The number of orbits used exceeds the number allocatedVisit DC added to repeat the three failed exposures in visit 4C. The request was filed in HOPR 92176.1486087115----- Attempting Submission 2 (Wed Mar 09 21:25:04 GMT 2022) -----repeat visit addedULLYSES SMC O7 to O9 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-STARMAIN SEQUENCE ONOAV148 : [M2002]_27731, AV 148, AzV 148
Previous name : AV 148
Input file: SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
SIMBAD link (AzV 148): https://simbad.u-strasbg.fr/simbad/sim-id?Ident=AzV+148&submit=submit+id
SpT = O8.5 V
COS/G130M/c1096 : rn-max(WM-Basic(O9 V, Z=0.004, Teff=32359, log_lum=5.00, log_g=4.00) (extinction smcbar=0.070), flux1160 +- 30.0A flux=3.1e-13 Flam)
COS/G130M/c1291 : rn-max(WM-Basic(O9 V, Z=0.004, Teff=32359, log_lum=5.00, log_g=4.00) (extinction smcbar=0.070), flux1360 +- 30.0A flux=2.8e-13 Flam)
COS/G160M/c1611 : rn-max(WM-Basic(O9 V, Z=0.004, Teff=32359, log_lum=5.00, log_g=4.00) (extinction smcbar=0.070), flux1700 +- 5.0A flux=1.7e-13 Flam)
COS/G185M/c1921 : rn-max(WM-Basic(O9 V, Z=0.004, Teff=32359, log_lum=5.00, log_g=4.00) (extinction smcbar=0.070), flux1700 +- 5.0A flux=1.7e-13 Flam)
COS/G185M/c1953 : rn-max(WM-Basic(O9 V, Z=0.004, Teff=32359, log_lum=5.00, log_g=4.00) (extinction smcbar=0.070), flux1700 +- 5.0A flux=1.7e-13 Flam)
COS/G185M/c1986 : rn-max(WM-Basic(O9 V, Z=0.004, Teff=32359, log_lum=5.00, log_g=4.00) (extinction smcbar=0.070), flux1700 +- 5.0A flux=1.7e-13 Flam)
STIS/E140M/c1425 : rn-max(WM-Basic(O9 V, Z=0.004, Teff=32359, log_lum=5.00, log_g=4.00) (extinction smcbar=0.070), flux1360 +- 30.0A flux=2.8e-13 Flam)
STIS/E230M/c1978 : rn-max(WM-Basic(O9 V, Z=0.004, Teff=32359, log_lum=5.00, log_g=4.00) (extinction smcbar=0.070), flux1700 +- 5.0A flux=1.7e-13 Flam)
STIS/E230M/c2707 : rn-max(WM-Basic(O9 V, Z=0.004, Teff=32359, log_lum=5.00, log_g=4.00) (extinction smcbar=0.070), flux1700 +- 5.0A flux=1.7e-13 Flam)
Coordinate pedigree: Gaia
v sin i = 60
Calculation performed 2020-02-24T18:00:06, v0.4
-------------------------------------------------------------------------------
tstatus; AV148; P/COS approved for submission ; S/ins not started; P/RS 23/10/20; S/xx DD/MM/YY
tcheck; APT/SIMBAD target names:; AV148, 'AzV 148'
tcheck; Target info verification status?; OK ...
spectral type in SIMBAD is B0, but accuracy D, and co-ordinates and names are fine.
tcheck; Coordinates & P.M. updated?; Yes - GAIA DR2
tcheck; Adopted SED compared to Observations?; OK ...
COS c1291 data exist and therefore the model was scaled by a factor of about 0.8 to match the FUV data, retaining E(B-V)=0.07M2002-27731AZV-148J2000SpT=O8.5 V; E(B-V)=0.07; U=12.9; B=13.9; V=14.1; F1160=3.13e-13; F1360=2.76e-13; F1700=1.71e-13EXT-STARMAIN SEQUENCE ONOAV468 : [M2002]_72941, AV 468, AzV 468
Previous name : AV 468
Input file: SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
SIMBAD link (AzV 468): https://simbad.u-strasbg.fr/simbad/sim-id?Ident=AzV+468&submit=submit+id
SpT = O9 V
COS/G130M/c1096 : rn-max(WM-Basic(O9 V, Z=0.004, Teff=32359, log_lum=5.00, log_g=4.00) (extinction smcbar=0.020), flux1160 +- 30.0A flux=2.9e-13 Flam)
COS/G130M/c1291 : rn-max(WM-Basic(O9 V, Z=0.004, Teff=32359, log_lum=5.00, log_g=4.00) (extinction smcbar=0.020), flux1360 +- 30.0A flux=2.1e-13 Flam)
COS/G160M/c1611 : rn-max(WM-Basic(O9 V, Z=0.004, Teff=32359, log_lum=5.00, log_g=4.00) (extinction smcbar=0.020), flux1700 +- 5.0A flux=1.1e-13 Flam)
COS/G185M/c1921 : rn-max(WM-Basic(O9 V, Z=0.004, Teff=32359, log_lum=5.00, log_g=4.00) (extinction smcbar=0.020), flux1700 +- 5.0A flux=1.1e-13 Flam)
COS/G185M/c1953 : rn-max(WM-Basic(O9 V, Z=0.004, Teff=32359, log_lum=5.00, log_g=4.00) (extinction smcbar=0.020), flux1700 +- 5.0A flux=1.1e-13 Flam)
COS/G185M/c1986 : rn-max(WM-Basic(O9 V, Z=0.004, Teff=32359, log_lum=5.00, log_g=4.00) (extinction smcbar=0.020), flux1700 +- 5.0A flux=1.1e-13 Flam)
STIS/E140M/c1425 : rn-max(WM-Basic(O9 V, Z=0.004, Teff=32359, log_lum=5.00, log_g=4.00) (extinction smcbar=0.020), flux1360 +- 30.0A flux=2.1e-13 Flam)
STIS/E230M/c1978 : rn-max(WM-Basic(O9 V, Z=0.004, Teff=32359, log_lum=5.00, log_g=4.00) (extinction smcbar=0.020), flux1700 +- 5.0A flux=1.1e-13 Flam)
STIS/E230M/c2707 : rn-max(WM-Basic(O9 V, Z=0.004, Teff=32359, log_lum=5.00, log_g=4.00) (extinction smcbar=0.020), flux1700 +- 5.0A flux=1.1e-13 Flam)
Coordinate pedigree: Gaia
v sin i = 50
Calculation performed 2020-02-24T18:01:58, v0.4
-------------------------------------------------------------------------------
tstatus; AV468; P/COS approved for submission ; S/ins not started; P/RS 23/10/20; S/xx DD/MM/YY
tcheck; APT/SIMBAD target names: ; AV468, 'AzV 468'
tcheck; Target info verification status?; OK ...
spectral type is O8.5V in SIMBAD
tcheck; Coordinates & P.M. updated?; Yes - GAIA DR2
tcheck; Adopted SED compared to Observations?; OK ...
COS c1291 data exist and therefore the model was scaled by a factor of about 0.8 to match the FUV data, retaining E(B-V)=0.02AV-468M2002-72941J2000SpT=O9 V; E(B-V)=0.02; U=13.8; B=14.9; V=15.1; F1160=2.91e-13; F1360=2.09e-13; F1700=1.12e-13EXT-STARMAIN SEQUENCE ONONGC346-ELS-31 : NGC 346-031, NGC346_31, Cl* NGC 346 ELS 031
Previous name : NGC 346-031
Input file: SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
SIMBAD link (Cl* NGC 346 ELS 031): https://simbad.u-strasbg.fr/simbad/sim-id?Ident=Cl*+NGC+346+ELS+031&submit=submit+id
SpT = O7 V
COS/G130M/c1096 : rn-max(WM-Basic(O7 V, Z=0.004, Teff=39811, log_lum=5.42, log_g=4.00) (extinction smcbar=0.010), flux1160 +- 30.0A flux=1.5e-13 Flam)
COS/G130M/c1291 : rn-max(WM-Basic(O7 V, Z=0.004, Teff=39811, log_lum=5.42, log_g=4.00) (extinction smcbar=0.010), flux1360 +- 30.0A flux=1.3e-13 Flam)
COS/G160M/c1611 : rn-max(WM-Basic(O7 V, Z=0.004, Teff=39811, log_lum=5.42, log_g=4.00) (extinction smcbar=0.010), flux1700 +- 5.0A flux=8.9e-14 Flam)
COS/G185M/c1921 : rn-max(WM-Basic(O7 V, Z=0.004, Teff=39811, log_lum=5.42, log_g=4.00) (extinction smcbar=0.010), flux1700 +- 5.0A flux=8.9e-14 Flam)
COS/G185M/c1953 : rn-max(WM-Basic(O7 V, Z=0.004, Teff=39811, log_lum=5.42, log_g=4.00) (extinction smcbar=0.010), flux1700 +- 5.0A flux=8.9e-14 Flam)
COS/G185M/c1986 : rn-max(WM-Basic(O7 V, Z=0.004, Teff=39811, log_lum=5.42, log_g=4.00) (extinction smcbar=0.010), flux1700 +- 5.0A flux=8.9e-14 Flam)
STIS/E140M/c1425 : rn-max(WM-Basic(O7 V, Z=0.004, Teff=39811, log_lum=5.42, log_g=4.00) (extinction smcbar=0.010), flux1360 +- 30.0A flux=1.3e-13 Flam)
STIS/E230M/c1978 : rn-max(WM-Basic(O7 V, Z=0.004, Teff=39811, log_lum=5.42, log_g=4.00) (extinction smcbar=0.010), flux1700 +- 5.0A flux=8.9e-14 Flam)
STIS/E230M/c2707 : rn-max(WM-Basic(O7 V, Z=0.004, Teff=39811, log_lum=5.42, log_g=4.00) (extinction smcbar=0.010), flux1700 +- 5.0A flux=8.9e-14 Flam)
Coordinate pedigree: Gaia
v sin i = 18
Calculation performed 2020-02-24T17:58:42, v0.4
-------------------------------------------------------------------------------
tstatus; NGC346-ELS-31; P/COS approved for submission ; S/ins not started; P/RS 23/10/20; S/xx DD/MM/YY
tcheck; APT/SIMBAD target names: ; NGC346-ELS-31, '[M2002] SMC 47478'
tcheck; Target info verification status?; OK ...
spectral type is O8Vz in SIMBAD
tcheck; Coordinates & P.M. updated?; Yes - GAIA DR2
tcheck; Adopted SED compared to Observations?; OK ...
COS c1291 data exist, and changing E(B-V) to 0.05 provided a sufficient match to the FUV dataNGC346-31NGC-346-031J2000SpT=O7 V; E(B-V)=0.01; B=14.8; V=15.0; F1160=1.53e-13; F1360=1.29e-13; F1700=8.89e-14EXT-STARMAIN SEQUENCE ONONGC346-ELS-46 : NGC 346-046, NGC346_46, Cl* NGC 346 ELS 046
Previous name : NGC 346-046
Input file: SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
SIMBAD link (Cl* NGC 346 ELS 046): https://simbad.u-strasbg.fr/simbad/sim-id?Ident=Cl*+NGC+346+ELS+046&submit=submit+id
SpT = O7 Vn
COS/G130M/c1096 : rn-max(WM-Basic(O7 V, Z=0.004, Teff=39811, log_lum=5.42, log_g=4.00), flux1160 +- 30.0A flux=1.7e-13 Flam)
COS/G130M/c1291 : rn-max(WM-Basic(O7 V, Z=0.004, Teff=39811, log_lum=5.42, log_g=4.00), flux1360 +- 30.0A flux=1.3e-13 Flam)
COS/G160M/c1611 : rn-max(WM-Basic(O7 V, Z=0.004, Teff=39811, log_lum=5.42, log_g=4.00), flux1700 +- 5.0A flux=7.5e-14 Flam)
COS/G185M/c1921 : rn-max(WM-Basic(O7 V, Z=0.004, Teff=39811, log_lum=5.42, log_g=4.00), flux1700 +- 5.0A flux=7.5e-14 Flam)
COS/G185M/c1953 : rn-max(WM-Basic(O7 V, Z=0.004, Teff=39811, log_lum=5.42, log_g=4.00), flux1700 +- 5.0A flux=7.5e-14 Flam)
COS/G185M/c1986 : rn-max(WM-Basic(O7 V, Z=0.004, Teff=39811, log_lum=5.42, log_g=4.00), flux1700 +- 5.0A flux=7.5e-14 Flam)
STIS/E140M/c1425 : rn-max(WM-Basic(O7 V, Z=0.004, Teff=39811, log_lum=5.42, log_g=4.00), flux1360 +- 30.0A flux=1.3e-13 Flam)
STIS/E230M/c1978 : rn-max(WM-Basic(O7 V, Z=0.004, Teff=39811, log_lum=5.42, log_g=4.00), flux1700 +- 5.0A flux=7.5e-14 Flam)
STIS/E230M/c2707 : rn-max(WM-Basic(O7 V, Z=0.004, Teff=39811, log_lum=5.42, log_g=4.00), flux1700 +- 5.0A flux=7.5e-14 Flam)
Coordinate pedigree: Gaia
v sin i = 340
Calculation performed 2020-02-24T17:58:28, v0.4
-------------------------------------------------------------------------------
tstatus; NGC346-ELS-46; P/COS approved for submission ; S/ins not started; P/RS 23/10/20; S/xx DD/MM/YY
tcheck; APT/SIMBAD target names: ; NGC346-ELS-46, 'Cl* NGC 346 ELS 46'
tcheck; Target info verification status?; OK
tcheck; Coordinates & P.M. updated?; Yes - GAIA DR2
tcheck; Adopted SED compared to Observations?; OK ...
COS c1291 data exist, and changing E(B-V) to 0.05 provided a sufficient match to the FUV dataCL-NGC-346-ELS-046NGC346-46J2000SpT=O7 Vn; E(B-V)=-0.01; B=15.2; V=15.4; F1160=1.71e-13; F1360=1.27e-13; F1700=7.51e-14The scheduling data was generated by CASM 30.1.CASM was run in Phase II mode./private/var/folders/s6/sm4z5cyx5qg9425w4_w30knw0001d1/T/OPVisit12914738498515010859.xmlvstatus; 1C; AV148; P/COS approved for submission ; P/RS 23/10/20 ; intrev: completed ; P/CP 03/12/20
vcheck; Enter targ name & Inst. & Resp. Sci.; AV148 ; COS ; RS
vcheck; ETC numbers entered in APT?; Yes
vcheck; Any screening violations?; None but ...
with the original model SED the spectroscopic ACQ with c1291 violates count rate for irregularly variable sources. This is not an issue.
vcheck; S/N ETC calcs done & documented?; The original model spectrum was scaled by a factor of 0.8 to match the existing COS data and was used to check for the screening limit. The scaled spectrum was used in the ETC calculations. The buffer times used are less than 2/3 the value for the brighter case.
vcheck; Field images checked & saved?; Yes
vcheck; Selected ACQ strategy?; COS G130M/1291 PSA 1.0 sec ...
There is one relatively bright star in the field that would pose a safety issue for the PSA in the case of ACQ/IM with the BOA.
vcheck; Possible ACQ or Sci spoilers?; No
vcheck; Field BOT clear?; There is one unknown source reported by GSCII for the spectroscopic ACQ. However an inspection of the DSS, 2MASS and Galex images along with the stars in the Zaritsky catalog showed they were no bright stars that would pose a problem.
vcheck; Visual BOT check for stars not in catalog?; OK
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 = 3(Tic-Visit
:proposal-id 16372
:visit-id "1C"
:proposal-version -1
:trans-version "20211222"
:date "09-Mar-2022 16:18:20.0"
: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 1156864
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16372
:visit-id "1C"
:obset-id "1C"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16372
:visit-id "1C"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2592
: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 16372
:visit-id "1C"
:orbit-number 2
:pcs-time 392
:si-vis-utilization 2597
:al-overhead-at-end 0
:internal-dur-at-end 124
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2989
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16372
:visit-id "1C"
:orbit-number 3
:pcs-time 392
:si-vis-utilization 2597
: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
)true30rn-max(WM-Basic(O9 V, Z=0.004, Teff=32359, log_lum=5.00, log_g=4.00) (extinction smcbar=0.070), flux1160 +- 30.0A flux=3.1e-13 Flam); cos,fuv,g130m,c1096,psa,mjd#59305; fp-pos=None, segment=None)
From file SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
Spectral type: O8.5 V --> O9 V
SED = AV148_COS_G130M_c1096_sed.fits
For exptime=5538.8 s, spectral region:
1080.0 +- 0.5 A achieves SNR=20.0/resel
global countrate (brightest segment): 2801.5 cts/s/segment
brightest pixel: 0.053 cts/s/pix at 1235.0 A
Calculation performed 2020-02-24T18:00:15, v0.4rn-max(WM-Basic(O9 V, Z=0.004, Teff=32359, log_lum=5.00, log_g=4.00) (extinction smcbar=0.070), flux1160 +- 30.0A flux=3.1e-13 Flam); cos,fuv,g130m,c1096,psa,mjd#59305; fp-pos=None, segment=None)
From file SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
Spectral type: O8.5 V --> O9 V
SED = AV148_COS_G130M_c1096_sed.fits
For exptime=5538.8 s, spectral region:
1080.0 +- 0.5 A achieves SNR=20.0/resel
global countrate (brightest segment): 2801.5 cts/s/segment
brightest pixel: 0.053 cts/s/pix at 1235.0 A
Calculation performed 2020-02-24T18:00:15, v0.4rn-max(WM-Basic(O9 V, Z=0.004, Teff=32359, log_lum=5.00, log_g=4.00) (extinction smcbar=0.070), flux1160 +- 30.0A flux=3.1e-13 Flam); cos,fuv,g130m,c1096,psa,mjd#59305; fp-pos=None, segment=None)
From file SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
Spectral type: O8.5 V --> O9 V
SED = AV148_COS_G130M_c1096_sed.fits
For exptime=5538.8 s, spectral region:
1080.0 +- 0.5 A achieves SNR=20.0/resel
global countrate (brightest segment): 2801.5 cts/s/segment
brightest pixel: 0.053 cts/s/pix at 1235.0 A
Calculation performed 2020-02-24T18:00:15, v0.4rn-max(WM-Basic(O9 V, Z=0.004, Teff=32359, log_lum=5.00, log_g=4.00) (extinction smcbar=0.070), flux1160 +- 30.0A flux=3.1e-13 Flam); cos,fuv,g130m,c1096,psa,mjd#59305; fp-pos=None, segment=None)
From file SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
Spectral type: O8.5 V --> O9 V
SED = AV148_COS_G130M_c1096_sed.fits
For exptime=5538.8 s, spectral region:
1080.0 +- 0.5 A achieves SNR=20.0/resel
global countrate (brightest segment): 2801.5 cts/s/segment
brightest pixel: 0.053 cts/s/pix at 1235.0 A
Calculation performed 2020-02-24T18:00:15, v0.4rn-max(WM-Basic(O9 V, Z=0.004, Teff=32359, log_lum=5.00, log_g=4.00) (extinction smcbar=0.070), flux1160 +- 30.0A flux=3.1e-13 Flam); cos,fuv,g130m,c1096,psa,mjd#59305; fp-pos=None, segment=None)
From file SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
Spectral type: O8.5 V --> O9 V
SED = AV148_COS_G130M_c1096_sed.fits
For exptime=5538.8 s, spectral region:
1080.0 +- 0.5 A achieves SNR=20.0/resel
global countrate (brightest segment): 2801.5 cts/s/segment
brightest pixel: 0.053 cts/s/pix at 1235.0 A
Calculation performed 2020-02-24T18:00:15, v0.4rn-max(WM-Basic(O9 V, Z=0.004, Teff=32359, log_lum=5.00, log_g=4.00) (extinction smcbar=0.070), flux1160 +- 30.0A flux=3.1e-13 Flam); cos,fuv,g130m,c1096,psa,mjd#59305; fp-pos=None, segment=None)
From file SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
Spectral type: O8.5 V --> O9 V
SED = AV148_COS_G130M_c1096_sed.fits
For exptime=5538.8 s, spectral region:
1080.0 +- 0.5 A achieves SNR=20.0/resel
global countrate (brightest segment): 2801.5 cts/s/segment
brightest pixel: 0.053 cts/s/pix at 1235.0 A
Calculation performed 2020-02-24T18:00:15, v0.4The scheduling data was generated by CASM 30.1.CASM was run in Phase II mode./private/var/folders/s6/sm4z5cyx5qg9425w4_w30knw0001d1/T/OPVisit3547113147903891335.xmlvstatus; 2C; AV468; P/COS approved for submission ; P/RS 23/10/20 ; intrev: completed ; P/CP 03/12/20
vcheck; Enter targ name & Inst. & Resp. Sci.; AV468 ; 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 1.0 sec ...
There is one relatively bright star in the field that would pose a safety issue for the PSA in the case of ACQ/IM with the BOA. Also the target is too bright for MIRROR_B/PSA ACQ/IM.
vcheck; Possible ACQ or Sci spoilers?; No
vcheck; Field BOT clear?; Yes
vcheck; Visual BOT check for stars not in catalog?; OK
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 = 3(Tic-Visit
:proposal-id 16372
:visit-id "2C"
:proposal-version -1
:trans-version "20211222"
:date "09-Mar-2022 16:18:21.0"
: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 1156864
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16372
:visit-id "2C"
:obset-id "2C"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16372
:visit-id "2C"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2592
: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 16372
:visit-id "2C"
:orbit-number 2
:pcs-time 392
:si-vis-utilization 2597
:al-overhead-at-end 0
:internal-dur-at-end 124
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2989
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16372
:visit-id "2C"
:orbit-number 3
:pcs-time 392
:si-vis-utilization 2597
: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
)true30rn-max(WM-Basic(O9 V, Z=0.004, Teff=32359, log_lum=5.00, log_g=4.00) (extinction smcbar=0.020), flux1160 +- 30.0A flux=2.9e-13 Flam); cos,fuv,g130m,c1096,psa,mjd#59305; fp-pos=None, segment=None)
From file SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
Spectral type: O9 V --> O9 V
SED = AV468_COS_G130M_c1096_sed.fits
For exptime=5229.9 s, spectral region:
1080.0 +- 0.5 A achieves SNR=20.0/resel
global countrate (brightest segment): 2542.3 cts/s/segment
brightest pixel: 0.045 cts/s/pix at 1235.0 A
Calculation performed 2020-02-24T18:02:07, v0.4rn-max(WM-Basic(O9 V, Z=0.004, Teff=32359, log_lum=5.00, log_g=4.00) (extinction smcbar=0.020), flux1160 +- 30.0A flux=2.9e-13 Flam); cos,fuv,g130m,c1096,psa,mjd#59305; fp-pos=None, segment=None)
From file SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
Spectral type: O9 V --> O9 V
SED = AV468_COS_G130M_c1096_sed.fits
For exptime=5229.9 s, spectral region:
1080.0 +- 0.5 A achieves SNR=20.0/resel
global countrate (brightest segment): 2542.3 cts/s/segment
brightest pixel: 0.045 cts/s/pix at 1235.0 A
Calculation performed 2020-02-24T18:02:07, v0.4rn-max(WM-Basic(O9 V, Z=0.004, Teff=32359, log_lum=5.00, log_g=4.00) (extinction smcbar=0.020), flux1160 +- 30.0A flux=2.9e-13 Flam); cos,fuv,g130m,c1096,psa,mjd#59305; fp-pos=None, segment=None)
From file SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
Spectral type: O9 V --> O9 V
SED = AV468_COS_G130M_c1096_sed.fits
For exptime=5229.9 s, spectral region:
1080.0 +- 0.5 A achieves SNR=20.0/resel
global countrate (brightest segment): 2542.3 cts/s/segment
brightest pixel: 0.045 cts/s/pix at 1235.0 A
Calculation performed 2020-02-24T18:02:07, v0.4rn-max(WM-Basic(O9 V, Z=0.004, Teff=32359, log_lum=5.00, log_g=4.00) (extinction smcbar=0.020), flux1160 +- 30.0A flux=2.9e-13 Flam); cos,fuv,g130m,c1096,psa,mjd#59305; fp-pos=None, segment=None)
From file SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
Spectral type: O9 V --> O9 V
SED = AV468_COS_G130M_c1096_sed.fits
For exptime=5229.9 s, spectral region:
1080.0 +- 0.5 A achieves SNR=20.0/resel
global countrate (brightest segment): 2542.3 cts/s/segment
brightest pixel: 0.045 cts/s/pix at 1235.0 A
Calculation performed 2020-02-24T18:02:07, v0.4rn-max(WM-Basic(O9 V, Z=0.004, Teff=32359, log_lum=5.00, log_g=4.00) (extinction smcbar=0.020), flux1160 +- 30.0A flux=2.9e-13 Flam); cos,fuv,g130m,c1096,psa,mjd#59305; fp-pos=None, segment=None)
From file SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
Spectral type: O9 V --> O9 V
SED = AV468_COS_G130M_c1096_sed.fits
For exptime=5229.9 s, spectral region:
1080.0 +- 0.5 A achieves SNR=20.0/resel
global countrate (brightest segment): 2542.3 cts/s/segment
brightest pixel: 0.045 cts/s/pix at 1235.0 A
Calculation performed 2020-02-24T18:02:07, v0.4rn-max(WM-Basic(O9 V, Z=0.004, Teff=32359, log_lum=5.00, log_g=4.00) (extinction smcbar=0.020), flux1160 +- 30.0A flux=2.9e-13 Flam); cos,fuv,g130m,c1096,psa,mjd#59305; fp-pos=None, segment=None)
From file SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
Spectral type: O9 V --> O9 V
SED = AV468_COS_G130M_c1096_sed.fits
For exptime=5229.9 s, spectral region:
1080.0 +- 0.5 A achieves SNR=20.0/resel
global countrate (brightest segment): 2542.3 cts/s/segment
brightest pixel: 0.045 cts/s/pix at 1235.0 A
Calculation performed 2020-02-24T18:02:07, v0.4The scheduling data was generated by CASM 30.1.CASM was run in Phase II mode./private/var/folders/s6/sm4z5cyx5qg9425w4_w30knw0001d1/T/OPVisit12824929417141013254.xmlvstatus; 3C; NGC346-ELS-31; P/COS approved for submission ; P/RS 23/10/20 ; intrev: completed ; P/CP 03/12/20
vcheck; Enter targ name & Inst. & Resp. Sci.; NGC346-ELS-31 ; 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 1.2 sec conservatively based on single detector ...
There are two relatively bright stars in the field that would pose a safety issue for the PSA in the case of ACQ/IM with the BOA. Also the target is too bright for MIRROR_B/PSA ACQ/IM.
vcheck; Possible ACQ or Sci spoilers?; No
vcheck; Field BOT clear?; Yes
vcheck; Visual BOT check for stars not in catalog?; OK
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 = 51646115686000144.1361461610761(Tic-Visit
:proposal-id 16372
:visit-id "3C"
:proposal-version -1
:trans-version "20211222"
:date "09-Mar-2022 16:18:22.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 5
:saa-model "31"
:si-bright-earth-limb-angle 20.0
:data-volume 1113440
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16372
:visit-id "3C"
:obset-id "3C"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16372
:visit-id "3C"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2592
: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 16372
:visit-id "3C"
: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 16372
:visit-id "3C"
:orbit-number 3
: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 16372
:visit-id "3C"
:orbit-number 4
: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 16372
:visit-id "3C"
:orbit-number 5
:pcs-time 392
:si-vis-utilization 2597
:al-overhead-at-end 0
:internal-dur-at-end 382
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2989
:pcs-gap 0
)true50rn-max(WM-Basic(O7 V, Z=0.004, Teff=39811, log_lum=5.42, log_g=4.00) (extinction smcbar=0.010), flux1160 +- 30.0A flux=1.5e-13 Flam); cos,fuv,g130m,c1096,psa,mjd#59305; fp-pos=None, segment=None)
From file SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
Spectral type: O7 V --> O7 V
SED = NGC346-ELS-31_COS_G130M_c1096_sed.fits
For exptime=10629.0 s, spectral region:
1080.0 +- 0.5 A achieves SNR=20.0/resel
global countrate (brightest segment): 1309.1 cts/s/segment
brightest pixel: 0.019 cts/s/pix at 1205.0 A
Calculation performed 2020-02-24T17:58:50, v0.4rn-max(WM-Basic(O7 V, Z=0.004, Teff=39811, log_lum=5.42, log_g=4.00) (extinction smcbar=0.010), flux1160 +- 30.0A flux=1.5e-13 Flam); cos,fuv,g130m,c1096,psa,mjd#59305; fp-pos=None, segment=None)
From file SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
Spectral type: O7 V --> O7 V
SED = NGC346-ELS-31_COS_G130M_c1096_sed.fits
For exptime=10629.0 s, spectral region:
1080.0 +- 0.5 A achieves SNR=20.0/resel
global countrate (brightest segment): 1309.1 cts/s/segment
brightest pixel: 0.019 cts/s/pix at 1205.0 A
Calculation performed 2020-02-24T17:58:50, v0.4rn-max(WM-Basic(O7 V, Z=0.004, Teff=39811, log_lum=5.42, log_g=4.00) (extinction smcbar=0.010), flux1160 +- 30.0A flux=1.5e-13 Flam); cos,fuv,g130m,c1096,psa,mjd#59305; fp-pos=None, segment=None)
From file SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
Spectral type: O7 V --> O7 V
SED = NGC346-ELS-31_COS_G130M_c1096_sed.fits
For exptime=10629.0 s, spectral region:
1080.0 +- 0.5 A achieves SNR=20.0/resel
global countrate (brightest segment): 1309.1 cts/s/segment
brightest pixel: 0.019 cts/s/pix at 1205.0 A
Calculation performed 2020-02-24T17:58:50, v0.4rn-max(WM-Basic(O7 V, Z=0.004, Teff=39811, log_lum=5.42, log_g=4.00) (extinction smcbar=0.010), flux1160 +- 30.0A flux=1.5e-13 Flam); cos,fuv,g130m,c1096,psa,mjd#59305; fp-pos=None, segment=None)
From file SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
Spectral type: O7 V --> O7 V
SED = NGC346-ELS-31_COS_G130M_c1096_sed.fits
For exptime=10629.0 s, spectral region:
1080.0 +- 0.5 A achieves SNR=20.0/resel
global countrate (brightest segment): 1309.1 cts/s/segment
brightest pixel: 0.019 cts/s/pix at 1205.0 A
Calculation performed 2020-02-24T17:58:50, v0.4rn-max(WM-Basic(O7 V, Z=0.004, Teff=39811, log_lum=5.42, log_g=4.00) (extinction smcbar=0.010), flux1160 +- 30.0A flux=1.5e-13 Flam); cos,fuv,g130m,c1096,psa,mjd#59305; fp-pos=None, segment=None)
From file SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
Spectral type: O7 V --> O7 V
SED = NGC346-ELS-31_COS_G130M_c1096_sed.fits
For exptime=10629.0 s, spectral region:
1080.0 +- 0.5 A achieves SNR=20.0/resel
global countrate (brightest segment): 1309.1 cts/s/segment
brightest pixel: 0.019 cts/s/pix at 1205.0 A
Calculation performed 2020-02-24T17:58:50, v0.4rn-max(WM-Basic(O7 V, Z=0.004, Teff=39811, log_lum=5.42, log_g=4.00) (extinction smcbar=0.010), flux1160 +- 30.0A flux=1.5e-13 Flam); cos,fuv,g130m,c1096,psa,mjd#59305; fp-pos=None, segment=None)
From file SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
Spectral type: O7 V --> O7 V
SED = NGC346-ELS-31_COS_G130M_c1096_sed.fits
For exptime=10629.0 s, spectral region:
1080.0 +- 0.5 A achieves SNR=20.0/resel
global countrate (brightest segment): 1309.1 cts/s/segment
brightest pixel: 0.019 cts/s/pix at 1205.0 A
Calculation performed 2020-02-24T17:58:50, v0.4rn-max(WM-Basic(O7 V, Z=0.004, Teff=39811, log_lum=5.42, log_g=4.00) (extinction smcbar=0.010), flux1160 +- 30.0A flux=1.5e-13 Flam); cos,fuv,g130m,c1096,psa,mjd#59305; fp-pos=None, segment=None)
From file SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
Spectral type: O7 V --> O7 V
SED = NGC346-ELS-31_COS_G130M_c1096_sed.fits
For exptime=10629.0 s, spectral region:
1080.0 +- 0.5 A achieves SNR=20.0/resel
global countrate (brightest segment): 1309.1 cts/s/segment
brightest pixel: 0.019 cts/s/pix at 1205.0 A
Calculation performed 2020-02-24T17:58:50, v0.4rn-max(WM-Basic(O7 V, Z=0.004, Teff=39811, log_lum=5.42, log_g=4.00) (extinction smcbar=0.010), flux1160 +- 30.0A flux=1.5e-13 Flam); cos,fuv,g130m,c1096,psa,mjd#59305; fp-pos=None, segment=None)
From file SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
Spectral type: O7 V --> O7 V
SED = NGC346-ELS-31_COS_G130M_c1096_sed.fits
For exptime=10629.0 s, spectral region:
1080.0 +- 0.5 A achieves SNR=20.0/resel
global countrate (brightest segment): 1309.1 cts/s/segment
brightest pixel: 0.019 cts/s/pix at 1205.0 A
Calculation performed 2020-02-24T17:58:50, v0.4The scheduling data was generated by CASM 30.1.CASM was run in Phase II mode./private/var/folders/s6/sm4z5cyx5qg9425w4_w30knw0001d1/T/OPVisit16802919098579454316.xmlvstatus; 4C; NGC346-ELS-46; P/COS approved for submission ; P/RS 23/10/20 ; intrev: completed ; P/CP 03/12/20
vcheck; Enter targ name & Inst. & Resp. Sci.; NGC346-ELS-46 ; 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 1.2 sec conservatively based on single detector ...
There is one relatively bright star in the field that would pose a safety issue for the PSA in the case of ACQ/IM with the BOA. Also the target is too bright for MIRROR_B/PSA ACQ/IM.
vcheck; Possible ACQ or Sci spoilers?; No
vcheck; Field BOT clear?; Yes
vcheck; Visual BOT check for stars not in catalog?; OK
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 = 41646447052000148.3190457684404(Tic-Visit
:proposal-id 16372
:visit-id "4C"
:proposal-version -1
:trans-version "20211222"
:date "09-Mar-2022 16:18:23.0"
: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 800224
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16372
:visit-id "4C"
:obset-id "4C"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16372
:visit-id "4C"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2592
: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 16372
:visit-id "4C"
:orbit-number 2
:pcs-time 392
:si-vis-utilization 2597
: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 16372
:visit-id "4C"
:orbit-number 3
:pcs-time 392
:si-vis-utilization 2597
: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 16372
:visit-id "4C"
:orbit-number 4
:pcs-time 392
:si-vis-utilization 2597
:al-overhead-at-end 0
:internal-dur-at-end 382
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2989
:pcs-gap 0
)true40rn-max(WM-Basic(O7 V, Z=0.004, Teff=39811, log_lum=5.42, log_g=4.00), flux1160 +- 30.0A flux=1.7e-13 Flam); cos,fuv,g130m,c1096,psa,mjd#59305; fp-pos=None, segment=None)
From file SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
Spectral type: O7 Vn --> O7 V
SED = NGC346-ELS-46_COS_G130M_c1096_sed.fits
For exptime=10120.5 s, spectral region:
1080.0 +- 0.5 A achieves SNR=20.0/resel
global countrate (brightest segment): 1328.9 cts/s/segment
brightest pixel: 0.019 cts/s/pix at 1205.0 A
Calculation performed 2020-02-24T17:58:36, v0.4The scheduling data was generated by CASM 30.1.CASM was run in Phase II mode./private/var/folders/s6/sm4z5cyx5qg9425w4_w30knw0001d1/T/OPVisit7755833170656256395.xmlvstatus; 4C; NGC346-ELS-46; P/COS approved for submission ; P/RS 23/10/20 ; intrev: completed ; P/CP 03/12/20
vcheck; Enter targ name & Inst. & Resp. Sci.; NGC346-ELS-46 ; 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 1.2 sec conservatively based on single detector ...
There is one relatively bright star in the field that would pose a safety issue for the PSA in the case of ACQ/IM with the BOA. Also the target is too bright for MIRROR_B/PSA ACQ/IM.
vcheck; Possible ACQ or Sci spoilers?; No
vcheck; Field BOT clear?; Yes
vcheck; Visual BOT check for stars not in catalog?; OK
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 16372
:visit-id "DC"
:proposal-version -1
:trans-version "20211222"
:date "09-Mar-2022 16:18:23.0"
: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 582800
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16372
:visit-id "DC"
:obset-id "DC"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16372
:visit-id "DC"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2596
:al-overhead-at-end 0
:internal-dur-at-end 38
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2989
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16372
:visit-id "DC"
:orbit-number 2
:pcs-time 392
:si-vis-utilization 2597
: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 16372
:visit-id "DC"
:orbit-number 3
:pcs-time 392
:si-vis-utilization 2597
:al-overhead-at-end 0
:internal-dur-at-end 382
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2989
:pcs-gap 0
)true30rn-max(WM-Basic(O7 V, Z=0.004, Teff=39811, log_lum=5.42, log_g=4.00), flux1160 +- 30.0A flux=1.7e-13 Flam); cos,fuv,g130m,c1096,psa,mjd#59305; fp-pos=None, segment=None)
From file SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
Spectral type: O7 Vn --> O7 V
SED = NGC346-ELS-46_COS_G130M_c1096_sed.fits
For exptime=10120.5 s, spectral region:
1080.0 +- 0.5 A achieves SNR=20.0/resel
global countrate (brightest segment): 1328.9 cts/s/segment
brightest pixel: 0.019 cts/s/pix at 1205.0 A
Calculation performed 2020-02-24T17:58:36, v0.4rn-max(WM-Basic(O7 V, Z=0.004, Teff=39811, log_lum=5.42, log_g=4.00), flux1160 +- 30.0A flux=1.7e-13 Flam); cos,fuv,g130m,c1096,psa,mjd#59305; fp-pos=None, segment=None)
From file SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
Spectral type: O7 Vn --> O7 V
SED = NGC346-ELS-46_COS_G130M_c1096_sed.fits
For exptime=10120.5 s, spectral region:
1080.0 +- 0.5 A achieves SNR=20.0/resel
global countrate (brightest segment): 1328.9 cts/s/segment
brightest pixel: 0.019 cts/s/pix at 1205.0 A
Calculation performed 2020-02-24T17:58:36, v0.4rn-max(WM-Basic(O7 V, Z=0.004, Teff=39811, log_lum=5.42, log_g=4.00), flux1160 +- 30.0A flux=1.7e-13 Flam); cos,fuv,g130m,c1096,psa,mjd#59305; fp-pos=None, segment=None)
From file SMC_2020Feb20/input/SMC_all_do1_NewCoords_pids.csv
Spectral type: O7 Vn --> O7 V
SED = NGC346-ELS-46_COS_G130M_c1096_sed.fits
For exptime=10120.5 s, spectral region:
1080.0 +- 0.5 A achieves SNR=20.0/resel
global countrate (brightest segment): 1328.9 cts/s/segment
brightest pixel: 0.019 cts/s/pix at 1205.0 A
Calculation performed 2020-02-24T17:58:36, v0.4