Duplicated failed visit 1C, relabeled it AC for the first repeat. Ref: HOPR 91881
Changed 1C to AC in visit status line642952065----- Attempting Submission 1 (Tue Jul 14 15:22:55 GMT 2020) -----
Your proposal could not be saved.
Submission aborted.
----- Attempting Submission 2 (Wed Dec 16 23:40:38 GMT 2020) -----
----- Attempting Submission 3 (Thu Dec 17 18:58:48 GMT 2020) -----ULLYSES SMC B1 Stars COSThe Space Telescope Science Institute (STScI) Director has decided to devote up to 1000 orbits of Director's Discretionary time in observing Cycles 27-29 to a new Hubble Ultraviolet Legacy program focused on star formation and associated stellar physics. This new program, ULLYSES (UV Legacy Library of Young Stars as Essential Standards), will provide a UV spectroscopic reference sample of young (< 10 Myr) high- and low-mass stars. It will target over ~150 OB stars in the Magellanic Clouds and lower metallicity galaxies in the Local Group, and ~40 T Tauri stars and brown dwarfs in the Milky Way. In addition, ULLYSES will monitor 4 typical T Tauri stars over different rotational phases through at least three rotation periods, and over timescales of months to years. The resulting library will provide template spectra of massive stars at metallicities substantially below the well studied, while the low mass sample will cover a wide range of ages, accretion rates, and masses, including objects down to well below 0.5 M_sun. The legacy of this large UV dataset on the first 10 Myr of stellar evolution will be enhanced by complementary datasets obtained by the scientific community. In addition to the core goals of the program related to stellar astrophysics of low and high mass stars, this data will also enable exciting science in the fields of ISM, CGM, jets, and exoplanets. ULLYSES will be modeled after the Frontier Fields program: all data obtained will be non-proprietary. The implementation team at STScI is developing high-level science data products and a sophisticated database and website for disseminating data from the ULLYSES program and ancillary datasets for the ULLYSES target sample from space and ground-based facilities.This proposal includes a subset of the massive ULLYSES stars being observed in the Magellanic clouds.
Depending on target brightness, the main FUV spectral range will generally use either the STIS E140M setting or the combination of the COS c1291 + c1611 settings. Sufficiently bright stars without good FUSE data in the archive will also be observed with the COS c1096 setting to provide coverage at shorter wavelengths. Where time permits, stars of type O9 or later will also be observed with STIS E230M/1978, while for supergiants of spectral type B5 or later E230M/2707 may also be included. Where possible, targets of a given spectral type were selected to span both a range in extinction and in rotation rates to support a variety of stellar and ISM studies.
Signal-to-noise requirements used to determine the desired exposures times were defined as follows:
COS/G130M/c1096: 20 / nine-pixel resel at 1080 A
COS/G130M/c1291: 30 / six-pixel resel at 1150 A
COS/G160M/c1611: 30 / six-pixel resel at 1590 A
COS/G185M/c1953: 30 / three-pixel resel at 1860 A
COS/G185M/c1986: 30 / three-pixel resel at 1980 A
STIS/E140M/c1425: 20 / two-pixel resel at 1200 A
STIS/E230M/c1978: 20 / two-pixel resel at 1800 A
STIS/E230M/c2707: 20 / two-pixel resel at 2800 A
The actual implemented exposure times may be adjusted to efficiently use HST orbits, but should always provide at least 80% of the desired time as defined by the above requirements.
Additional details about the scientific motivation and technical implementation strategy of the ULLYSES observations can be found at http://www.stsci.edu/stsci-research/research-topics-and-programs/ullyses. The ULLYSES program is based on the recommendations of a working group led by Sally Oey; the full text of that group's report can be found at http://www.stsci.edu/files/live/sites/www/files/home/stsci-research/research-topics-and-programs/ullyses/_documents/HSTUV-report-ULLYSES.pdf.0falseSUPPORTEDEXT-STARB0-B2 V-IVNO2DFS-3694 : [2dFS]-3694, [2dFS]_3694, 2dFS 3694
Previous name : [2dFS]-3694
Input file: SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
SIMBAD link (2dFS 3694): https://simbad.u-strasbg.fr/simbad/sim-id?Ident=2dFS+3694&submit=submit+id
SpT = B1 IV
COS/G130M/c1096 : rn(WM-Basic(B1 V, Z=0.004, Teff=26303, log_lum=4.45, log_g=4.00) (extinction smcbar=0.070), johnson U mag=12.800 vegamag)
COS/G130M/c1291 : rn(WM-Basic(B1 V, Z=0.004, Teff=26303, log_lum=4.45, log_g=4.00) (extinction smcbar=0.070), johnson U mag=12.800 vegamag)
COS/G160M/c1611 : rn(WM-Basic(B1 V, Z=0.004, Teff=26303, log_lum=4.45, log_g=4.00) (extinction smcbar=0.070), johnson U mag=12.800 vegamag)
COS/G185M/c1921 : rn(WM-Basic(B1 V, Z=0.004, Teff=26303, log_lum=4.45, log_g=4.00) (extinction smcbar=0.070), johnson U mag=12.800 vegamag)
COS/G185M/c1953 : rn(WM-Basic(B1 V, Z=0.004, Teff=26303, log_lum=4.45, log_g=4.00) (extinction smcbar=0.070), johnson U mag=12.800 vegamag)
COS/G185M/c1986 : rn(WM-Basic(B1 V, Z=0.004, Teff=26303, log_lum=4.45, log_g=4.00) (extinction smcbar=0.070), johnson U mag=12.800 vegamag)
STIS/E140M/c1425 : rn(WM-Basic(B1 V, Z=0.004, Teff=26303, log_lum=4.45, log_g=4.00) (extinction smcbar=0.070), johnson U mag=12.800 vegamag)
STIS/E230M/c1978 : rn(WM-Basic(B1 V, Z=0.004, Teff=26303, log_lum=4.45, log_g=4.00) (extinction smcbar=0.070), johnson U mag=12.800 vegamag)
STIS/E230M/c2707 : rn(WM-Basic(B1 V, Z=0.004, Teff=26303, log_lum=4.45, log_g=4.00) (extinction smcbar=0.070), johnson U mag=12.800 vegamag)
Coordinate pedigree: Gaia
v sin i = 120
Calculation performed 2020-02-24T17:51:02, v0.4
-------------------------------------------------------------------------------
tstatus; 2DFS-3694; P/COS Approved for submission ; S/ins not started; P/RS 28/06/20; S/xx DD/MM/YY
tcheck; APT/SIMBAD target names: ; 2DFS-3694, 2dFS 3694, [M2002] SMC 81522
tcheck; Target info verification status?; Verified
tcheck; Coordinates & P.M. updated?; Updated, GAIA DR2
tcheck; Adopted SED compared to Observations?; OK - No FUV data, matches photometryJ2000SpT=B1 IV; E(B-V)=0.07; U=12.8; B=13.7; V=13.9EXT-STARB0-B2 III-INOAV175 : [M2002]_37732, AV 175, AzV 175
Previous name : AV 175
Input file: SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
SIMBAD link (AzV 175): https://simbad.u-strasbg.fr/simbad/sim-id?Ident=AzV+175&submit=submit+id
SpT = B1 IIW
COS/G130M/c1096 : rn-max(WM-Basic(B0.5 I, Z=0.004, Teff=24547, log_lum=5.40, log_g=2.95) (extinction smcbar=0.160), flux1160 +- 30.0A flux=1.1e-13 Flam)
COS/G130M/c1291 : rn-max(WM-Basic(B0.5 I, Z=0.004, Teff=24547, log_lum=5.40, log_g=2.95) (extinction smcbar=0.160), flux1360 +- 30.0A flux=1.4e-13 Flam)
COS/G160M/c1611 : rn-max(WM-Basic(B0.5 I, Z=0.004, Teff=24547, log_lum=5.40, log_g=2.95) (extinction smcbar=0.160), flux1700 +- 5.0A flux=1.2e-13 Flam)
COS/G185M/c1921 : rn-max(WM-Basic(B0.5 I, Z=0.004, Teff=24547, log_lum=5.40, log_g=2.95) (extinction smcbar=0.160), flux1700 +- 5.0A flux=1.2e-13 Flam)
COS/G185M/c1953 : rn-max(WM-Basic(B0.5 I, Z=0.004, Teff=24547, log_lum=5.40, log_g=2.95) (extinction smcbar=0.160), flux1700 +- 5.0A flux=1.2e-13 Flam)
COS/G185M/c1986 : rn-max(WM-Basic(B0.5 I, Z=0.004, Teff=24547, log_lum=5.40, log_g=2.95) (extinction smcbar=0.160), flux2200 +- 5.0A flux=7.8e-14 Flam)
STIS/E140M/c1425 : rn-max(WM-Basic(B0.5 I, Z=0.004, Teff=24547, log_lum=5.40, log_g=2.95) (extinction smcbar=0.160), flux1360 +- 30.0A flux=1.4e-13 Flam)
STIS/E230M/c1978 : rn-max(WM-Basic(B0.5 I, Z=0.004, Teff=24547, log_lum=5.40, log_g=2.95) (extinction smcbar=0.160), flux2200 +- 5.0A flux=7.8e-14 Flam)
STIS/E230M/c2707 : rn-max(WM-Basic(B0.5 I, Z=0.004, Teff=24547, log_lum=5.40, log_g=2.95) (extinction smcbar=0.160), flux2200 +- 5.0A flux=7.8e-14 Flam)
Coordinate pedigree: Gaia
v sin i = 51
Calculation performed 2020-02-24T17:50:02, v0.4
-------------------------------------------------------------------------------
tstatus; AV175; P/COS Approved for submission; S/ins not started; P/RS 28/06/20; S/xx DD/MM/YY
tcheck; APT/SIMBAD target names: ; AV175, AzV 175, SK 64
tcheck; Target info verification status?; Verified
tcheck; Coordinates & P.M. updated?; Updated, GAIA DR2
tcheck; Adopted SED compared to Observations?; OK, in the sense no brightness issues ...
However, the 1291 SED overestimates the IUE flux longward of 1500A while the 1611 SED underestimates the flux shortward of 1500A (by a factor of around 1.5). It is probably fine to use the 1611 SED, since if the target is brighter we will achieve higher signal.AZV-175M2002-37732J2000SpT=B1 IIW; E(B-V)=0.16; U=12.6; B=13.4; V=13.5; F1160=1.11e-13; F1360=1.38e-13; F1700=1.16e-13; F2200=7.78e-14EXT-STARB0-B2 III-INOAV224 : [M2002]_45809, AV 224, AzV 224
Previous name : AV 224
Input file: SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
SIMBAD link (AzV 224): https://simbad.u-strasbg.fr/simbad/sim-id?Ident=AzV+224&submit=submit+id
SpT = B1 III
COS/G130M/c1096 : rn(WM-Basic(B1 III, Z=0.004, Teff=24547, log_lum=4.80, log_g=3.47) (extinction smcbar=0.110), johnson U mag=13.020 vegamag)
COS/G130M/c1291 : rn(WM-Basic(B1 III, Z=0.004, Teff=24547, log_lum=4.80, log_g=3.47) (extinction smcbar=0.110), johnson U mag=13.020 vegamag)
COS/G160M/c1611 : rn(WM-Basic(B1 III, Z=0.004, Teff=24547, log_lum=4.80, log_g=3.47) (extinction smcbar=0.110), johnson U mag=13.020 vegamag)
COS/G185M/c1921 : rn(WM-Basic(B1 III, Z=0.004, Teff=24547, log_lum=4.80, log_g=3.47) (extinction smcbar=0.110), johnson U mag=13.020 vegamag)
COS/G185M/c1953 : rn(WM-Basic(B1 III, Z=0.004, Teff=24547, log_lum=4.80, log_g=3.47) (extinction smcbar=0.110), johnson U mag=13.020 vegamag)
COS/G185M/c1986 : rn(WM-Basic(B1 III, Z=0.004, Teff=24547, log_lum=4.80, log_g=3.47) (extinction smcbar=0.110), johnson U mag=13.020 vegamag)
STIS/E140M/c1425 : rn(WM-Basic(B1 III, Z=0.004, Teff=24547, log_lum=4.80, log_g=3.47) (extinction smcbar=0.110), johnson U mag=13.020 vegamag)
STIS/E230M/c1978 : rn(WM-Basic(B1 III, Z=0.004, Teff=24547, log_lum=4.80, log_g=3.47) (extinction smcbar=0.110), johnson U mag=13.020 vegamag)
STIS/E230M/c2707 : rn(WM-Basic(B1 III, Z=0.004, Teff=24547, log_lum=4.80, log_g=3.47) (extinction smcbar=0.110), johnson U mag=13.020 vegamag)
Coordinate pedigree: Gaia
v sin i = 299
Calculation performed 2020-02-24T17:50:47, v0.4
-------------------------------------------------------------------------------
tstatus; AV224; P/COS Approved for submission ; S/ins not started; P/RS 28/06/20; S/xx DD/MM/YY
tcheck; APT/SIMBAD target names: ; AV224, AzV 224
tcheck; Target info verification status?; Verified...
SIMBAD gives target type as B1e and Vmag 14.21
tcheck; Coordinates & P.M. updated?; Updated, GAIA DR2
tcheck; Adopted SED compared to Observations?; OK - No FUV data, matches photometryM2002-45809AV-224J2000SpT=B1 III; E(B-V)=0.11; U=13.0; B=14.0; V=14.1EXT-STARB0-B2 V-IVNONGC346-ELS-35 : NGC 346-035, NGC346_35, Cl* NGC 346 ELS 035
Previous name : NGC 346-035
Input file: SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
SIMBAD link (Cl* NGC 346 ELS 035): https://simbad.u-strasbg.fr/simbad/sim-id?Ident=Cl*+NGC+346+ELS+035&submit=submit+id
SpT = B1 V
COS/G130M/c1096 : rn(WM-Basic(B1 V, Z=0.004, Teff=26303, log_lum=4.45, log_g=4.00) (extinction smcbar=0.030), johnson B mag=14.860 vegamag)
COS/G130M/c1291 : rn(WM-Basic(B1 V, Z=0.004, Teff=26303, log_lum=4.45, log_g=4.00) (extinction smcbar=0.030), johnson B mag=14.860 vegamag)
COS/G160M/c1611 : rn(WM-Basic(B1 V, Z=0.004, Teff=26303, log_lum=4.45, log_g=4.00) (extinction smcbar=0.030), johnson B mag=14.860 vegamag)
COS/G185M/c1921 : rn(WM-Basic(B1 V, Z=0.004, Teff=26303, log_lum=4.45, log_g=4.00) (extinction smcbar=0.030), johnson B mag=14.860 vegamag)
COS/G185M/c1953 : rn(WM-Basic(B1 V, Z=0.004, Teff=26303, log_lum=4.45, log_g=4.00) (extinction smcbar=0.030), johnson B mag=14.860 vegamag)
COS/G185M/c1986 : rn(WM-Basic(B1 V, Z=0.004, Teff=26303, log_lum=4.45, log_g=4.00) (extinction smcbar=0.030), johnson B mag=14.860 vegamag)
STIS/E140M/c1425 : rn(WM-Basic(B1 V, Z=0.004, Teff=26303, log_lum=4.45, log_g=4.00) (extinction smcbar=0.030), johnson B mag=14.860 vegamag)
STIS/E230M/c1978 : rn(WM-Basic(B1 V, Z=0.004, Teff=26303, log_lum=4.45, log_g=4.00) (extinction smcbar=0.030), johnson B mag=14.860 vegamag)
STIS/E230M/c2707 : rn(WM-Basic(B1 V, Z=0.004, Teff=26303, log_lum=4.45, log_g=4.00) (extinction smcbar=0.030), johnson B mag=14.860 vegamag)
Coordinate pedigree: Gaia
v sin i = 145
Calculation performed 2020-02-24T17:51:45, v0.4
-------------------------------------------------------------------------------
tstatus; NGC346-ELS-35; P/COS Approved for submission ; S/ins not started; P/RS 28/06/20; S/xx DD/MM/YY
tcheck; APT/SIMBAD target names: ; NGC346-ELS-35, OGLE SMC108.3 14382, 2dFS 1418
tcheck; Target info verification status?; Verified
tcheck; Coordinates & P.M. updated?; Yes, GAIA DR2
tcheck; Adopted SED compared to Observations?; OK - No FUV data, matches photometryCL-NGC-346-ELS-035NGC-346-035J2000SpT=B1 V; E(B-V)=0.03; B=14.9; V=15.1EXT-STARB0-B2 III-IBENOSK173 : [2dFS]-3747, [2dFS]_3747, 2dFS 3747
Previous name : [2dFS]-3747
Input file: SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
SIMBAD link (2dFS 3747): https://simbad.u-strasbg.fr/simbad/sim-id?Ident=2dFS+3747&submit=submit+id
SpT = B0.7 (II)e
COS/G130M/c1096 : rn(WM-Basic(B0.5 I, Z=0.004, Teff=24547, log_lum=5.40, log_g=2.95) (extinction smcbar=0.070), johnson U mag=12.440 vegamag)
COS/G130M/c1291 : rn(WM-Basic(B0.5 I, Z=0.004, Teff=24547, log_lum=5.40, log_g=2.95) (extinction smcbar=0.070), johnson U mag=12.440 vegamag)
COS/G160M/c1611 : rn(WM-Basic(B0.5 I, Z=0.004, Teff=24547, log_lum=5.40, log_g=2.95) (extinction smcbar=0.070), johnson U mag=12.440 vegamag)
COS/G185M/c1921 : rn(WM-Basic(B0.5 I, Z=0.004, Teff=24547, log_lum=5.40, log_g=2.95) (extinction smcbar=0.070), johnson U mag=12.440 vegamag)
COS/G185M/c1953 : rn(WM-Basic(B0.5 I, Z=0.004, Teff=24547, log_lum=5.40, log_g=2.95) (extinction smcbar=0.070), johnson U mag=12.440 vegamag)
COS/G185M/c1986 : rn(WM-Basic(B0.5 I, Z=0.004, Teff=24547, log_lum=5.40, log_g=2.95) (extinction smcbar=0.070), johnson U mag=12.440 vegamag)
STIS/E140M/c1425 : rn(WM-Basic(B0.5 I, Z=0.004, Teff=24547, log_lum=5.40, log_g=2.95) (extinction smcbar=0.070), johnson U mag=12.440 vegamag)
STIS/E230M/c1978 : rn(WM-Basic(B0.5 I, Z=0.004, Teff=24547, log_lum=5.40, log_g=2.95) (extinction smcbar=0.070), johnson U mag=12.440 vegamag)
STIS/E230M/c2707 : rn(WM-Basic(B0.5 I, Z=0.004, Teff=24547, log_lum=5.40, log_g=2.95) (extinction smcbar=0.070), johnson U mag=12.440 vegamag)
Coordinate pedigree: Gaia
Calculation performed 2020-02-24T17:49:10, v0.4
-------------------------------------------------------------------------------
tstatus; SK173; P/COS Approved for submission ; S/ins not started; P/RS 28/06/20; S/xx DD/MM/YY
tcheck; APT/SIMBAD target names: ; SK173, 2dFS 3747
tcheck; Target info verification status?; Verified ...
SIMBAD gives spectral type as B1-2(Ib)e? however with quality D
tcheck; Coordinates & P.M. updated?; Updated, GAIA DR2
tcheck; Adopted SED compared to Observations?; OK - No FUV data, matches photometry2DFS-3747J2000SpT=B0.7 (II)e; E(B-V)=0.07; U=12.4; B=13.4; V=13.6The scheduling data was generated by CASM 28.2.CASM was run in Phase II mode.vstatus; 1C; 2DFS-3694; P/COS Approved for submission; P/RS 04/07/20 ; intrev: complete ; COS/CP 13/07/20
vcheck; Enter targ name & Inst. & Resp. Sci.; 2DFS-3694 ; 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?; COS G130M/1291 PSA Spectroscopic ACQ 1 s ...
Imaging ACQ would need BOA, and be complicated by bright star in the field violating PSA health and safety.
vcheck; Possible ACQ or Sci spoilers?; No
vcheck; Field BOT clear?; Yes; 7 safe field sources reported. ...
The target itself is listed as posing a safety issue for c1291 observations, but that is due to the assumption of an O5V source.
Examination of the field, and the catalogs of Massey et al. (2002), Evans (2004) the 2dFS catalog, and Ramachandran et al. (2019) indicate that there is one other B0 star in the BOA macroaperture with a visual magnitude 0f 16.48.
vcheck; Visual BOT check for stars not in catalog?; OK
vcheck; Orbit packing finalized?; Done
vcheck; Buffer times optimized?; Done
vcheck; Verify visit grouping correct; None needed
vcheck; Is visit ready for int. review?; Yes
Allocated COS orbits = 21597431436000294.0(Tic-Visit
:proposal-id 16101
:visit-id "1C"
:proposal-version -1
:trans-version "20200518"
:date "13-Jul-2020 14:54:42.0"
: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 1304720
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16101
:visit-id "1C"
:obset-id "1C"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16101
:visit-id "1C"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2596
:al-overhead-at-end 0
:internal-dur-at-end 105
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2989
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16101
:visit-id "1C"
:orbit-number 2
:pcs-time 392
:si-vis-utilization 2597
:al-overhead-at-end 0
:internal-dur-at-end 360
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2989
:pcs-gap 0
)true20rn(WM-Basic(B1 V, Z=0.004, Teff=26303, log_lum=4.45, log_g=4.00) (extinction smcbar=0.070), johnson U mag=12.800 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: B1 IV --> B1 V
SED = 2DFS-3694_COS_G130M_c1291_sed.fits
For exptime=887.3 s, spectral region:
1150.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 4562.4 cts/s/segment
brightest pixel: 0.072 cts/s/pix at 1265.0 A
Calculation performed 2020-02-24T17:51:06, v0.4rn(WM-Basic(B1 V, Z=0.004, Teff=26303, log_lum=4.45, log_g=4.00) (extinction smcbar=0.070), johnson U mag=12.800 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: B1 IV --> B1 V
SED = 2DFS-3694_COS_G130M_c1291_sed.fits
For exptime=887.3 s, spectral region:
1150.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 4562.4 cts/s/segment
brightest pixel: 0.072 cts/s/pix at 1265.0 A
Calculation performed 2020-02-24T17:51:06, v0.4rn(WM-Basic(B1 V, Z=0.004, Teff=26303, log_lum=4.45, log_g=4.00) (extinction smcbar=0.070), johnson U mag=12.800 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: B1 IV --> B1 V
SED = 2DFS-3694_COS_G160M_c1611_sed.fits
For exptime=1362.8 s, spectral region:
1590.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 2745.5 cts/s/segment
brightest pixel: 0.046 cts/s/pix at 1435.0 A
Calculation performed 2020-02-24T17:51:09, v0.4rn(WM-Basic(B1 V, Z=0.004, Teff=26303, log_lum=4.45, log_g=4.00) (extinction smcbar=0.070), johnson U mag=12.800 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: B1 IV --> B1 V
SED = 2DFS-3694_COS_G160M_c1611_sed.fits
For exptime=1362.8 s, spectral region:
1590.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 2745.5 cts/s/segment
brightest pixel: 0.046 cts/s/pix at 1435.0 A
Calculation performed 2020-02-24T17:51:09, v0.4The scheduling data was generated by CASM 28.2.CASM was run in Phase II mode./private/var/folders/s6/sm4z5cyx5qg9425w4_w30knw0001d1/T/OPVisit5266615662664842956.xmlvstatus; AC; 2DFS-3694; P/COS Approved for submission; P/RS 04/07/20 ; intrev: complete ; COS/CP 13/07/20
vcheck; Enter targ name & Inst. & Resp. Sci.; 2DFS-3694 ; 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?; COS G130M/1291 PSA Spectroscopic ACQ 1 s ...
Imaging ACQ would need BOA, and be complicated by bright star in the field violating PSA health and safety.
vcheck; Possible ACQ or Sci spoilers?; No
vcheck; Field BOT clear?; Yes; 7 safe field sources reported. ...
The target itself is listed as posing a safety issue for c1291 observations, but that is due to the assumption of an O5V source.
Examination of the field, and the catalogs of Massey et al. (2002), Evans (2004) the 2dFS catalog, and Ramachandran et al. (2019) indicate that there is one other B0 star in the BOA macroaperture with a visual magnitude 0f 16.48.
vcheck; Visual BOT check for stars not in catalog?; OK
vcheck; Orbit packing finalized?; Done
vcheck; Buffer times optimized?; Done
vcheck; Verify visit grouping correct; None needed
vcheck; Is visit ready for int. review?; Yes
Allocated COS orbits = 2(Tic-Visit
:proposal-id 16101
:visit-id "AC"
:proposal-version -1
:trans-version "20200619"
:date "17-Dec-2020 13:57:23.0"
: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 1304720
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16101
:visit-id "AC"
:obset-id "AC"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16101
:visit-id "AC"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2596
:al-overhead-at-end 0
:internal-dur-at-end 105
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2989
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16101
:visit-id "AC"
:orbit-number 2
:pcs-time 392
:si-vis-utilization 2597
:al-overhead-at-end 0
:internal-dur-at-end 360
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2989
:pcs-gap 0
)true20rn(WM-Basic(B1 V, Z=0.004, Teff=26303, log_lum=4.45, log_g=4.00) (extinction smcbar=0.070), johnson U mag=12.800 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: B1 IV --> B1 V
SED = 2DFS-3694_COS_G130M_c1291_sed.fits
For exptime=887.3 s, spectral region:
1150.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 4562.4 cts/s/segment
brightest pixel: 0.072 cts/s/pix at 1265.0 A
Calculation performed 2020-02-24T17:51:06, v0.4rn(WM-Basic(B1 V, Z=0.004, Teff=26303, log_lum=4.45, log_g=4.00) (extinction smcbar=0.070), johnson U mag=12.800 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: B1 IV --> B1 V
SED = 2DFS-3694_COS_G130M_c1291_sed.fits
For exptime=887.3 s, spectral region:
1150.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 4562.4 cts/s/segment
brightest pixel: 0.072 cts/s/pix at 1265.0 A
Calculation performed 2020-02-24T17:51:06, v0.4rn(WM-Basic(B1 V, Z=0.004, Teff=26303, log_lum=4.45, log_g=4.00) (extinction smcbar=0.070), johnson U mag=12.800 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: B1 IV --> B1 V
SED = 2DFS-3694_COS_G160M_c1611_sed.fits
For exptime=1362.8 s, spectral region:
1590.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 2745.5 cts/s/segment
brightest pixel: 0.046 cts/s/pix at 1435.0 A
Calculation performed 2020-02-24T17:51:09, v0.4rn(WM-Basic(B1 V, Z=0.004, Teff=26303, log_lum=4.45, log_g=4.00) (extinction smcbar=0.070), johnson U mag=12.800 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: B1 IV --> B1 V
SED = 2DFS-3694_COS_G160M_c1611_sed.fits
For exptime=1362.8 s, spectral region:
1590.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 2745.5 cts/s/segment
brightest pixel: 0.046 cts/s/pix at 1435.0 A
Calculation performed 2020-02-24T17:51:09, v0.4The scheduling data was generated by CASM 28.2.CASM was run in Phase II mode.vstatus; 2C; AV175; P/COS Approved for submission; P/RS 05/07/20 ; intrev: complete ; COS/CP 13/07/20
vcheck; Enter targ name & Inst. & Resp. Sci.; AV175 ; 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?; G130M/1291 Spectroscopic ACQ ...
Several stars in larger macro-aperture that pose a safety issue for PSA observations.
vcheck; Possible ACQ or Sci spoilers?; No
vcheck; Field BOT clear?; Yes ; 19 safe and 1 unknown reported ...
Zaritsky et al. (2002) shows the presence of a V=17.14 star within the PSA macro-aperture, and several sources with V between 17 and 18th magnitude in the BOA macro-aperture.
vcheck; Visual BOT check for stars not in catalog?; Okay
vcheck; Orbit packing finalized?; Done
vcheck; Buffer times optimized?; Done
vcheck; Verify visit grouping correct; None needed
vcheck; Is visit ready for int. review?; Yes
Allocated COS orbits = 31598244356000301.3393796012097(Tic-Visit
:proposal-id 16101
:visit-id "2C"
:proposal-version -1
:trans-version "20200518"
:date "13-Jul-2020 14:54:45.0"
: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 1122128
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16101
:visit-id "2C"
:obset-id "2C"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16101
:visit-id "2C"
: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 16101
:visit-id "2C"
: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 16101
:visit-id "2C"
:orbit-number 3
:pcs-time 392
:si-vis-utilization 2595
:al-overhead-at-end 0
:internal-dur-at-end 341
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2989
:pcs-gap 0
)true30rn-max(WM-Basic(B0.5 I, Z=0.004, Teff=24547, log_lum=5.40, log_g=2.95) (extinction smcbar=0.160), flux1360 +- 30.0A flux=1.4e-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: B1 IIW --> B0.5 I
SED = AV175_COS_G130M_c1291_sed.fits
For exptime=2597.2 s, spectral region:
1150.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 2065.4 cts/s/segment
brightest pixel: 0.033 cts/s/pix at 1275.0 A
Calculation performed 2020-02-24T17:50:05, v0.4rn-max(WM-Basic(B0.5 I, Z=0.004, Teff=24547, log_lum=5.40, log_g=2.95) (extinction smcbar=0.160), flux1360 +- 30.0A flux=1.4e-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: B1 IIW --> B0.5 I
SED = AV175_COS_G130M_c1291_sed.fits
For exptime=2597.2 s, spectral region:
1150.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 2065.4 cts/s/segment
brightest pixel: 0.033 cts/s/pix at 1275.0 A
Calculation performed 2020-02-24T17:50:05, v0.4rn-max(WM-Basic(B0.5 I, Z=0.004, Teff=24547, log_lum=5.40, log_g=2.95) (extinction smcbar=0.160), flux1360 +- 30.0A flux=1.4e-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: B1 IIW --> B0.5 I
SED = AV175_COS_G130M_c1291_sed.fits
For exptime=2597.2 s, spectral region:
1150.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 2065.4 cts/s/segment
brightest pixel: 0.033 cts/s/pix at 1275.0 A
Calculation performed 2020-02-24T17:50:05, v0.4rn-max(WM-Basic(B0.5 I, Z=0.004, Teff=24547, log_lum=5.40, log_g=2.95) (extinction smcbar=0.160), flux1700 +- 5.0A flux=1.2e-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: B1 IIW --> B0.5 I
SED = AV175_COS_G160M_c1611_sed.fits
For exptime=2479.5 s, spectral region:
1590.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 1428.1 cts/s/segment
brightest pixel: 0.022 cts/s/pix at 1435.0 A
Calculation performed 2020-02-24T17:50:08, v0.4The scheduling data was generated by CASM 28.2.CASM was run in Phase II mode.vstatus; 3C; AV224; P/COS Approved for submission ; P/RS 05/07/20 ; intrev: complete ; COS/CP 13/07/20
vcheck; Enter targ name & Inst. & Resp. Sci.; AV224 ; 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?; G130M/1291 spectroscopic ACQ ...
Several stars in larger macro-aperture that pose a safety issue for PSA observations.
vcheck; Possible ACQ or Sci spoilers?; No
vcheck; Field BOT clear?; Yes ; Health and safety violation reported for target in c1291 observations because of O5V assumption, and 16 safe targets in the field ... Zaritsky et al (2002) reports a V=18.6 star in the smaller macro-aperture, and several stars between V=16.5 and 18.0 in the larger macro-aperture.
vcheck; Visual BOT check for stars not in catalog?; Okay
vcheck; Orbit packing finalized?; Done ...
The c1611 exposures were separated into individual FPPOS with two FPPOS=2 exposures to pack the orbits
vcheck; Buffer times optimized?; Done
vcheck; Verify visit grouping correct; None needed
vcheck; Is visit ready for int. review?; Yes
Allocated COS orbits = 31598279714000314.878205924422(Tic-Visit
:proposal-id 16101
:visit-id "3C"
:proposal-version -1
:trans-version "20200518"
:date "13-Jul-2020 14:54:49.0"
: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 1487392
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16101
:visit-id "3C"
:obset-id "3C"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16101
:visit-id "3C"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2569
: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 16101
:visit-id "3C"
:orbit-number 2
:pcs-time 392
:si-vis-utilization 2597
: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 16101
:visit-id "3C"
:orbit-number 3
:pcs-time 392
:si-vis-utilization 2587
:al-overhead-at-end 0
:internal-dur-at-end 350
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2989
:pcs-gap 0
)true30rn(WM-Basic(B1 III, Z=0.004, Teff=24547, log_lum=4.80, log_g=3.47) (extinction smcbar=0.110), johnson U mag=13.020 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: B1 III --> B1 III
SED = AV224_COS_G130M_c1291_sed.fits
For exptime=2317.2 s, spectral region:
1150.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 2016.1 cts/s/segment
brightest pixel: 0.032 cts/s/pix at 1272.0 A
Calculation performed 2020-02-24T17:50:51, v0.4rn(WM-Basic(B1 III, Z=0.004, Teff=24547, log_lum=4.80, log_g=3.47) (extinction smcbar=0.110), johnson U mag=13.020 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: B1 III --> B1 III
SED = AV224_COS_G130M_c1291_sed.fits
For exptime=2317.2 s, spectral region:
1150.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 2016.1 cts/s/segment
brightest pixel: 0.032 cts/s/pix at 1272.0 A
Calculation performed 2020-02-24T17:50:51, v0.4rn(WM-Basic(B1 III, Z=0.004, Teff=24547, log_lum=4.80, log_g=3.47) (extinction smcbar=0.110), johnson U mag=13.020 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: B1 III --> B1 III
SED = AV224_COS_G130M_c1291_sed.fits
For exptime=2317.2 s, spectral region:
1150.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 2016.1 cts/s/segment
brightest pixel: 0.032 cts/s/pix at 1272.0 A
Calculation performed 2020-02-24T17:50:51, v0.4rn(WM-Basic(B1 III, Z=0.004, Teff=24547, log_lum=4.80, log_g=3.47) (extinction smcbar=0.110), johnson U mag=13.020 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: B1 III --> B1 III
SED = AV224_COS_G160M_c1611_sed.fits
For exptime=2400.2 s, spectral region:
1590.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 1511.7 cts/s/segment
brightest pixel: 0.024 cts/s/pix at 1435.0 A
Calculation performed 2020-02-24T17:50:54, v0.4rn(WM-Basic(B1 III, Z=0.004, Teff=24547, log_lum=4.80, log_g=3.47) (extinction smcbar=0.110), johnson U mag=13.020 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: B1 III --> B1 III
SED = AV224_COS_G160M_c1611_sed.fits
For exptime=2400.2 s, spectral region:
1590.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 1511.7 cts/s/segment
brightest pixel: 0.024 cts/s/pix at 1435.0 A
Calculation performed 2020-02-24T17:50:54, v0.4rn(WM-Basic(B1 III, Z=0.004, Teff=24547, log_lum=4.80, log_g=3.47) (extinction smcbar=0.110), johnson U mag=13.020 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: B1 III --> B1 III
SED = AV224_COS_G160M_c1611_sed.fits
For exptime=2400.2 s, spectral region:
1590.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 1511.7 cts/s/segment
brightest pixel: 0.024 cts/s/pix at 1435.0 A
Calculation performed 2020-02-24T17:50:54, v0.4rn(WM-Basic(B1 III, Z=0.004, Teff=24547, log_lum=4.80, log_g=3.47) (extinction smcbar=0.110), johnson U mag=13.020 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: B1 III --> B1 III
SED = AV224_COS_G160M_c1611_sed.fits
For exptime=2400.2 s, spectral region:
1590.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 1511.7 cts/s/segment
brightest pixel: 0.024 cts/s/pix at 1435.0 A
Calculation performed 2020-02-24T17:50:54, v0.4rn(WM-Basic(B1 III, Z=0.004, Teff=24547, log_lum=4.80, log_g=3.47) (extinction smcbar=0.110), johnson U mag=13.020 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: B1 III --> B1 III
SED = AV224_COS_G160M_c1611_sed.fits
For exptime=2400.2 s, spectral region:
1590.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 1511.7 cts/s/segment
brightest pixel: 0.024 cts/s/pix at 1435.0 A
Calculation performed 2020-02-24T17:50:54, v0.4The scheduling data was generated by CASM 28.2.CASM was run in Phase II mode.vstatus; 4C; NGC346-ELS-35; P/COS Approved for submission ; P/RS 05/07/20 ; intrev: complete ; COS/CP 13/07/20
vcheck; Enter targ name & Inst. & Resp. Sci.; NGC346-ELS-35 ; 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?; G130M/1291 Spectroscopic ACQ ...
Two bright stars in the larger macro-aperture would require orient constraints, and save only about 30 seconds exposure time.
vcheck; Possible ACQ or Sci spoilers?; No
vcheck; Field BOT clear?; Yes ; reports 24 safe sources in the field ...
Zaritsky et al. (2002) reports a V=18.4 star within the smaller macro-aperture, and V=14.94 and V=17.9 sources in the larger macro-aperture
vcheck; Visual BOT check for stars not in catalog?; Okay
vcheck; Orbit packing finalized?; Done ...
To get all exposures in two orbits, the exposure times were reduced by 4 percent for c1291 and by 2.5 percent for c1611 relative to default exposure times.
vcheck; Buffer times optimized?; Done
vcheck; Verify visit grouping correct; None needed
vcheck; Is visit ready for int. review?; Yes
Allocated COS orbits = 21598124234000312.868030078889(Tic-Visit
:proposal-id 16101
:visit-id "4C"
:proposal-version -1
:trans-version "20200518"
:date "13-Jul-2020 14:54:52.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 2
:saa-model "31"
:si-bright-earth-limb-angle 20.0
:data-volume 800352
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16101
:visit-id "4C"
:obset-id "4C"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16101
:visit-id "4C"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2595
:al-overhead-at-end 0
:internal-dur-at-end 57
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2989
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16101
:visit-id "4C"
:orbit-number 2
:pcs-time 392
:si-vis-utilization 2597
:al-overhead-at-end 0
:internal-dur-at-end 341
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2989
:pcs-gap 0
)true20rn(WM-Basic(B1 V, Z=0.004, Teff=26303, log_lum=4.45, log_g=4.00) (extinction smcbar=0.030), johnson B mag=14.860 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: B1 V --> B1 V
SED = NGC346-ELS-35_COS_G130M_c1291_sed.fits
For exptime=1348.2 s, spectral region:
1150.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 2879.9 cts/s/segment
brightest pixel: 0.042 cts/s/pix at 1265.0 A
Calculation performed 2020-02-24T17:51:48, v0.4rn(WM-Basic(B1 V, Z=0.004, Teff=26303, log_lum=4.45, log_g=4.00) (extinction smcbar=0.030), johnson B mag=14.860 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: B1 V --> B1 V
SED = NGC346-ELS-35_COS_G130M_c1291_sed.fits
For exptime=1348.2 s, spectral region:
1150.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 2879.9 cts/s/segment
brightest pixel: 0.042 cts/s/pix at 1265.0 A
Calculation performed 2020-02-24T17:51:48, v0.4rn(WM-Basic(B1 V, Z=0.004, Teff=26303, log_lum=4.45, log_g=4.00) (extinction smcbar=0.030), johnson B mag=14.860 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: B1 V --> B1 V
SED = NGC346-ELS-35_COS_G160M_c1611_sed.fits
For exptime=2780.3 s, spectral region:
1590.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 1420.2 cts/s/segment
brightest pixel: 0.024 cts/s/pix at 1435.0 A
Calculation performed 2020-02-24T17:51:51, v0.4rn(WM-Basic(B1 V, Z=0.004, Teff=26303, log_lum=4.45, log_g=4.00) (extinction smcbar=0.030), johnson B mag=14.860 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: B1 V --> B1 V
SED = NGC346-ELS-35_COS_G160M_c1611_sed.fits
For exptime=2780.3 s, spectral region:
1590.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 1420.2 cts/s/segment
brightest pixel: 0.024 cts/s/pix at 1435.0 A
Calculation performed 2020-02-24T17:51:51, v0.4The scheduling data was generated by CASM 28.2.CASM was run in Phase II mode.vstatus; 5C; SK173; P/COS Approved for submission; P/RS 06/07/20 ; intrev: complete ; COS/CP 13/07/20
vcheck; Enter targ name & Inst. & Resp. Sci.; SK173 ; 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?; G130M/1291 spectroscopic ACQ ...
There is one field star with V=18.53 that will likely NOT pose a threat to the imaging ACQ since the catalogs of Oey et al. (2004) and Ramachandran et al. (2019) do not identify any O or B stars in the larger macro-aperture except for the target. However, there is ample time to achieve the required S/N in the 2 orbits allocated, so to the spectroscopic ACQ was chosen as the conservative BOP option.
vcheck; Possible ACQ or Sci spoilers?; No
vcheck; Field BOT clear?; Yes ; ten safe field sources reported
vcheck; Visual BOT check for stars not in catalog?; Okay
vcheck; Orbit packing finalized?; Done
vcheck; Buffer times optimized?; Done
vcheck; Verify visit grouping correct; None needed
vcheck; Is visit ready for int. review?; Yes
Allocated COS orbits = 21598708582000313.4618197874994(Tic-Visit
:proposal-id 16101
:visit-id "5C"
:proposal-version -1
:trans-version "20200518"
:date "13-Jul-2020 14:54:54.0"
: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 1539520
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16101
:visit-id "5C"
:obset-id "5C"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16101
:visit-id "5C"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2594
: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 16101
:visit-id "5C"
:orbit-number 2
:pcs-time 392
:si-vis-utilization 2595
:al-overhead-at-end 0
:internal-dur-at-end 369
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2989
:pcs-gap 0
)true20rn(WM-Basic(B0.5 I, Z=0.004, Teff=24547, log_lum=5.40, log_g=2.95) (extinction smcbar=0.070), johnson U mag=12.440 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: B0.7 (II)e --> B0.5 I
SED = SK173_COS_G130M_c1291_sed.fits
For exptime=830.8 s, spectral region:
1150.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 4835.7 cts/s/segment
brightest pixel: 0.078 cts/s/pix at 1267.0 A
Calculation performed 2020-02-24T17:49:13, v0.4rn(WM-Basic(B0.5 I, Z=0.004, Teff=24547, log_lum=5.40, log_g=2.95) (extinction smcbar=0.070), johnson U mag=12.440 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: B0.7 (II)e --> B0.5 I
SED = SK173_COS_G130M_c1291_sed.fits
For exptime=830.8 s, spectral region:
1150.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 4835.7 cts/s/segment
brightest pixel: 0.078 cts/s/pix at 1267.0 A
Calculation performed 2020-02-24T17:49:13, v0.4rn(WM-Basic(B0.5 I, Z=0.004, Teff=24547, log_lum=5.40, log_g=2.95) (extinction smcbar=0.070), johnson U mag=12.440 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: B0.7 (II)e --> B0.5 I
SED = SK173_COS_G160M_c1611_sed.fits
For exptime=1143.7 s, spectral region:
1590.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 3347.4 cts/s/segment
brightest pixel: 0.054 cts/s/pix at 1435.0 A
Calculation performed 2020-02-24T17:49:16, v0.4rn(WM-Basic(B0.5 I, Z=0.004, Teff=24547, log_lum=5.40, log_g=2.95) (extinction smcbar=0.070), johnson U mag=12.440 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: B0.7 (II)e --> B0.5 I
SED = SK173_COS_G160M_c1611_sed.fits
For exptime=1143.7 s, spectral region:
1590.0 +- 0.5 A achieves SNR=30.0/resel
global countrate (brightest segment): 3347.4 cts/s/segment
brightest pixel: 0.054 cts/s/pix at 1435.0 A
Calculation performed 2020-02-24T17:49:16, v0.4