The list of Investigators does not match the STScI records for this program.
INEFFICIENT ORDERING OF FP-POS POSITIONS
INEFFICIENT ORDERING OF FP-POS POSITIONS
INEFFICIENT ORDERING OF FP-POS POSITIONS
INEFFICIENT ORDERING OF FP-POS POSITIONS10-Jan-2022:
27 orbits were allocated, but only 26 are needed526569938----- Attempting Submission 1 (Mon Jan 10 19:42:14 GMT 2022) -----List of investigators reflects changes to ULLYSES staff
Inefficient FP-POS changes are always hidden within occultationULLYSES M-Type T Tauri Survey Stars in Lupus III: Part 2The 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 STARNOSZ103 : HBC 618
Region: Lupus III
Simbad: http://simbad.u-strasbg.fr/simbad/sim-id?Ident=sz103&submit=submit+id
Target coordinates are from Gaia DR2.
Spectral type: M4 ; A_V: 0.7 ; Distance (pc): 200
M*: 0.22 ; log(dm/dt): -8.99
Input file: lowmass_survey_Input-gaia.csv
sz103_lya2_etc_scaled_pAV0.50.txt
Calculation performed 2021-10-21T02:38:32, v0.8
-------------------------------------------------------------------------------
tstatus; SZ103; P/COS approved for submission; S/STIS approved for submission; P/WF 10/01/22; S/WF 10/01/22
tcheck; APT/SIMBAD target names: ; 2MASS J16083026-3906111; HBC 618
tcheck; Target info verification status?; OK
tcheck; Coordinates & P.M. verified, epoch checked?; yes
tcheck; Adopted SED compared to Observations?; yes ...
VRI photometry is only 12-61% of CTTS template; use M4 model in opticalHBC-618J2000SpT=M4; A_V=0.70; V=16.58; J=11.38START TAURI STARPRE-MAIN SEQUENCE STARNOSZ110 : V1193 Sco
Region: Lupus III
Simbad: http://simbad.u-strasbg.fr/simbad/sim-id?Ident=sz110&submit=submit+id
Target coordinates are from Gaia DR2.
Spectral type: M4 ; A_V: 0.0 ; Distance (pc): 200
M*: 0.22 ; log(dm/dt): -8.53
Input file: lowmass_survey_Input-gaia.csv
sz110_lya2_etc_scaled_pAV0.50.txt
Calculation performed 2021-10-21T02:38:41, v0.8
-------------------------------------------------------------------------------
tstatus; SZ110; P/COS approved for submission; S/STIS approved for submission; P/WF 10/01/22; S/WF 10/01/22
tcheck; APT/SIMBAD target names: ; HBC 621; V1193 Sco
tcheck; Target info verification status?; OK
tcheck; Coordinates & P.M. verified, epoch checked?; yes
tcheck; Adopted SED compared to Observations?; yes ...
BVRI photometry is only 16-59% of CTTS template; use M4 model in opticalV1193-SCOJ2000SpT=M4; A_V=0.00; B=15.95; V=14.99; J=10.97START TAURI STARPRE-MAIN SEQUENCE STARNOSZ99
Region: Lupus III
Simbad: http://simbad.u-strasbg.fr/simbad/sim-id?Ident=sz99&submit=submit+id
Target coordinates are from Gaia DR2.
Spectral type: M4 ; A_V: 0.0 ; Distance (pc): 200
M*: 0.23 ; log(dm/dt): -9.41
Input file: lowmass_survey_Input-gaia.csv
sz99_lya2_etc_scaled_pAV0.50.txt
Calculation performed 2021-10-21T02:38:22, v0.8
-------------------------------------------------------------------------------
tstatus; SZ99; P/COS approved for submission; S/STIS approved for submission; P/WF 10/01/22; S/WF 10/01/22
tcheck; APT/SIMBAD target names: ; 2MASS J16082404-3905494
tcheck; Target info verification status?; OK
tcheck; Coordinates & P.M. verified, epoch checked?; yes
tcheck; Adopted SED compared to Observations?; Adopted SED compared to Observations?; yes ...
BVRI photometry is only 7-25% of CTTS template; use M4 model in optical
For the M dwarf check of Sz 99, we use A_V = 0.4, reported by Mortier et al. (2011, MNRAS, 418, 1194); henceforth M11. This is more reasonable than the A_V = 0.0 reported by Alcala et al. (2014, A&A, 561, A2); henceforth A14. Both M11 and A14 compare spectra of Sz 99 to templates to derive A_V. M11 use a field dwarf as a template, which almost certainly has A_V = 0. A14 use TWA 9B as a template and do not seem to allow for the fact that it may have A_V > 0. This does not affect exposure time estimates, since these were conservatively calculated assuming A_V = 0.5.J2000SpT=M4; A_V=0.00; B=17.69; V=17.05; J=11.93STARA4-A9 III-INOThis object was generated by the targetselector and retrieved from the SIMBAD database.
Manually added coordinate uncertainties, parallax, and data in "other fluxes"
Offset acquisition star for Sz 103HR-5999HD-144668J2000SpT=A7III; A_V=0.33; U=7.66; B=7.41; V=7.05; J=5.91/Users/wfischer/Box/ullyses_tech/ullyses_proposals/survey_c29/16856/OP-cache/ULLYSES_16856-v1C.xmlTiming link suitability includes constraints ([Group (1C 1D 1E 1F 1G 1S) Within 2.0 days])The scheduling data was generated by CASM 29.2.CASM was run in Phase II mode.vstatus; 1C; SZ103; P/COS approved for submission; P/WF 10/01/22 ; intrev: complete ; P/JRD 10/01/22
vcheck; Enter targ name & Inst. & Resp. Sci.; Sz 103 ; COS ; WF
vcheck; ETC numbers entered in APT?; yes ...
see comments in the STIS acquisition for details about the hybrid model used
vcheck; Any screening violations?; no
vcheck; M-dwarf check complete and added to box folder?; yes ...
located at: ~/Box/ullyses_tech/ullyses_proposals/survey_c29/16856/sz-103/mdwarf/
vcheck; S/N ETC calcs done & documented?; yes
vcheck; Field images checked & saved?; yes, no GALEX coverage ...
located at: ~/Box/ullyses_tech/ullyses_proposals/survey_c29/16856/sz-103/
vcheck; Selected ACQ strategy?; yes; BOA/MirrorB on offset target V856 Sco
vcheck; Possible ACQ or Sci spoilers?; no
vcheck; Field BOT clear?; yes ...
see ~/Box/ullyses_tech/ullyses_proposals/survey_c29/16856/sz-103/field/
vcheck; Visual BOT check for stars not in catalog?; yes
vcheck; Orbit packing finalized?; yes ...
G130M gets 114% of requested time; G160M gets 86% of requested time
vcheck; Buffer times optimized?; yes
vcheck; Verify visit grouping correct; yes
vcheck; phase constraint for ground based observations added?; N/A
vcheck; BETWEENS for coordinated observations added?; yes
vcheck; Is visit ready for int. review?; yes
Allocated COS orbits = 14(Tic-Visit
:proposal-id 16856
:visit-id "1C"
:proposal-version -1
:trans-version "20210514"
:date "10-Jan-2022 14:23:57.0"
: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 252288
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16856
:visit-id "1C"
:obset-id "1C"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16856
:visit-id "1C"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2534
:al-overhead-at-end 0
:internal-dur-at-end 114
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2927
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16856
:visit-id "1C"
:orbit-number 2
:pcs-time 392
:si-vis-utilization 2535
:al-overhead-at-end 0
:internal-dur-at-end 114
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2927
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16856
:visit-id "1C"
:orbit-number 3
:pcs-time 392
:si-vis-utilization 2535
:al-overhead-at-end 0
:internal-dur-at-end 410
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2927
:pcs-gap 0
)true30Due to M dwarf rules, perform an offset acquisition on V856 Sco (HD 144668; HR 5999), the southern of the pair of bright stars in the region. SIMBAD says it's an A7III star with U = 7.66. With X-Shooter data, Fairlamb et al. (2015) found T_eff = 8500 K and A_V = 0.33. For the ETC calculation, use the Pickles A5III (T_eff = 8452.79 K) model with E(B-V) = A_V / 3.1 = 0.11, normalized to U = 7.66. With BOA/MirrorB (ETC 1548163), the brightest pixel is 9.286 cts/s, so the star could be 5 times brighter and still not violate the limit. The exposure time to hit the recommended S/N = 30 is 13.5 sec, which is doubled to guard against faintness.
See ~/Box/ullyses_tech/ullyses_proposals/survey_c29/16856/sz-103/offset/offset_notes.rtf for additional notes and plots.ETC exposure time is 3128 s per G130M setting. This exposure will be coadded with others.
Worst-case ETC run (1666793) gives 0.09 cts/s in brightest pixel and buffer time of 6108 s
M dwarf flare ETC run (1666794) gives 0.18 cts/s in brightest pixel
Buffer time set to exposure time
sz103_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: M4 ; A_V: 0.7 ; Distance (pc): 200
M*: 0.22 ; log(dm/dt): -8.99
For exptime=6254.5 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): 291.0 cts/s/segment
brightest pixel: 0.005 cts/s/pix at 1304.8 A
Calculation performed 2021-10-21T02:38:31, v0.23ETC exposure time is 3128 s per G130M setting. This exposure will be coadded with others.
Worst-case ETC run (1666793) gives 0.09 cts/s in brightest pixel and buffer time of 6108 s
M dwarf flare ETC run (1666794) gives 0.18 cts/s in brightest pixel
Buffer time set to exposure time
sz103_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: M4 ; A_V: 0.7 ; Distance (pc): 200
M*: 0.22 ; log(dm/dt): -8.99
For exptime=6254.5 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): 291.0 cts/s/segment
brightest pixel: 0.005 cts/s/pix at 1304.8 A
Calculation performed 2021-10-21T02:38:31, v0.23ETC exposure time is 3128 s per G130M setting. This exposure will be coadded with others.
Worst-case ETC run (1666793) gives 0.09 cts/s in brightest pixel and buffer time of 6108 s
M dwarf flare ETC run (1666794) gives 0.18 cts/s in brightest pixel
Buffer time set to exposure time
sz103_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: M4 ; A_V: 0.7 ; Distance (pc): 200
M*: 0.22 ; log(dm/dt): -8.99
For exptime=6254.5 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): 291.0 cts/s/segment
brightest pixel: 0.005 cts/s/pix at 1304.8 A
Calculation performed 2021-10-21T02:38:31, v0.23/Users/wfischer/Box/ullyses_tech/ullyses_proposals/survey_c29/16856/OP-cache/ULLYSES_16856-v1D.xmlTiming link suitability includes constraints ([Group (1C 1D 1E 1F 1G 1S) Within 2.0 days])The scheduling data was generated by CASM 29.2.CASM was run in Phase II mode.vstatus; 1D; SZ103; P/COS approved for submission; P/WF 10/01/22 ; intrev: complete ; P/JRD 10/01/22
vcheck; Enter targ name & Inst. & Resp. Sci.; Sz 103 ; COS ; WF
vcheck; ETC numbers entered in APT?; yes ...
see comments in the STIS acquisition for details about the hybrid model used
vcheck; Any screening violations?; no
vcheck; M-dwarf check complete and added to box folder?; yes ...
located at: ~/Box/ullyses_tech/ullyses_proposals/survey_c29/16856/sz-103/mdwarf/
vcheck; S/N ETC calcs done & documented?; yes
vcheck; Field images checked & saved?; yes, no GALEX coverage ...
located at: ~/Box/ullyses_tech/ullyses_proposals/survey_c29/16856/sz-103/
vcheck; Selected ACQ strategy?; yes; BOA/MirrorB on offset target V856 Sco
vcheck; Possible ACQ or Sci spoilers?; no
vcheck; Field BOT clear?; yes ...
see ~/Box/ullyses_tech/ullyses_proposals/survey_c29/16856/sz-103/field/
vcheck; Visual BOT check for stars not in catalog?; yes
vcheck; Orbit packing finalized?; yes ...
G130M gets 114% of requested time; G160M gets 86% of requested time
vcheck; Buffer times optimized?; yes
vcheck; Verify visit grouping correct; yes
vcheck; phase constraint for ground based observations added?; N/A
vcheck; BETWEENS for coordinated observations added?; yes
vcheck; Is visit ready for int. review?; yes
Allocated COS orbits = 14(Tic-Visit
:proposal-id 16856
:visit-id "1D"
:proposal-version -1
:trans-version "20210514"
:date "10-Jan-2022 14:23:58.0"
: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 252288
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16856
:visit-id "1D"
:obset-id "1D"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16856
:visit-id "1D"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2534
:al-overhead-at-end 0
:internal-dur-at-end 114
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2927
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16856
:visit-id "1D"
:orbit-number 2
:pcs-time 392
:si-vis-utilization 2535
:al-overhead-at-end 0
:internal-dur-at-end 114
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2927
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16856
:visit-id "1D"
:orbit-number 3
:pcs-time 392
:si-vis-utilization 2535
:al-overhead-at-end 0
:internal-dur-at-end 410
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2927
:pcs-gap 0
)true30Due to M dwarf rules, perform an offset acquisition on V856 Sco (HD 144668; HR 5999), the southern of the pair of bright stars in the region. SIMBAD says it's an A7III star with U = 7.66. With X-Shooter data, Fairlamb et al. (2015) found T_eff = 8500 K and A_V = 0.33. For the ETC calculation, use the Pickles A5III (T_eff = 8452.79 K) model with E(B-V) = A_V / 3.1 = 0.11, normalized to U = 7.66. With BOA/MirrorB (ETC 1548163), the brightest pixel is 9.286 cts/s, so the star could be 5 times brighter and still not violate the limit. The exposure time to hit the recommended S/N = 30 is 13.5 sec, which is doubled to guard against faintness.
See ~/Box/ullyses_tech/ullyses_proposals/survey_c29/16856/sz-103/offset/offset_notes.rtf for additional notes and plots.ETC exposure time is 3128 s per G130M setting. This exposure will be coadded with others.
Worst-case ETC run (1666793) gives 0.09 cts/s in brightest pixel and buffer time of 6108 s
M dwarf flare ETC run (1666794) gives 0.18 cts/s in brightest pixel
Buffer time set to exposure time
sz103_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: M4 ; A_V: 0.7 ; Distance (pc): 200
M*: 0.22 ; log(dm/dt): -8.99
For exptime=6254.5 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): 291.0 cts/s/segment
brightest pixel: 0.005 cts/s/pix at 1304.8 A
Calculation performed 2021-10-21T02:38:31, v0.23ETC exposure time is 3128 s per G130M setting. This exposure will be coadded with others.
Worst-case ETC run (1666793) gives 0.09 cts/s in brightest pixel and buffer time of 6108 s
M dwarf flare ETC run (1666794) gives 0.18 cts/s in brightest pixel
Buffer time set to exposure time
sz103_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: M4 ; A_V: 0.7 ; Distance (pc): 200
M*: 0.22 ; log(dm/dt): -8.99
For exptime=6254.5 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): 291.0 cts/s/segment
brightest pixel: 0.005 cts/s/pix at 1304.8 A
Calculation performed 2021-10-21T02:38:31, v0.23ETC exposure time is 3128 s per G130M setting. This exposure will be coadded with others.
Worst-case ETC run (1666793) gives 0.09 cts/s in brightest pixel and buffer time of 6108 s
M dwarf flare ETC run (1666794) gives 0.18 cts/s in brightest pixel
Buffer time set to exposure time
sz103_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: M4 ; A_V: 0.7 ; Distance (pc): 200
M*: 0.22 ; log(dm/dt): -8.99
For exptime=6254.5 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): 291.0 cts/s/segment
brightest pixel: 0.005 cts/s/pix at 1304.8 A
Calculation performed 2021-10-21T02:38:31, v0.23/Users/wfischer/Box/ullyses_tech/ullyses_proposals/survey_c29/16856/OP-cache/ULLYSES_16856-v1E.xmlTiming link suitability includes constraints ([Group (1C 1D 1E 1F 1G 1S) Within 2.0 days])The scheduling data was generated by CASM 29.2.CASM was run in Phase II mode.vstatus; 1E; SZ103; P/COS approved for submission; P/WF 10/01/22 ; intrev: complete ; P/JRD 10/01/22
vcheck; Enter targ name & Inst. & Resp. Sci.; Sz 103 ; COS ; WF
vcheck; ETC numbers entered in APT?; yes ...
see comments in the STIS acquisition for details about the hybrid model used
vcheck; Any screening violations?; no
vcheck; M-dwarf check complete and added to box folder?; yes ...
located at: ~/Box/ullyses_tech/ullyses_proposals/survey_c29/16856/sz-103/mdwarf/
vcheck; S/N ETC calcs done & documented?; yes
vcheck; Field images checked & saved?; yes, no GALEX coverage ...
located at: ~/Box/ullyses_tech/ullyses_proposals/survey_c29/16856/sz-103/
vcheck; Selected ACQ strategy?; yes; BOA/MirrorB on offset target V856 Sco
vcheck; Possible ACQ or Sci spoilers?; no
vcheck; Field BOT clear?; yes ...
see ~/Box/ullyses_tech/ullyses_proposals/survey_c29/16856/sz-103/field/
vcheck; Visual BOT check for stars not in catalog?; yes
vcheck; Orbit packing finalized?; yes ...
G130M gets 114% of requested time; G160M gets 86% of requested time
vcheck; Buffer times optimized?; yes
vcheck; Verify visit grouping correct; yes
vcheck; phase constraint for ground based observations added?; N/A
vcheck; BETWEENS for coordinated observations added?; yes
vcheck; Is visit ready for int. review?; yes
Allocated COS orbits = 14(Tic-Visit
:proposal-id 16856
:visit-id "1E"
:proposal-version -1
:trans-version "20210514"
:date "10-Jan-2022 14:23:59.0"
: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 252288
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16856
:visit-id "1E"
:obset-id "1E"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16856
:visit-id "1E"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2534
:al-overhead-at-end 0
:internal-dur-at-end 114
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2927
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16856
:visit-id "1E"
:orbit-number 2
:pcs-time 392
:si-vis-utilization 2535
:al-overhead-at-end 0
:internal-dur-at-end 114
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2927
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16856
:visit-id "1E"
:orbit-number 3
:pcs-time 392
:si-vis-utilization 2535
:al-overhead-at-end 0
:internal-dur-at-end 410
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2927
:pcs-gap 0
)true30Due to M dwarf rules, perform an offset acquisition on V856 Sco (HD 144668; HR 5999), the southern of the pair of bright stars in the region. SIMBAD says it's an A7III star with U = 7.66. With X-Shooter data, Fairlamb et al. (2015) found T_eff = 8500 K and A_V = 0.33. For the ETC calculation, use the Pickles A5III (T_eff = 8452.79 K) model with E(B-V) = A_V / 3.1 = 0.11, normalized to U = 7.66. With BOA/MirrorB (ETC 1548163), the brightest pixel is 9.286 cts/s, so the star could be 5 times brighter and still not violate the limit. The exposure time to hit the recommended S/N = 30 is 13.5 sec, which is doubled to guard against faintness.
See ~/Box/ullyses_tech/ullyses_proposals/survey_c29/16856/sz-103/offset/offset_notes.rtf for additional notes and plots.ETC exposure time is 2650 s per G160M setting. This exposure will be coadded with others.
Worst-case ETC run (1666796) gives 0.03 cts/s in brightest pixel and buffer time of 17452 s
M dwarf flare ETC run (1666797) gives 0.34 cts/s in brightest pixel
Buffer time set to exposure time
sz103_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: M4 ; A_V: 0.7 ; Distance (pc): 200
M*: 0.22 ; log(dm/dt): -8.99
For exptime=5300.2 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): 67.7 cts/s/segment
brightest pixel: 0.002 cts/s/pix at 1446.2 A
Calculation performed 2021-10-21T02:38:28, v0.23ETC exposure time is 2650 s per G160M setting. This exposure will be coadded with others.
Worst-case ETC run (1666796) gives 0.03 cts/s in brightest pixel and buffer time of 17452 s
M dwarf flare ETC run (1666797) gives 0.34 cts/s in brightest pixel
Buffer time set to exposure time
sz103_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: M4 ; A_V: 0.7 ; Distance (pc): 200
M*: 0.22 ; log(dm/dt): -8.99
For exptime=5300.2 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): 67.7 cts/s/segment
brightest pixel: 0.002 cts/s/pix at 1446.2 A
Calculation performed 2021-10-21T02:38:28, v0.23ETC exposure time is 2712 s per G160M setting. This exposure will be coadded with others.
Worst-case ETC run (1666799) gives 0.03 cts/s in brightest pixel and buffer time of 19046 s
M dwarf flare ETC run (1666800) gives 0.34 cts/s in brightest pixel
Buffer time set to exposure time
sz103_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: M4 ; A_V: 0.7 ; Distance (pc): 200
M*: 0.22 ; log(dm/dt): -8.99
For exptime=5424.6 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): 66.9 cts/s/segment
brightest pixel: 0.001 cts/s/pix at 1446.2 A
Calculation performed 2021-10-21T02:38:29, v0.23/Users/wfischer/Box/ullyses_tech/ullyses_proposals/survey_c29/16856/OP-cache/ULLYSES_16856-v1F.xmlTiming link suitability includes constraints ([Group (1C 1D 1E 1F 1G 1S) Within 2.0 days])The scheduling data was generated by CASM 29.2.CASM was run in Phase II mode.vstatus; 1F; SZ103; P/COS approved for submission; P/WF 10/01/22 ; intrev: complete ; P/JRD 10/01/22
vcheck; Enter targ name & Inst. & Resp. Sci.; Sz 103 ; COS ; WF
vcheck; ETC numbers entered in APT?; yes ...
see comments in the STIS acquisition for details about the hybrid model used
vcheck; Any screening violations?; no
vcheck; M-dwarf check complete and added to box folder?; yes ...
located at: ~/Box/ullyses_tech/ullyses_proposals/survey_c29/16856/sz-103/mdwarf/
vcheck; S/N ETC calcs done & documented?; yes
vcheck; Field images checked & saved?; yes, no GALEX coverage ...
located at: ~/Box/ullyses_tech/ullyses_proposals/survey_c29/16856/sz-103/
vcheck; Selected ACQ strategy?; yes; BOA/MirrorB on offset target V856 Sco
vcheck; Possible ACQ or Sci spoilers?; no
vcheck; Field BOT clear?; yes ...
see ~/Box/ullyses_tech/ullyses_proposals/survey_c29/16856/sz-103/field/
vcheck; Visual BOT check for stars not in catalog?; yes
vcheck; Orbit packing finalized?; yes ...
G130M gets 114% of requested time; G160M gets 86% of requested time
vcheck; Buffer times optimized?; yes
vcheck; Verify visit grouping correct; yes
vcheck; phase constraint for ground based observations added?; N/A
vcheck; BETWEENS for coordinated observations added?; yes
vcheck; Is visit ready for int. review?; yes
Allocated COS orbits = 14(Tic-Visit
:proposal-id 16856
:visit-id "1F"
:proposal-version -1
:trans-version "20210514"
:date "10-Jan-2022 14:24:00.0"
: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 252288
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16856
:visit-id "1F"
:obset-id "1F"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16856
:visit-id "1F"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2534
:al-overhead-at-end 0
:internal-dur-at-end 114
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2927
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16856
:visit-id "1F"
:orbit-number 2
:pcs-time 392
:si-vis-utilization 2535
:al-overhead-at-end 0
:internal-dur-at-end 114
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2927
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16856
:visit-id "1F"
:orbit-number 3
:pcs-time 392
:si-vis-utilization 2535
:al-overhead-at-end 0
:internal-dur-at-end 410
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2927
:pcs-gap 0
)true30Due to M dwarf rules, perform an offset acquisition on V856 Sco (HD 144668; HR 5999), the southern of the pair of bright stars in the region. SIMBAD says it's an A7III star with U = 7.66. With X-Shooter data, Fairlamb et al. (2015) found T_eff = 8500 K and A_V = 0.33. For the ETC calculation, use the Pickles A5III (T_eff = 8452.79 K) model with E(B-V) = A_V / 3.1 = 0.11, normalized to U = 7.66. With BOA/MirrorB (ETC 1548163), the brightest pixel is 9.286 cts/s, so the star could be 5 times brighter and still not violate the limit. The exposure time to hit the recommended S/N = 30 is 13.5 sec, which is doubled to guard against faintness.
See ~/Box/ullyses_tech/ullyses_proposals/survey_c29/16856/sz-103/offset/offset_notes.rtf for additional notes and plots.ETC exposure time is 2650 s per G160M setting. This exposure will be coadded with others.
Worst-case ETC run (1666796) gives 0.03 cts/s in brightest pixel and buffer time of 17452 s
M dwarf flare ETC run (1666797) gives 0.34 cts/s in brightest pixel
Buffer time set to exposure time
sz103_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: M4 ; A_V: 0.7 ; Distance (pc): 200
M*: 0.22 ; log(dm/dt): -8.99
For exptime=5300.2 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): 67.7 cts/s/segment
brightest pixel: 0.002 cts/s/pix at 1446.2 A
Calculation performed 2021-10-21T02:38:28, v0.23ETC exposure time is 2650 s per G160M setting. This exposure will be coadded with others.
Worst-case ETC run (1666796) gives 0.03 cts/s in brightest pixel and buffer time of 17452 s
M dwarf flare ETC run (1666797) gives 0.34 cts/s in brightest pixel
Buffer time set to exposure time
sz103_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: M4 ; A_V: 0.7 ; Distance (pc): 200
M*: 0.22 ; log(dm/dt): -8.99
For exptime=5300.2 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): 67.7 cts/s/segment
brightest pixel: 0.002 cts/s/pix at 1446.2 A
Calculation performed 2021-10-21T02:38:28, v0.23ETC exposure time is 2712 s per G160M setting. This exposure will be coadded with others.
Worst-case ETC run (1666799) gives 0.03 cts/s in brightest pixel and buffer time of 19046 s
M dwarf flare ETC run (1666800) gives 0.34 cts/s in brightest pixel
Buffer time set to exposure time
sz103_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: M4 ; A_V: 0.7 ; Distance (pc): 200
M*: 0.22 ; log(dm/dt): -8.99
For exptime=5424.6 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): 66.9 cts/s/segment
brightest pixel: 0.001 cts/s/pix at 1446.2 A
Calculation performed 2021-10-21T02:38:29, v0.23/Users/wfischer/Box/ullyses_tech/ullyses_proposals/survey_c29/16856/OP-cache/ULLYSES_16856-v1G.xmlTiming link suitability includes constraints ([Group (1C 1D 1E 1F 1G 1S) Within 2.0 days])The scheduling data was generated by CASM 29.2.CASM was run in Phase II mode.vstatus; 1G; SZ103; P/COS approved for submission; P/WF 10/01/22 ; intrev: complete ; P/JRD 10/01/22
vcheck; Enter targ name & Inst. & Resp. Sci.; Sz 103 ; COS ; WF
vcheck; ETC numbers entered in APT?; yes ...
see comments in the STIS acquisition for details about the hybrid model used
vcheck; Any screening violations?; no
vcheck; M-dwarf check complete and added to box folder?; yes ...
located at: ~/Box/ullyses_tech/ullyses_proposals/survey_c29/16856/sz-103/mdwarf/
vcheck; S/N ETC calcs done & documented?; yes
vcheck; Field images checked & saved?; yes, no GALEX coverage ...
located at: ~/Box/ullyses_tech/ullyses_proposals/survey_c29/16856/sz-103/
vcheck; Selected ACQ strategy?; yes; BOA/MirrorB on offset target V856 Sco
vcheck; Possible ACQ or Sci spoilers?; no
vcheck; Field BOT clear?; yes ...
see ~/Box/ullyses_tech/ullyses_proposals/survey_c29/16856/sz-103/field/
vcheck; Visual BOT check for stars not in catalog?; yes
vcheck; Orbit packing finalized?; yes ...
G130M gets 114% of requested time; G160M gets 86% of requested time
vcheck; Buffer times optimized?; yes
vcheck; Verify visit grouping correct; yes
vcheck; phase constraint for ground based observations added?; N/A
vcheck; BETWEENS for coordinated observations added?; yes
vcheck; Is visit ready for int. review?; yes
Allocated COS orbits = 14(Tic-Visit
:proposal-id 16856
:visit-id "1G"
:proposal-version -1
:trans-version "20210514"
:date "10-Jan-2022 14:24:01.0"
:trans-errors '(:WARNINGS 1 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 2
:saa-model "31"
:si-bright-earth-limb-angle 20.0
:data-volume 52416
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16856
:visit-id "1G"
:obset-id "1G"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16856
:visit-id "1G"
: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 16856
:visit-id "1G"
:orbit-number 2
:pcs-time 392
:si-vis-utilization 2535
:al-overhead-at-end 0
:internal-dur-at-end 334
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2927
:pcs-gap 0
)true20Due to M dwarf rules, perform an offset acquisition on V856 Sco (HD 144668; HR 5999), the southern of the pair of bright stars in the region. SIMBAD says it's an A7III star with U = 7.66. With X-Shooter data, Fairlamb et al. (2015) found T_eff = 8500 K and A_V = 0.33. For the ETC calculation, use the Pickles A5III (T_eff = 8452.79 K) model with E(B-V) = A_V / 3.1 = 0.11, normalized to U = 7.66. With BOA/MirrorB (ETC 1548163), the brightest pixel is 9.286 cts/s, so the star could be 5 times brighter and still not violate the limit. The exposure time to hit the recommended S/N = 30 is 13.5 sec, which is doubled to guard against faintness.
See ~/Box/ullyses_tech/ullyses_proposals/survey_c29/16856/sz-103/offset/offset_notes.rtf for additional notes and plots.ETC exposure time is 2712 s per G160M setting. This exposure will be coadded with others.
Worst-case ETC run (1666799) gives 0.03 cts/s in brightest pixel and buffer time of 19046 s
M dwarf flare ETC run (1666800) gives 0.34 cts/s in brightest pixel
Buffer time set to 2/3 of worst-case result
sz103_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: M4 ; A_V: 0.7 ; Distance (pc): 200
M*: 0.22 ; log(dm/dt): -8.99
For exptime=5424.6 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): 66.9 cts/s/segment
brightest pixel: 0.001 cts/s/pix at 1446.2 A
Calculation performed 2021-10-21T02:38:29, v0.23ETC exposure time is 2712 s per G160M setting. This exposure will be coadded with others.
Worst-case ETC run (1666799) gives 0.03 cts/s in brightest pixel and buffer time of 19046 s
M dwarf flare ETC run (1666800) gives 0.34 cts/s in brightest pixel
Buffer time set to 2/3 of worst-case result
sz103_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: M4 ; A_V: 0.7 ; Distance (pc): 200
M*: 0.22 ; log(dm/dt): -8.99
For exptime=5424.6 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): 66.9 cts/s/segment
brightest pixel: 0.001 cts/s/pix at 1446.2 A
Calculation performed 2021-10-21T02:38:29, v0.23ETC exposure time is 2712 s per G160M setting. This exposure will be coadded with others.
Worst-case ETC run (1666799) gives 0.03 cts/s in brightest pixel and buffer time of 19046 s
M dwarf flare ETC run (1666800) gives 0.34 cts/s in brightest pixel
Buffer time set to 2/3 of worst-case result
sz103_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: M4 ; A_V: 0.7 ; Distance (pc): 200
M*: 0.22 ; log(dm/dt): -8.99
For exptime=5424.6 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): 66.9 cts/s/segment
brightest pixel: 0.001 cts/s/pix at 1446.2 A
Calculation performed 2021-10-21T02:38:29, v0.23ETC exposure time is 2712 s per G160M setting. This exposure will be coadded with others.
Worst-case ETC run (1666799) gives 0.03 cts/s in brightest pixel and buffer time of 19046 s
M dwarf flare ETC run (1666800) gives 0.34 cts/s in brightest pixel
Buffer time set to 2/3 of worst-case result
sz103_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: M4 ; A_V: 0.7 ; Distance (pc): 200
M*: 0.22 ; log(dm/dt): -8.99
For exptime=5424.6 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): 66.9 cts/s/segment
brightest pixel: 0.001 cts/s/pix at 1446.2 A
Calculation performed 2021-10-21T02:38:29, v0.23/Users/wfischer/Box/ullyses_tech/ullyses_proposals/survey_c29/16856/OP-cache/ULLYSES_16856-v1S.xmlTiming link suitability includes constraints ([Group (1C 1D 1E 1F 1G 1S) Within 2.0 days])The scheduling data was generated by CASM 29.2.CASM was run in Phase II mode.vstatus; 1S; SZ103; S/STIS approved for submission; S/WF 10/01/22 ; intrev: complete ; S/JRD 10/01/22
vcheck; Enter targ name & Inst. & Resp. Sci.; Sz 103 ; STIS ; WF
vcheck; ETC numbers entered in APT?; yes ...
see comments in the STIS acquisition for details about the hybrid model used
vcheck; Any screening violations?; no
vcheck; M-dwarf check complete and added to box folder?; yes ...
located at: ~/Box/ullyses_tech/ullyses_proposals/survey_c29/16856/sz-103/mdwarf/
vcheck; S/N ETC calcs done & documented?; yes
vcheck; Field images checked & saved?; yes, no GALEX coverage ...
located at: ~/Box/ullyses_tech/ullyses_proposals/survey_c29/16856/sz-103/
vcheck; Selected ACQ strategy?; yes, F28X50LP
vcheck; Possible ACQ or Sci spoilers?; no
vcheck; Field BOT clear?; yes, nothing in the G230L macroaperture
vcheck; Visual BOT check for stars not in catalog?; yes
vcheck; Orbit packing finalized?; yes ...
both orbits are needed; exposure times were increased to 131% of ETC result for G430L and doubled for other gratings ...
use of MAMA + CCD in same visit is needed to ensure near-simultaneous measurement of NUV and optical continuum in this rapidly variable source
vcheck; Buffer times optimized?; yes
vcheck; Verify visit grouping correct; yes
vcheck; phase constraint for ground based observations added?; N/A
vcheck; BETWEENS for coordinated observations added?; yes
vcheck; Is visit ready for int. review?; yes
Allocated STIS orbits = 2 (constrained in input CSV)(Tic-Visit
:proposal-id 16856
:visit-id "1S"
:proposal-version -1
:trans-version "20210514"
:date "10-Jan-2022 14:24:02.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 2
:saa-model "24"
:si-bright-earth-limb-angle 20.0
:data-volume 576240
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16856
:visit-id "1S"
:obset-id "1S"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16856
:visit-id "1S"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2534
:al-overhead-at-end 116
:internal-dur-at-end 773
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2927
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16856
:visit-id "1S"
:orbit-number 2
:pcs-time 392
:si-vis-utilization 2534
:al-overhead-at-end 119
:internal-dur-at-end 399
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2927
:pcs-gap 0
)true20Nominal ETC run gives 0.20 sec for S/N = 40
Worst-case ETC run (1548748) gives saturation in 11.4 sec
Used a hybrid model: CTTS template below 3700 A; M4 dwarf scaled to V = 16.58 above 3700 A
For S/N calcs, A_V = 1.2 is used instead of nominal A_V = 0.7; see sz110_lya2_etc_scaled_pAV0.50_M4phot.txt
For BOP calcs, nominal A_V is used and both components are scaled up by 4x; see sz110_lya2_x4.00_etc_M4phot.txt
Above SEDs and an IDL program to make them are in ~/Box/ullyses_tech/ullyses_proposals/survey_c29/16856/sz-103/seds/Exposure time of 299 s was doubled to 598 s
Worst-case ETC run (1666803) gives 2.72 cts/s in brightest pixel and buffer time of 763 s
M dwarf flare ETC run (1666804) gives 6.5 cts/s in brightest pixel
Buffer time set to just under half the exposure time
sz103_lya2_etc_scaled_pAV0.50.txt; stis,nuvmama,g230l,c2376,52x2,mjd#59670
Input file: lowmass_survey_Input-gaia.csv
Spectral type: M4 ; A_V: 0.7 ; Distance (pc): 200
M*: 0.22 ; log(dm/dt): -8.99
For exptime=299.2 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): 2345.0 cts/s/segment
brightest pixel: 0.282 cts/s/pix at 2796.8 A
Calculation performed 2021-10-21T02:38:31, v0.23ETC exposure time is 1932 s. This exposure will be coadded with a longer one.
ETC exposure time is larger than automatically calculated below due to use of an M dwarf SED
Worst-case ETC run (1666808) gives saturation in 4160 s
Used GAIN = 4 to guard against saturation on emission lines in 1281 s (ETC 1666809)
sz103_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: M4 ; A_V: 0.7 ; Distance (pc): 200
M*: 0.22 ; log(dm/dt): -8.99
For exptime=98.1 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): 37862.9 cts/s/segment
brightest pixel: 11.945 cts/s/pix at 4560.5 A
Calculation performed 2021-10-21T02:38:31, v0.23Exposure time of 116 s was doubled to 232 s
Exposure time is larger than automatically calculated below due to use of an M dwarf SED
Worst-case ETC run (1666813) gives saturation in 950 s
Used CR-SPLIT = 4 and GAIN = 4 to guard against saturation on emission lines in 166 s (ETC 1666814)
sz103_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: M4 ; A_V: 0.7 ; Distance (pc): 200
M*: 0.22 ; log(dm/dt): -8.99
For exptime=7.1 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): 71333.6 cts/s/segment
brightest pixel: 106.038 cts/s/pix at 6563.9 A
Calculation performed 2021-10-21T02:38:32, v0.23ETC exposure time is 1932 s. This exposure will be coadded with another one to reach 131% of this.
ETC exposure time is larger than automatically calculated below due to use of an M dwarf SED
Worst-case ETC run (1666808) gives saturation in 4160 s
Used CR-SPLIT = 4 and GAIN = 4 to guard against saturation on emission lines in 1281 s (ETC 1666809)
sz103_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: M4 ; A_V: 0.7 ; Distance (pc): 200
M*: 0.22 ; log(dm/dt): -8.99
For exptime=98.1 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): 37862.9 cts/s/segment
brightest pixel: 11.945 cts/s/pix at 4560.5 A
Calculation performed 2021-10-21T02:38:31, v0.23/Users/wfischer/Box/ullyses_tech/ullyses_proposals/survey_c29/16856/OP-cache/ULLYSES_16856-v2C.xmlTiming link suitability includes constraints ([Group (2C 2S) Within 1.0 days])The scheduling data was generated by CASM 29.2.CASM was run in Phase II mode.vstatus; 2C; SZ110; P/COS approved for submission; P/WF 10/01/22 ; intrev: complete ; P/JRD 10/01/22
vcheck; Enter targ name & Inst. & Resp. Sci.; Sz 110 ; COS ; WF
vcheck; ETC numbers entered in APT?; yes ...
see comments in the COS acquisition for details about the hybrid model used
vcheck; Any screening violations?; no
vcheck; M-dwarf check complete and added to box folder?; yes ...
located at: ~/Box/ullyses_tech/ullyses_proposals/survey_c29/16856/sz-110/mdwarf/
vcheck; S/N ETC calcs done & documented?; yes
vcheck; Field images checked & saved?; yes, no GALEX coverage ...
located at: ~/Box/ullyses_tech/ullyses_proposals/survey_c29/16856/sz-110/
vcheck; Selected ACQ strategy?; yes; dispersed with G230L/2635 ...
see ~/Box/ullyses_tech/ullyses_proposals/survey_c29/16856/sz-110/acq_strategies.xlsx for assessment of strategies
vcheck; Possible ACQ or Sci spoilers?; no
vcheck; Field BOT clear?; yes ...
see ~/Box/ullyses_tech/ullyses_proposals/survey_c29/16856/sz-110/field/
vcheck; Visual BOT check for stars not in catalog?; yes
vcheck; Orbit packing finalized?; yes ...
Both gratings are at 147% of requested times
vcheck; Buffer times optimized?; yes, all are texp - 110 sec
vcheck; Verify visit grouping correct; yes
vcheck; phase constraint for ground based observations added?; N/A
vcheck; BETWEENS for coordinated observations added?; yes
vcheck; Is visit ready for int. review?; yes
Allocated COS orbits = 2(Tic-Visit
:proposal-id 16856
:visit-id "2C"
:proposal-version -1
:trans-version "20210514"
:date "10-Jan-2022 14:24:04.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 2
:saa-model "31"
:si-bright-earth-limb-angle 20.0
:data-volume 626400
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16856
:visit-id "2C"
:obset-id "2C"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16856
:visit-id "2C"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2534
: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 2927
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16856
:visit-id "2C"
:orbit-number 2
:pcs-time 392
:si-vis-utilization 2535
: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
)true20Exposure time doubled from 37 s in case target is faint
Worst-case ETC run (1666745) gives 5.1 cts/s in brightest pixel
M dwarf flare ETC run (1666747) gives 4.8 cts/s in brightest pixel
Used a hybrid model: CTTS template below 3700 A; M4 dwarf scaled to B = 15.945 above 3700 A
For S/N calcs, A_V = 0.5 is used instead of nominal A_V = 0.0; see sz110_lya2_etc_scaled_pAV0.50_M4phot.txt
For BOP calcs, nominal A_V is used and both components are scaled up by 4x; see sz110_lya2_x4.00_etc_M4phot.txt
Above SEDs and an IDL program to make them are in ~/Box/ullyses_tech/ullyses_proposals/survey_c29/16856/sz-110/seds/
For M dwarf flaring, see ~/Box/ullyses_tech/ullyses_proposals/survey_c29/16856/sz-110/mdwarf/Exposure time doubled from 51 s in case target is faint
Worst-case ETC run (1666746) gives 5.1 cts/s in brightest pixel
M dwarf flare ETC run (1666748) gives 4.8 cts/s in brightest pixel
Used a hybrid model: CTTS template below 3700 A; M4 dwarf scaled to B = 15.945 above 3700 A
For S/N calcs, A_V = 0.5 is used instead of nominal A_V = 0.0; see sz110_lya2_etc_scaled_pAV0.50_M4phot.txt
For BOP calcs, nominal A_V is used and both components are scaled up by 4x; see sz110_lya2_x4.00_etc_M4phot.txt
Above SEDs and an IDL program to make them are in ~/Box/ullyses_tech/ullyses_proposals/survey_c29/16856/sz-110/seds/
For M dwarf flaring, see ~/Box/ullyses_tech/ullyses_proposals/survey_c29/16856/sz-110/mdwarf/Exposure time of 229 s per G160M setting was doubled to 458 s and extended to help fill the orbit
Worst-case ETC run (1666644) gives 0.36 cts/s in brightest pixel and buffer time of 2464 s
M dwarf flare ETC run (1666645) gives 2.43 cts/s in brightest pixel
Buffer time is exp time - 110 s
sz110_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: M4 ; A_V: 0.0 ; Distance (pc): 200
M*: 0.22 ; log(dm/dt): -8.53
For exptime=457.6 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): 130.0 cts/s/segment
brightest pixel: 0.025 cts/s/pix at 1446.2 A
Calculation performed 2021-10-21T02:38:39, v0.23Exposure time of 229 s per G160M setting was doubled to 458 s and extended to help fill the orbit
Worst-case ETC run (1666644) gives 0.36 cts/s in brightest pixel and buffer time of 2464 s
M dwarf flare ETC run (1666645) gives 2.43 cts/s in brightest pixel
Buffer time is exp time - 110 s
sz110_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: M4 ; A_V: 0.0 ; Distance (pc): 200
M*: 0.22 ; log(dm/dt): -8.53
For exptime=457.6 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): 130.0 cts/s/segment
brightest pixel: 0.025 cts/s/pix at 1446.2 A
Calculation performed 2021-10-21T02:38:39, v0.23Exposure time of 224 s per G160M setting was doubled to 448 s and extended to help fill the orbit
Worst-case ETC run (1666641) gives 0.38 cts/s in brightest pixel and buffer time of 2081 s
M dwarf flare ETC run (1666642) gives 2.41 cts/s in brightest pixel
Buffer time is exp time - 110 s
sz110_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: M4 ; A_V: 0.0 ; Distance (pc): 200
M*: 0.22 ; log(dm/dt): -8.53
For exptime=447.2 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): 142.4 cts/s/segment
brightest pixel: 0.027 cts/s/pix at 1446.2 A
Calculation performed 2021-10-21T02:38:37, v0.23Exposure time of 224 s per G160M setting was doubled to 448 s and extended to help fill the orbit
Worst-case ETC run (1666641) gives 0.38 cts/s in brightest pixel and buffer time of 2081 s
M dwarf flare ETC run (1666642) gives 2.41 cts/s in brightest pixel
Buffer time is exp time - 110 s
sz110_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: M4 ; A_V: 0.0 ; Distance (pc): 200
M*: 0.22 ; log(dm/dt): -8.53
For exptime=447.2 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): 142.4 cts/s/segment
brightest pixel: 0.027 cts/s/pix at 1446.2 A
Calculation performed 2021-10-21T02:38:37, v0.23Exposure time of 115 s per G130M setting was doubled to 230 s and extended to help fill the orbit
Worst-case ETC run (1666639) gives 0.50 cts/s in brightest pixel and buffer time of 660 s
M dwarf flare ETC run (1666638) gives 1.66 cts/s in brightest pixel
Buffer time is exp time - 110 s
sz110_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: M4 ; A_V: 0.0 ; Distance (pc): 200
M*: 0.22 ; log(dm/dt): -8.53
For exptime=229.9 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): 555.6 cts/s/segment
brightest pixel: 0.103 cts/s/pix at 1304.8 A
Calculation performed 2021-10-21T02:38:41, v0.23Exposure time of 115 s per G130M setting was doubled to 230 s and extended to help fill the orbit
Worst-case ETC run (1666639) gives 0.50 cts/s in brightest pixel and buffer time of 660 s
M dwarf flare ETC run (1666638) gives 1.66 cts/s in brightest pixel
Buffer time is exp time - 110 s
sz110_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: M4 ; A_V: 0.0 ; Distance (pc): 200
M*: 0.22 ; log(dm/dt): -8.53
For exptime=229.9 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): 555.6 cts/s/segment
brightest pixel: 0.103 cts/s/pix at 1304.8 A
Calculation performed 2021-10-21T02:38:41, v0.23/Users/wfischer/Box/ullyses_tech/ullyses_proposals/survey_c29/16856/OP-cache/ULLYSES_16856-v2S.xmlTiming link suitability includes constraints ([Group (2C 2S) Within 1.0 days])The scheduling data was generated by CASM 29.2.CASM was run in Phase II mode.vstatus; 2S; SZ110; S/STIS approved for submission; S/WF 10/01/22 ; intrev: complete ; S/JRD 10/01/22
vcheck; Enter targ name & Inst. & Resp. Sci.; Sz 110 ; STIS ; WF
vcheck; ETC numbers entered in APT?; yes ...
see comments in the COS acquisition for details about the hybrid model used
vcheck; Any screening violations?; no
vcheck; M-dwarf check complete and added to box folder?; yes ...
located at: ~/Box/ullyses_tech/ullyses_proposals/survey_c29/16856/sz-110/mdwarf/
vcheck; S/N ETC calcs done & documented?; yes
vcheck; Field images checked & saved?; yes, no GALEX coverage ...
located at: box/ullyses_tech/ullyses_proposals/survey_c29/16856/sz-110/
vcheck; Selected ACQ strategy?; yes, F28X50LP
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 ...
Exposure times were increased to about 5.9x ETC results. Only one orbit needed.
vcheck; Buffer times optimized?; yes
vcheck; Verify visit grouping correct; yes
vcheck; phase constraint for ground based observations added?; N/A
vcheck; BETWEENS for coordinated observations added?; yes
vcheck; Is visit ready for int. review?; yes
Allocated STIS orbits = 2 (constrained in input CSV)(Tic-Visit
:proposal-id 16856
:visit-id "2S"
:proposal-version -1
:trans-version "20210514"
:date "10-Jan-2022 14:24:05.0"
: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 484224
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16856
:visit-id "2S"
:obset-id "2S"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16856
: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
)true10Nominal ETC run gives 0.03 s for S/N = 40
Worst-case ETC run (1666648) gives saturation in 1.9 sExposure time of 40 s was doubled to 80 s and extended to help fill the orbit
Worst-case ETC run (1666650) gives 19.9 cts/s in brightest pixel and buffer time of 389 s
M dwarf flare ETC run (1666651) gives 17.5 cts/s in brightest pixel
Buffer time set to just under half the exposure time
sz110_lya2_etc_scaled_pAV0.50.txt; stis,nuvmama,g230l,c2376,52x2,mjd#59670
Input file: lowmass_survey_Input-gaia.csv
Spectral type: M4 ; A_V: 0.0 ; Distance (pc): 200
M*: 0.22 ; log(dm/dt): -8.53
For exptime=39.8 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): 2587.6 cts/s/segment
brightest pixel: 2.042 cts/s/pix at 2796.8 A
Calculation performed 2021-10-21T02:38:41, v0.23Exposure time of 139 s was doubled to 278 s and extended to help fill the orbit
Exposure time is larger than automatically calculated below due to use of an M dwarf SED
Worst-case ETC run (1666654) gives saturation in 783 s
Used CR-SPLIT = 4 and GAIN = 4 to guard against saturation on emission lines in 312 s (ETC 1666656)
sz110_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: M4 ; A_V: 0.0 ; Distance (pc): 200
M*: 0.22 ; log(dm/dt): -8.53
For exptime=20.7 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): 60180.5 cts/s/segment
brightest pixel: 48.962 cts/s/pix at 4560.5 A
Calculation performed 2021-10-21T02:38:41, v0.23Exposure time of 14 s was doubled to 28 s and extended to help fill the orbit
Exposure time is larger than automatically calculated below due to use of an M dwarf SED
Worst-case ETC run (1666658) gives saturation in 156 s
Used GAIN = 4 to guard against saturation on emission lines in 63 s (ETC 1666659)
sz110_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: M4 ; A_V: 0.0 ; Distance (pc): 200
M*: 0.22 ; log(dm/dt): -8.53
For exptime=2.1 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): 131388.6 cts/s/segment
brightest pixel: 279.580 cts/s/pix at 6563.9 A
Calculation performed 2021-10-21T02:38:41, v0.23/Users/wfischer/Box/ullyses_tech/ullyses_proposals/survey_c29/16856/OP-cache/ULLYSES_16856-v3C.xmlTiming link suitability includes constraints ([Group (3C 3D 3S) Within 1.0 days])The scheduling data was generated by CASM 29.2.CASM was run in Phase II mode.vstatus; 3C; SZ99; P/COS approved for submission; P/WF 10/01/22 ; intrev: complete ; P/JRD 10/01/22
vcheck; Enter targ name & Inst. & Resp. Sci.; Sz 99 ; COS ; WF
vcheck; ETC numbers entered in APT?; yes ...
see comments in the COS acquisition for details about the hybrid model used
vcheck; Any screening violations?; no
vcheck; M-dwarf check complete and added to box folder?; yes ...
located at: ~/Box/ullyses_tech/ullyses_proposals/survey_c29/16856/sz-99/mdwarf/
vcheck; S/N ETC calcs done & documented?; yes
vcheck; Field images checked & saved?; yes, no GALEX coverage ...
located at: ~/Box/ullyses_tech/ullyses_proposals/survey_c29/16856/sz-99/
vcheck; Selected ACQ strategy?; yes; PSA/MirrorB
vcheck; Possible ACQ or Sci spoilers?; no
vcheck; Field BOT clear?; yes, nothing in the macroapertures
vcheck; Visual BOT check for stars not in catalog?; yes
vcheck; Orbit packing finalized?; yes ...
G130M gets 108% of requested time and G160M gets 85% of requested time
vcheck; Buffer times optimized?; yes, all are texp - 110 sec
vcheck; Verify visit grouping correct; yes
vcheck; phase constraint for ground based observations added?; N/A
vcheck; BETWEENS for coordinated observations added?; yes
vcheck; Is visit ready for int. review?; yes
Allocated COS orbits = 5(Tic-Visit
:proposal-id 16856
:visit-id "3C"
:proposal-version -1
:trans-version "20210514"
:date "10-Jan-2022 14:24:06.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 2
:saa-model "31"
:si-bright-earth-limb-angle 20.0
:data-volume 191488
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16856
:visit-id "3C"
:obset-id "3C"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16856
:visit-id "3C"
: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 16856
:visit-id "3C"
:orbit-number 2
:pcs-time 392
:si-vis-utilization 2535
:al-overhead-at-end 0
:internal-dur-at-end 334
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2927
:pcs-gap 0
)true20Exposure time doubled from 89 s in case target is faint
Worst-case ETC run (1666757) gives 6.9 cts/s in brightest pixel
M dwarf flare ETC run (1666758) gives 97 cts/s in brightest pixel
Used a hybrid model: CTTS template below 3700 A; M4 dwarf scaled to B = 17.687 above 3700 A
For S/N calcs, A_V = 0.5 is used instead of nominal A_V = 0.0; see sz99_lya2_etc_scaled_pAV0.50_M4phot.txt
For BOP calcs, nominal A_V is used and both components are scaled up by 4x; see sz99_lya2_x4.00_etc_M4phot.txt
Above SEDs and an IDL program to make them are in ~/Box/ullyses_tech/ullyses_proposals/survey_c29/16856/sz-99/seds/
For M dwarf flaring, see ~/Box/ullyses_tech/ullyses_proposals/survey_c29/16856/sz-99/mdwarf/Exposure time of 865 s per G130M setting was doubled to 1730 s and extended to fill the orbit
Worst-case ETC run (1666761) gives 0.10 cts/s in brightest pixel and buffer time of 3409 s
M dwarf flare ETC run (1666762) gives 0.30 cts/s in brightest pixel
Buffer time is exp time - 110 s
sz99_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: M4 ; A_V: 0.0 ; Distance (pc): 200
M*: 0.23 ; log(dm/dt): -9.41
For exptime=1730.6 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): 315.5 cts/s/segment
brightest pixel: 0.013 cts/s/pix at 1304.8 A
Calculation performed 2021-10-21T02:38:22, v0.23Exposure time of 1050 s per G160M setting was doubled to 2100 s and extended to fill the orbit
Worst-case ETC run (1666764) gives 0.05 cts/s in brightest pixel and buffer time of 10487 s
M dwarf flare ETC run (1666765) gives 0.56 cts/s in brightest pixel
Buffer time is exp time - 110 s
sz99_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: M4 ; A_V: 0.0 ; Distance (pc): 200
M*: 0.23 ; log(dm/dt): -9.41
For exptime=2098.8 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): 74.5 cts/s/segment
brightest pixel: 0.003 cts/s/pix at 1446.2 A
Calculation performed 2021-10-21T02:38:18, v0.23/Users/wfischer/Box/ullyses_tech/ullyses_proposals/survey_c29/16856/OP-cache/ULLYSES_16856-v3D.xmlTiming link suitability includes constraints ([Group (3C 3D 3S) Within 1.0 days])The scheduling data was generated by CASM 29.2.CASM was run in Phase II mode.vstatus; 3D; SZ99; P/COS approved for submission; P/WF 10/01/22 ; intrev: complete ; P/JRD 10/01/22
vcheck; Enter targ name & Inst. & Resp. Sci.; Sz 99 ; COS ; WF
vcheck; ETC numbers entered in APT?; yes ...
see comments in the COS acquisition for details about the hybrid model used
vcheck; Any screening violations?; no
vcheck; M-dwarf check complete and added to box folder?; yes ...
located at: ~/Box/ullyses_tech/ullyses_proposals/survey_c29/16856/sz-99/mdwarf/
vcheck; S/N ETC calcs done & documented?; yes
vcheck; Field images checked & saved?; yes, no GALEX coverage ...
located at: ~/Box/ullyses_tech/ullyses_proposals/survey_c29/16856/sz-99/
vcheck; Selected ACQ strategy?; yes; PSA/MirrorB
vcheck; Possible ACQ or Sci spoilers?; no
vcheck; Field BOT clear?; yes, nothing in the macroapertures
vcheck; Visual BOT check for stars not in catalog?; yes
vcheck; Orbit packing finalized?; yes ...
G130M gets 108% of requested time and G160M gets 85% of requested time
vcheck; Buffer times optimized?; yes, all are texp - 110 sec
vcheck; Verify visit grouping correct; yes
vcheck; phase constraint for ground based observations added?; N/A
vcheck; BETWEENS for coordinated observations added?; yes
vcheck; Is visit ready for int. review?; yes
Allocated COS orbits = 5(Tic-Visit
:proposal-id 16856
:visit-id "3D"
:proposal-version -1
:trans-version "20210514"
:date "10-Jan-2022 14:24:07.0"
: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 365504
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16856
:visit-id "3D"
:obset-id "3D"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16856
:visit-id "3D"
: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 16856
:visit-id "3D"
:orbit-number 2
:pcs-time 392
:si-vis-utilization 2535
: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 16856
:visit-id "3D"
:orbit-number 3
:pcs-time 392
:si-vis-utilization 2535
:al-overhead-at-end 0
:internal-dur-at-end 334
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2927
:pcs-gap 0
)true30Exposure time doubled from 89 s in case target is faint
Worst-case ETC run (1666757) gives 6.9 cts/s in brightest pixel
M dwarf flare ETC run (1666758) gives 97 cts/s in brightest pixel
Used a hybrid model: CTTS template below 3700 A; M4 dwarf scaled to B = 17.687 above 3700 A
For S/N calcs, A_V = 0.5 is used instead of nominal A_V = 0.0; see sz99_lya2_etc_scaled_pAV0.50_M4phot.txt
For BOP calcs, nominal A_V is used and both components are scaled up by 4x; see sz99_lya2_x4.00_etc_M4phot.txt
Above SEDs and an IDL program to make them are in ~/Box/ullyses_tech/ullyses_proposals/survey_c29/16856/sz-99/seds/
For M dwarf flaring, see ~/Box/ullyses_tech/ullyses_proposals/survey_c29/16856/sz-99/mdwarf/Exposure time of 865 s per G130M setting was doubled to 1730 s and extended to fill the orbit
Worst-case ETC run (1666761) gives 0.10 cts/s in brightest pixel and buffer time of 3409 s
M dwarf flare ETC run (1666762) gives 0.30 cts/s in brightest pixel
Buffer time is exp time - 110 s
sz99_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: M4 ; A_V: 0.0 ; Distance (pc): 200
M*: 0.23 ; log(dm/dt): -9.41
For exptime=1730.6 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): 315.5 cts/s/segment
brightest pixel: 0.013 cts/s/pix at 1304.8 A
Calculation performed 2021-10-21T02:38:22, v0.23Exposure time of 1074 s per G160M setting was doubled to 2148 s and extended to fill the orbit
Worst-case ETC run (1666767) gives 0.05 cts/s in brightest pixel and buffer time of 12035 s
M dwarf flare ETC run (1666768) gives 0.56 cts/s in brightest pixel
Buffer time is exp time - 110 s
sz99_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: M4 ; A_V: 0.0 ; Distance (pc): 200
M*: 0.23 ; log(dm/dt): -9.41
For exptime=2147.8 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): 72.4 cts/s/segment
brightest pixel: 0.003 cts/s/pix at 1446.2 A
Calculation performed 2021-10-21T02:38:20, v0.23ETC exposure time is 1074 s per G160M setting. This exposure will be coadded with a longer one.
Worst-case ETC run (1666767) gives 0.05 cts/s in brightest pixel and buffer time of 12035 s
M dwarf flare ETC run (1666768) gives 0.56 cts/s in brightest pixel
Buffer time is exp time - 110 s
sz99_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: M4 ; A_V: 0.0 ; Distance (pc): 200
M*: 0.23 ; log(dm/dt): -9.41
For exptime=2147.8 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): 72.4 cts/s/segment
brightest pixel: 0.003 cts/s/pix at 1446.2 A
Calculation performed 2021-10-21T02:38:20, v0.23ETC exposure time is 1050 s per G160M setting. This exposure will be coadded with a longer one.
Worst-case ETC run (1666764) gives 0.05 cts/s in brightest pixel and buffer time of 10487 s
M dwarf flare ETC run (1666765) gives 0.56 cts/s in brightest pixel
Buffer time is exp time - 110 s
sz99_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: M4 ; A_V: 0.0 ; Distance (pc): 200
M*: 0.23 ; log(dm/dt): -9.41
For exptime=2098.8 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): 74.5 cts/s/segment
brightest pixel: 0.003 cts/s/pix at 1446.2 A
Calculation performed 2021-10-21T02:38:18, v0.23/Users/wfischer/Box/ullyses_tech/ullyses_proposals/survey_c29/16856/OP-cache/ULLYSES_16856-v3S.xmlTiming link suitability includes constraints ([Group (3C 3D 3S) Within 1.0 days])The scheduling data was generated by CASM 29.2.CASM was run in Phase II mode.vstatus; 3S; SZ99; S/STIS approved for submission; S/WF 10/01/22 ; intrev: complete ; S/JRD 10/01/22
vcheck; Enter targ name & Inst. & Resp. Sci.; Sz 99 ; STIS ; WF
vcheck; ETC numbers entered in APT?; yes ...
see comments in the COS acquisition for details about the hybrid model used
vcheck; Any screening violations?; no
vcheck; M-dwarf check complete and added to box folder?; yes ...
located at: ~/Box/ullyses_tech/ullyses_proposals/survey_c29/16856/sz-99/mdwarf/
vcheck; S/N ETC calcs done & documented?; yes
vcheck; Field images checked & saved?; yes, no GALEX coverage ...
located at: ~/Box/ullyses_tech/ullyses_proposals/survey_c29/16856/sz-110/
vcheck; Selected ACQ strategy?; yes, F28X50LP
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 ...
both orbits are needed; exposure times were increased to 3x ETC result for G430L and about 5.9x for other gratings ...
use of MAMA + CCD in same visit is needed to ensure near-simultaneous measurement of NUV and optical continuum in this rapidly variable source
vcheck; Buffer times optimized?; yes
vcheck; Verify visit grouping correct; yes
vcheck; phase constraint for ground based observations added?; N/A
vcheck; BETWEENS for coordinated observations added?; yes
vcheck; Is visit ready for int. review?; yes
Allocated STIS orbits = 2 (constrained in input CSV)(Tic-Visit
:proposal-id 16856
:visit-id "3S"
:proposal-version -1
:trans-version "20210514"
:date "07-Jan-2022 17:12:01.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 2
:saa-model "24"
:si-bright-earth-limb-angle 20.0
:data-volume 660176
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16856
:visit-id "3S"
:obset-id "3S"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16856
:visit-id "3S"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2534
:al-overhead-at-end 116
:internal-dur-at-end 773
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2927
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16856
:visit-id "3S"
:orbit-number 2
:pcs-time 392
:si-vis-utilization 2534
:al-overhead-at-end 119
:internal-dur-at-end 399
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2927
:pcs-gap 0
)true20Nominal ETC run gives 0.2 sec for S/N = 40
Worst-case ETC run (1666779) gives saturation in 9.5 secExposure time of 170 s was doubled to 340 s and extended to help fill the orbit
Worst-case ETC run (1666776) gives 4.8 cts/s in brightest pixel and buffer time of 713 s
M dwarf flare ETC run (1666777) gives 5.7 cts/s in brightest pixel
Buffer time: STIS observations are based on B=17.69, V=17.05. But there is literature photometry V=16.00. In case this 2.5x brighter measurement is more accurate, we apply an additional factor of 1/2.5 = 0.4 beyond the usual factor of 0.8: 700 x 0.4 x 0.8 = 224 sec.
sz99_lya2_etc_scaled_pAV0.50.txt; stis,nuvmama,g230l,c2376,52x2,mjd#59670
Input file: lowmass_survey_Input-gaia.csv
Spectral type: M4 ; A_V: 0.0 ; Distance (pc): 200
M*: 0.23 ; log(dm/dt): -9.41
For exptime=170.0 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): 2362.6 cts/s/segment
brightest pixel: 0.487 cts/s/pix at 2796.8 A
Calculation performed 2021-10-21T02:38:22, v0.23Exposure time of 69 s was doubled to 138 s and extended to help fill the orbit
Exposure time is larger than automatically calculated below due to use of an M dwarf SED
Worst-case ETC run (1666786) gives saturation in 778 s
Used GAIN = 4 to guard against saturation on emission lines in 152 s (ETC 1666787)
sz99_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: M4 ; A_V: 0.0 ; Distance (pc): 200
M*: 0.23 ; log(dm/dt): -9.41
For exptime=6.8 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): 71272.6 cts/s/segment
brightest pixel: 115.583 cts/s/pix at 6563.9 A
Calculation performed 2021-10-21T02:38:22, v0.23Exposure time of 742 s was doubled to 1484 s and extended to fill the orbit
Exposure time is larger than automatically calculated below due to use of an M dwarf SED
Worst-case ETC run (1666782) gives saturation in 2650 s
Used CR-SPLIT = 4 and GAIN = 4 to guard against saturation on emission lines in 1029 s (ETC 1666783)
sz99_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: M4 ; A_V: 0.0 ; Distance (pc): 200
M*: 0.23 ; log(dm/dt): -9.41
For exptime=70.6 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): 39079.2 cts/s/segment
brightest pixel: 14.863 cts/s/pix at 4560.5 A
Calculation performed 2021-10-21T02:38:22, v0.23