For the best data quality, it is generally required to use all four FP-POS positions when observing at a given COS cenwave. See the COS Instrument Handbook for exceptions that may apply to observations with G130M/1291 or G160M.Re-submission 3: Added Visit AC, which is an exact copy of the failed Visit 1C as authorized by the TTRB under the auspices of HOPR-92547.
Re-submission 2: Corrected names of new Visits 1D and 2D in their respective vstatus lines.
Re-submission 1: Visits 1D and 2D provide 1 orbit of additional exposure time with the COS G130M/1096 configuration for BI265 and SK-69D212, respectively.1533265529----- Attempting Submission 1 (Fri Oct 07 15:30:41 GMT 2022) -----
----- Attempting Submission 2 (Tue Mar 07 18:22:21 GMT 2023) -----
----- Attempting Submission 3 (Tue Mar 07 21:07:38 GMT 2023) -----
----- Attempting Submission 4 (Thu May 25 13:22:25 GMT 2023) -----Investigators have changed through the implementation period of ULLYSES.
Visit 3C uses G130M/1291.ULLYSES LMC O5 Giants - COSThe Space Telescope Science Institute (STScI) Director has decided to devote up to 1000 orbits of Director's Discretionary time in observing Cycles 27-29 to a new Hubble Ultraviolet Legacy program focused on star formation and associated stellar physics. This new program, ULLYSES (UV Legacy Library of Young Stars as Essential Standards), will provide a UV spectroscopic reference sample of young (< 10 Myr) high- and low-mass stars. It will target over ~150 OB stars in the Magellanic Clouds and lower metallicity galaxies in the Local Group, and ~40 T Tauri stars and brown dwarfs in the Milky Way. In addition, ULLYSES will monitor 4 typical T Tauri stars over different rotational phases through at least three rotation periods, and over timescales of months to years. The resulting library will provide template spectra of massive stars at metallicities substantially below the well studied, while the low mass sample will cover a wide range of ages, accretion rates, and masses, including objects down to well below 0.5 M_sun. The legacy of this large UV dataset on the first 10 Myr of stellar evolution will be enhanced by complementary datasets obtained by the scientific community. In addition to the core goals of the program related to stellar astrophysics of low and high mass stars, this data will also enable exciting science in the fields of ISM, CGM, jets, and exoplanets. ULLYSES will be modeled after the Frontier Fields program: all data obtained will be non-proprietary. The implementation team at STScI is developing high-level science data products and a sophisticated database and website for disseminating data from the ULLYSES program and ancillary datasets for the ULLYSES target sample from space and ground-based facilities.This proposal includes a subset of the massive ULLYSES stars being observed in the Magellanic clouds.
Depending on target brightness, the main FUV spectral range will generally use either the STIS E140M setting or the combination of the COS c1291 + c1611 settings. Sufficiently bright stars without good FUSE data in the archive will also be observed with the COS c1096 setting to provide coverage at shorter wavelengths. Where time permits, stars of type O9 or later will also be observed with STIS E230M/1978, while for supergiants of spectral type B5 or later E230M/2707 may also be included. Where possible, targets of a given spectral type were selected to span both a range in extinction and in rotation rates to support a variety of stellar and ISM studies.
Signal-to-noise requirements used to determine the desired exposures times were defined as follows:
COS/G130M/c1096: 20 / nine-pixel resel at 1080 A
COS/G130M/c1291: 30 / six-pixel resel at 1150 A
COS/G160M/c1611: 30 / six-pixel resel at 1590 A
COS/G185M/c1953: 30 / three-pixel resel at 1860 A
COS/G185M/c1986: 30 / three-pixel resel at 1980 A
STIS/E140M/c1425: 20 / two-pixel resel at 1200 A
STIS/E230M/c1978: 20 / two-pixel resel at 1800 A
STIS/E230M/c2707: 20 / two-pixel resel at 2800 A
The actual implemented exposure times may be adjusted to efficiently use HST orbits, but should always provide at least 80% of the desired time as defined by the above requirements.
Additional details about the scientific motivation and technical implementation strategy of the ULLYSES observations can be found at http://www.stsci.edu/stsci-research/research-topics-and-programs/ullyses. The ULLYSES program is based on the recommendations of a working group led by Sally Oey; the full text of that group's report can be found at http://www.stsci.edu/files/live/sites/www/files/home/stsci-research/research-topics-and-programs/ullyses/_documents/HSTUV-report-ULLYSES.pdf.0falseSUPPORTEDSTARGIANT OOFNOBI265 : AAOMEGA-361, BI 265
Previous name : BI265
Input file: ULLYSES_Cycle29_MassiveStar_ProgramInput_v5.csv
SpT = O5 III(fc)
COS/G130M/c1096 : rn(PoWR-OB-new(PoWR_40000_3.80_m7.00_Z0.50.fits, lmc-ob-i 40-38, Z=0.500 solar, Teff=40000, log_lum=5.64, log_g=3.80, log_mdot=-7.00) (extinction lmcavg=0.130), flux1160 +- 2.0A flux=7.1e-13 Flam)
Coordinate pedigree: Gaia DR2
Calculation performed 2021-10-25T00:57:56, v0.9
-------------------------------------------------------------------------------
tstatus; BI265; P/COS approved for submission; S/ins not started; P/RS 29/08/22; S/xx DD/MM/YY
tcheck; APT/SIMBAD target names: ; BI265 'BI 265'
tcheck; Target info verification status?; OK
tcheck; Coordinates & P.M. verified, epoch checked?; Yes Gaia DR3
tcheck; Adopted SED compared to Observations?; Yes ...
BI265_adopted_sed.fits PoWR model matched to STIS and UBVAAOMEGA-361BI-265J2000SpT=O5 III(fc); E(B-V)=0.13; U=11.42; B=12.43; V=12.58; F1160=7.060e-13; F1360=5.780e-13; F1700=4.710e-13STARSUPERGIANT OOFNOSK-69D212 : SK -69 212
Previous name : Sk -69 212
Input file: ULLYSES_Cycle29_MassiveStar_ProgramInput_v5.csv
SpT = O5 In(f)p
COS/G130M/c1096 : rn(PoWR-OB-new(PoWR_39000_3.80_m7.00_Z0.50.fits, lmc-ob-i 39-38, Z=0.500 solar, Teff=39000, log_lum=5.54, log_g=3.80, log_mdot=-7.00) (extinction lmcavg=0.230), flux1160 +- 2.0A flux=5.5e-13 Flam)
Coordinate pedigree: Gaia DR2
Calculation performed 2021-10-25T00:57:37, v0.9
-------------------------------------------------------------------------------
tstatus; SK-69D212; P/COS approved for submission; S/ins not started; P/RS 29/08/22; S/xx DD/MM/YY
tcheck; APT/SIMBAD target names: ; SK-69D212 'SK -69 212'
tcheck; Target info verification status?; OK
tcheck; Coordinates & P.M. verified, epoch checked?; Yes Gaia DR3
tcheck; Adopted SED compared to Observations?; Yes ...
SK-69D212_adopted_sed.fits PoWR model matching STIS and UBVSK-69-212J2000SpT=O5 In(f)p; E(B-V)=0.23; U=11.31; B=12.26; V=12.31; F1160=5.460e-13; F1360=4.930e-13; F1700=4.570e-13STARGIANT OOFNOVFTS-244 : VFTS 244
Previous name : VFTS-244
Input file: ULLYSES_Cycle29_MassiveStar_ProgramInput_v5.csv
SpT = O5 III(n)(fc)
Note: Some exptime deducted due to outside program(s).
COS/G130M/c1291 : rn(PoWR-OB-new(PoWR_41000_3.80_m7.00_Z0.50.fits, lmc-ob-i 41-38, Z=0.500 solar, Teff=41000, log_lum=5.73, log_g=3.80, log_mdot=-7.00) (extinction lmc30dor=0.180), flux1360 +- 2.0A flux=1e-13 Flam)
COS/G160M/c1611 : rn(PoWR-OB-new(PoWR_41000_3.80_m7.00_Z0.50.fits, lmc-ob-i 41-38, Z=0.500 solar, Teff=41000, log_lum=5.73, log_g=3.80, log_mdot=-7.00) (extinction lmc30dor=0.180), flux1700 +- 2.0A flux=1e-13 Flam)
Coordinate pedigree: Gaia DR2
Calculation performed 2021-10-25T00:57:46, v0.9
-------------------------------------------------------------------------------
tstatus; VFTS-244; P/COS approved for submission; S/ins not started; P/RS 29/08/22; S/xx DD/MM/YY
tcheck; APT/SIMBAD target names: ; VFTS-244 'VFTS 244'
tcheck; Target info verification status?; OK
tcheck; Coordinates & P.M. verified, epoch checked?; Yes Gaia DR3
tcheck; Adopted SED compared to Observations?; Yes ...
VFTS-244_adopted_sed.fits PoWR model matched to STIS, F336W and UBV2MASS-J05380840-6905446J2000SpT=O5 III(n)(fc); E(B-V)=0.18; B=13.94; V=14.04; F1160=1.110e-13; F1360=1.050e-13; F1700=1.020e-13The scheduling data was generated by CASM 31.0.CASM was run in Phase II mode./private/var/folders/81/nbsn78xx3tzfyhsmxnp50pk80004gh/T/OPVisit18429853043383154039.xmlvstatus; 1C; BI265; P/COS approved for submission; P/RS 29/08/22 ; intrev: complete ; P/AF 06/10/22
vcheck; Enter targ name & Inst. & Resp. Sci.; BI265 ; COS ; RS
vcheck; ETC numbers entered in APT?; Yes
vcheck; Any screening violations?; No ...
count-rate warning for irregularly variable sources in the c1291 spectral acquisition calculation
vcheck; S/N ETC calcs done & documented?; N/A
vcheck; Field images checked & saved?; Yes
vcheck; Selected ACQ strategy?; Yes spectroscopic acq using G130M/1291 ...
several stars in the field that are too bright for PSA while obtaining imaging acq
vcheck; Possible ACQ or Sci spoilers?; No
vcheck; Field BOT clear?; Yes ...
both the Zaritsky catalog and Gaia show that sources flagged unknown are safe
vcheck; Visual BOT check for stars not in catalog?; Okay
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 = 21682230483000130.0(Tic-Visit
:proposal-id 16816
:visit-id "1C"
:proposal-version -1
:trans-version "20220630"
:date "25-May-2023 09:16:12.0"
: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 1252496
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16816
:visit-id "1C"
:obset-id "1C"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16816
:visit-id "1C"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2573
:al-overhead-at-end 0
:internal-dur-at-end 76
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2970
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16816
:visit-id "1C"
:orbit-number 2
:pcs-time 392
:si-vis-utilization 2578
:al-overhead-at-end 0
:internal-dur-at-end 379
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2970
:pcs-gap 0
)true20Exposure time calculated.Exposure time calculated.rn(PoWR-OB-new(PoWR_40000_3.80_m7.00_Z0.50.fits, lmc-ob-i 40-38, Z=0.500 solar, Teff=40000, log_lum=5.64, log_g=3.80, log_mdot=-7.00) (extinction lmcavg=0.130), flux1160 +- 2.0A flux=7.1e-13 Flam); cos,fuv,g130m,c1096,psa,mjd#59670; fp-pos=None, segment=None)
From file ULLYSES_Cycle29_MassiveStar_ProgramInput_v5.csv
Spectral type: O5 III(fc)
SED = BI265_COS_G130M_c1096_sed.fits
For exptime=2774.1 s, spectral region:
1080.0 +- 0.5 A achieves SNR=20.0/resel
global countrate (brightest segment): 7574.9 cts/s/segment
brightest pixel: 0.153 cts/s/pix at 1220.0 A
Calculation performed 2021-10-25T00:58:01, v0.9rn(PoWR-OB-new(PoWR_40000_3.80_m7.00_Z0.50.fits, lmc-ob-i 40-38, Z=0.500 solar, Teff=40000, log_lum=5.64, log_g=3.80, log_mdot=-7.00) (extinction lmcavg=0.130), flux1160 +- 2.0A flux=7.1e-13 Flam); cos,fuv,g130m,c1096,psa,mjd#59670; fp-pos=None, segment=None)
From file ULLYSES_Cycle29_MassiveStar_ProgramInput_v5.csv
Spectral type: O5 III(fc)
SED = BI265_COS_G130M_c1096_sed.fits
For exptime=2774.1 s, spectral region:
1080.0 +- 0.5 A achieves SNR=20.0/resel
global countrate (brightest segment): 7574.9 cts/s/segment
brightest pixel: 0.153 cts/s/pix at 1220.0 A
Calculation performed 2021-10-25T00:58:01, v0.9rn(PoWR-OB-new(PoWR_40000_3.80_m7.00_Z0.50.fits, lmc-ob-i 40-38, Z=0.500 solar, Teff=40000, log_lum=5.64, log_g=3.80, log_mdot=-7.00) (extinction lmcavg=0.130), flux1160 +- 2.0A flux=7.1e-13 Flam); cos,fuv,g130m,c1096,psa,mjd#59670; fp-pos=None, segment=None)
From file ULLYSES_Cycle29_MassiveStar_ProgramInput_v5.csv
Spectral type: O5 III(fc)
SED = BI265_COS_G130M_c1096_sed.fits
For exptime=2774.1 s, spectral region:
1080.0 +- 0.5 A achieves SNR=20.0/resel
global countrate (brightest segment): 7574.9 cts/s/segment
brightest pixel: 0.153 cts/s/pix at 1220.0 A
Calculation performed 2021-10-25T00:58:01, v0.9rn(PoWR-OB-new(PoWR_40000_3.80_m7.00_Z0.50.fits, lmc-ob-i 40-38, Z=0.500 solar, Teff=40000, log_lum=5.64, log_g=3.80, log_mdot=-7.00) (extinction lmcavg=0.130), flux1160 +- 2.0A flux=7.1e-13 Flam); cos,fuv,g130m,c1096,psa,mjd#59670; fp-pos=None, segment=None)
From file ULLYSES_Cycle29_MassiveStar_ProgramInput_v5.csv
Spectral type: O5 III(fc)
SED = BI265_COS_G130M_c1096_sed.fits
For exptime=2774.1 s, spectral region:
1080.0 +- 0.5 A achieves SNR=20.0/resel
global countrate (brightest segment): 7574.9 cts/s/segment
brightest pixel: 0.153 cts/s/pix at 1220.0 A
Calculation performed 2021-10-25T00:58:01, v0.9The scheduling data was generated by CASM 31.0.CASM was run in Phase II mode./private/var/folders/81/nbsn78xx3tzfyhsmxnp50pk80004gh/T/OPVisit17694548768227723321.xmlvstatus; 1C; BI265; P/COS approved for submission; P/RS 29/08/22 ; intrev: complete ; P/AF 06/10/22
vcheck; Enter targ name & Inst. & Resp. Sci.; BI265 ; COS ; RS
vcheck; ETC numbers entered in APT?; Yes
vcheck; Any screening violations?; No ...
count-rate warning for irregularly variable sources in the c1291 spectral acquisition calculation
vcheck; S/N ETC calcs done & documented?; N/A
vcheck; Field images checked & saved?; Yes
vcheck; Selected ACQ strategy?; Yes spectroscopic acq using G130M/1291 ...
several stars in the field that are too bright for PSA while obtaining imaging acq
vcheck; Possible ACQ or Sci spoilers?; No
vcheck; Field BOT clear?; Yes ...
both the Zaritsky catalog and Gaia show that sources flagged unknown are safe
vcheck; Visual BOT check for stars not in catalog?; Okay
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 = 2
Update May 25,2023 (AF): Visit AC is an exact copy of Visit 1C, as authorized by the TTRB in response to HOPR-92547.(Tic-Visit
:proposal-id 16816
:visit-id "AC"
:proposal-version -1
:trans-version "20220630"
:date "25-May-2023 09:11:56.0"
: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 1252496
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16816
:visit-id "AC"
:obset-id "AC"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16816
:visit-id "AC"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2573
:al-overhead-at-end 0
:internal-dur-at-end 76
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2970
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16816
:visit-id "AC"
:orbit-number 2
:pcs-time 392
:si-vis-utilization 2578
:al-overhead-at-end 0
:internal-dur-at-end 379
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2970
:pcs-gap 0
)true20Exposure time calculated.Exposure time calculated.rn(PoWR-OB-new(PoWR_40000_3.80_m7.00_Z0.50.fits, lmc-ob-i 40-38, Z=0.500 solar, Teff=40000, log_lum=5.64, log_g=3.80, log_mdot=-7.00) (extinction lmcavg=0.130), flux1160 +- 2.0A flux=7.1e-13 Flam); cos,fuv,g130m,c1096,psa,mjd#59670; fp-pos=None, segment=None)
From file ULLYSES_Cycle29_MassiveStar_ProgramInput_v5.csv
Spectral type: O5 III(fc)
SED = BI265_COS_G130M_c1096_sed.fits
For exptime=2774.1 s, spectral region:
1080.0 +- 0.5 A achieves SNR=20.0/resel
global countrate (brightest segment): 7574.9 cts/s/segment
brightest pixel: 0.153 cts/s/pix at 1220.0 A
Calculation performed 2021-10-25T00:58:01, v0.9rn(PoWR-OB-new(PoWR_40000_3.80_m7.00_Z0.50.fits, lmc-ob-i 40-38, Z=0.500 solar, Teff=40000, log_lum=5.64, log_g=3.80, log_mdot=-7.00) (extinction lmcavg=0.130), flux1160 +- 2.0A flux=7.1e-13 Flam); cos,fuv,g130m,c1096,psa,mjd#59670; fp-pos=None, segment=None)
From file ULLYSES_Cycle29_MassiveStar_ProgramInput_v5.csv
Spectral type: O5 III(fc)
SED = BI265_COS_G130M_c1096_sed.fits
For exptime=2774.1 s, spectral region:
1080.0 +- 0.5 A achieves SNR=20.0/resel
global countrate (brightest segment): 7574.9 cts/s/segment
brightest pixel: 0.153 cts/s/pix at 1220.0 A
Calculation performed 2021-10-25T00:58:01, v0.9rn(PoWR-OB-new(PoWR_40000_3.80_m7.00_Z0.50.fits, lmc-ob-i 40-38, Z=0.500 solar, Teff=40000, log_lum=5.64, log_g=3.80, log_mdot=-7.00) (extinction lmcavg=0.130), flux1160 +- 2.0A flux=7.1e-13 Flam); cos,fuv,g130m,c1096,psa,mjd#59670; fp-pos=None, segment=None)
From file ULLYSES_Cycle29_MassiveStar_ProgramInput_v5.csv
Spectral type: O5 III(fc)
SED = BI265_COS_G130M_c1096_sed.fits
For exptime=2774.1 s, spectral region:
1080.0 +- 0.5 A achieves SNR=20.0/resel
global countrate (brightest segment): 7574.9 cts/s/segment
brightest pixel: 0.153 cts/s/pix at 1220.0 A
Calculation performed 2021-10-25T00:58:01, v0.9rn(PoWR-OB-new(PoWR_40000_3.80_m7.00_Z0.50.fits, lmc-ob-i 40-38, Z=0.500 solar, Teff=40000, log_lum=5.64, log_g=3.80, log_mdot=-7.00) (extinction lmcavg=0.130), flux1160 +- 2.0A flux=7.1e-13 Flam); cos,fuv,g130m,c1096,psa,mjd#59670; fp-pos=None, segment=None)
From file ULLYSES_Cycle29_MassiveStar_ProgramInput_v5.csv
Spectral type: O5 III(fc)
SED = BI265_COS_G130M_c1096_sed.fits
For exptime=2774.1 s, spectral region:
1080.0 +- 0.5 A achieves SNR=20.0/resel
global countrate (brightest segment): 7574.9 cts/s/segment
brightest pixel: 0.153 cts/s/pix at 1220.0 A
Calculation performed 2021-10-25T00:58:01, v0.9The scheduling data was generated by CASM 31.0.CASM was run in Phase II mode./private/var/folders/81/nbsn78xx3tzfyhsmxnp50pk80004gh/T/OPVisit6709092565057407467.xmlvstatus; 1D; BI265; P/COS approved for submission; P/RS 29/08/22 ; intrev: complete ; P/AF 06/10/22
vcheck; Enter targ name & Inst. & Resp. Sci.; BI265 ; COS ; RS
vcheck; ETC numbers entered in APT?; Yes
vcheck; Any screening violations?; No ...
count-rate warning for irregularly variable sources in the c1291 spectral acquisition calculation
vcheck; S/N ETC calcs done & documented?; N/A
vcheck; Field images checked & saved?; Yes
vcheck; Selected ACQ strategy?; Yes spectroscopic acq using G130M/1291 ...
several stars in the field that are too bright for PSA while obtaining imaging acq
vcheck; Possible ACQ or Sci spoilers?; No
vcheck; Field BOT clear?; Yes ...
both the Zaritsky catalog and Gaia show that sources flagged unknown are safe
vcheck; Visual BOT check for stars not in catalog?; Okay
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 = 2
7/3/23 AF: Visit 1D provides 1 orbit of additional exposure time with the COS G130M/1096 configuration. To implement Visit 1D:
- the dispersed light target acquisition from Visit 1C was copied "as is"
- the exposure time for FP-POS=ALL was adjusted to fit the single-orbit allocation: 413 s per FP-POS. A re-optimized value of the buffer time was found to be 272 s.1684300305000150.32467149438878(Tic-Visit
:proposal-id 16816
:visit-id "1D"
:proposal-version -1
:trans-version "20220630"
:date "25-May-2023 09:16:16.0"
: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 487152
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16816
:visit-id "1D"
:obset-id "1D"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16816
:visit-id "1D"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2577
:al-overhead-at-end 0
:internal-dur-at-end 388
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2970
:pcs-gap 0
)true10Exposure time calculated.Exposure time calculated.rn(PoWR-OB-new(PoWR_40000_3.80_m7.00_Z0.50.fits, lmc-ob-i 40-38, Z=0.500 solar, Teff=40000, log_lum=5.64, log_g=3.80, log_mdot=-7.00) (extinction lmcavg=0.130), flux1160 +- 2.0A flux=7.1e-13 Flam); cos,fuv,g130m,c1096,psa,mjd#59670; fp-pos=None, segment=None)
From file ULLYSES_Cycle29_MassiveStar_ProgramInput_v5.csv
Spectral type: O5 III(fc)
SED = BI265_COS_G130M_c1096_sed.fits
For exptime=2774.1 s, spectral region:
1080.0 +- 0.5 A achieves SNR=20.0/resel
global countrate (brightest segment): 7574.9 cts/s/segment
brightest pixel: 0.153 cts/s/pix at 1220.0 A
Calculation performed 2021-10-25T00:58:01, v0.9The scheduling data was generated by CASM 31.0.CASM was run in Phase II mode./private/var/folders/81/nbsn78xx3tzfyhsmxnp50pk80004gh/T/OPVisit6235205417072529016.xmlvstatus; 2C; SK-69D212; P/COS approved for submission; P/RS 29/08/22 ; intrev: complete ; P/AF 06/10/22
vcheck; Enter targ name & Inst. & Resp. Sci.; SK-69D212 ; COS ; RS
vcheck; ETC numbers entered in APT?; Yes
vcheck; Any screening violations?; No ...
count-rate warning for irregularly variable sources in the c1291 spectral acquisition calculation
vcheck; S/N ETC calcs done & documented?; N/A
vcheck; Field images checked & saved?; Yes
vcheck; Selected ACQ strategy?; Yes spectroscopic acq with G130M/1291 ...
several stars in the field that would be too bright for PSA if imaging acq is used
vcheck; Possible ACQ or Sci spoilers?; No
vcheck; Field BOT clear?; Yes ...
there are a few bright stars within 8 arcsec of the target, one is a known O7V star [ST-92]2-51 which is about 4.65 arcsec away and has V=14.9 ...
there is another uncataloged star at about the same distance and same V mag, these two stars are 5 and 7 in gaiaBOT ...
even under the assumption that these are O5V stars the countrates are below the bright-object limit for the modes being used (COS.sp.1821390 and 1821391)
vcheck; Visual BOT check for stars not in catalog?; Okay
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 = 2(Tic-Visit
:proposal-id 16816
:visit-id "2C"
:proposal-version -1
:trans-version "20220630"
:date "25-May-2023 09:16:19.0"
: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 1235120
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16816
:visit-id "2C"
:obset-id "2C"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16816
:visit-id "2C"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2576
: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 2970
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16816
:visit-id "2C"
:orbit-number 2
:pcs-time 392
:si-vis-utilization 2578
:al-overhead-at-end 0
:internal-dur-at-end 379
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2970
:pcs-gap 0
)true20Exposure time calculated.Exposure time calculated.rn(PoWR-OB-new(PoWR_39000_3.80_m7.00_Z0.50.fits, lmc-ob-i 39-38, Z=0.500 solar, Teff=39000, log_lum=5.54, log_g=3.80, log_mdot=-7.00) (extinction lmcavg=0.230), flux1160 +- 2.0A flux=5.5e-13 Flam); cos,fuv,g130m,c1096,psa,mjd#59670; fp-pos=None, segment=None)
From file ULLYSES_Cycle29_MassiveStar_ProgramInput_v5.csv
Spectral type: O5 In(f)p
SED = SK-69D212_COS_G130M_c1096_sed.fits
For exptime=4240.5 s, spectral region:
1080.0 +- 0.5 A achieves SNR=20.0/resel
global countrate (brightest segment): 6007.9 cts/s/segment
brightest pixel: 0.132 cts/s/pix at 1226.5 A
Calculation performed 2021-10-25T00:57:43, v0.9rn(PoWR-OB-new(PoWR_39000_3.80_m7.00_Z0.50.fits, lmc-ob-i 39-38, Z=0.500 solar, Teff=39000, log_lum=5.54, log_g=3.80, log_mdot=-7.00) (extinction lmcavg=0.230), flux1160 +- 2.0A flux=5.5e-13 Flam); cos,fuv,g130m,c1096,psa,mjd#59670; fp-pos=None, segment=None)
From file ULLYSES_Cycle29_MassiveStar_ProgramInput_v5.csv
Spectral type: O5 In(f)p
SED = SK-69D212_COS_G130M_c1096_sed.fits
For exptime=4240.5 s, spectral region:
1080.0 +- 0.5 A achieves SNR=20.0/resel
global countrate (brightest segment): 6007.9 cts/s/segment
brightest pixel: 0.132 cts/s/pix at 1226.5 A
Calculation performed 2021-10-25T00:57:43, v0.9rn(PoWR-OB-new(PoWR_39000_3.80_m7.00_Z0.50.fits, lmc-ob-i 39-38, Z=0.500 solar, Teff=39000, log_lum=5.54, log_g=3.80, log_mdot=-7.00) (extinction lmcavg=0.230), flux1160 +- 2.0A flux=5.5e-13 Flam); cos,fuv,g130m,c1096,psa,mjd#59670; fp-pos=None, segment=None)
From file ULLYSES_Cycle29_MassiveStar_ProgramInput_v5.csv
Spectral type: O5 In(f)p
SED = SK-69D212_COS_G130M_c1096_sed.fits
For exptime=4240.5 s, spectral region:
1080.0 +- 0.5 A achieves SNR=20.0/resel
global countrate (brightest segment): 6007.9 cts/s/segment
brightest pixel: 0.132 cts/s/pix at 1226.5 A
Calculation performed 2021-10-25T00:57:43, v0.9rn(PoWR-OB-new(PoWR_39000_3.80_m7.00_Z0.50.fits, lmc-ob-i 39-38, Z=0.500 solar, Teff=39000, log_lum=5.54, log_g=3.80, log_mdot=-7.00) (extinction lmcavg=0.230), flux1160 +- 2.0A flux=5.5e-13 Flam); cos,fuv,g130m,c1096,psa,mjd#59670; fp-pos=None, segment=None)
From file ULLYSES_Cycle29_MassiveStar_ProgramInput_v5.csv
Spectral type: O5 In(f)p
SED = SK-69D212_COS_G130M_c1096_sed.fits
For exptime=4240.5 s, spectral region:
1080.0 +- 0.5 A achieves SNR=20.0/resel
global countrate (brightest segment): 6007.9 cts/s/segment
brightest pixel: 0.132 cts/s/pix at 1226.5 A
Calculation performed 2021-10-25T00:57:43, v0.9The scheduling data was generated by CASM 31.0.CASM was run in Phase II mode./private/var/folders/81/nbsn78xx3tzfyhsmxnp50pk80004gh/T/OPVisit315052655915599141.xmlvstatus; 2D; SK-69D212; P/COS approved for submission; P/RS 29/08/22 ; intrev: complete ; P/AF 06/10/22
vcheck; Enter targ name & Inst. & Resp. Sci.; SK-69D212 ; COS ; RS
vcheck; ETC numbers entered in APT?; Yes
vcheck; Any screening violations?; No ...
count-rate warning for irregularly variable sources in the c1291 spectral acquisition calculation
vcheck; S/N ETC calcs done & documented?; N/A
vcheck; Field images checked & saved?; Yes
vcheck; Selected ACQ strategy?; Yes spectroscopic acq with G130M/1291 ...
several stars in the field that would be too bright for PSA if imaging acq is used
vcheck; Possible ACQ or Sci spoilers?; No
vcheck; Field BOT clear?; Yes ...
there are a few bright stars within 8 arcsec of the target, one is a known O7V star [ST-92]2-51 which is about 4.65 arcsec away and has V=14.9 ...
there is another uncataloged star at about the same distance and same V mag, these two stars are 5 and 7 in gaiaBOT ...
even under the assumption that these are O5V stars the countrates are below the bright-object limit for the modes being used (COS.sp.1821390 and 1821391)
vcheck; Visual BOT check for stars not in catalog?; Okay
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 = 2
7/3/23 AF: Visit 2D provides 1 orbit of additional exposure time with the COS G130M/1096 configuration. To implement Visit 2D:
- the dispersed light target acquisition from Visit 2C was copied "as is"
- the exposure time for FP-POS=ALL was adjusted to fit the single-orbit allocation: 419 s per FP-POS. A re-optimized value of the buffer time was found to be 309 s.1684893082000157.84984060780943(Tic-Visit
:proposal-id 16816
:visit-id "2D"
:proposal-version -1
:trans-version "20220630"
:date "25-May-2023 09:16:22.0"
: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 452400
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16816
:visit-id "2D"
:obset-id "2D"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16816
:visit-id "2D"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2574
:al-overhead-at-end 0
:internal-dur-at-end 379
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2970
:pcs-gap 0
)true10Exposure time calculated.Exposure time calculated.rn(PoWR-OB-new(PoWR_39000_3.80_m7.00_Z0.50.fits, lmc-ob-i 39-38, Z=0.500 solar, Teff=39000, log_lum=5.54, log_g=3.80, log_mdot=-7.00) (extinction lmcavg=0.230), flux1160 +- 2.0A flux=5.5e-13 Flam); cos,fuv,g130m,c1096,psa,mjd#59670; fp-pos=None, segment=None)
From file ULLYSES_Cycle29_MassiveStar_ProgramInput_v5.csv
Spectral type: O5 In(f)p
SED = SK-69D212_COS_G130M_c1096_sed.fits
For exptime=4240.5 s, spectral region:
1080.0 +- 0.5 A achieves SNR=20.0/resel
global countrate (brightest segment): 6007.9 cts/s/segment
brightest pixel: 0.132 cts/s/pix at 1226.5 A
Calculation performed 2021-10-25T00:57:43, v0.9The scheduling data was generated by CASM 31.0.CASM was run in Phase II mode./private/var/folders/81/nbsn78xx3tzfyhsmxnp50pk80004gh/T/OPVisit6260615866827919037.xmlvstatus; 3C; VFTS-244; P/COS approved for submission; P/RS 29/08/22 ; intrev: complete ; P/AF 06/10/22
vcheck; Enter targ name & Inst. & Resp. Sci.; VFTS-244 ; 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 spectroscopic acq with G130M/1291 ...
several stars in the field that would be too bright for PSA if imaging acq is used
vcheck; Possible ACQ or Sci spoilers?; No
vcheck; Field BOT clear?; Yes
vcheck; Visual BOT check for stars not in catalog?; Yes okay
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 = 21685321061000162.1329553843591(Tic-Visit
:proposal-id 16816
:visit-id "3C"
:proposal-version -1
:trans-version "20220630"
:date "25-May-2023 09:16:26.0"
: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 782896
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16816
:visit-id "3C"
:obset-id "3C"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16816
:visit-id "3C"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2577
:al-overhead-at-end 0
:internal-dur-at-end 57
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2970
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16816
:visit-id "3C"
:orbit-number 2
:pcs-time 392
:si-vis-utilization 2578
:al-overhead-at-end 0
:internal-dur-at-end 369
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2970
:pcs-gap 0
)true20Exposure time calculated.Exposure time calculated.rn(PoWR-OB-new(PoWR_41000_3.80_m7.00_Z0.50.fits, lmc-ob-i 41-38, Z=0.500 solar, Teff=41000, log_lum=5.73, log_g=3.80, log_mdot=-7.00) (extinction lmc30dor=0.180), flux1360 +- 2.0A flux=1e-13 Flam); cos,fuv,g130m,c1291,psa,mjd#59670; fp-pos=None, segment=None)
From file ULLYSES_Cycle29_MassiveStar_ProgramInput_v5.csv
Spectral type: O5 III(n)(fc)
SED = VFTS-244_COS_G130M_c1291_sed.fits
For exptime=1590.5 s, spectral region:
1150.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 2083.6 cts/s/segment
brightest pixel: 0.046 cts/s/pix at 1243.5 A
Calculation performed 2021-10-25T00:57:49, v0.9rn(PoWR-OB-new(PoWR_41000_3.80_m7.00_Z0.50.fits, lmc-ob-i 41-38, Z=0.500 solar, Teff=41000, log_lum=5.73, log_g=3.80, log_mdot=-7.00) (extinction lmc30dor=0.180), flux1360 +- 2.0A flux=1e-13 Flam); cos,fuv,g130m,c1291,psa,mjd#59670; fp-pos=None, segment=None)
From file ULLYSES_Cycle29_MassiveStar_ProgramInput_v5.csv
Spectral type: O5 III(n)(fc)
SED = VFTS-244_COS_G130M_c1291_sed.fits
For exptime=1590.5 s, spectral region:
1150.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 2083.6 cts/s/segment
brightest pixel: 0.046 cts/s/pix at 1243.5 A
Calculation performed 2021-10-25T00:57:49, v0.9rn(PoWR-OB-new(PoWR_41000_3.80_m7.00_Z0.50.fits, lmc-ob-i 41-38, Z=0.500 solar, Teff=41000, log_lum=5.73, log_g=3.80, log_mdot=-7.00) (extinction lmc30dor=0.180), flux1700 +- 2.0A flux=1e-13 Flam); cos,fuv,g160m,c1611,psa,mjd#59670; fp-pos=None, segment=None)
From file ULLYSES_Cycle29_MassiveStar_ProgramInput_v5.csv
Spectral type: O5 III(n)(fc)
SED = VFTS-244_COS_G160M_c1611_sed.fits
For exptime=2058.0 s, spectral region:
1590.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 1631.7 cts/s/segment
brightest pixel: 0.027 cts/s/pix at 1423.5 A
Calculation performed 2021-10-25T00:57:51, v0.9