ia --> B8 I
SED = AV200_COS_G160M_c1611_sed.fits
For exptime=2196.0 s, spectral region:
1590.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 1329.0 cts/s/segment
brightest pixel: 0.019 cts/s/pix at 1447.0 A
Calculation performed 2020-02-24T17:55:04, v0.4rn-max(ck04models(B8I,Teff=11278,metallicity=0.004,logG=2.26) (extinction smcbar=0.080), flux1700 +- 5.0A flux=1e-13 Flam); cos,nuv,g185m,c1953,psa,mjd#59305
From file SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
Spectral type: B8Ia --> B8 I
SED = AV200_COS_G185M_c1953_sed.fits
For exptime=1650.8 s, spectral region:
1860.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 1554.5 cts/s/segment
brightest pixel: 0.111 cts/s/pix at 1971.0 A
Calculation performed 2020-02-24T17:55:05, v0.4rn-max(ck04models(B8I,Teff=11278,metallicity=0.004,logG=2.26) (extinction smcbar=0.080), flux2200 +- 5.0A flux=9.2e-14 Flam); cos,nuv,g185m,c1986,psa,mjd#59305
From file SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
Spectral type: B8Ia --> B8 I
SED = AV200_COS_G185M_c1986_sed.fits
For exptime=1544.4 s, spectral region:
1980.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 1499.9 cts/s/segment
brightest pixel: 0.099 cts/s/pix at 1976.0 A
Calculation performed 2020-02-24T17:55:06, v0.4vstatus; 1D; AV200;P/COS approved for submission; P/CP 02/11/20 ; intrev: complete ; P/AF 14/07/21
vcheck; Enter targ name & Inst. & Resp. Sci.; AV200 ; COS ; 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
vcheck; Selected ACQ strategy?; G130M/c1291 dispersed
vcheck; Possible ACQ or Sci spoilers?; None
vcheck; Field BOT clear?; Yes, with explanation ...
GSC 2 "unknowns" lack GSC color info, but can be easily shown to be safe using Zaritsky catalog.
Brightest U band Zaritsky objects near target:
In PSA macro-aperture:
UBVI = 18.191, 17.199, 16.061, 14.651
UBVI = 18.134, 18.721, 18.685, 18.570 at 9.17" from target PA=205.7D > BOP limiting star
But unreddened O star llimit for all COS modes is much brighter than this: see ETC 1417065, 1417089, 1431784, and 1431798
anything fainter than V=14.5 is safe in PSA
In BOA brightest U band measure in Zaritsky is
UVBI = 14.995, 16.003, 16.069, 16.209 at 18" from target
But anything fainter than V=9.25 is safe for BOA
All Zaritsky stars without U mags are fainter than V=18.2
vcheck; Visual BOT check for stars not in catalog?; non-found; see figure av200_gsc2_zaritsky.png in box folder
vcheck; Orbit packing finalized?; ...
can fit about 85% of requested c1291 into a single 3 orbit visit; remaining exposures fit into a second 3 orbit visit with a bit of time to spare. (113% of requested c1611, 104% of c1953, 109% of c1986)
vcheck; Buffer times optimized?; yes
vcheck; Verify visit grouping correct; N/A
vcheck; Is visit ready for int. review?; Yes
Allocated COS orbits = 6 do as 3+3(Tic-Visit
:proposal-id 16375
:visit-id "1D"
:proposal-version -1
:trans-version "20210514"
:date "02-Nov-2021 11:52:24.0"
: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 1287536
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16375
:visit-id "1D"
:obset-id "1D"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16375
:visit-id "1D"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2594
: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 2989
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16375
:visit-id "1D"
:orbit-number 2
:pcs-time 392
:si-vis-utilization 2593
: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 16375
:visit-id "1D"
:orbit-number 3
:pcs-time 392
:si-vis-utilization 2597
:al-overhead-at-end 0
:internal-dur-at-end 363
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2989
:pcs-gap 0
)false30rn-max(ck04models(B8I,Teff=11278,metallicity=0.004,logG=2.26) (extinction smcbar=0.080), flux1700 +- 5.0A flux=1e-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: B8Ia --> B8 I
SED = AV200_COS_G160M_c1611_sed.fits
For exptime=2196.0 s, spectral region:
1590.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 1329.0 cts/s/segment
brightest pixel: 0.019 cts/s/pix at 1447.0 A
Calculation performed 2020-02-24T17:55:04, v0.4rn-max(ck04models(B8I,Teff=11278,metallicity=0.004,logG=2.26) (extinction smcbar=0.080), flux1700 +- 5.0A flux=1e-13 Flam); cos,nuv,g185m,c1953,psa,mjd#59305
From file SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
Spectral type: B8Ia --> B8 I
SED = AV200_COS_G185M_c1953_sed.fits
For exptime=1650.8 s, spectral region:
1860.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 1554.5 cts/s/segment
brightest pixel: 0.111 cts/s/pix at 1971.0 A
Calculation performed 2020-02-24T17:55:05, v0.4rn-max(ck04models(B8I,Teff=11278,metallicity=0.004,logG=2.26) (extinction smcbar=0.080), flux2200 +- 5.0A flux=9.2e-14 Flam); cos,nuv,g185m,c1986,psa,mjd#59305
From file SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
Spectral type: B8Ia --> B8 I
SED = AV200_COS_G185M_c1986_sed.fits
For exptime=1544.4 s, spectral region:
1980.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 1499.9 cts/s/segment
brightest pixel: 0.099 cts/s/pix at 1976.0 A
Calculation performed 2020-02-24T17:55:06, v0.4The scheduling data was generated by CASM 29.2.CASM was run in Phase II mode.vstatus; 1S; AV200; S/STIS approved for submission; S/CP 02/11/20 ; intrev: complete ; P/AF 14/07/21
vcheck; Enter targ name & Inst. & Resp. Sci.; AV200 ; 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 - see COS
vcheck; Selected ACQ strategy?; F28X50LP, 0.5s should yield S/N~125
vcheck; Possible ACQ or Sci spoilers?; none (previous G430L acq shows no other objects in 5"x5" acq box)
vcheck; Field BOT clear?; yes; BOT shows target as unknown
vcheck; Visual BOT check for stars not in catalog?; clear -- Gaia DR3 has nothing else with G<18 within 5"
vcheck; Orbit packing finalized?; Yes
vcheck; Buffer times optimized?; Yes
vcheck; Verify visit grouping correct; N/A
vcheck; Is visit ready for int. review?; yes
Allocated STIS orbits = 1163519509600015.319928891849287(Tic-Visit
:proposal-id 16375
:visit-id "1S"
:proposal-version -1
:trans-version "20210514"
:date "02-Nov-2021 11:52:25.0"
: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 16375
:visit-id "1S"
:obset-id "1S"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16375
:visit-id "1S"
: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
)true10See also exposure oec696jbq from proposal 16230The model for the COS c1291 agrees better with the IUE flux in this wavelength range than does the 2200 Angstrom normalization intended for this grating.
rn-max(ck04models(B8I,Teff=11278,metallicity=0.004,logG=2.26) (extinction smcbar=0.080), flux2200 +- 5.0A flux=9.2e-14 Flam); stis,nuvmama,e230m,c2707,0.2x0.2,mjd#59305
From file SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
Spectral type: B8Ia --> B8 I
SED = AV200_STIS_E230M_c2707_sed.fits
For exptime=2118.4 s, spectral region:
2800.0 +- 0.5 A achieves SNR=20.0/resel
global countrate (brightest segment): 4324.1 cts/s/segment
brightest pixel: 0.054 cts/s/pix at 2647.5 A
Calculation performed 2020-02-24T17:55:10, v0.4
ETC calculation using IUE spectrum yields similar results -- 0.076|4.9k cts/s, S/N~25 near 2800A (1517446)vstatus; 1S; AV200; S/STIS approved for submission; S/CP 02/11/20 ; intrev: complete ; P/AF 14/07/21
vcheck; Enter targ name & Inst. & Resp. Sci.; AV200 ; 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 - see COS
vcheck; Selected ACQ strategy?; F28X50LP, 0.5s should yield S/N~125
vcheck; Possible ACQ or Sci spoilers?; none (previous G430L acq shows no other objects in 5"x5" acq box)
vcheck; Field BOT clear?; yes; BOT shows target as unknown
vcheck; Visual BOT check for stars not in catalog?; clear -- Gaia DR3 has nothing else with G<18 within 5"
vcheck; Orbit packing finalized?; Yes
vcheck; Buffer times optimized?; Yes
vcheck; Verify visit grouping correct; N/A
vcheck; Is visit ready for int. review?; yes
Allocated STIS orbits = 1(Tic-Visit
:proposal-id 16375
:visit-id "1S"
:proposal-version -1
:trans-version "20210514"
:date "02-Nov-2021 11:52:25.0"
: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 16375
:visit-id "1S"
:obset-id "1S"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16375
:visit-id "1S"
: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
)false10See also exposure oec696jbq from proposal 16230The model for the COS c1291 agrees better with the IUE flux in this wavelength range than does the 2200 Angstrom normalization intended for this grating.
rn-max(ck04models(B8I,Teff=11278,metallicity=0.004,logG=2.26) (extinction smcbar=0.080), flux2200 +- 5.0A flux=9.2e-14 Flam); stis,nuvmama,e230m,c2707,0.2x0.2,mjd#59305
From file SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
Spectral type: B8Ia --> B8 I
SED = AV200_STIS_E230M_c2707_sed.fits
For exptime=2118.4 s, spectral region:
2800.0 +- 0.5 A achieves SNR=20.0/resel
global countrate (brightest segment): 4324.1 cts/s/segment
brightest pixel: 0.054 cts/s/pix at 2647.5 A
Calculation performed 2020-02-24T17:55:10, v0.4
ETC calculation using IUE spectrum yields similar results -- 0.076|4.9k cts/s, S/N~25 near 2800A (1517446)The scheduling data was generated by CASM 29.2.CASM was run in Phase II mode.vstatus; 2C; AV314; P/COS approved for submission; P/CP 03/11/20 ; intrev: complete ; P/AF 14/07/21
vcheck; Enter targ name & Inst. & Resp. Sci.; AV314 ; COS ; CP
vcheck; ETC numbers entered in APT?; Done
vcheck; Any screening violations?; No
vcheck; S/N ETC calcs done & documented?; Yes
vcheck; Field images checked & saved?; yes
vcheck; Selected ACQ strategy?; Do dispersed G160M c1611 exposure to optimize efficiency and orbit packing
vcheck; Possible ACQ or Sci spoilers?; none
vcheck; Field BOT clear?; yes ...
3 unknowns flagged; one is target, the other (S0XG331178) is not visible in GSC2 image and has N-plate mag=17.93 (no F or J plate mag so apparently a very faint, very red object)
The third is a relatively bright star that is marked as both safe and unknown (not a point source) for c1291, but Zaritsky gives UBVI=13.19, 14.362, 14.543, 14.924, and an unreddened O star with U=13.19 is safe (COS.sp.1470942)
All other stars (except for the target) in macro-aperture are fainter than this one
vcheck; Visual BOT check for stars not in catalog?; None found
vcheck; Orbit packing finalized?; yes ...
achieved 90% of requested c1291, 88% of c1611, 96% of c1953, 98% of c1986.
1st two FP-POS of c1953 are a bit shorter than the last two positions (311s vs 366s per FP-POS)
vcheck; Buffer times optimized?; yes
vcheck; Verify visit grouping correct; N/A
vcheck; Is visit ready for int. review?; Yes
Allocated COS orbits = 3163496633100011.759384778947293(Tic-Visit
:proposal-id 16375
:visit-id "2C"
:proposal-version -1
:trans-version "20210514"
:date "02-Nov-2021 11:52:26.0"
: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 1183200
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16375
:visit-id "2C"
:obset-id "2C"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16375
:visit-id "2C"
: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 16375
:visit-id "2C"
:orbit-number 2
:pcs-time 392
:si-vis-utilization 2596
: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 16375
:visit-id "2C"
:orbit-number 3
:pcs-time 392
:si-vis-utilization 2596
:al-overhead-at-end 0
:internal-dur-at-end 363
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2989
:pcs-gap 0
)true30c1291 needs 1.3s (COS.sa.1470835)
c1611 needs 1.0s (COS.sa.1470836)rn-max(ck04models(B5I,Teff=13600,metallicity=0.004,logG=2.5), flux1700 +- 5.0A flux=1.5e-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: B5Iab --> B5 I
SED = AV314_COS_G160M_c1611_sed.fits
For exptime=1457.7 s, spectral region:
1590.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 2260.6 cts/s/segment
brightest pixel: 0.034 cts/s/pix at 1447.0 A
Calculation performed 2020-02-24T17:54:15, v0.4rn-max(ck04models(B5I,Teff=13600,metallicity=0.004,logG=2.5), flux1360 +- 30.0A flux=1.8e-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: B5Iab --> B5 I
SED = AV314_COS_G130M_c1291_sed.fits
For exptime=1648.3 s, spectral region:
1150.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 2195.8 cts/s/segment
brightest pixel: 0.042 cts/s/pix at 1255.0 A
Calculation performed 2020-02-24T17:54:13, v0.4rn-max(ck04models(B5I,Teff=13600,metallicity=0.004,logG=2.5), flux1360 +- 30.0A flux=1.8e-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: B5Iab --> B5 I
SED = AV314_COS_G130M_c1291_sed.fits
For exptime=1648.3 s, spectral region:
1150.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 2195.8 cts/s/segment
brightest pixel: 0.042 cts/s/pix at 1255.0 A
Calculation performed 2020-02-24T17:54:13, v0.4rn-max(ck04models(B5I,Teff=13600,metallicity=0.004,logG=2.5), flux1360 +- 30.0A flux=1.8e-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: B5Iab --> B5 I
SED = AV314_COS_G130M_c1291_sed.fits
For exptime=1648.3 s, spectral region:
1150.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 2195.8 cts/s/segment
brightest pixel: 0.042 cts/s/pix at 1255.0 A
Calculation performed 2020-02-24T17:54:13, v0.4rn-max(ck04models(B5I,Teff=13600,metallicity=0.004,logG=2.5), flux1700 +- 5.0A flux=1.5e-13 Flam); cos,nuv,g185m,c1953,psa,mjd#59305
From file SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
Spectral type: B5Iab --> B5 I
SED = AV314_COS_G185M_c1953_sed.fits
For exptime=1404.7 s, spectral region:
1860.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 1623.3 cts/s/segment
brightest pixel: 0.123 cts/s/pix at 1872.0 A
Calculation performed 2020-02-24T17:54:16, v0.4rn-max(ck04models(B5I,Teff=13600,metallicity=0.004,logG=2.5), flux2200 +- 5.0A flux=1e-13 Flam); cos,nuv,g185m,c1986,psa,mjd#59305
From file SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
Spectral type: B5Iab --> B5 I
SED = AV314_COS_G185M_c1986_sed.fits
For exptime=1309.4 s, spectral region:
1980.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 1609.7 cts/s/segment
brightest pixel: 0.124 cts/s/pix at 1875.0 A
Calculation performed 2020-02-24T17:54:16, v0.4The scheduling data was generated by CASM 29.2.CASM was run in Phase II mode.vstatus; 2C; AV314; P/COS approved for submission; P/CP 03/11/20 ; intrev: complete ; P/AF 14/07/21
vcheck; Enter targ name & Inst. & Resp. Sci.; AV314 ; COS ; CP
vcheck; ETC numbers entered in APT?; Done
vcheck; Any screening violations?; No
vcheck; S/N ETC calcs done & documented?; Yes
vcheck; Field images checked & saved?; yes
vcheck; Selected ACQ strategy?; Do dispersed G160M c1611 exposure to optimize efficiency and orbit packing
vcheck; Possible ACQ or Sci spoilers?; none
vcheck; Field BOT clear?; yes ...
3 unknowns flagged; one is target, the other (S0XG331178) is not visible in GSC2 image and has N-plate mag=17.93 (no F or J plate mag so apparently a very faint, very red object)
The third is a relatively bright star that is marked as both safe and unknown (not a point source) for c1291, but Zaritsky gives UBVI=13.19, 14.362, 14.543, 14.924, and an unreddened O star with U=13.19 is safe (COS.sp.1470942)
All other stars (except for the target) in macro-aperture are fainter than this one
vcheck; Visual BOT check for stars not in catalog?; None found
vcheck; Orbit packing finalized?; yes ...
achieved 90% of requested c1291, 88% of c1611, 96% of c1953, 98% of c1986.
1st two FP-POS of c1953 are a bit shorter than the last two positions (311s vs 366s per FP-POS)
vcheck; Buffer times optimized?; yes
vcheck; Verify visit grouping correct; N/A
vcheck; Is visit ready for int. review?; Yes
Allocated COS orbits = 3(Tic-Visit
:proposal-id 16375
:visit-id "BC"
:proposal-version -1
:trans-version "20210514"
:date "02-Nov-2021 11:39:50.0"
: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 356800
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16375
:visit-id "BC"
:obset-id "BC"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16375
:visit-id "BC"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2596
: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 16375
:visit-id "BC"
:orbit-number 2
:pcs-time 392
:si-vis-utilization 2597
:al-overhead-at-end 0
:internal-dur-at-end 372
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2989
:pcs-gap 0
)true20c1291 needs 1.3s (COS.sa.1470835)
c1611 needs 1.0s (COS.sa.1470836)rn-max(ck04models(B5I,Teff=13600,metallicity=0.004,logG=2.5), flux1700 +- 5.0A flux=1.5e-13 Flam); cos,nuv,g185m,c1953,psa,mjd#59305
From file SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
Spectral type: B5Iab --> B5 I
SED = AV314_COS_G185M_c1953_sed.fits
For exptime=1404.7 s, spectral region:
1860.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 1623.3 cts/s/segment
brightest pixel: 0.123 cts/s/pix at 1872.0 A
Calculation performed 2020-02-24T17:54:16, v0.4rn-max(ck04models(B5I,Teff=13600,metallicity=0.004,logG=2.5), flux1700 +- 5.0A flux=1.5e-13 Flam); cos,nuv,g185m,c1953,psa,mjd#59305
From file SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
Spectral type: B5Iab --> B5 I
SED = AV314_COS_G185M_c1953_sed.fits
For exptime=1404.7 s, spectral region:
1860.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 1623.3 cts/s/segment
brightest pixel: 0.123 cts/s/pix at 1872.0 A
Calculation performed 2020-02-24T17:54:16, v0.4rn-max(ck04models(B5I,Teff=13600,metallicity=0.004,logG=2.5), flux1700 +- 5.0A flux=1.5e-13 Flam); cos,nuv,g185m,c1953,psa,mjd#59305
From file SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
Spectral type: B5Iab --> B5 I
SED = AV314_COS_G185M_c1953_sed.fits
For exptime=1404.7 s, spectral region:
1860.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 1623.3 cts/s/segment
brightest pixel: 0.123 cts/s/pix at 1872.0 A
Calculation performed 2020-02-24T17:54:16, v0.4rn-max(ck04models(B5I,Teff=13600,metallicity=0.004,logG=2.5), flux1700 +- 5.0A flux=1.5e-13 Flam); cos,nuv,g185m,c1953,psa,mjd#59305
From file SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
Spectral type: B5Iab --> B5 I
SED = AV314_COS_G185M_c1953_sed.fits
For exptime=1404.7 s, spectral region:
1860.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 1623.3 cts/s/segment
brightest pixel: 0.123 cts/s/pix at 1872.0 A
Calculation performed 2020-02-24T17:54:16, v0.4rn-max(ck04models(B5I,Teff=13600,metallicity=0.004,logG=2.5), flux1700 +- 5.0A flux=1.5e-13 Flam); cos,nuv,g185m,c1953,psa,mjd#59305
From file SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
Spectral type: B5Iab --> B5 I
SED = AV314_COS_G185M_c1953_sed.fits
For exptime=1404.7 s, spectral region:
1860.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 1623.3 cts/s/segment
brightest pixel: 0.123 cts/s/pix at 1872.0 A
Calculation performed 2020-02-24T17:54:16, v0.4rn-max(ck04models(B5I,Teff=13600,metallicity=0.004,logG=2.5), flux2200 +- 5.0A flux=1e-13 Flam); cos,nuv,g185m,c1986,psa,mjd#59305
From file SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
Spectral type: B5Iab --> B5 I
SED = AV314_COS_G185M_c1986_sed.fits
For exptime=1309.4 s, spectral region:
1980.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 1609.7 cts/s/segment
brightest pixel: 0.124 cts/s/pix at 1875.0 A
Calculation performed 2020-02-24T17:54:16, v0.4The scheduling data was generated by CASM 29.2.CASM was run in Phase II mode.vstatus; 2S; AV314; S/STIS approved for submission; S/CP 03/11/20 ; intrev: complete ; P/AF 14/07/21
vcheck; Enter targ name & Inst. & Resp. Sci.; AV314 ; 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
vcheck; Selected ACQ strategy?; F28X50LP, 0.5s should yield S/N~120
vcheck; Possible ACQ or Sci spoilers?; no -- previous G430L acq shows no other objects in 5"x5" acq box
vcheck; Field BOT clear?; yes -- Gaia DR3 has nothing else with G<17.7 within 5"
vcheck; Visual BOT check for stars not in catalog?; none
vcheck; Orbit packing finalized?; yes, get 93% of requested time for c2707
vcheck; Buffer times optimized?; yes
vcheck; Verify visit grouping correct; N/A
vcheck; Is visit ready for int. review?; yes
Allocated STIS orbits = 1164002189300062.400000000000006(Tic-Visit
:proposal-id 16375
:visit-id "2S"
:proposal-version -1
:trans-version "20210514"
:date "02-Nov-2021 11:52:27.0"
: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 16375
:visit-id "2S"
:obset-id "2S"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16375
:visit-id "2S"
: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
)true10see also TA exposure oec691hlq from proposal 16230rn-max(ck04models(B5I,Teff=13600,metallicity=0.004,logG=2.5), flux2200 +- 5.0A flux=1e-13 Flam); stis,nuvmama,e230m,c2707,0.2x0.2,mjd#59305
From file SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
Spectral type: B5Iab --> B5 I
SED = AV314_STIS_E230M_c2707_sed.fits
For exptime=2335.3 s, spectral region:
2800.0 +- 0.5 A achieves SNR=20.0/resel
global countrate (brightest segment): 4147.8 cts/s/segment
brightest pixel: 0.047 cts/s/pix at 2648.0 A
Calculation performed 2020-02-24T17:54:20, v0.4
ETC calculation using IUE spectrum yield similar results -- 0.061|4.4k cts/s, S/N~21 near 2800A (1517447)The scheduling data was generated by CASM 29.2.CASM was run in Phase II mode./private/var/folders/76/cvxxp9r10s96wsxp4w001ydh0001y0/T/OPVisit8423461246809065838.xmlvstatus; 2S; AV314; S/STIS approved for submission; S/CP 03/11/20 ; intrev: complete ; P/AF 14/07/21
vcheck; Enter targ name & Inst. & Resp. Sci.; AV314 ; 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
vcheck; Selected ACQ strategy?; F28X50LP, 0.5s should yield S/N~120
vcheck; Possible ACQ or Sci spoilers?; no -- previous G430L acq shows no other objects in 5"x5" acq box
vcheck; Field BOT clear?; yes -- Gaia DR3 has nothing else with G<17.7 within 5"
vcheck; Visual BOT check for stars not in catalog?; none
vcheck; Orbit packing finalized?; yes, get 93% of requested time for c2707
vcheck; Buffer times optimized?; yes
vcheck; Verify visit grouping correct; N/A
vcheck; Is visit ready for int. review?; yes
Allocated STIS orbits = 1(Tic-Visit
:proposal-id 16375
:visit-id "BS"
:proposal-version -1
:trans-version "20210514"
:date "23-Dec-2021 16:45:19.0"
: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 16375
:visit-id "BS"
:obset-id "BS"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16375
:visit-id "BS"
: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
)true10see also TA exposure oec691hlq from proposal 16230rn-max(ck04models(B5I,Teff=13600,metallicity=0.004,logG=2.5), flux2200 +- 5.0A flux=1e-13 Flam); stis,nuvmama,e230m,c2707,0.2x0.2,mjd#59305
From file SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
Spectral type: B5Iab --> B5 I
SED = AV314_STIS_E230M_c2707_sed.fits
For exptime=2335.3 s, spectral region:
2800.0 +- 0.5 A achieves SNR=20.0/resel
global countrate (brightest segment): 4147.8 cts/s/segment
brightest pixel: 0.047 cts/s/pix at 2648.0 A
Calculation performed 2020-02-24T17:54:20, v0.4
ETC calculation using IUE spectrum yield similar results -- 0.061|4.4k cts/s, S/N~21 near 2800A (1517447)The scheduling data was generated by CASM 29.2.CASM was run in Phase II mode.vstatus; 3C; AV343; P/COS approved for submission ; P/RS 24/06/21 ; intrev: complete ; P/AF 14/07/21
vcheck; Enter targ name & Inst. & Resp. Sci.; AV343 ; COS ; RS
vcheck; ETC numbers entered in APT?; Yes
vcheck; Any screening violations?; No
vcheck; S/N ETC calcs done & documented?; N/A
vcheck; Field images checked & saved?; Yes
vcheck; Selected ACQ strategy?;
NUV ACQ/PEAKD COS.sa.1473724 6 s; ACQ/PEAKXD 18s COS.sa.1473725; both c1941
vcheck; Possible ACQ or Sci spoilers?; no
vcheck; Field BOT clear?; yes, only the target is flagged
close companion in PSA macro-aperture that is not in GSC2 has V=16.169, U=15.146 in Zaritsky
vcheck; Visual BOT check for stars not in catalog?; OK (if we use Zaritsky rather than just GSC2)
vcheck; Orbit packing finalized?; Yes
vcheck; Buffer times optimized?; Yes
vcheck; Verify visit grouping correct; N/A
vcheck; Is visit ready for int. review?; Yes
Allocated COS orbits = 4(Tic-Visit
:proposal-id 16375
:visit-id "3C"
:proposal-version -1
:trans-version "20210514"
:date "02-Nov-2021 11:52:29.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 4
:saa-model "31"
:si-bright-earth-limb-angle 20.0
:data-volume 1165696
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16375
:visit-id "3C"
:obset-id "3C"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16375
:visit-id "3C"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2596
: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 16375
:visit-id "3C"
:orbit-number 2
:pcs-time 392
:si-vis-utilization 2597
: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 16375
:visit-id "3C"
:orbit-number 3
:pcs-time 392
:si-vis-utilization 2597
: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 2989
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16375
:visit-id "3C"
:orbit-number 4
:pcs-time 392
:si-vis-utilization 2597
:al-overhead-at-end 0
:internal-dur-at-end 420
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2989
:pcs-gap 0
)true40With revised SED requires 4180s or 2090 per FP-POS
rn(ck04models(B6I,Teff=12826,metallicity=0.004,logG=2.5) (extinction smcbar=0.020), johnson U mag=12.320 vegamag); 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: B6Iab --> B6 I
SED = AV343_COS_G130M_c1291_sed.fits
For exptime=2979.1 s, spectral region:
1150.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 1572.7 cts/s/segment
brightest pixel: 0.027 cts/s/pix at 1277.0 A
Calculation performed 2020-02-24T17:54:37, v0.4rn(ck04models(B6I,Teff=12826,metallicity=0.004,logG=2.5) (extinction smcbar=0.020), johnson U mag=12.320 vegamag); 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: B6Iab --> B6 I
SED = AV343_COS_G130M_c1291_sed.fits
For exptime=2979.1 s, spectral region:
1150.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 1572.7 cts/s/segment
brightest pixel: 0.027 cts/s/pix at 1277.0 A
Calculation performed 2020-02-24T17:54:37, v0.4rn(ck04models(B6I,Teff=12826,metallicity=0.004,logG=2.5) (extinction smcbar=0.020), johnson U mag=12.320 vegamag); 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: B6Iab --> B6 I
SED = AV343_COS_G130M_c1291_sed.fits
For exptime=2979.1 s, spectral region:
1150.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 1572.7 cts/s/segment
brightest pixel: 0.027 cts/s/pix at 1277.0 A
Calculation performed 2020-02-24T17:54:37, v0.4with revised model requies 2603s or 650 per FP-POS
rn(ck04models(B6I,Teff=12826,metallicity=0.004,logG=2.5) (extinction smcbar=0.020), johnson U mag=12.320 vegamag); 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: B6Iab --> B6 I
SED = AV343_COS_G160M_c1611_sed.fits
For exptime=1978.1 s, spectral region:
1590.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 1619.0 cts/s/segment
brightest pixel: 0.024 cts/s/pix at 1447.0 A
Calculation performed 2020-02-24T17:54:40, v0.4with revised SED requires 2079s
rn(ck04models(B6I,Teff=12826,metallicity=0.004,logG=2.5) (extinction smcbar=0.020), johnson U mag=12.320 vegamag); cos,nuv,g185m,c1986,psa,mjd#59305
From file SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
Spectral type: B6Iab --> B6 I
SED = AV343_COS_G185M_c1986_sed.fits
For exptime=1591.6 s, spectral region:
1980.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 1487.6 cts/s/segment
brightest pixel: 0.100 cts/s/pix at 1875.0 A
Calculation performed 2020-02-24T17:54:41, v0.4with revised SED requires 2079s
rn(ck04models(B6I,Teff=12826,metallicity=0.004,logG=2.5) (extinction smcbar=0.020), johnson U mag=12.320 vegamag); cos,nuv,g185m,c1986,psa,mjd#59305
From file SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
Spectral type: B6Iab --> B6 I
SED = AV343_COS_G185M_c1986_sed.fits
For exptime=1591.6 s, spectral region:
1980.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 1487.6 cts/s/segment
brightest pixel: 0.100 cts/s/pix at 1875.0 A
Calculation performed 2020-02-24T17:54:41, v0.4with revised sed requires 2386s
rn(ck04models(B6I,Teff=12826,metallicity=0.004,logG=2.5) (extinction smcbar=0.020), johnson U mag=12.320 vegamag); cos,nuv,g185m,c1953,psa,mjd#59305
From file SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
Spectral type: B6Iab --> B6 I
SED = AV343_COS_G185M_c1953_sed.fits
For exptime=1818.0 s, spectral region:
1860.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 1475.1 cts/s/segment
brightest pixel: 0.096 cts/s/pix at 1872.0 A
Calculation performed 2020-02-24T17:54:41, v0.4with revised sed requires 2386s
rn(ck04models(B6I,Teff=12826,metallicity=0.004,logG=2.5) (extinction smcbar=0.020), johnson U mag=12.320 vegamag); cos,nuv,g185m,c1953,psa,mjd#59305
From file SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
Spectral type: B6Iab --> B6 I
SED = AV343_COS_G185M_c1953_sed.fits
For exptime=1818.0 s, spectral region:
1860.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 1475.1 cts/s/segment
brightest pixel: 0.096 cts/s/pix at 1872.0 A
Calculation performed 2020-02-24T17:54:41, v0.4The scheduling data was generated by CASM 29.2.CASM was run in Phase II mode.vstatus; 3S; AV343; S/STIS approved for submission; S/DW 22/05/21 ; intrev: complete ; P/AF 14/07/21
vcheck; Enter targ name & Inst. & Resp. Sci.; AV343 ; STIS ; DW
vcheck; ETC numbers entered in APT?; yes
vcheck; Any screening violations?; no -- GSC2 and GALEX list as safe, ETC confirms
vcheck; S/N ETC calcs done & documented?; yes
vcheck; Field images checked & saved?; yes
vcheck; Selected ACQ strategy?; F28x50LP, 0.5s should yield S/N~115
vcheck; Possible ACQ or Sci spoilers?; no -- previous G430L acq shows no other objects in 5"x5" acq box
vcheck; Field BOT clear?; yes -- clearance region dominated by saturated core of target
vcheck; Visual BOT check for stars not in catalog?; yes ...
Gaia DR3 has star with G=16.1 at 5.1", all others within 10" are much fainter
vcheck; Orbit packing finalized?; yes
vcheck; Buffer times optimized?; yes
vcheck; Verify visit grouping correct; n/a
vcheck; Is visit ready for int. review?; yes
Allocated STIS orbits = 1163926366700057.79263808335321(Tic-Visit
:proposal-id 16375
:visit-id "3S"
:proposal-version -1
:trans-version "20210514"
:date "02-Nov-2021 11:52:30.0"
: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 435312
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16375
:visit-id "3S"
:obset-id "3S"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16375
: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
)true10Revised SED based on IUE spectrum requires 3511s
rn(ck04models(B6I,Teff=12826,metallicity=0.004,logG=2.5) (extinction smcbar=0.020), johnson U mag=12.320 vegamag); stis,nuvmama,e230m,c2707,0.2x0.2,mjd#59305
From file SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
Spectral type: B6Iab --> B6 I
SED = AV343_STIS_E230M_c2707_sed.fits
For exptime=2695.6 s, spectral region:
2800.0 +- 0.5 A achieves SNR=20.0/resel
global countrate (brightest segment): 3915.3 cts/s/segment
brightest pixel: 0.042 cts/s/pix at 2647.5 A
Calculation performed 2020-02-24T17:54:45, v0.4
ETC calculations using IUE spectrum yield similar results -- 0.037|3.6k cts/s, S/N~17 near 2800A (1517451)The scheduling data was generated by CASM 29.2.CASM was run in Phase II mode./private/var/folders/76/cvxxp9r10s96wsxp4w001ydh0001y0/T/OPVisit9638143728436424859.xmlvstatus; 3S; AV343; S/STIS approved for submission; S/DW 22/05/21 ; intrev: complete ; P/AF 14/07/21
vcheck; Enter targ name & Inst. & Resp. Sci.; AV343 ; STIS ; DW
vcheck; ETC numbers entered in APT?; yes
vcheck; Any screening violations?; no -- GSC2 and GALEX list as safe, ETC confirms
vcheck; S/N ETC calcs done & documented?; yes
vcheck; Field images checked & saved?; yes
vcheck; Selected ACQ strategy?; F28x50LP, 0.5s should yield S/N~115
vcheck; Possible ACQ or Sci spoilers?; no -- previous G430L acq shows no other objects in 5"x5" acq box
vcheck; Field BOT clear?; yes -- clearance region dominated by saturated core of target
vcheck; Visual BOT check for stars not in catalog?; yes ...
Gaia DR3 has star with G=16.1 at 5.1", all others within 10" are much fainter
vcheck; Orbit packing finalized?; yes
vcheck; Buffer times optimized?; yes
vcheck; Verify visit grouping correct; n/a
vcheck; Is visit ready for int. review?; yes
Allocated STIS orbits = 1(Tic-Visit
:proposal-id 16375
:visit-id "CS"
:proposal-version -1
:trans-version "20210514"
:date "23-Dec-2021 16:45:31.0"
: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 435312
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16375
:visit-id "CS"
:obset-id "CS"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16375
:visit-id "CS"
: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
)true10Revised SED based on IUE spectrum requires 3511s
rn(ck04models(B6I,Teff=12826,metallicity=0.004,logG=2.5) (extinction smcbar=0.020), johnson U mag=12.320 vegamag); stis,nuvmama,e230m,c2707,0.2x0.2,mjd#59305
From file SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
Spectral type: B6Iab --> B6 I
SED = AV343_STIS_E230M_c2707_sed.fits
For exptime=2695.6 s, spectral region:
2800.0 +- 0.5 A achieves SNR=20.0/resel
global countrate (brightest segment): 3915.3 cts/s/segment
brightest pixel: 0.042 cts/s/pix at 2647.5 A
Calculation performed 2020-02-24T17:54:45, v0.4
ETC calculations using IUE spectrum yield similar results -- 0.037|3.6k cts/s, S/N~17 near 2800A (1517451)The scheduling data was generated by CASM 29.2.CASM was run in Phase II mode.vstatus; 4C; AV445; P/COS approved for submission; P/CP 03/06/21 ; intrev: complete ; P/AF 14/07/21
vcheck; Enter targ name & Inst. & Resp. Sci.; AV445 ; COS ; CP
vcheck; ETC numbers entered in APT?; yes ...
sed comparisons in AV445_c1291_sed.png and AV445_revised_sed.png
vcheck; Any screening violations?; no
vcheck; S/N ETC calcs done & documented?; yes
vcheck; Field images checked & saved?; yes av445-gsc2-cos.png
vcheck; Selected ACQ strategy?; c1291 dispersed
vcheck; Possible ACQ or Sci spoilers?; no
vcheck; Field BOT clear?; Yes ...
Except for target all stars visible in image are found by GSC2 BOT and declared safe.
vcheck; Visual BOT check for stars not in catalog?; None found
vcheck; Orbit packing finalized?; yes ...
using revised exposure estimtes obtained c1291 100%, c1611 96%, c1953 124%, c1986 126%. Used auto-adjust so 1st two sub-exposures of c1953 are a bit longer than the next two.
vcheck; Buffer times optimized?; Yes
vcheck; Verify visit grouping correct; N/A
vcheck; Is visit ready for int. review?; yes
Allocated COS orbits = 3(Tic-Visit
:proposal-id 16375
:visit-id "4C"
:proposal-version -1
:trans-version "20210514"
:date "02-Nov-2021 11:52:31.0"
: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 1200496
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16375
:visit-id "4C"
:obset-id "4C"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16375
:visit-id "4C"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2595
: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 2989
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16375
:visit-id "4C"
:orbit-number 2
:pcs-time 392
:si-vis-utilization 2597
: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 16375
:visit-id "4C"
:orbit-number 3
:pcs-time 392
:si-vis-utilization 2596
:al-overhead-at-end 0
:internal-dur-at-end 363
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2989
:pcs-gap 0
)true30rn-max(ck04models(B5I,Teff=13600,metallicity=0.004,logG=2.5) (extinction smcbar=0.030), 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: B5 (Iab) --> B5 I
SED = AV445_COS_G130M_c1291_sed.fits
For exptime=1552.8 s, spectral region:
1150.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 2657.5 cts/s/segment
brightest pixel: 0.048 cts/s/pix at 1277.0 A
Calculation performed 2020-02-24T17:54:25, v0.4rn-max(ck04models(B5I,Teff=13600,metallicity=0.004,logG=2.5) (extinction smcbar=0.030), 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: B5 (Iab) --> B5 I
SED = AV445_COS_G130M_c1291_sed.fits
For exptime=1552.8 s, spectral region:
1150.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 2657.5 cts/s/segment
brightest pixel: 0.048 cts/s/pix at 1277.0 A
Calculation performed 2020-02-24T17:54:25, v0.4rn-max(ck04models(B5I,Teff=13600,metallicity=0.004,logG=2.5) (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: B5 (Iab) --> B5 I
SED = AV445_COS_G160M_c1611_sed.fits
For exptime=1221.5 s, spectral region:
1590.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 2613.3 cts/s/segment
brightest pixel: 0.038 cts/s/pix at 1447.0 A
Calculation performed 2020-02-24T17:54:28, v0.4rn-max(ck04models(B5I,Teff=13600,metallicity=0.004,logG=2.5) (extinction smcbar=0.030), flux1700 +- 5.0A flux=1.8e-13 Flam); cos,nuv,g185m,c1953,psa,mjd#59305
From file SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
Spectral type: B5 (Iab) --> B5 I
SED = AV445_COS_G185M_c1953_sed.fits
For exptime=1106.2 s, spectral region:
1860.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 1818.9 cts/s/segment
brightest pixel: 0.156 cts/s/pix at 1872.0 A
Calculation performed 2020-02-24T17:54:28, v0.4rn-max(ck04models(B5I,Teff=13600,metallicity=0.004,logG=2.5) (extinction smcbar=0.030), flux2200 +- 5.0A flux=1.3e-13 Flam); cos,nuv,g185m,c1986,psa,mjd#59305
From file SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
Spectral type: B5 (Iab) --> B5 I
SED = AV445_COS_G185M_c1986_sed.fits
For exptime=1069.9 s, spectral region:
1980.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 1759.2 cts/s/segment
brightest pixel: 0.149 cts/s/pix at 1875.0 A
Calculation performed 2020-02-24T17:54:29, v0.4The scheduling data was generated by CASM 29.2.CASM was run in Phase II mode.vstatus; 4S; AV445; S/STIS approved for submission; S/DW 22/05/21 ; intrev:complete ; P/AF 14/07/21
vcheck; Enter targ name & Inst. & Resp. Sci.; AV445 ; STIS ; DW
vcheck; ETC numbers entered in APT?; yes
vcheck; Any screening violations?; no -- GSC2 lists as safe, confirmed via ETC
vcheck; S/N ETC calcs done & documented?; yes
vcheck; Field images checked & saved?; yes av445-gsc2-stis.png, others
vcheck; Selected ACQ strategy?; F28x50LP, 0.5s, I or V band normalization -- should yield S/N~135
vcheck; Possible ACQ or Sci spoilers?; none -- clearance region dominated by saturated core of target
vcheck; Field BOT clear?; yes
vcheck; Visual BOT check for stars not in catalog?; OK ...
Gaia DR3 has star with G=15.7 at 9.4", all others within 10" are much fainter
vcheck; Orbit packing finalized?; yes, get 130% of estimated time
vcheck; Buffer times optimized?; yes
vcheck; Verify visit grouping correct; N/A
vcheck; Is visit ready for int. review?; Yes
Allocated STIS orbits = 1164018199900063.0(Tic-Visit
:proposal-id 16375
:visit-id "4S"
:proposal-version -1
:trans-version "20210514"
:date "02-Nov-2021 11:52:32.0"
: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 16375
:visit-id "4S"
:obset-id "4S"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16375
:visit-id "4S"
: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(B5I,Teff=13600,metallicity=0.004,logG=2.5) (extinction smcbar=0.030), flux2200 +- 5.0A flux=1.3e-13 Flam); stis,nuvmama,e230m,c2707,0.2x0.2,mjd#59305
From file SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
Spectral type: B5 (Iab) --> B5 I
SED = AV445_STIS_E230M_c2707_sed.fits
For exptime=1681.0 s, spectral region:
2800.0 +- 0.5 A achieves SNR=20.0/resel
global countrate (brightest segment): 4741.8 cts/s/segment
brightest pixel: 0.062 cts/s/pix at 2648.0 A
Calculation performed 2020-02-24T17:54:33, v0.4
ETC calculations using IUE spectrum yield similar results -- 0.069|4.8k cts/s, S/N~24 near 2800A (1517448)The scheduling data was generated by CASM 29.2.CASM was run in Phase II mode.vstatus; 5C; SK179; P/COS approved for submission; P/RS 17/06/21 ; intrev: complete ; P/AF 14/07/21
vcheck; Enter targ name & Inst. & Resp. Sci.; SK179 ; COS ; RS
vcheck; ETC numbers entered in APT?; Yes
vcheck; Any screening violations?; No
vcheck; S/N ETC calcs done & documented?; N/A
vcheck; Field images checked & saved?; Yes
vcheck; Selected ACQ strategy?; Yes
vcheck; Possible ACQ or Sci spoilers?; No
vcheck; Field BOT clear?; GSC BOT finds one unknown, but it is the target
vcheck; Visual BOT check for stars not in catalog?; 2nd brightest star in field may have a fainter companion not in GSC2, but this is in the BOA region and fainter than safe star in PSA region - no coverage by Zaritsky
vcheck; Orbit packing finalized?; Yes
vcheck; Buffer times optimized?; Yes
vcheck; Verify visit grouping correct; N/A
vcheck; Is visit ready for int. review?; Yes
Allocated COS orbits = 4 (2 FUV + 2 NUV)1630184900000312.5(Tic-Visit
:proposal-id 16375
:visit-id "5C"
:proposal-version -1
:trans-version "20210514"
:date "02-Nov-2021 11:52:33.0"
: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 956848
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16375
:visit-id "5C"
:obset-id "5C"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16375
:visit-id "5C"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2596
: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 16375
:visit-id "5C"
:orbit-number 2
:pcs-time 392
:si-vis-utilization 2594
:al-overhead-at-end 0
:internal-dur-at-end 353
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2989
:pcs-gap 0
)true20rn(ck04models(B6I,Teff=12826,metallicity=0.004,logG=2.5), johnson U mag=12.240 vegamag); 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: B6 I --> B6 I
SED = SK179_COS_G130M_c1291_sed.fits
For exptime=2084.7 s, spectral region:
1150.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 2033.8 cts/s/segment
brightest pixel: 0.036 cts/s/pix at 1277.0 A
Calculation performed 2020-02-24T17:54:49, v0.4rn(ck04models(B6I,Teff=12826,metallicity=0.004,logG=2.5), johnson U mag=12.240 vegamag); 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: B6 I --> B6 I
SED = SK179_COS_G130M_c1291_sed.fits
For exptime=2084.7 s, spectral region:
1150.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 2033.8 cts/s/segment
brightest pixel: 0.036 cts/s/pix at 1277.0 A
Calculation performed 2020-02-24T17:54:49, v0.4rn(ck04models(B6I,Teff=12826,metallicity=0.004,logG=2.5), johnson U mag=12.240 vegamag); 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: B6 I --> B6 I
SED = SK179_COS_G160M_c1611_sed.fits
For exptime=1600.8 s, spectral region:
1590.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 2031.6 cts/s/segment
brightest pixel: 0.030 cts/s/pix at 1447.0 A
Calculation performed 2020-02-24T17:54:52, v0.4The scheduling data was generated by CASM 29.2.CASM was run in Phase II mode.vstatus; 5D; SK179; P/COS approved for submission; P/RS 17/06/21 ; intrev: complete; P/AF 14/07/21
vcheck; Enter targ name & Inst. & Resp. Sci.; SK179 ; COS ; RS
vcheck; ETC numbers entered in APT?; Yes
vcheck; Any screening violations?; No
vcheck; S/N ETC calcs done & documented?; N/A
vcheck; Field images checked & saved?; Yes
vcheck; Selected ACQ strategy?; Yes
vcheck; Possible ACQ or Sci spoilers?; No
vcheck; Field BOT clear?; GSC BOT finds one unknown, but it is the target
vcheck; Visual BOT check for stars not in catalog?; 2nd brightest star in field may have a fainter companion not in GSC2, but this is in the BOA region and fainter than safe star in PSA region - no coverage by Zaritsky
vcheck; Orbit packing finalized?; Yes
vcheck; Buffer times optimized?; Yes
vcheck; Verify visit grouping correct; N/A
vcheck; Is visit ready for int. review?; Yes
Allocated COS orbits = 4 (2 FUV + 2 NUV)16348932320004.652729597886889(Tic-Visit
:proposal-id 16375
:visit-id "5D"
:proposal-version -1
:trans-version "20210514"
:date "02-Nov-2021 11:52:34.0"
: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 765632
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16375
:visit-id "5D"
:obset-id "5D"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16375
:visit-id "5D"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 3129
: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 3525
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16375
:visit-id "5D"
:orbit-number 2
:pcs-time 392
:si-vis-utilization 3133
:al-overhead-at-end 0
:internal-dur-at-end 344
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3525
:pcs-gap 0
)true20rn(ck04models(B6I,Teff=12826,metallicity=0.004,logG=2.5), johnson U mag=12.240 vegamag); cos,nuv,g185m,c1986,psa,mjd#59305
From file SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
Spectral type: B6 I --> B6 I
SED = SK179_COS_G185M_c1986_sed.fits
For exptime=1345.9 s, spectral region:
1980.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 1588.1 cts/s/segment
brightest pixel: 0.119 cts/s/pix at 1875.0 A
Calculation performed 2020-02-24T17:54:53, v0.4rn(ck04models(B6I,Teff=12826,metallicity=0.004,logG=2.5), johnson U mag=12.240 vegamag); cos,nuv,g185m,c1953,psa,mjd#59305
From file SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
Spectral type: B6 I --> B6 I
SED = SK179_COS_G185M_c1953_sed.fits
For exptime=1517.8 s, spectral region:
1860.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 1575.1 cts/s/segment
brightest pixel: 0.114 cts/s/pix at 1872.0 A
Calculation performed 2020-02-24T17:54:53, v0.4The scheduling data was generated by CASM 29.2.CASM was run in Phase II mode.vstatus; 5S; SK179; S/STIS approved for submission; S/DW 22/05/21 ; intrev:complete; P/AF 14/07/21
vcheck; Enter targ name & Inst. & Resp. Sci.; SK179 ; STIS ; DW
vcheck; ETC numbers entered in APT?; yes
vcheck; Any screening violations?; no -- GSC2 lists 1 unknown (target) -- cleared via ETC
vcheck; S/N ETC calcs done & documented?; yes
vcheck; Field images checked & saved?; yes
vcheck; Selected ACQ strategy?; F28x50LP, 0.5s should yield S/N~110
vcheck; Possible ACQ or Sci spoilers?; no -- previous G430L acq shows no other objects in 5"x5" acq box
vcheck; Field BOT clear?; yes -- clearance region is dominated by saturated core of target
vcheck; Visual BOT check for stars not in catalog?; yes ...
Gaia DR3 has star with G=15.3 at 8.1", all others within 10" are much fainter
vcheck; Orbit packing finalized?; yes, get 90% of estimated time in a 1 orbit visit
vcheck; Buffer times optimized?; yes
vcheck; Verify visit grouping correct; n/a
vcheck; Is visit ready for int. review?; yes
Allocated STIS orbits = 11630301955000313.0984553556077(Tic-Visit
:proposal-id 16375
:visit-id "5S"
:proposal-version -1
:trans-version "20210514"
:date "02-Nov-2021 11:52:34.0"
: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 435312
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16375
:visit-id "5S"
:obset-id "5S"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16375
:visit-id "5S"
: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(ck04models(B6I,Teff=12826,metallicity=0.004,logG=2.5), johnson U mag=12.240 vegamag); stis,nuvmama,e230m,c2707,0.2x0.2,mjd#59305
From file SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
Spectral type: B6 I --> B6 I
SED = SK179_STIS_E230M_c2707_sed.fits
For exptime=2410.5 s, spectral region:
2800.0 +- 0.5 A achieves SNR=20.0/resel
global countrate (brightest segment): 4096.8 cts/s/segment
brightest pixel: 0.047 cts/s/pix at 2647.5 A
Calculation performed 2020-02-24T17:54:58, v0.4
ETC calculations using IUE spectrum yield similar results -- 0.049|4.2k cts/s, S/N~20 near 2800A (1517449)