The list of Investigators does not match the STScI records for this program.
REFERENCE-FRAME MUST BE ICRS OR GSC1 FOR SMALL APERTURE0----- Attempting Submission 1 (Thu Dec 16 21:21:31 GMT 2021) -----[1] "Warning (Form): The list of Investigators does not match the STScI records for this program."
This list has been updated since the initial generation of the program and should now currently reflect the correct author list.
[2] "Warning (Orbit Planner): REFERENCE-FRAME MUST BE ICRS OR GSC1 FOR SMALL APERTURE"
This star is included as an offset target for COS acquisition of Sz 84. Its reference data (including coordinates) are taken from SIMBAD, which references its GAIA DR2 values.ULLYSES T Tauri Survey Stars in Lupus IIThe 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 low mass ULLYSES survey stars. Each target will be observed with the COS c1291 + c1589 + c1623 settings, as well as with STIS G230L, G430L, and G750L. All observations will normally be constrained to occur within 1 day.
Signal-to-noise requirements used to determine the desired exposures times were defined as follows:
COS/G130M/c1291: N V 1239 +- 1 A -- S/N=10/6-pix-resel at the peak of the line
COS/G160M/c1589: C IV 1549 +- 1 A -- S/N=20/6-pix-resel at the peak of the line (combined c1589 & c1623)
COS/G160M/c1623: C IV 1549 +- 1 A -- S/N=20/6-pix-resel at the peak of the line (combined c1589 & c1623)
STIS/G230L/52X2: Mg II 2800 +-15 A -- S/N=20/2-pix-resel at the peak of the line
STIS/G430L/52X2: continuum average 4000 +-5 A -- S/N=20/2-pix-resel (2 reads)
STIS/G750L/52X2: continuum average 5700 +-5 A -- S/N=20/2-pix-resel (2 reads)
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.0falseSUPPORTEDSTART TAURI STARPRE-MAIN SEQUENCE STARNORXJ1556.1-3655
Region: Lupus II
Simbad: http://simbad.u-strasbg.fr/simbad/sim-id?Ident=rxj15561-3655&submit=submit+id
Target coordinates are from Gaia DR2.
Spectral type: M1 ; A_V: 1.0 ; Distance (pc): 150
M*: 0.5 ; log(dm/dt): -7.92
Input file: lowmass_survey_Input-gaia.csv
rxj15561-3655_lya2_etc_scaled_pAV0.50.txt
Calculation performed 2021-10-21T02:37:44, v0.8
-------------------------------------------------------------------------------
tstatus; RXJ1556.1-3655; P/COS work started; S/STIS work started; P/AH 27/10/21; S/xx DD/MM/YY
tcheck; APT/SIMBAD target names: ; RXJ1556.1-3655 ...
Default SIMBAD name is WRAY 15-1384, aka 2MASS J15560210-3655282
tcheck; Target info verification status?; OK ...
spectral type and magnitudes seem to be consistent
Flam(B) = 7.64e-11 at 4444 Angstroms and Flam(V) = 9.53e-11 at 5540 Angstroms from Vizier photometry viewer linked from SIMBAD
tcheck; Coordinates & P.M. verified, epoch checked?; OK ...
SIMBAD coordinates check out with what's here, SIMBAD PM values check out with what's here
tcheck; Adopted SED compared to Observations?; Yes ...
located at: box/ullyses_tech/ullyses_proposals/survey_c29/16583/seds/RXJ1556.1-3655/J2000SpT=M1; A_V=1.00; B=14.79; V=13.70; J=10.40START TAURI STARPRE-MAIN SEQUENCE STARNOSZ82 : IM Lup
Region: Lupus II
Simbad: http://simbad.u-strasbg.fr/simbad/sim-id?Ident=sz82&submit=submit+id
Target coordinates are from Gaia DR2.
Spectral type: K5 ; A_V: 0.9 ; Distance (pc): 150
M*: 0.95 ; log(dm/dt): -8.04
Input file: lowmass_survey_Input-gaia.csv
sz82_lya2_etc_scaled_pAV0.50.txt
Calculation performed 2021-10-21T02:37:16, v0.8
-------------------------------------------------------------------------------
tstatus; SZ82; P/COS work started; S/STIS work started; P/AH 27/10/21; S/xx DD/MM/YY
tcheck; APT/SIMBAD target names: ; SZ82 ...
Default SIMBAD name is THA 15-12, aka 2MASS J15560921-3756057
tcheck; Target info verification status?; OK ...
spectral type and magnitudes seem to be consistent
Flam(B) = 3.65e-10 at 4444 Angstroms and Flam(V) = 7.18e-10 at 5540 Angstroms from Vizier photometry viewer linked from SIMBAD
tcheck; Coordinates & P.M. verified, epoch checked?; OK ...
SIMBAD coordinates check out with what's here, SIMBAD PM values check out with what's here
tcheck; Adopted SED compared to Observations?; Yes ...
located at: box/ullyses_tech/ullyses_proposals/survey_c29/16583/seds/Sz82/IM-LUPJ2000SpT=K5; A_V=0.90; B=12.99; V=11.63; J=8.783START TAURI STARPRE-MAIN SEQUENCE STARNOSZ84
Region: Lupus II
Simbad: http://simbad.u-strasbg.fr/simbad/sim-id?Ident=sz84&submit=submit+id
Target coordinates are from Gaia DR2.
Spectral type: M5 ; A_V: 0.0 ; Distance (pc): 150
M*: 0.16 ; log(dm/dt): -9.21
Input file: lowmass_survey_Input-gaia.csv
sz84_lya2_etc_scaled_pAV0.50.txt
Calculation performed 2021-10-21T02:39:10, v0.8
-------------------------------------------------------------------------------
tstatus; SZ84; P/COS work started; S/STIS work started; P/AH 27/10/21; S/xx DD/MM/YY
tcheck; APT/SIMBAD target names: ; SZ84 ...
Default SIMBAD name is SZ 84, aka 2MASS J15580252-3736026
tcheck; Target info verification status?; OK ...
spectral type and magnitudes seem to be consistent
Flam(B) = 1.98e-11 at 4444 Angstroms and Flam(V) = 1.09e-11 at 5540 Angstroms from Vizier photometry viewer
tcheck; Coordinates & P.M. verified, epoch checked?; OK ...
SIMBAD coordinates check out with what's here, SIMBAD PM values check out with what's here
tcheck; Adopted SED compared to Observations?; Yes ...
located at: box/ullyses_tech/ullyses_proposals/survey_c29/16583/seds/Sz84/J2000SpT=M5; A_V=0.00; B=17.56; V=16.12; J=10.93STARK III-INOThis object was generated by the targetselector and retrieved from the SIMBAD database.GAIA-DR2-60102164304486378242MASS-J15580075-3737365J2000SpT=K0; A_V=1.78; B=14.91; V=13.172; R=12.733; G=12.4371; J=9.912; H=9.131; K=8.862Timing link suitability includes constraints ([Group (1C 1D 1S) Within 2.0 days])The scheduling data was generated by CASM 29.2.CASM was run in Phase II mode.vstatus; 1C; RXJ1556.1-3655; P/COS ready for internal review; P/AH 27/10/21 ; intrev: not started ; ?/rr DD/MM/YY
vcheck; Enter targ name & Inst. & Resp. Sci.; RXJ1556.1-3655 ; COS ; AH
vcheck; ETC numbers entered in APT?; Yes
vcheck; Any screening violations?; No
vcheck; M-dwarf check complete and added to box folder?; Yes ...
located at: box/ullyses_tech/ullyses_proposals/survey/revised-mstar-bop.xls
vcheck; S/N ETC calcs done & documented?; Yes
vcheck; Field images checked & saved?; Yes ...
located at: box/ullyses_tech/ullyses_proposals/survey_c29/16853/images/RXJ1556.1-3655
vcheck; Selected ACQ strategy?; PSA, MIRRORB, S/N=40
vcheck; Possible ACQ or Sci spoilers?; No
vcheck; Field BOT clear?; Yes ...
GSC II assumes O5V spectral type; ETC calculations cleared
vcheck; Visual BOT check for stars not in catalog?; Yes
vcheck; Orbit packing finalized?; Yes
vcheck; Buffer times optimized?; Yes
vcheck; Verify visit grouping correct; Yes ...
COS visit has GROUP 1C,1D,1S WITHIN 2D
vcheck; phase constraint for ground based observations added?; N/A
vcheck; BETWEENS for coordinated observations added?; Yes ...
26 MAR 2022 00:00 to 29 JUL 2023 00:00
vcheck; Is visit ready for int. review?; Yes
Allocated COS orbits = 6(Tic-Visit
:proposal-id 16853
:visit-id "1C"
:proposal-version -1
:trans-version "20210514"
:date "16-Dec-2021 16:16:08.0"
: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 121952
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16853
:visit-id "1C"
:obset-id "1C"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16853
:visit-id "1C"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2524
: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 2927
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16853
:visit-id "1C"
:orbit-number 2
:pcs-time 392
:si-vis-utilization 2535
: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 2927
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16853
:visit-id "1C"
:orbit-number 3
:pcs-time 392
:si-vis-utilization 2533
:al-overhead-at-end 0
:internal-dur-at-end 372
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2927
:pcs-gap 0
)true30BOP check with 4x spectrum COS.ta.1667051, B.P. = 19.958
M dwarf flare spectrum COS.ta.1667052, B.P. = 4.932
Baseline SED with S/N = 40 COS.ta.1667050 requires 114.3301 seconds (x2 = 228.6602 seconds, rounded to 228.7 seconds), B.P. = 1.959BOP check with 4x spectrum COS.sp.1667059, B.P. = 0.062
M dwarf flare spectrum COS.sp.1667291, B.P. = 0.011
Baseline SED (scaled with additional A_v = 0.50) calculation for G160M/c1589: COS.sp.1667058, B.P. = 0.005.
Total S/N achieved in G160M exposures ~22.8/resel @1548.4243 A
rxj15561-3655_lya2_etc_scaled_pAV0.50.txt; cos,fuv,g160m,c1589,psa,mjd#59670; fp-pos=None, segment=None)
Input file: lowmass_survey_Input-gaia.csv
Spectral type: M1 ; A_V: 1.0 ; Distance (pc): 150
M*: 0.5 ; log(dm/dt): -7.92
For exptime=1036.8 s, spectral region:
1549.0 +- 1.0 A achieves SNR=20.0 / 6-pix-resel for combined c1589 & c1623
The exptime for this c1589 exposure has been halved because c1589 & c1623 target the same line.
A factor of 2.0 has been applied to the exptime in each exposure.
global countrate (brightest segment): 69.6 cts/s/segment
brightest pixel: 0.005 cts/s/pix at 1548.4 A
Calculation performed 2021-10-21T02:37:40, v0.23BOP check with 4x spectrum COS.sp.1667059, B.P. = 0.062
M dwarf flare spectrum COS.sp.1667291, B.P. = 0.011
Baseline SED (scaled with additional A_v = 0.50) calculation for G160M/c1589: COS.sp.1667058, B.P. = 0.005.
Total S/N achieved in G160M exposures ~22.8/resel @1548.4243 A
rxj15561-3655_lya2_etc_scaled_pAV0.50.txt; cos,fuv,g160m,c1589,psa,mjd#59670; fp-pos=None, segment=None)
Input file: lowmass_survey_Input-gaia.csv
Spectral type: M1 ; A_V: 1.0 ; Distance (pc): 150
M*: 0.5 ; log(dm/dt): -7.92
For exptime=1036.8 s, spectral region:
1549.0 +- 1.0 A achieves SNR=20.0 / 6-pix-resel for combined c1589 & c1623
The exptime for this c1589 exposure has been halved because c1589 & c1623 target the same line.
A factor of 2.0 has been applied to the exptime in each exposure.
global countrate (brightest segment): 69.6 cts/s/segment
brightest pixel: 0.005 cts/s/pix at 1548.4 A
Calculation performed 2021-10-21T02:37:40, v0.23BOP check with 4x spectrum COS.sp.1667065, B.P. = 0.090
M dwarf flare spectrum COS.sp.1667293, B.P. = 0.090
Baseline SED (scaled with additional A_v = 0.50) calculation for G130M/c1291: COS.sp.1667064, B.P. = 0.090.
Total S/N achieved in G130M exposures ~13.5/resel @1238.9430 A
rxj15561-3655_lya2_etc_scaled_pAV0.50.txt; cos,fuv,g130m,c1291,psa,mjd#59670; fp-pos=None, segment=None)
Input file: lowmass_survey_Input-gaia.csv
Spectral type: M1 ; A_V: 1.0 ; Distance (pc): 150
M*: 0.5 ; log(dm/dt): -7.92
For exptime=4775.0 s, spectral region:
1239.0 +- 1.0 A achieves SNR=10.0 / 6-pix-resel
A factor of 2.0 has been applied to the exptime in each exposure.
global countrate (brightest segment): 285.2 cts/s/segment
brightest pixel: 0.002 cts/s/pix at 1304.9 A
Calculation performed 2021-10-21T02:37:44, v0.23BOP check with 4x spectrum COS.sp.1667065, B.P. = 0.090
M dwarf flare spectrum COS.sp.1667293, B.P. = 0.090
Baseline SED (scaled with additional A_v = 0.50) calculation for G130M/c1291: COS.sp.1667064, B.P. = 0.090.
Total S/N achieved in G130M exposures ~13.5/resel @1238.9430 A
rxj15561-3655_lya2_etc_scaled_pAV0.50.txt; cos,fuv,g130m,c1291,psa,mjd#59670; fp-pos=None, segment=None)
Input file: lowmass_survey_Input-gaia.csv
Spectral type: M1 ; A_V: 1.0 ; Distance (pc): 150
M*: 0.5 ; log(dm/dt): -7.92
For exptime=4775.0 s, spectral region:
1239.0 +- 1.0 A achieves SNR=10.0 / 6-pix-resel
A factor of 2.0 has been applied to the exptime in each exposure.
global countrate (brightest segment): 285.2 cts/s/segment
brightest pixel: 0.002 cts/s/pix at 1304.9 A
Calculation performed 2021-10-21T02:37:44, v0.23Timing link suitability includes constraints ([Group (1C 1D 1S) Within 2.0 days])The scheduling data was generated by CASM 29.2.CASM was run in Phase II mode.vstatus; 1D; RXJ1556.1-3655; P/COS ready for internal review; P/AH 27/10/21 ; intrev: not started ; ?/rr DD/MM/YY
vcheck; Enter targ name & Inst. & Resp. Sci.; RXJ1556.1-3655 ; COS ; AH
vcheck; ETC numbers entered in APT?; Yes
vcheck; Any screening violations?; No
vcheck; M-dwarf check complete and added to box folder?; Yes ...
located at: box/ullyses_tech/ullyses_proposals/survey/revised-mstar-bop.xls
vcheck; S/N ETC calcs done & documented?; Yes
vcheck; Field images checked & saved?; Yes ...
located at: box/ullyses_tech/ullyses_proposals/survey_c29/16853/images/RXJ1556.1-3655
vcheck; Selected ACQ strategy?; PSA, MIRRORB, S/N=40
vcheck; Possible ACQ or Sci spoilers?; No
vcheck; Field BOT clear?; Yes ...
GSC II assumes O5V spectral type; ETC calculations cleared
vcheck; Visual BOT check for stars not in catalog?; Yes
vcheck; Orbit packing finalized?; Yes
vcheck; Buffer times optimized?; Yes
vcheck; Verify visit grouping correct; Yes ...
COS visit has GROUP 1D,1C,1S WITHIN 2D
vcheck; phase constraint for ground based observations added?; N/A
vcheck; BETWEENS for coordinated observations added?; Yes ...
26 MAR 2022 00:00 to 29 JUL 2023 00:00
vcheck; Is visit ready for int. review?; Yes
Allocated COS orbits = 6(Tic-Visit
:proposal-id 16853
:visit-id "1D"
:proposal-version -1
:trans-version "20210514"
:date "16-Dec-2021 16:16:09.0"
: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 121952
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16853
:visit-id "1D"
:obset-id "1D"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16853
:visit-id "1D"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2534
: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 2927
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16853
:visit-id "1D"
:orbit-number 2
:pcs-time 392
:si-vis-utilization 2535
: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 2927
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16853
:visit-id "1D"
:orbit-number 3
:pcs-time 392
:si-vis-utilization 2533
:al-overhead-at-end 0
:internal-dur-at-end 372
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2927
:pcs-gap 0
)true30BOP check with 4x spectrum COS.ta.1667051, B.P. = 19.958
M dwarf flare spectrum COS.ta.1667052, B.P. = 4.932
Baseline SED with S/N = 40 COS.ta.1667050 requires 114.3301 seconds (x2 = 228.6602 seconds, rounded to 228.7 seconds), B.P. = 1.959BOP check with 4x spectrum COS.sp.1667062, B.P. = 0.063
M dwarf flare spectrum COS.sp.1667292, B.P. = 0.011
Baseline SED (scaled with additional A_v = 0.50) calculation for G160M/c1623: COS.sp.1667061, B.P. = 0.005.
Total S/N achieved in G160M exposures ~22.8/resel @1548.4243 A
rxj15561-3655_lya2_etc_scaled_pAV0.50.txt; cos,fuv,g160m,c1623,psa,mjd#59670; fp-pos=None, segment=None)
Input file: lowmass_survey_Input-gaia.csv
Spectral type: M1 ; A_V: 1.0 ; Distance (pc): 150
M*: 0.5 ; log(dm/dt): -7.92
For exptime=1029.8 s, spectral region:
1549.0 +- 1.0 A achieves SNR=20.0 / 6-pix-resel for combined c1589 & c1623
The exptime for this c1623 exposure has been halved because c1589 & c1623 target the same line.
A factor of 2.0 has been applied to the exptime in each exposure.
global countrate (brightest segment): 69.1 cts/s/segment
brightest pixel: 0.005 cts/s/pix at 1548.4 A
Calculation performed 2021-10-21T02:37:42, v0.23BOP check with 4x spectrum COS.sp.1667062, B.P. = 0.063
M dwarf flare spectrum COS.sp.1667292, B.P. = 0.011
Baseline SED (scaled with additional A_v = 0.50) calculation for G160M/c1623: COS.sp.1667061, B.P. = 0.005.
Total S/N achieved in G160M exposures ~22.8/resel @1548.4243 A
rxj15561-3655_lya2_etc_scaled_pAV0.50.txt; cos,fuv,g160m,c1623,psa,mjd#59670; fp-pos=None, segment=None)
Input file: lowmass_survey_Input-gaia.csv
Spectral type: M1 ; A_V: 1.0 ; Distance (pc): 150
M*: 0.5 ; log(dm/dt): -7.92
For exptime=1029.8 s, spectral region:
1549.0 +- 1.0 A achieves SNR=20.0 / 6-pix-resel for combined c1589 & c1623
The exptime for this c1623 exposure has been halved because c1589 & c1623 target the same line.
A factor of 2.0 has been applied to the exptime in each exposure.
global countrate (brightest segment): 69.1 cts/s/segment
brightest pixel: 0.005 cts/s/pix at 1548.4 A
Calculation performed 2021-10-21T02:37:42, v0.23BOP check with 4x spectrum COS.sp.1667065, B.P. = 0.090
M dwarf flare spectrum COS.sp.1667293, B.P. = 0.090
Baseline SED (scaled with additional A_v = 0.50) calculation for G130M/c1291: COS.sp.1667064, B.P. = 0.090.
Total S/N achieved in G130M exposures ~13.5/resel @1238.9430 A
rxj15561-3655_lya2_etc_scaled_pAV0.50.txt; cos,fuv,g130m,c1291,psa,mjd#59670; fp-pos=None, segment=None)
Input file: lowmass_survey_Input-gaia.csv
Spectral type: M1 ; A_V: 1.0 ; Distance (pc): 150
M*: 0.5 ; log(dm/dt): -7.92
For exptime=4775.0 s, spectral region:
1239.0 +- 1.0 A achieves SNR=10.0 / 6-pix-resel
A factor of 2.0 has been applied to the exptime in each exposure.
global countrate (brightest segment): 285.2 cts/s/segment
brightest pixel: 0.002 cts/s/pix at 1304.9 A
Calculation performed 2021-10-21T02:37:44, v0.23BOP check with 4x spectrum COS.sp.1667065, B.P. = 0.090
M dwarf flare spectrum COS.sp.1667293, B.P. = 0.090
Baseline SED (scaled with additional A_v = 0.50) calculation for G130M/c1291: COS.sp.1667064, B.P. = 0.090.
Total S/N achieved in G130M exposures ~13.5/resel @1238.9430 A
rxj15561-3655_lya2_etc_scaled_pAV0.50.txt; cos,fuv,g130m,c1291,psa,mjd#59670; fp-pos=None, segment=None)
Input file: lowmass_survey_Input-gaia.csv
Spectral type: M1 ; A_V: 1.0 ; Distance (pc): 150
M*: 0.5 ; log(dm/dt): -7.92
For exptime=4775.0 s, spectral region:
1239.0 +- 1.0 A achieves SNR=10.0 / 6-pix-resel
A factor of 2.0 has been applied to the exptime in each exposure.
global countrate (brightest segment): 285.2 cts/s/segment
brightest pixel: 0.002 cts/s/pix at 1304.9 A
Calculation performed 2021-10-21T02:37:44, v0.23Timing link suitability includes constraints ([Group (1C 1D 1S) Within 2.0 days])The scheduling data was generated by CASM 29.2.CASM was run in Phase II mode.vstatus; 1S; RXJ1556.1-3655; S/STIS ready for internal review; S/AH 27/10/21 ; intrev: not started ; ?/rr DD/MM/YY
vcheck; Enter targ name & Inst. & Resp. Sci.; RXJ1556.1-3655 ; STIS ; AH
vcheck; ETC numbers entered in APT?; Yes
vcheck; Any screening violations?; No
vcheck; M-dwarf check complete and added to box folder?; Yes ...
located at: box/ullyses_tech/ullyses_proposals/survey/revised-mstar-bop.xls
vcheck; S/N ETC calcs done & documented?; Yes
vcheck; Field images checked & saved?; Yes ...
located at: box/ullyses_tech/ullyses_proposals/survey_c29/16853/images/RXJ1556.1-3655
vcheck; Selected ACQ strategy?; R-mag with F28X50LP, S/N=80
vcheck; Possible ACQ or Sci spoilers?; No
vcheck; Field BOT clear?; Yes
vcheck; Visual BOT check for stars not in catalog?; Yes
vcheck; Orbit packing finalized?; Yes
vcheck; Buffer times optimized?; Yes
vcheck; Verify visit grouping correct; Yes ...
STIS visit has GROUP 1S,1C,1D WITHIN 2D
vcheck; phase constraint for ground based observations added?; N/A
vcheck; BETWEENS for coordinated observations added?; Yes ...
26 MAR 2022 00:00 to 29 JUL 2023 00:00
vcheck; Is visit ready for int. review?; Yes
Allocated STIS orbits = 1(Tic-Visit
:proposal-id 16853
:visit-id "1S"
:proposal-version -1
:trans-version "20210514"
:date "16-Dec-2021 16:16:11.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 1
:saa-model "24"
:si-bright-earth-limb-angle 20.0
:data-volume 377824
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16853
:visit-id "1S"
:obset-id "1S"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16853
:visit-id "1S"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2534
:al-overhead-at-end 116
:internal-dur-at-end 1192
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2927
:pcs-gap 0
)true104x BOP check: STIS.ta.1667088, B.P. = 85,473.623
Baseline SED (Castelli-Kurucz M2V 3500 4.5 spectrum renormalized to Johnson V = 13.70 vegamag) with S/N = 80: STIS.ta.1667087 requires 0.0866 seconds (x2 = 0.1732 seconds, rounded to 0.2 seconds), B.P. = 25,717.072BOP check with 4x spectrum: STIS.sp.1667082, B.P. = 7.729
M dwarf flare spectrum STIS.sp.1667295, B.P. = 0.803
Baseline ETC calc with spectrum: STIS.sp.1667081, B.P. = 0.796
rxj15561-3655_lya2_etc_scaled_pAV0.50.txt; stis,nuvmama,g230l,c2376,52x2,mjd#59670
Input file: lowmass_survey_Input-gaia.csv
Spectral type: M1 ; A_V: 1.0 ; Distance (pc): 150
M*: 0.5 ; log(dm/dt): -7.92
For exptime=102.9 s, spectral region:
2800.0 +- 15.0 A achieves SNR=20.0 / 2-pix-resel
A factor of 2.0 has been applied to the exptime in each exposure.
global countrate (brightest segment): 2489.6 cts/s/segment
brightest pixel: 0.796 cts/s/pix at 2788.8 A
Calculation performed 2021-10-21T02:37:44, v0.23Calculation with Castelli-Kurucz M2V 3500 4.5 stellar model, normalized to Johnson/V = 13.70, for G430L: STIS.sp.1667089, B.P. = 16.071
BOP calculation with Castelli-Kurucz M2V 3500 4.5 stellar model, normalized to Johnson/V = 13.70 - 1.5 = 12.20: STIS.sp.1667090, B.P. = 65.778.
rxj15561-3655_lya2_etc_scaled_pAV0.50.txt; stis,ccd,g430l,c4300,52x2,mjd#59670
WARNING: operating mode = ACCUM
Input file: lowmass_survey_Input-gaia.csv
Spectral type: M1 ; A_V: 1.0 ; Distance (pc): 150
M*: 0.5 ; log(dm/dt): -7.92
For exptime=35.8 s, n_reads=2, spectral region:
4000.0 +- 5.0 A achieves SNR=20.0 / 2-pix-resel
A factor of 2.0 has been applied to the exptime in each exposure.
global countrate (brightest segment): 52517.0 cts/s/segment
brightest pixel: 33.961 cts/s/pix at 4871.0 A
Calculation performed 2021-10-21T02:37:44, v0.23Calculation with Castelli-Kurucz M2V 3500 4.5 stellar model, normalized to Johnson/V = 13.70, for G750L: STIS.sp.1667093, B.P. = 82.776
BOP calculation with Castelli-Kurucz M2V 3500 4.5 stellar model, normalized to Johnson/R = 13.70 - 1.5 = 12.20: STIS.sp.1667094, B.P. = 273.993.
rxj15561-3655_lya2_etc_scaled_pAV0.50.txt; stis,ccd,g750l,c7751,52x2,mjd#59670
WARNING: operating mode = ACCUM
Input file: lowmass_survey_Input-gaia.csv
Spectral type: M1 ; A_V: 1.0 ; Distance (pc): 150
M*: 0.5 ; log(dm/dt): -7.92
For exptime=2.6 s, n_reads=2, spectral region:
5700.0 +- 5.0 A achieves SNR=20.0 / 2-pix-resel
A factor of 2.0 has been applied to the exptime in each exposure.
global countrate (brightest segment): 149217.1 cts/s/segment
brightest pixel: 295.729 cts/s/pix at 6563.9 A
Calculation performed 2021-10-21T02:37:44, v0.23Timing link suitability includes constraints ([Group (2C 2D 2S) Within 2.0 days])The scheduling data was generated by CASM 29.2.CASM was run in Phase II mode.vstatus; 2C; SZ82; P/COS ready for internal review; P/AH 27/10/21 ; intrev: not started ; ?/rr DD/MM/YY
vcheck; Enter targ name & Inst. & Resp. Sci.; SZ82 ; COS ; AH
vcheck; ETC numbers entered in APT?; Yes
vcheck; Any screening violations?; No
vcheck; M-dwarf check complete and added to box folder?; Yes ...
located at: box/ullyses_tech/ullyses_proposals/survey/revised-mstar-bop.xls
vcheck; S/N ETC calcs done & documented?; Yes
vcheck; Field images checked & saved?; Yes ...
located at: box/ullyses_tech/ullyses_proposals/survey_c29/16853/images/Sz82
vcheck; Selected ACQ strategy?; PSA, MIRRORB, S/N=40
vcheck; Possible ACQ or Sci spoilers?; No
vcheck; Field BOT clear?; Yes ...
GSC II assumes O5V spectral type; ETC calculations cleared
vcheck; Visual BOT check for stars not in catalog?; Yes
vcheck; Orbit packing finalized?; Yes
vcheck; Buffer times optimized?; Yes
vcheck; Verify visit grouping correct; Yes ...
COS visit has GROUP 2C,2D,2S WITHIN 2D
vcheck; phase constraint for ground based observations added?; N/A
vcheck; BETWEENS for coordinated observations added?; Yes ...
26 MAR 2022 00:00 to 29 JUL 2023 00:00
vcheck; Is visit ready for int. review?; Yes
Allocated COS orbits = 6(Tic-Visit
:proposal-id 16853
:visit-id "2C"
:proposal-version -1
:trans-version "20210514"
:date "16-Dec-2021 16:16:12.0"
: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 121952
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16853
:visit-id "2C"
:obset-id "2C"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16853
:visit-id "2C"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2524
: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 2927
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16853
:visit-id "2C"
:orbit-number 2
:pcs-time 392
:si-vis-utilization 2535
: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 2927
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16853
:visit-id "2C"
:orbit-number 3
:pcs-time 392
:si-vis-utilization 2533
:al-overhead-at-end 0
:internal-dur-at-end 372
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2927
:pcs-gap 0
)true30BOP check with 4x spectrum COS.ta.1667099, B.P. = 18.976
Baseline SED with S/N = 40 COS.ta.1667098 requires 120.5142 seconds (x2 = 241.0284 seconds, rounded to 241.0 seconds), B.P. = 1.859BOP check with 4x spectrum COS.sp.1545230, B.P. = 0.064
Baseline SED (scaled with additional A_v = 0.50) calculation for G160M/c1589: COS.sp.1545229, B.P. = 0.005. Total S/N achieved in G160M exposures ~23.0/resel @1548.5 A
sz82_lya2_etc_scaled_pAV0.50.txt; cos,fuv,g160m,c1589,psa,mjd#59670; fp-pos=None, segment=None)
Input file: lowmass_survey_Input-gaia.csv
Spectral type: K5 ; A_V: 0.9 ; Distance (pc): 150
M*: 0.95 ; log(dm/dt): -8.04
For exptime=1009.5 s, spectral region:
1549.0 +- 1.0 A achieves SNR=20.0 / 6-pix-resel for combined c1589 & c1623
The exptime for this c1589 exposure has been halved because c1589 & c1623 target the same line.
A factor of 2.0 has been applied to the exptime in each exposure.
global countrate (brightest segment): 69.6 cts/s/segment
brightest pixel: 0.005 cts/s/pix at 1548.4 A
Calculation performed 2021-10-21T02:37:12, v0.23BOP check with 4x spectrum COS.sp.1545230, B.P. = 0.064
Baseline SED (scaled with additional A_v = 0.50) calculation for G160M/c1589: COS.sp.1545229, B.P. = 0.005. Total S/N achieved in G160M exposures ~23.0/resel @1548.5 A
sz82_lya2_etc_scaled_pAV0.50.txt; cos,fuv,g160m,c1589,psa,mjd#59670; fp-pos=None, segment=None)
Input file: lowmass_survey_Input-gaia.csv
Spectral type: K5 ; A_V: 0.9 ; Distance (pc): 150
M*: 0.95 ; log(dm/dt): -8.04
For exptime=1009.5 s, spectral region:
1549.0 +- 1.0 A achieves SNR=20.0 / 6-pix-resel for combined c1589 & c1623
The exptime for this c1589 exposure has been halved because c1589 & c1623 target the same line.
A factor of 2.0 has been applied to the exptime in each exposure.
global countrate (brightest segment): 69.6 cts/s/segment
brightest pixel: 0.005 cts/s/pix at 1548.4 A
Calculation performed 2021-10-21T02:37:12, v0.23BOP check with 4x spectrum COS.sp.1667108, B.P. = 0.090
Baseline SED (scaled with additional A_v = 0.50) calculation for G130M/c1291: COS.sp.1667107, B.P. = 0.090. Total S/N achieved in G130M exposures ~13.4/resel @1238.9430 A
sz82_lya2_etc_scaled_pAV0.50.txt; cos,fuv,g130m,c1291,psa,mjd#59670; fp-pos=None, segment=None)
Input file: lowmass_survey_Input-gaia.csv
Spectral type: K5 ; A_V: 0.9 ; Distance (pc): 150
M*: 0.95 ; log(dm/dt): -8.04
For exptime=4565.8 s, spectral region:
1239.0 +- 1.0 A achieves SNR=10.0 / 6-pix-resel
A factor of 2.0 has been applied to the exptime in each exposure.
global countrate (brightest segment): 285.3 cts/s/segment
brightest pixel: 0.002 cts/s/pix at 1304.9 A
Calculation performed 2021-10-21T02:37:16, v0.23BOP check with 4x spectrum COS.sp.1667108, B.P. = 0.090
Baseline SED (scaled with additional A_v = 0.50) calculation for G130M/c1291: COS.sp.1667107, B.P. = 0.090. Total S/N achieved in G130M exposures ~13.4/resel @1238.9430 A
sz82_lya2_etc_scaled_pAV0.50.txt; cos,fuv,g130m,c1291,psa,mjd#59670; fp-pos=None, segment=None)
Input file: lowmass_survey_Input-gaia.csv
Spectral type: K5 ; A_V: 0.9 ; Distance (pc): 150
M*: 0.95 ; log(dm/dt): -8.04
For exptime=4565.8 s, spectral region:
1239.0 +- 1.0 A achieves SNR=10.0 / 6-pix-resel
A factor of 2.0 has been applied to the exptime in each exposure.
global countrate (brightest segment): 285.3 cts/s/segment
brightest pixel: 0.002 cts/s/pix at 1304.9 A
Calculation performed 2021-10-21T02:37:16, v0.23Timing link suitability includes constraints ([Group (2C 2D 2S) Within 2.0 days])The scheduling data was generated by CASM 29.2.CASM was run in Phase II mode.vstatus; 2D; SZ82; P/COS ready for internal review; P/AH 27/10/21 ; intrev: not started ; ?/rr DD/MM/YY
vcheck; Enter targ name & Inst. & Resp. Sci.; SZ82 ; COS ; AH
vcheck; ETC numbers entered in APT?; Yes
vcheck; Any screening violations?; No
vcheck; M-dwarf check complete and added to box folder?; Yes ...
located at: box/ullyses_tech/ullyses_proposals/survey/revised-mstar-bop.xls
vcheck; S/N ETC calcs done & documented?; Yes
vcheck; Field images checked & saved?; Yes ...
located at: box/ullyses_tech/ullyses_proposals/survey_c29/16853/images/Sz82
vcheck; Selected ACQ strategy?; PSA, MIRRORB, S/N=40
vcheck; Possible ACQ or Sci spoilers?; No
vcheck; Field BOT clear?; Yes ...
GSC II assumes O5V spectral type; ETC calculations cleared
vcheck; Visual BOT check for stars not in catalog?; Yes
vcheck; Orbit packing finalized?; Yes
vcheck; Buffer times optimized?; Yes
vcheck; Verify visit grouping correct; Yes ...
COS visit has GROUP 2D,2C,2S WITHIN 2D
vcheck; phase constraint for ground based observations added?; N/A
vcheck; BETWEENS for coordinated observations added?; Yes ...
26 MAR 2022 00:00 to 29 JUL 2023 00:00
vcheck; Is visit ready for int. review?; Yes
Allocated COS orbits = 6(Tic-Visit
:proposal-id 16853
:visit-id "2D"
:proposal-version -1
:trans-version "20210514"
:date "16-Dec-2021 16:16:13.0"
: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 121952
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16853
:visit-id "2D"
:obset-id "2D"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16853
:visit-id "2D"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2534
: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 2927
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16853
:visit-id "2D"
:orbit-number 2
:pcs-time 392
:si-vis-utilization 2535
: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 2927
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16853
:visit-id "2D"
:orbit-number 3
:pcs-time 392
:si-vis-utilization 2533
:al-overhead-at-end 0
:internal-dur-at-end 372
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2927
:pcs-gap 0
)true30BOP check with 4x spectrum COS.ta.1667099, B.P. = 18.976
Baseline SED with S/N = 40 COS.ta.1667098 requires 120.5142 seconds (x2 = 241.0284 seconds, rounded to 241.0 seconds), B.P. = 1.859BOP check with 4x spectrum COS.sp.1545232, B.P. = 0.064
Baseline SED (scaled with additional A_v = 0.50) calculation for G160M/c1623: COS.sp.1545231, B.P. = 0.005. Total S/N achieved in G160M exposures ~23.0/resel @1548.5 A
sz82_lya2_etc_scaled_pAV0.50.txt; cos,fuv,g160m,c1623,psa,mjd#59670; fp-pos=None, segment=None)
Input file: lowmass_survey_Input-gaia.csv
Spectral type: K5 ; A_V: 0.9 ; Distance (pc): 150
M*: 0.95 ; log(dm/dt): -8.04
For exptime=1002.7 s, spectral region:
1549.0 +- 1.0 A achieves SNR=20.0 / 6-pix-resel for combined c1589 & c1623
The exptime for this c1623 exposure has been halved because c1589 & c1623 target the same line.
A factor of 2.0 has been applied to the exptime in each exposure.
global countrate (brightest segment): 69.0 cts/s/segment
brightest pixel: 0.005 cts/s/pix at 1548.4 A
Calculation performed 2021-10-21T02:37:14, v0.23BOP check with 4x spectrum COS.sp.1545232, B.P. = 0.064
Baseline SED (scaled with additional A_v = 0.50) calculation for G160M/c1623: COS.sp.1545231, B.P. = 0.005. Total S/N achieved in G160M exposures ~23.0/resel @1548.5 A
sz82_lya2_etc_scaled_pAV0.50.txt; cos,fuv,g160m,c1623,psa,mjd#59670; fp-pos=None, segment=None)
Input file: lowmass_survey_Input-gaia.csv
Spectral type: K5 ; A_V: 0.9 ; Distance (pc): 150
M*: 0.95 ; log(dm/dt): -8.04
For exptime=1002.7 s, spectral region:
1549.0 +- 1.0 A achieves SNR=20.0 / 6-pix-resel for combined c1589 & c1623
The exptime for this c1623 exposure has been halved because c1589 & c1623 target the same line.
A factor of 2.0 has been applied to the exptime in each exposure.
global countrate (brightest segment): 69.0 cts/s/segment
brightest pixel: 0.005 cts/s/pix at 1548.4 A
Calculation performed 2021-10-21T02:37:14, v0.23BOP check with 4x spectrum COS.sp.1667108, B.P. = 0.090
Baseline SED (scaled with additional A_v = 0.50) calculation for G130M/c1291: COS.sp.1667107, B.P. = 0.090. Total S/N achieved in G130M exposures ~13.4/resel @1238.9430 A
sz82_lya2_etc_scaled_pAV0.50.txt; cos,fuv,g130m,c1291,psa,mjd#59670; fp-pos=None, segment=None)
Input file: lowmass_survey_Input-gaia.csv
Spectral type: K5 ; A_V: 0.9 ; Distance (pc): 150
M*: 0.95 ; log(dm/dt): -8.04
For exptime=4565.8 s, spectral region:
1239.0 +- 1.0 A achieves SNR=10.0 / 6-pix-resel
A factor of 2.0 has been applied to the exptime in each exposure.
global countrate (brightest segment): 285.3 cts/s/segment
brightest pixel: 0.002 cts/s/pix at 1304.9 A
Calculation performed 2021-10-21T02:37:16, v0.23BOP check with 4x spectrum COS.sp.1667108, B.P. = 0.090
Baseline SED (scaled with additional A_v = 0.50) calculation for G130M/c1291: COS.sp.1667107, B.P. = 0.090. Total S/N achieved in G130M exposures ~13.4/resel @1238.9430 A
sz82_lya2_etc_scaled_pAV0.50.txt; cos,fuv,g130m,c1291,psa,mjd#59670; fp-pos=None, segment=None)
Input file: lowmass_survey_Input-gaia.csv
Spectral type: K5 ; A_V: 0.9 ; Distance (pc): 150
M*: 0.95 ; log(dm/dt): -8.04
For exptime=4565.8 s, spectral region:
1239.0 +- 1.0 A achieves SNR=10.0 / 6-pix-resel
A factor of 2.0 has been applied to the exptime in each exposure.
global countrate (brightest segment): 285.3 cts/s/segment
brightest pixel: 0.002 cts/s/pix at 1304.9 A
Calculation performed 2021-10-21T02:37:16, v0.23Timing link suitability includes constraints ([Group (2C 2D 2S) Within 2.0 days])The scheduling data was generated by CASM 29.2.CASM was run in Phase II mode.vstatus; 2S; SZ82; S/STIS ready for internal review; S/AH 27/10/21 ; intrev: not started ; ?/rr DD/MM/YY
vcheck; Enter targ name & Inst. & Resp. Sci.; SZ82 ; STIS ; AH
vcheck; ETC numbers entered in APT?; Yes
vcheck; Any screening violations?; No
vcheck; M-dwarf check complete and added to box folder?; Yes ...
located at: box/ullyses_tech/ullyses_proposals/survey/revised-mstar-bop.xls
vcheck; S/N ETC calcs done & documented?; Yes
vcheck; Field images checked & saved?; Yes ...
located at: box/ullyses_tech/ullyses_proposals/survey_c29/16853/images/Sz82
vcheck; Selected ACQ strategy?; V-mag with F28X50LP, S/N=80
vcheck; Possible ACQ or Sci spoilers?; No
vcheck; Field BOT clear?; Yes
vcheck; Visual BOT check for stars not in catalog?; Yes
vcheck; Orbit packing finalized?; Yes
vcheck; Buffer times optimized?; Yes
vcheck; Verify visit grouping correct; Yes ...
STIS visit has GROUP 2S,2C,2D WITHIN 2D
vcheck; phase constraint for ground based observations added?; N/A
vcheck; BETWEENS for coordinated observations added?; Yes ...
26 MAR 2022 00:00 to 29 JUL 2023 00:00
vcheck; Is visit ready for int. review?; Yes
Allocated STIS orbits = 1(Tic-Visit
:proposal-id 16853
:visit-id "2S"
:proposal-version -1
:trans-version "20210514"
:date "16-Dec-2021 16:16:14.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 1
:saa-model "24"
:si-bright-earth-limb-angle 20.0
:data-volume 377840
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16853
:visit-id "2S"
:obset-id "2S"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16853
:visit-id "2S"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2534
:al-overhead-at-end 116
:internal-dur-at-end 1192
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2927
:pcs-gap 0
)true104x BOP check: STIS.ta.1667111, B.P. = 1,248.150, with F25ND3 filter
Baseline SED (K5V 4250 4.5 spectrum renormalized to Johnson V = 11.63 vegamag) with S/N = 80: STIS.ta.1667110 requires 6.4698 seconds (x2 =12.9396 seconds, rounded to 12.9 seconds) , B.P. = 377.956BOP check with 4x spectrum: STIS.sp.1667116, B.P. = 0.697
Baseline ETC calc with spectrum: STIS.sp.1667115, B.P. = 0.093
sz82_lya2_etc_scaled_pAV0.50.txt; stis,nuvmama,g230l,c2376,52x2,mjd#59670
Input file: lowmass_survey_Input-gaia.csv
Spectral type: K5 ; A_V: 0.9 ; Distance (pc): 150
M*: 0.95 ; log(dm/dt): -8.04
For exptime=109.5 s, spectral region:
2800.0 +- 15.0 A achieves SNR=20.0 / 2-pix-resel
A factor of 2.0 has been applied to the exptime in each exposure.
global countrate (brightest segment): 2479.6 cts/s/segment
brightest pixel: 0.749 cts/s/pix at 2788.8 A
Calculation performed 2021-10-21T02:37:16, v0.23Calculation with Castelli-Kurucz K5V 4250 4.5 stellar model, normalized to Johnson/V = 11.63, for G430L: STIS.sp.1667117, B.P. = 92.412
BOP calculation with Castelli-Kurucz K5V 4250 4.5 stellar model, normalized to Johnson/V = 11.63 - 1.5 = 10.13: STIS.sp.1667118, B.P. = 382.639.
sz82_lya2_etc_scaled_pAV0.50.txt; stis,ccd,g430l,c4300,52x2,mjd#59670
WARNING: operating mode = ACCUM
Input file: lowmass_survey_Input-gaia.csv
Spectral type: K5 ; A_V: 0.9 ; Distance (pc): 150
M*: 0.95 ; log(dm/dt): -8.04
For exptime=37.2 s, n_reads=2, spectral region:
4000.0 +- 5.0 A achieves SNR=20.0 / 2-pix-resel
A factor of 2.0 has been applied to the exptime in each exposure.
global countrate (brightest segment): 51189.8 cts/s/segment
brightest pixel: 32.056 cts/s/pix at 4871.0 A
Calculation performed 2021-10-21T02:37:16, v0.23Calculation with Castelli-Kurucz K5V 4250 4.5 stellar model, normalized to Johnson/V = 11.63, for G750L: STIS.sp.1667119, B.P. = 230.316
BOP calculation with Castelli-Kurucz K5V 4250 4.5 stellar model, normalized to Johnson/V = 11.63 - 1.5 = 10.13: STIS.sp.1667120, B.P. = 783.101.
sz82_lya2_etc_scaled_pAV0.50.txt; stis,ccd,g750l,c7751,52x2,mjd#59670
WARNING: operating mode = ACCUM
Input file: lowmass_survey_Input-gaia.csv
Spectral type: K5 ; A_V: 0.9 ; Distance (pc): 150
M*: 0.95 ; log(dm/dt): -8.04
For exptime=2.8 s, n_reads=2, spectral region:
5700.0 +- 5.0 A achieves SNR=20.0 / 2-pix-resel
A factor of 2.0 has been applied to the exptime in each exposure.
global countrate (brightest segment): 141994.5 cts/s/segment
brightest pixel: 281.897 cts/s/pix at 6563.9 A
Calculation performed 2021-10-21T02:37:16, v0.23Timing link suitability includes constraints ([Group (3C 3S) Within 1.0 days])The scheduling data was generated by CASM 29.2.CASM was run in Phase II mode.vstatus; 3C; SZ84; P/COS ready for internal review; P/AH 27/10/21 ; intrev: not started ; ?/rr DD/MM/YY
vcheck; Enter targ name & Inst. & Resp. Sci.; SZ84 ; COS ; AH
vcheck; ETC numbers entered in APT?; Yes
vcheck; Any screening violations?; No
vcheck; M-dwarf check complete and added to box folder?; Yes ...
located at: box/ullyses_tech/ullyses_proposals/survey/revised-mstar-bop.xls
vcheck; S/N ETC calcs done & documented?; Yes
vcheck; Field images checked & saved?; Yes ...
located at: box/ullyses_tech/ullyses_proposals/survey_c29/16853/images/Sz84
vcheck; Selected ACQ strategy?; PSA, MIRRORB, S/N=40
vcheck; Possible ACQ or Sci spoilers?; No
vcheck; Field BOT clear?; Yes
vcheck; Visual BOT check for stars not in catalog?; Yes
vcheck; Orbit packing finalized?; Yes
vcheck; Buffer times optimized?; Yes
vcheck; Verify visit grouping correct; Yes ...
COS visit has GROUP 3C,3S WITHIN 1D
vcheck; phase constraint for ground based observations added?; N/A
vcheck; BETWEENS for coordinated observations added?; Yes ...
26 MAR 2022 00:00 to 29 JUL 2023 00:00
vcheck; Is visit ready for int. review?; Yes
Allocated COS orbits = 3(Tic-Visit
:proposal-id 16853
:visit-id "3C"
:proposal-version -1
:trans-version "20210514"
:date "16-Dec-2021 16:16:16.0"
:trans-errors '(:WARNINGS 1 :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 278496
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16853
:visit-id "3C"
:obset-id "3C"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16853
:visit-id "3C"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2533
: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 2927
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16853
:visit-id "3C"
:orbit-number 2
:pcs-time 392
:si-vis-utilization 2534
: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 2927
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16853
:visit-id "3C"
:orbit-number 3
:pcs-time 392
:si-vis-utilization 2522
: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 2927
:pcs-gap 0
)true30BOP check with 4x spectrum COS.ta.1679234, B.P. = 39.943
Baseline SED with S/N = 40 COS.ta.1679225 requires 40.5446 seconds (x2 = 81.0892 seconds, rounded to 81.1 seconds), B.P. = 5.496BOP check with 4x spectrum COS.ta.1679236, B.P. = 0.183
M dwarf flare spectrum COS.ta.1679237, B.P. = 0.846
Baseline SED (scaled with additional A_v = 0.50) calculation for G130M/c1291: COS.ta.1679235, B.P. = 0.090.
Total S/N achieved in G130M exposures ~17.5/resel @1238.8743 A
sz84_lya2_etc_scaled_pAV0.50.txt; cos,fuv,g130m,c1291,psa,mjd#59670; fp-pos=None, segment=None)
Input file: lowmass_survey_Input-gaia.csv
Spectral type: M5 ; A_V: 0.0 ; Distance (pc): 150
M*: 0.16 ; log(dm/dt): -9.21
For exptime=613.6 s, spectral region:
1239.0 +- 1.0 A achieves SNR=10.0 / 6-pix-resel
A factor of 2.0 has been applied to the exptime in each exposure.
global countrate (brightest segment): 380.5 cts/s/segment
brightest pixel: 0.037 cts/s/pix at 1304.8 A
Calculation performed 2021-10-21T02:39:09, v0.23BOP check with 4x spectrum COS.ta.1679236, B.P. = 0.183
M dwarf flare spectrum COS.ta.1679237, B.P. = 0.846
Baseline SED (scaled with additional A_v = 0.50) calculation for G130M/c1291: COS.ta.1679235, B.P. = 0.090.
Total S/N achieved in G130M exposures ~17.5/resel @1238.8743 A
sz84_lya2_etc_scaled_pAV0.50.txt; cos,fuv,g130m,c1291,psa,mjd#59670; fp-pos=None, segment=None)
Input file: lowmass_survey_Input-gaia.csv
Spectral type: M5 ; A_V: 0.0 ; Distance (pc): 150
M*: 0.16 ; log(dm/dt): -9.21
For exptime=613.6 s, spectral region:
1239.0 +- 1.0 A achieves SNR=10.0 / 6-pix-resel
A factor of 2.0 has been applied to the exptime in each exposure.
global countrate (brightest segment): 380.5 cts/s/segment
brightest pixel: 0.037 cts/s/pix at 1304.8 A
Calculation performed 2021-10-21T02:39:09, v0.23BOP check with 4x spectrum COS.sp.1667167, B.P. = 0.137
M dwarf flare spectrum COS.sp.1667168, B.P. = 1.528
Baseline SED (scaled with additional A_v = 0.50) calculation for G160M/c1589: COS.sp.1667166, B.P. = 0.010.
Total S/N achieved in G160M exposures ~33.2/resel @1548.4366 A
sz84_lya2_etc_scaled_pAV0.50.txt; cos,fuv,g160m,c1589,psa,mjd#59670; fp-pos=None, segment=None)
Input file: lowmass_survey_Input-gaia.csv
Spectral type: M5 ; A_V: 0.0 ; Distance (pc): 150
M*: 0.16 ; log(dm/dt): -9.21
For exptime=829.6 s, spectral region:
1549.0 +- 1.0 A achieves SNR=20.0 / 6-pix-resel for combined c1589 & c1623
The exptime for this c1589 exposure has been halved because c1589 & c1623 target the same line.
A factor of 2.0 has been applied to the exptime in each exposure.
global countrate (brightest segment): 95.4 cts/s/segment
brightest pixel: 0.010 cts/s/pix at 1446.2 A
Calculation performed 2021-10-21T02:39:05, v0.23BOP check with 4x spectrum COS.sp.1667167, B.P. = 0.137
M dwarf flare spectrum COS.sp.1667168, B.P. = 1.528
Baseline SED (scaled with additional A_v = 0.50) calculation for G160M/c1589: COS.sp.1667166, B.P. = 0.010.
Total S/N achieved in G160M exposures ~33.2/resel @1548.4366 A
sz84_lya2_etc_scaled_pAV0.50.txt; cos,fuv,g160m,c1589,psa,mjd#59670; fp-pos=None, segment=None)
Input file: lowmass_survey_Input-gaia.csv
Spectral type: M5 ; A_V: 0.0 ; Distance (pc): 150
M*: 0.16 ; log(dm/dt): -9.21
For exptime=829.6 s, spectral region:
1549.0 +- 1.0 A achieves SNR=20.0 / 6-pix-resel for combined c1589 & c1623
The exptime for this c1589 exposure has been halved because c1589 & c1623 target the same line.
A factor of 2.0 has been applied to the exptime in each exposure.
global countrate (brightest segment): 95.4 cts/s/segment
brightest pixel: 0.010 cts/s/pix at 1446.2 A
Calculation performed 2021-10-21T02:39:05, v0.23BOP check with 4x spectrum COS.sp.1667171, B.P. = 0.130
M dwarf flare spectrum COS.sp.1667172, B.P. = 1.539
Baseline SED (scaled with additional A_v = 0.50) calculation for G160M/c1623: COS.sp.1667170, B.P. = 0.009.
Total S/N achieved in G160M exposures ~33.2/resel @1548.4366 A
sz84_lya2_etc_scaled_pAV0.50.txt; cos,fuv,g160m,c1623,psa,mjd#59670; fp-pos=None, segment=None)
Input file: lowmass_survey_Input-gaia.csv
Spectral type: M5 ; A_V: 0.0 ; Distance (pc): 150
M*: 0.16 ; log(dm/dt): -9.21
For exptime=849.0 s, spectral region:
1549.0 +- 1.0 A achieves SNR=20.0 / 6-pix-resel for combined c1589 & c1623
The exptime for this c1623 exposure has been halved because c1589 & c1623 target the same line.
A factor of 2.0 has been applied to the exptime in each exposure.
global countrate (brightest segment): 89.9 cts/s/segment
brightest pixel: 0.009 cts/s/pix at 1446.2 A
Calculation performed 2021-10-21T02:39:07, v0.23BOP check with 4x spectrum COS.sp.1667171, B.P. = 0.130
M dwarf flare spectrum COS.sp.1667172, B.P. = 1.539
Baseline SED (scaled with additional A_v = 0.50) calculation for G160M/c1623: COS.sp.1667170, B.P. = 0.009.
Total S/N achieved in G160M exposures ~33.2/resel @1548.4366 A
sz84_lya2_etc_scaled_pAV0.50.txt; cos,fuv,g160m,c1623,psa,mjd#59670; fp-pos=None, segment=None)
Input file: lowmass_survey_Input-gaia.csv
Spectral type: M5 ; A_V: 0.0 ; Distance (pc): 150
M*: 0.16 ; log(dm/dt): -9.21
For exptime=849.0 s, spectral region:
1549.0 +- 1.0 A achieves SNR=20.0 / 6-pix-resel for combined c1589 & c1623
The exptime for this c1623 exposure has been halved because c1589 & c1623 target the same line.
A factor of 2.0 has been applied to the exptime in each exposure.
global countrate (brightest segment): 89.9 cts/s/segment
brightest pixel: 0.009 cts/s/pix at 1446.2 A
Calculation performed 2021-10-21T02:39:07, v0.23Timing link suitability includes constraints ([Group (3C 3S) Within 1.0 days])The scheduling data was generated by CASM 29.2.CASM was run in Phase II mode.vstatus; 3S;SZ84; P/STIS ready for internal review; P/AH 27/10/21 ; intrev: not started ; ?/rr DD/MM/YY
vcheck; Enter targ name & Inst. & Resp. Sci.; SZ84 ; STIS ; AH
vcheck; ETC numbers entered in APT?; Yes
vcheck; Any screening violations?; No
vcheck; M-dwarf check complete and added to box folder?; Yes ...
located at: box/ullyses_tech/ullyses_proposals/survey/revised-mstar-bop.xls
vcheck; S/N ETC calcs done & documented?; Yes
vcheck; Field images checked & saved?; Yes ...
located at: box/ullyses_tech/ullyses_proposals/survey_c29/16853/images/Sz84
vcheck; Selected ACQ strategy?; V-mag with F28X50LP, S/N=80
vcheck; Possible ACQ or Sci spoilers?; No
vcheck; Field BOT clear?; Yes
vcheck; Visual BOT check for stars not in catalog?; Yes
vcheck; Orbit packing finalized?; Yes
vcheck; Buffer times optimized?; Yes
vcheck; Verify visit grouping correct; Yes ...
STIS visit has GROUP 3S,3C WITHIN 1D
vcheck; phase constraint for ground based observations added?; N/A
vcheck; BETWEENS for coordinated observations added?; Yes ...
26 MAR 2022 00:00 to 29 JUL 2023 00:00
vcheck; Is visit ready for int. review?; Yes
Allocated STIS orbits = 2 (constrained in input CSV)(Tic-Visit
:proposal-id 16853
:visit-id "3S"
:proposal-version -1
:trans-version "20210514"
:date "16-Dec-2021 16:16:17.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 1
:saa-model "24"
:si-bright-earth-limb-angle 20.0
:data-volume 377824
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16853
:visit-id "3S"
:obset-id "3S"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16853
:visit-id "3S"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2534
:al-overhead-at-end 116
:internal-dur-at-end 1192
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2927
:pcs-gap 0
)true104x BOP check: STIS.ta.1667306, B.P. = 9,014.183
Baseline SED (Castelli-Kurucz M6V 3500 5.0 spectrum renormalized to Johnson V = 16.12 vegamag) with S/N = 80: STIS.ta.1667305 requires 1.0219 seconds (x2 = 2.0438 seconds, rounded to 2.0 seconds), B.P. = 2,264.317BOP check with 4x spectrum: STIS.sp.1667316, B.P. = 11.593
M dwarf flare spectrum STIS.sp.1667317, B.P. = 7.712
Baseline ETC calc with spectrum: STIS.sp.1667315, B.P. = 1.196
sz84_lya2_etc_scaled_pAV0.50.txt; stis,nuvmama,g230l,c2376,52x2,mjd#59670
Input file: lowmass_survey_Input-gaia.csv
Spectral type: M5 ; A_V: 0.0 ; Distance (pc): 150
M*: 0.16 ; log(dm/dt): -9.21
For exptime=68.2 s, spectral region:
2800.0 +- 15.0 A achieves SNR=20.0 / 2-pix-resel
A factor of 2.0 has been applied to the exptime in each exposure.
global countrate (brightest segment): 2439.4 cts/s/segment
brightest pixel: 1.196 cts/s/pix at 2796.8 A
Calculation performed 2021-10-21T02:39:09, v0.23Calculation with Castelli-Kurucz M6V 3500 5.0 stellar model, normalized to Johnson/V = 16.12, for G430L: STIS.sp.1667318, B.P. = 1.762
BOP calculation with Castelli-Kurucz M6V 3500 5.0 stellar model, normalized to Johnson/V = 16.12 - 1.5 = 14.62: STIS.sp.1667319, B.P. = 6.928.
sz84_lya2_etc_scaled_pAV0.50.txt; stis,ccd,g430l,c4300,52x2,mjd#59670
WARNING: operating mode = ACCUM
Input file: lowmass_survey_Input-gaia.csv
Spectral type: M5 ; A_V: 0.0 ; Distance (pc): 150
M*: 0.16 ; log(dm/dt): -9.21
For exptime=29.4 s, n_reads=2, spectral region:
4000.0 +- 5.0 A achieves SNR=20.0 / 2-pix-resel
A factor of 2.0 has been applied to the exptime in each exposure.
global countrate (brightest segment): 51280.9 cts/s/segment
brightest pixel: 34.619 cts/s/pix at 4560.5 A
Calculation performed 2021-10-21T02:39:10, v0.23Calculation with Castelli-Kurucz M6V 3500 5.0 stellar model, normalized to Johnson/V = 16.12, for G750L: STIS.sp.1667320, B.P. = 6.855
BOP calculation with Castelli-Kurucz M6V 3500 5.0 stellar model, normalized to Johnson/V = 16.12 - 1.5 = 14.62: STIS.sp.1667321, B.P. = 27.200.
sz84_lya2_etc_scaled_pAV0.50.txt; stis,ccd,g750l,c7751,52x2,mjd#59670
WARNING: operating mode = ACCUM
Input file: lowmass_survey_Input-gaia.csv
Spectral type: M5 ; A_V: 0.0 ; Distance (pc): 150
M*: 0.16 ; log(dm/dt): -9.21
For exptime=2.9 s, n_reads=2, spectral region:
5700.0 +- 5.0 A achieves SNR=20.0 / 2-pix-resel
A factor of 2.0 has been applied to the exptime in each exposure.
global countrate (brightest segment): 119645.6 cts/s/segment
brightest pixel: 251.137 cts/s/pix at 6563.9 A
Calculation performed 2021-10-21T02:39:10, v0.23