Removed all phase requirements
Changed CCD gain back to 4 for the external G430L/G750L exposures
Some cleanup in the comment lines.
-----------------------
Hello Tricia:
I've fixed the betweens to better match the TESS timing and changed the STIS G430L and G750L to GAIN=1.
Charles
This is the real version of this program rather than the placeholder.
It is being submitted by Will Fischer, since Charles Proffitt is on vacation.1237917262----- Attempting Submission 2 (Thu Sep 17 00:39:06 GMT 2020) -----
----- Attempting Submission 3 (Wed Oct 14 03:01:28 GMT 2020) -----
----- Attempting Submission 4 (Tue Oct 27 17:00:14 GMT 2020) -----ULLYSES K-type T Tauri stars in Orion OBIb Star Forming RegionThe 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 + c1611 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=15/6-pix-resel at the peak of the line
COS/G160M/c1611: C IV 1549 +- 1 A -- S/N=30/6-pix-resel at the peak of the line
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.
To obtain near simultaneous coverage, all visits to a given target should be grouped within 1 day.
The visits in this proposal are all constrained to occur between 19 November and 17 December 2020 to be simultaneous with planned TESS observations.
We also wish to attempt to obtain simultaneous coverage with telescopes of the LCOGT network. Unfortuneately, this network has an approximately 2 to 3 hour gap in coverage for the Orion targets due to the lack of an observataory at an appropriate longitude. We will therefore add a period and a phase constraint to these obervations to prevent the HST observations from being schedulled during this daily gap. The period when the Orion stars can be observed by this networks starts when they reach ~ airmass of 2 from the Sutherland observatory in South Africa, and ends about 21 hours later due to the start of morning twilight in Siding Springs Australia. Originally we had planned to enforce this scheduling restriction using APT phase constraints, but instead the Program Coordinator will manually restrict the planning windows in the LRP to achieve the desired effect. This is less error prone and more flexible as these constraints, unlike APT ones, can be relaxed during the schedule building process.
At each TESS perigee, there are two LAHO (low-altitude housekeeping operations) contacts. TESSscience observations stop 10 minutes before the beginning of the first LAHO and resume 5 minutes before the end of the second LAHO. Times of LAHO contacts are posted on the TESS operations calendar at https://calendar.google.com/calendar/b/0/r/week?cid=a21va3YydDM0dmpsc2w2Ymw2Z29vdWE2OGNAZ3JvdXAuY2FsZW5kYXIuZ29vZ2xlLmNvbQ approximately 3 months in advance.
We will require that our visits start at least 45minutes prior to the start of any gap in TESS operations.
For TESS sector 32,
LAHO Passes
(1) 19-Nov-2020 08:45-13:45 start 5m before LAHO end
(2) 02-Dec-2020 10:45-15:45 stop 10m before LAHO start
(3) 03-Dec-2020 05:45-10:45 start 5m before LAHO end
(4) 16-Dec-2020 17:45-22:45 stop 10m before LAHO start
TESS start/stop times
19-Nov-2020:13:40 to 02-Dec-2020:10:35
03-Nov-2020:10:40 to 16-Dec-2020:17:35
Constrain end of HST BETWEENs to be 55m, 2h30m, and 4h5m before TESS end for 1, 2, and 3 orbit visits to allow HST to complete before TESS end
HST-1 orbit: subtract 50 minutes from end times
19-Nov-2020:13:40 to 02-Dec-2020:09:40
03-Nov-2020:10:40 to 16-Dec-2020:16:40
HST-2 orbit: subtract 2h25m from end times
19-Nov-2020:13:40 to 02-Dec-2020:08:05
03-Nov-2020:10:40 to 16-Dec-2020:15:05
HST-3 orbit: subtract 4h from end times
19-Nov-2020:13:40 to 02-Dec-2020:06:30
03-Nov-2020:10:40 to 16-Dec-2020:13:300falseSUPPORTEDSTART TAURI STARPRE-MAIN SEQUENCE STARNOCVSO-107 : J05322578-0036533
Region: Ori OB1b
Simbad: https://simbad.u-strasbg.fr/simbad/sim-id?Ident=2MASS+J05322578-0036533&submit=submit+id
Target coordinates are from Gaia DR2.
Spectral type: K7 ; A_V: 0.32 ; Distance (pc): 440
M*: 0.77 ; log(dm/dt): -7.96
Input file: combined_todo_survey_tess_sort_v2_Gaia_J_CP_edit.csv
cvso107_lya2_etc.txt
Calculation performed 2020-07-30T14:21:25, v0.4
-------------------------------------------------------------------------------
tstatus; CVSO-107; P/COS approved for submission; S/STIS Ready for internal review; P/CP 11/08/20; S/CP 11/08/20
tcheck; APT/SIMBAD target names: ; Kiso A-0904 4
tcheck; Target info verification status?; Good
tcheck; Coordinates & P.M. verified, epoch checked?; Yes
tcheck; Adopted SED compared to Observations?; Yes ...
BVI data within a factor of 2 of predictions (cvso-107-sed-vs-photo-revised.png). Continuum in observed G160M spectrum about a factor of two high (cvso-107-sed-vs-g160m.png), but overall count rate very low (about 30 cnts/s from source integrated over the whole spectrum), while brightest observed emission lines are actually a bit fainter in the real observation than in the prediction (cvso-107-sed-vs-g160m-detail.png).J05322578-0036533J2000SpT=K7; A_V=0.32; U=15.24; V=14.65; I=12.82; J=11.551START TAURI STARPRE-MAIN SEQUENCE STARNOCVSO-165 : J05390257-0120323
Region: Ori OB1b
Simbad: https://simbad.u-strasbg.fr/simbad/sim-id?Ident=2MASS+J05390257-0120323&submit=submit+id
Target coordinates are from Gaia DR2.
Spectral type: K6 ; A_V: 0.0 ; Distance (pc): 440
M*: 0.91 ; log(dm/dt): -8.43
Input file: combined_todo_survey_tess_sort_v2_Gaia_J_CP_edit.csv
cvso165_lya2_etc.txt
Calculation performed 2020-07-30T14:21:34, v0.4
-------------------------------------------------------------------------------
tstatus; CVSO-165; P/COS approved for submission; S/STIS Ready for internal review; P/CP 01/08/20; S/CP 01/08/20
tcheck; APT/SIMBAD target names: ; Kiso A-0904 76; CVSO 165
tcheck; Target info verification status?; good, but has a visual companion ...
companion at 5.432" and PA = 321.5,
G=15.054, Bp=15.5261, Rp = 14.3965, Bp - Rp=1.1296, Parallax=0.7217, SDSS u = 17.186
Gaia color matches~ K2.5V spectral type, but large distance suggests too luminous for a dwarf
vs intended target with
G=13.299, Bp=14.0800, Rp = 12.4122, Bp - Rp=1.6678, Parallax=2.9802, SDSS u = 16.725
can put both stars along STIS slit between 08 Dec and 30 Dec although only 8 Dec - 17 Dec overlaps with TESS
tcheck; Coordinates & P.M. verified, epoch checked?; Yes
tcheck; Adopted SED compared to Observations?; yes ...
UVI photometry all a factor of 2.17 to 2.37 above nominal scaled spectrum. See cvso-165-sed-vs-photo-revised.pngJ05390257-0120323J2000SpT=K6; A_V=0.00; U=15.25; V=13.73; I=12.33; J=11.1START TAURI STARPRE-MAIN SEQUENCE STARNOCVSO-58 : J05292326-0125153
Region: Ori OB1b
Simbad: https://simbad.u-strasbg.fr/simbad/sim-id?Ident=2MASS+J05292326-0125153&submit=submit+id
Target coordinates are from Gaia DR2.
Spectral type: K7 ; A_V: 0.12 ; Distance (pc): 440
M*: 0.78 ; log(dm/dt): -8.35
Input file: combined_todo_survey_tess_sort_v2_Gaia_J_CP_edit.csv
cvso58_lya2_etc.txt
Calculation performed 2020-07-30T14:21:50, v0.4
-------------------------------------------------------------------------------
tstatus; CVSO-58; P/COS approved for submission; S/STIS ready for internal review; P/CP 11/08/20; S/CP 11/08/20
tcheck; APT/SIMBAD target names: ; Kiso A-0903 176; [HCB2007] OB1b 209; CVSO 58
tcheck; Target info verification status?; Done
tcheck; Coordinates & P.M. verified, epoch checked?; Yes
tcheck; Adopted SED compared to Observations?; Yes, ...
Fair agreement between UVI photometry and adoped SED (within a factor of 2) cvso-58-sed-vs-photo-revised.png
Observed G160M spectrum has average continuum 2-3x higher than adopted SED (cvso-58-sed-vs-g160m.png), but still only 20 observed counts/s integrated over entire G160M spectrum.
but peak of brightest observed emission lines near 1550 Angstroms are a factor of a few lower than adopted SED (cvso-58-sed-vs-g160m-detail.png), and this is what determines BOP limits in this case.J05292326-0125153J2000SpT=K7; A_V=0.12; U=15.52; V=14.79; I=13.27; J=12.1START TAURI STARPRE-MAIN SEQUENCE STARNOCVSO-90 : J05312062-0049197
Region: Ori OB1b
Simbad: https://simbad.u-strasbg.fr/simbad/sim-id?Ident=2MASS+J05312062-0049197&submit=submit+id
Target coordinates are from Gaia DR2.
Spectral type: K7 ; A_V: 0.0 ; Distance (pc): 440
M*: 0.79 ; log(dm/dt): -7.75
Input file: combined_todo_survey_tess_sort_v2_Gaia_J_CP_edit.csv
cvso90_lya2_etc.txt
Calculation performed 2020-07-30T14:20:25, v0.4
-------------------------------------------------------------------------------
tstatus; CVSO-90; P/COS approved for submission; S/STIS ready for internal review; P/CP 12/08/20; S/CP 12/08/20
tcheck; APT/SIMBAD target names: ; Kiso A-0904 1 ; CVSO 90
tcheck; Target info verification status?; Good
tcheck; Coordinates & P.M. verified, epoch checked?; Yes
tcheck; Adopted SED compared to Observations?; yes ...
Observed U about 2.6x baseline SED, while observed VI about 0.45x baseline, COS c1611 continuum about 0.5x, while observed peak 1550 emission about 0.2x observed.J05312062-0049197KISO-A-0904-1J2000SpT=K7; A_V=0.00; U=14.02; V=14.6; I=13.37, J=12.1Timing link suitability includes constraints ([Group (1C 1D 1S) Within 1.0 days])The scheduling data was generated by CASM 28.2.CASM was run in Phase II mode./Users/proffitt/Box/ullyses_tech/ullyses_proposals/survey/16114/OP-cache/ULLYSES_16114-v1C.xmlvstatus; 1C; CVSO-107; P/COS approved for submission; P/CP 02/09/20 ; internal review complete ; C/DS 16/09/20
vcheck; Enter targ name & Inst. & Resp. Sci.; CVSO-107 ; COS ; CP
vcheck; ETC numbers entered in APT?; Yes
vcheck; Any screening violations?; No
vcheck; M-dwarf check complete and added to box folder?; N/A
vcheck; S/N ETC calcs done & documented?; Yes
vcheck; Field images checked & saved?; YES
vcheck; Selected ACQ strategy?; PSA/MIRROR
vcheck; Possible ACQ or Sci spoilers?; None
vcheck; Field BOT clear?; Yes ...
one unknown S1LN033093, has NpgMag (roughly I band) =18.1799 in GSC2, but does not appear in other images or catalogs (neither Gaia nor SDSS show any object here), so this is probably a very faint and very red object, so it is not of concern
vcheck; Visual BOT check for stars not in catalog?; Clear
vcheck; Orbit packing finalized?; Yes ..
Achieved 97.5% of requested c1291 and 98.3% of c1611 in two 2 orbit visits 1C and 1D.
vcheck; Buffer times optimized?; yes ...
set to exptime - 110 even though this is much shorter than requierd
vcheck; Verify visit grouping correct; GROUP 1S, 1C, 1D within 1 day
vcheck; phase constraint for ground based observations added?; Yes
vcheck; BETWEENS for coordinated observations added?; Between 19-nov-2020 and 17-dec-2020
vcheck; Is visit ready for int. review?; Yes
Allocated COS orbits = 4, (2+2 orbit visits)(Tic-Visit
:proposal-id 16114
:visit-id "1C"
:proposal-version -1
:trans-version "20200619"
:date "27-Oct-2020 12:02:19.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 2
:saa-model "31"
:si-bright-earth-limb-angle 20.0
:data-volume 278496
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16114
:visit-id "1C"
:obset-id "1C"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16114
:visit-id "1C"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2525
: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 2918
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16114
:visit-id "1C"
:orbit-number 2
:pcs-time 392
:si-vis-utilization 2525
:al-overhead-at-end 0
:internal-dur-at-end 331
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2918
:pcs-gap 0
)true20baseline at S/N 40 (2x requirement) COS.ta.1460360 needs 110.2 s, with B.P. = 2.034x BOP Check COS.sp.1460369 - B.P. is Lyman-alpha geocoronal
S/N check with nominal spectrum is COS.sp.1460374
cvso107_lya2_etc.txt; cos,fuv,g130m,c1291,psa,mjd#59305; fp-pos=None, segment=None)
Input file: combined_todo_survey_tess_sort_v2_Gaia_J_CP_edit.csv
Spectral type: K7 ; A_V: 0.32 ; Distance (pc): 440
M*: 0.77 ; log(dm/dt): -7.96
For exptime=2041.1 s, spectral region:
1239.0 +- 1.0 A achieves SNR=15.0 / 6-pix-resel
A factor of 2.0 has been applied to the exptime in each exposure.
global countrate (brightest segment): 314.4 cts/s/segment
brightest pixel: 0.007 cts/s/pix at 1304.9 A
Calculation performed 2020-07-30T14:21:25, v0.94x case for BOP COS.sp.1460364, B.P. 0.037 cnts/pixel/s
baseline for S/N COS.sp.1460366
cvso107_lya2_etc.txt; cos,fuv,g160m,c1611,psa,mjd#59305; fp-pos=None, segment=None)
Input file: combined_todo_survey_tess_sort_v2_Gaia_J_CP_edit.csv
Spectral type: K7 ; A_V: 0.32 ; Distance (pc): 440
M*: 0.77 ; log(dm/dt): -7.96
For exptime=2395.0 s, spectral region:
1549.0 +- 1.0 A achieves SNR=30.0 / 6-pix-resel
A factor of 2.0 has been applied to the exptime in each exposure.
global countrate (brightest segment): 86.6 cts/s/segment
brightest pixel: 0.009 cts/s/pix at 1548.4 A
Calculation performed 2020-07-30T14:21:22, v0.94x case for BOP COS.sp.1460364, B.P. 0.037 cnts/pixel/s
baseline for S/N COS.sp.1460366
cvso107_lya2_etc.txt; cos,fuv,g160m,c1611,psa,mjd#59305; fp-pos=None, segment=None)
Input file: combined_todo_survey_tess_sort_v2_Gaia_J_CP_edit.csv
Spectral type: K7 ; A_V: 0.32 ; Distance (pc): 440
M*: 0.77 ; log(dm/dt): -7.96
For exptime=2395.0 s, spectral region:
1549.0 +- 1.0 A achieves SNR=30.0 / 6-pix-resel
A factor of 2.0 has been applied to the exptime in each exposure.
global countrate (brightest segment): 86.6 cts/s/segment
brightest pixel: 0.009 cts/s/pix at 1548.4 A
Calculation performed 2020-07-30T14:21:22, v0.9Timing link suitability includes constraints ([Group (1C 1D 1S) Within 1.0 days])The scheduling data was generated by CASM 28.2.CASM was run in Phase II mode./Users/proffitt/Box/ullyses_tech/ullyses_proposals/survey/16114/OP-cache/ULLYSES_16114-v1D.xmlvstatus; 1C; CVSO-107; P/COS approved for submission; P/CP 02/09/20 ; internal review complete ; C/DS 16/09/20
See Visit 1C for a full filled out checklist
vcheck; Enter targ name & Inst. & Resp. Sci.; CVSO-107 ; COS ; CP
vcheck; ETC numbers entered in APT?; Yes
vcheck; Any screening violations?; No
vcheck; M-dwarf check complete and added to box folder?; N/A
vcheck; S/N ETC calcs done & documented?; Yes
vcheck; Field images checked & saved?; YES
vcheck; Selected ACQ strategy?; PSA/MIRROR
vcheck; Possible ACQ or Sci spoilers?; None
vcheck; Field BOT clear?; Yes ...
one unknown S1LN033093, has NpgMag (roughly I band) =18.1799 in GSC2, but does not appear in other images or catalogs (neither Gaia nor SDSS show any object here), so this is probably a very faint and very red object, so it is not of concern
vcheck; Visual BOT check for stars not in catalog?; Clear
vcheck; Orbit packing finalized?; ------
vcheck; Buffer times optimized?; ------
vcheck; Verify visit grouping correct; ------
vcheck; phase constraint for ground based observations added?; -------
vcheck; BETWEENS for coordinated observations added?; -------
vcheck; Is visit ready for int. review?; ------
Allocated COS orbits = 4(Tic-Visit
:proposal-id 16114
:visit-id "1D"
:proposal-version -1
:trans-version "20200619"
:date "27-Oct-2020 12:02:20.0"
: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 278496
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16114
:visit-id "1D"
:obset-id "1D"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16114
:visit-id "1D"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2525
: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 2918
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16114
:visit-id "1D"
:orbit-number 2
:pcs-time 392
:si-vis-utilization 2525
:al-overhead-at-end 0
:internal-dur-at-end 331
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2918
:pcs-gap 0
)true20baseline at S/N 40 (2x requirement) COS.ta.1460360 needs 110.2 s, with B.P. = 2.034x BOP Check COS.sp.1460369 - B.P. is Lyman-alpha geocoronal
S/N check with nominal spectrum is COS.sp.1460374
cvso107_lya2_etc.txt; cos,fuv,g130m,c1291,psa,mjd#59305; fp-pos=None, segment=None)
Input file: combined_todo_survey_tess_sort_v2_Gaia_J_CP_edit.csv
Spectral type: K7 ; A_V: 0.32 ; Distance (pc): 440
M*: 0.77 ; log(dm/dt): -7.96
For exptime=2041.1 s, spectral region:
1239.0 +- 1.0 A achieves SNR=15.0 / 6-pix-resel
A factor of 2.0 has been applied to the exptime in each exposure.
global countrate (brightest segment): 314.4 cts/s/segment
brightest pixel: 0.007 cts/s/pix at 1304.9 A
Calculation performed 2020-07-30T14:21:25, v0.94x case for BOP COS.sp.1460364, B.P. 0.037 cnts/pixel/s
baseline for S/N COS.sp.1460366
cvso107_lya2_etc.txt; cos,fuv,g160m,c1611,psa,mjd#59305; fp-pos=None, segment=None)
Input file: combined_todo_survey_tess_sort_v2_Gaia_J_CP_edit.csv
Spectral type: K7 ; A_V: 0.32 ; Distance (pc): 440
M*: 0.77 ; log(dm/dt): -7.96
For exptime=2395.0 s, spectral region:
1549.0 +- 1.0 A achieves SNR=30.0 / 6-pix-resel
A factor of 2.0 has been applied to the exptime in each exposure.
global countrate (brightest segment): 86.6 cts/s/segment
brightest pixel: 0.009 cts/s/pix at 1548.4 A
Calculation performed 2020-07-30T14:21:22, v0.94x case for BOP COS.sp.1460364, B.P. 0.037 cnts/pixel/s
baseline for S/N COS.sp.1460366
cvso107_lya2_etc.txt; cos,fuv,g160m,c1611,psa,mjd#59305; fp-pos=None, segment=None)
Input file: combined_todo_survey_tess_sort_v2_Gaia_J_CP_edit.csv
Spectral type: K7 ; A_V: 0.32 ; Distance (pc): 440
M*: 0.77 ; log(dm/dt): -7.96
For exptime=2395.0 s, spectral region:
1549.0 +- 1.0 A achieves SNR=30.0 / 6-pix-resel
A factor of 2.0 has been applied to the exptime in each exposure.
global countrate (brightest segment): 86.6 cts/s/segment
brightest pixel: 0.009 cts/s/pix at 1548.4 A
Calculation performed 2020-07-30T14:21:22, v0.9/private/var/folders/c1/kkl4zqqs11g637_3q3f43f2m000400/T/OPVisit6334672454240379571.xmlTiming link suitability includes constraints ([Group (1C 1D 1S) Within 1.0 days])The scheduling data was generated by CASM 28.2.CASM was run in Phase II mode.vstatus; 1S; CVSO-107; S/STIS approved for submission; P/CP 02/09/20 ; internal review complete ; S/DW 11/09/20
vcheck; Enter targ name & Inst. & Resp. Sci.; CVSO-107 ;STIS ; CP
vcheck; ETC numbers entered in APT?; Yes
vcheck; Any screening violations?; No
vcheck; M-dwarf check complete and added to box folder?; N/A
vcheck; S/N ETC calcs done & documented?; Yes
vcheck; Field images checked & saved?; Yes
vcheck; Selected ACQ strategy?; F28X50LP, S/N=80 using baseline SED
vcheck; Possible ACQ or Sci spoilers?; None
vcheck; Field BOT clear?; Yes ...
one unknown S1LN033093, has NpgMag (roughly I band) =18.1799 in GSC2, but does not appear in other images or catalogs (neither Gaia nor SDSS show any object
vcheck; Visual BOT check for stars not in catalog?; clear
vcheck; Orbit packing finalized?; yes
vcheck; Buffer times optimized?; yes
vcheck; Verify visit grouping correct; yes
vcheck; phase constraint for ground based observations added?; Yes
vcheck; BETWEENS for coordinated observations added?; yes
vcheck; Is visit ready for int. review?; Yes
Allocated STIS orbits = 1(Tic-Visit
:proposal-id 16114
:visit-id "1S"
:proposal-version -1
:trans-version "20200619"
:date "27-Oct-2020 12:53:42.0"
: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 341008
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16114
:visit-id "1S"
:obset-id "1S"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16114
:visit-id "1S"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2525
:al-overhead-at-end 116
:internal-dur-at-end 958
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2918
:pcs-gap 0
)true10STIS.ta.1460391 calculated for nominal spectrum with S/N = 804X for BOP check: STIS.sp.1460389; B.P. rate = 2.877 cnts/pix/s
Baseline for S/N calculation: STIS.sp.1460388
cvso107_lya2_etc.txt; stis,nuvmama,g230l,c2376,52x2,mjd#59305
Input file: combined_todo_survey_tess_sort_v2_Gaia_J_CP_edit.csv
Spectral type: K7 ; A_V: 0.32 ; Distance (pc): 440
M*: 0.77 ; log(dm/dt): -7.96
For exptime=113.8 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): 2493.8 cts/s/segment
brightest pixel: 0.721 cts/s/pix at 2788.8 A
Calculation performed 2020-07-30T14:21:25, v0.9
cited ETC used Lya x 4 -- with brightest 2.877, global 3035.4Normalizing a K7 star to V=14.78 and E(B-V)=0.152 with mwrv21 gives ETC STIS.sp.1463442 with texp=216s, so double to 432s.
cvso107_lya2_etc.txt; stis,ccd,g430l,c4300,52x2,mjd#59305
WARNING: operating mode = ACCUM
Input file: combined_todo_survey_tess_sort_v2_Gaia_J_CP_edit.csv
Spectral type: K7 ; A_V: 0.32 ; Distance (pc): 440
M*: 0.77 ; log(dm/dt): -7.96
For exptime=70.1 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): 38680.5 cts/s/segment
brightest pixel: 15.042 cts/s/pix at 4871.0 A
Calculation performed 2020-07-30T14:21:25, v0.9
cited ETC used Kstar, has brightest 5.258 at 5308.4 A, global 34.8kcvso107_lya2_etc.txt; stis,ccd,g750l,c7751,52x2,mjd#59305
WARNING: operating mode = ACCUM
Input file: combined_todo_survey_tess_sort_v2_Gaia_J_CP_edit.csv
Spectral type: K7 ; A_V: 0.32 ; Distance (pc): 440
M*: 0.77 ; log(dm/dt): -7.96
For exptime=7.6 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): 62235.0 cts/s/segment
brightest pixel: 93.576 cts/s/pix at 6563.9 A
Calculation performed 2020-07-30T14:21:25, v0.9
cited ETC used sed, with brightest, global as given abovecvso107_lya2_etc.txt; stis,ccd,g750l,c7751,52x2,mjd#59305
WARNING: operating mode = ACCUM
Input file: combined_todo_survey_tess_sort_v2_Gaia_J_CP_edit.csv
Spectral type: K7 ; A_V: 0.32 ; Distance (pc): 440
M*: 0.77 ; log(dm/dt): -7.96
For exptime=7.6 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): 62235.0 cts/s/segment
brightest pixel: 93.576 cts/s/pix at 6563.9 A
Calculation performed 2020-07-30T14:21:25, v0.9cvso107_lya2_etc.txt; stis,ccd,g750l,c7751,52x2,mjd#59305
WARNING: operating mode = ACCUM
Input file: combined_todo_survey_tess_sort_v2_Gaia_J_CP_edit.csv
Spectral type: K7 ; A_V: 0.32 ; Distance (pc): 440
M*: 0.77 ; log(dm/dt): -7.96
For exptime=7.6 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): 62235.0 cts/s/segment
brightest pixel: 93.576 cts/s/pix at 6563.9 A
Calculation performed 2020-07-30T14:21:25, v0.9Timing link suitability includes constraints ([Group (2C 2D 2S) Within 1.0 days])The scheduling data was generated by CASM 28.2.CASM was run in Phase II mode./Users/proffitt/Box/ullyses_tech/ullyses_proposals/survey/16114/OP-cache/ULLYSES_16114-v2C.xmlvstatus; 2C; CVSO-165;P/COS approved for submission; P/CP 02/09/20; internal review complete ; C/DS 16/09/20
vcheck; Enter targ name & Inst. & Resp. Sci.; CVSO-165 ; COS ; CP
vcheck; ETC numbers entered in APT?; Yes
vcheck; Any screening violations?; no
vcheck; M-dwarf check complete and added to box folder?; N/A
vcheck; S/N ETC calcs done & documented?; Yes
vcheck; Field images checked & saved?; Yes
vcheck; Selected ACQ strategy?; PSA MIRRORB, S/N=40 (2X normal to allow for fainter than expected target)
vcheck; Possible ACQ or Sci spoilers?; no, bluer and fainter companion at 5" can be shown to be safe (see comments in ACQ exposure)
vcheck; Field BOT clear?; Yes, GSC2 version of target shows up as unsafe, but target easily safe when estimated spectrum is used.
vcheck; Visual BOT check for stars not in catalog?; companion at 5" not in GSC2, but easily cleared with Gaia mag and color (see disucssion in target comments)
vcheck; Orbit packing finalized?; Yes ...
obtained 82.5% of c1291 goal, and 87.8% of c1611
vcheck; Buffer times optimized?; yes
vcheck; Verify visit grouping correct; Yes, 2S, 2C, 2D within 1 day
vcheck; phase constraint for ground based observations added?; yes
vcheck; BETWEENS for coordinated observations added?; yes
vcheck; Is visit ready for int. review?; Yes
Allocated COS orbits = 4(Tic-Visit
:proposal-id 16114
:visit-id "2C"
:proposal-version -1
:trans-version "20200619"
:date "27-Oct-2020 12:02:23.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 2
:saa-model "31"
:si-bright-earth-limb-angle 20.0
:data-volume 278496
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16114
:visit-id "2C"
:obset-id "2C"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16114
: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 2918
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16114
:visit-id "2C"
:orbit-number 2
:pcs-time 392
:si-vis-utilization 2525
:al-overhead-at-end 0
:internal-dur-at-end 331
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2918
:pcs-gap 0
)true20Use S/N= 40 (2x recommended) with baseline SED to allow for fainter than expected target.
Baseline calculation with CVSO-165_sed.fits: COS.ta.1460398, 157s for S/N = 40, B.P.=1.43
BOP calculation with cvso165_lya2_x4.00_etc.txt gives COS.ta.1460402, B.P. = 5.7
Calculation for blue companion to background star - assume U=15.25 is all due to a hot O3V companion of background ~K2 star - get COS.ta.1460401 with B.P. =30.7, so obs is safe even in this extreme case. If use sdss u=17.186 measured for companion and assume an O3 star get COS.ta.1460403 with B.P. = 10.BOP check spectrum cvso165_lya2_x4.00_etc.txt, COS.sp.1460408, B.P. still geo-coronal lyman alpha
Baseline CVSO-165_sed.fits for S/N, COS.sp.1460409
cvso165_lya2_etc.txt; cos,fuv,g130m,c1291,psa,mjd#59305; fp-pos=None, segment=None)
Input file: combined_todo_survey_tess_sort_v2_Gaia_J_CP_edit.csv
Spectral type: K6 ; A_V: 0.0 ; Distance (pc): 440
M*: 0.91 ; log(dm/dt): -8.43
For exptime=2301.2 s, spectral region:
1239.0 +- 1.0 A achieves SNR=15.0 / 6-pix-resel
A factor of 2.0 has been applied to the exptime in each exposure.
global countrate (brightest segment): 336.7 cts/s/segment
brightest pixel: 0.015 cts/s/pix at 1214.2 A
Calculation performed 2020-07-30T14:21:34, v0.94X for BOP: cvso165_lya2_x4.00_etc.txt, COS.sp.1460412
baseline for S/N CVSO-165_sed.fits, COS.sp.1460410, B.P. = 0.033 cnts/pixel/s
cvso165_lya2_etc.txt; cos,fuv,g160m,c1611,psa,mjd#59305; fp-pos=None, segment=None)
Input file: combined_todo_survey_tess_sort_v2_Gaia_J_CP_edit.csv
Spectral type: K6 ; A_V: 0.0 ; Distance (pc): 440
M*: 0.91 ; log(dm/dt): -8.43
For exptime=2680.0 s, spectral region:
1549.0 +- 1.0 A achieves SNR=30.0 / 6-pix-resel
A factor of 2.0 has been applied to the exptime in each exposure.
global countrate (brightest segment): 83.9 cts/s/segment
brightest pixel: 0.008 cts/s/pix at 1548.4 A
Calculation performed 2020-07-30T14:21:32, v0.94X for BOP: cvso165_lya2_x4.00_etc.txt, COS.sp.1460412
baseline for S/N CVSO-165_sed.fits, COS.sp.1460410, B.P. = 0.033 cnts/pixel/s
cvso165_lya2_etc.txt; cos,fuv,g160m,c1611,psa,mjd#59305; fp-pos=None, segment=None)
Input file: combined_todo_survey_tess_sort_v2_Gaia_J_CP_edit.csv
Spectral type: K6 ; A_V: 0.0 ; Distance (pc): 440
M*: 0.91 ; log(dm/dt): -8.43
For exptime=2680.0 s, spectral region:
1549.0 +- 1.0 A achieves SNR=30.0 / 6-pix-resel
A factor of 2.0 has been applied to the exptime in each exposure.
global countrate (brightest segment): 83.9 cts/s/segment
brightest pixel: 0.008 cts/s/pix at 1548.4 A
Calculation performed 2020-07-30T14:21:32, v0.9Timing link suitability includes constraints ([Group (2C 2D 2S) Within 1.0 days])The scheduling data was generated by CASM 28.2.CASM was run in Phase II mode./Users/proffitt/Box/ullyses_tech/ullyses_proposals/survey/16114/OP-cache/ULLYSES_16114-v2D.xmlvstatus; 2C; CVSO-165; P/COS approved for submission; P/CP 02/09/20; internal review complete ; C/DS 16/09/20
vcheck; Enter targ name & Inst. & Resp. Sci.; CVSO-165 ; COS ; CP
vcheck; ETC numbers entered in APT?; Yes
vcheck; Any screening violations?; no
vcheck; M-dwarf check complete and added to box folder?; N/A
vcheck; S/N ETC calcs done & documented?; Yes
vcheck; Field images checked & saved?; Yes
vcheck; Selected ACQ strategy?; PSA MIRRORB, S/N=40 (2X normal to allow for fainter than expected target)
vcheck; Possible ACQ or Sci spoilers?; ------
vcheck; Field BOT clear?; Yes, GSC2 version of target shows up as unsafe, but target easily safe when estimated spectrum is used.
vcheck; Visual BOT check for stars not in catalog?; companion at 5" not in GSC2, but easily cleared with Gaia mag and color (see disucssion in target comments)
vcheck; Orbit packing finalized?; Yes ...
obtained 82.5% of c1291 goal, and 87.8% of c1611
vcheck; Buffer times optimized?; yes
vcheck; Verify visit grouping correct; Yes, 2S, 2C, 2D within 1 day
vcheck; phase constraint for ground based observations added?; -------
vcheck; BETWEENS for coordinated observations added?; -------
vcheck; Is visit ready for int. review?; ------
Allocated COS orbits = 4(Tic-Visit
:proposal-id 16114
:visit-id "2D"
:proposal-version -1
:trans-version "20200619"
:date "27-Oct-2020 12:02:24.0"
: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 278496
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16114
:visit-id "2D"
:obset-id "2D"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16114
:visit-id "2D"
: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 2918
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16114
:visit-id "2D"
:orbit-number 2
:pcs-time 392
:si-vis-utilization 2525
:al-overhead-at-end 0
:internal-dur-at-end 331
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2918
:pcs-gap 0
)true20Use S/N= 40 (2x recommended) with baseline SED to allow for fainter than expected target.
Baseline calculation with CVSO-165_sed.fits: COS.ta.1460398, 157s for S/N = 40, B.P.=1.43
BOP calculation with cvso165_lya2_x4.00_etc.txt gives COS.ta.1460402, B.P. = 5.7
Calculation for blue companion to background star - assume U=15.25 is all due to a hot O3V companion of background ~K2 star - get COS.ta.1460401 with B.P. =30.7, so obs is safe even in this extreme case. If use sdss u=17.186 measured for companion and assume an O3 star get COS.ta.1460403 with B.P. = 10.BOP check spectrum cvso165_lya2_x4.00_etc.txt, COS.sp.1460408, B.P. still geo-coronal lyman alpha
Baseline CVSO-165_sed.fits for S/N, COS.sp.1460409
cvso165_lya2_etc.txt; cos,fuv,g130m,c1291,psa,mjd#59305; fp-pos=None, segment=None)
Input file: combined_todo_survey_tess_sort_v2_Gaia_J_CP_edit.csv
Spectral type: K6 ; A_V: 0.0 ; Distance (pc): 440
M*: 0.91 ; log(dm/dt): -8.43
For exptime=2301.2 s, spectral region:
1239.0 +- 1.0 A achieves SNR=15.0 / 6-pix-resel
A factor of 2.0 has been applied to the exptime in each exposure.
global countrate (brightest segment): 336.7 cts/s/segment
brightest pixel: 0.015 cts/s/pix at 1214.2 A
Calculation performed 2020-07-30T14:21:34, v0.94X for BOP: cvso165_lya2_x4.00_etc.txt, COS.sp.1460412
baseline for S/N CVSO-165_sed.fits, COS.sp.1460410, B.P. = 0.033 cnts/pixel/s
cvso165_lya2_etc.txt; cos,fuv,g160m,c1611,psa,mjd#59305; fp-pos=None, segment=None)
Input file: combined_todo_survey_tess_sort_v2_Gaia_J_CP_edit.csv
Spectral type: K6 ; A_V: 0.0 ; Distance (pc): 440
M*: 0.91 ; log(dm/dt): -8.43
For exptime=2680.0 s, spectral region:
1549.0 +- 1.0 A achieves SNR=30.0 / 6-pix-resel
A factor of 2.0 has been applied to the exptime in each exposure.
global countrate (brightest segment): 83.9 cts/s/segment
brightest pixel: 0.008 cts/s/pix at 1548.4 A
Calculation performed 2020-07-30T14:21:32, v0.94X for BOP: cvso165_lya2_x4.00_etc.txt, COS.sp.1460412
baseline for S/N CVSO-165_sed.fits, COS.sp.1460410, B.P. = 0.033 cnts/pixel/s
cvso165_lya2_etc.txt; cos,fuv,g160m,c1611,psa,mjd#59305; fp-pos=None, segment=None)
Input file: combined_todo_survey_tess_sort_v2_Gaia_J_CP_edit.csv
Spectral type: K6 ; A_V: 0.0 ; Distance (pc): 440
M*: 0.91 ; log(dm/dt): -8.43
For exptime=2680.0 s, spectral region:
1549.0 +- 1.0 A achieves SNR=30.0 / 6-pix-resel
A factor of 2.0 has been applied to the exptime in each exposure.
global countrate (brightest segment): 83.9 cts/s/segment
brightest pixel: 0.008 cts/s/pix at 1548.4 A
Calculation performed 2020-07-30T14:21:32, v0.9/private/var/folders/c1/kkl4zqqs11g637_3q3f43f2m000400/T/OPVisit1057977171640345139.xmlTiming link suitability includes constraints ([Group (2C 2D 2S) Within 1.0 days])The scheduling data was generated by CASM 28.2.CASM was run in Phase II mode.vstatus; 2S; CVSO-165; S/STIS approved for submission; P/CP 11/08/20 ; internal review complete ; S/DW 11/09/20
vcheck; Enter targ name & Inst. & Resp. Sci.; CVSO-165 ; STIS ; CP
vcheck; ETC numbers entered in APT?; Yes
vcheck; Any screening violations?; No
vcheck; M-dwarf check complete and added to box folder?; N/A
vcheck; S/N ETC calcs done & documented?; Yes
vcheck; Field images checked & saved?; Yes
vcheck; Selected ACQ strategy?; F28X50LP, S/N=80
vcheck; Possible ACQ or Sci spoilers?; companion star is too faint to endanger ACQ, and well away along slit from primary target; companion has Gaia Rp 2 mags fainter than primary target
vcheck; Field BOT clear?; Yes
vcheck; Visual BOT check for stars not in catalog?; OK, companion is safe and well displaced
vcheck; Orbit packing finalized?; Yes
vcheck; Buffer times optimized?; yes
vcheck; Verify visit grouping correct; Yes, 2S, 2C, 2D within 1 day
vcheck; phase constraint for ground based observations added?; yes
vcheck; BETWEENS for coordinated observations added?; yes
vcheck; Is visit ready for int. review?; Yes
Allocated STIS orbits = 1(Tic-Visit
:proposal-id 16114
:visit-id "2S"
:proposal-version -1
:trans-version "20200619"
:date "27-Oct-2020 12:53:45.0"
: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 377808
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16114
:visit-id "2S"
:obset-id "2S"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16114
:visit-id "2S"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2525
:al-overhead-at-end 116
:internal-dur-at-end 1220
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2918
:pcs-gap 0
)true10STIS.ta.1460414 gives S/N=80 with F28x50LP for baseline spectrum in 0.41 sBOP calculation using 4X spectrum cvso165_lya2_x4.00_etc.txt gives STIS.sp.1460418 with B.P. = 2.053 cnts/pixel/s
Baseline calculation STIS.sp.1460417 gets S/N=40.84 at 2789
cvso165_lya2_etc.txt; stis,nuvmama,g230l,c2376,52x2,mjd#59305
Input file: combined_todo_survey_tess_sort_v2_Gaia_J_CP_edit.csv
Spectral type: K6 ; A_V: 0.0 ; Distance (pc): 440
M*: 0.91 ; log(dm/dt): -8.43
For exptime=160.5 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): 2436.6 cts/s/segment
brightest pixel: 0.515 cts/s/pix at 2790.4 A
Calculation performed 2020-07-30T14:21:34, v0.9
cited ETC used Lya x 4 -- with brightest 2.053, global 2806.4STIS.sp.1460416 needs 224.9s to reach S/N=10 at 4000 angstroms using baseline scaling
In this case, the stellar contiuum looks to be brighter than the , so STIS.sp.1463444 suggests only 66s needed~
We'll compromise and use 225s as the adopted exposure time to save more time for the G230L
cvso165_lya2_etc.txt; stis,ccd,g430l,c4300,52x2,mjd#59305
WARNING: operating mode = ACCUM
Input file: combined_todo_survey_tess_sort_v2_Gaia_J_CP_edit.csv
Spectral type: K6 ; A_V: 0.0 ; Distance (pc): 440
M*: 0.91 ; log(dm/dt): -8.43
For exptime=92.1 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): 35954.9 cts/s/segment
brightest pixel: 10.903 cts/s/pix at 4871.0 A
Calculation performed 2020-07-30T14:21:34, v0.9
cited ETC used sed, with brightest, global rates as given above -- but time not multiplied by 2STIS.sp.1460415 needs 26.1s with baseline SED to get S/N=20 at 5700 angstroms
cvso165_lya2_etc.txt; stis,ccd,g750l,c7751,52x2,mjd#59305
WARNING: operating mode = ACCUM
Input file: combined_todo_survey_tess_sort_v2_Gaia_J_CP_edit.csv
Spectral type: K6 ; A_V: 0.0 ; Distance (pc): 440
M*: 0.91 ; log(dm/dt): -8.43
For exptime=11.1 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): 53833.2 cts/s/segment
brightest pixel: 72.578 cts/s/pix at 6563.9 A
Calculation performed 2020-07-30T14:21:34, v0.9
cited ETC used sed, with brightest, global rates as given aboveAdded extra 52x0.1 fringe flat for use with the second star in the slitTiming link suitability includes constraints ([Group (3C 3D 3S) Within 1.0 days])The scheduling data was generated by CASM 28.2.CASM was run in Phase II mode./Users/proffitt/Box/ullyses_tech/ullyses_proposals/survey/16114/OP-cache/ULLYSES_16114-v3C.xmlvstatus; 3C; CVSO-58; P/COS approved for submission; P/CP 02/09/20; internal review complete ; C/DS 16/09/20
vcheck; Enter targ name & Inst. & Resp. Sci.; CVSO-58 ; COS ; CP
vcheck; ETC numbers entered in APT?; Yes
vcheck; Any screening violations?; No
vcheck; M-dwarf check complete and added to box folder?; N/A
vcheck; S/N ETC calcs done & documented?; yes
vcheck; Field images checked & saved?; yes
vcheck; Selected ACQ strategy?; PSA, MIRROB, S/N=40 requires texp=163.4s
vcheck; Possible ACQ or Sci spoilers?;None
vcheck; Field BOT clear?; yes
vcheck; Visual BOT check for stars not in catalog?; all clear
vcheck; Orbit packing finalized?; yes ...
Awkward to split our 6 exposures over 5 orbits. Got 81.8% of requested c1291 and 106.3% of c1611.
Split into 3+2 orbit visits. Split as follows
3 orbit visit 3C: c1291-4 1185s; c1611-1,2,3 1570s each with FP-2 split over two orbits
2 orbit visit 3D:c1291-3 1185s+273s; c1291-4, 274s; c1611-4 1570s
could get more ~100s more c1291 time if we're willing to live with uneven split between FPPOS 3 and 4 exposure times.
vcheck; Buffer times optimized?; yes
vcheck; Verify visit grouping correct; Group 3S, 3C, and 3D within 1 day
vcheck; phase constraint for ground based observations added?; yes
vcheck; BETWEENS for coordinated observations added?; Between 19 Nov 2020 and 17 Dec 2020
vcheck; Is visit ready for int. review?; Yes
Allocated COS orbits = 5(Tic-Visit
:proposal-id 16114
:visit-id "3C"
:proposal-version -1
:trans-version "20200619"
:date "27-Oct-2020 12:02:28.0"
: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 469888
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16114
:visit-id "3C"
:obset-id "3C"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16114
:visit-id "3C"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2525
: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 2918
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16114
:visit-id "3C"
:orbit-number 2
:pcs-time 392
:si-vis-utilization 2526
: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 2918
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16114
:visit-id "3C"
:orbit-number 3
:pcs-time 392
:si-vis-utilization 2524
:al-overhead-at-end 0
:internal-dur-at-end 331
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2918
:pcs-gap 0
)true30Baseline calc CVSO-58_sed.fits, S/N=40, COS.ta.1460423, B.P. = 1.374 cnts/pix/s, exptime=163.4s
BOP calc COS.ta.1460424, B.P. = 5.4774X BOP check: COS.sp.1460432, BP is lyman-alpha geo-coronal
Nominal S/N calculation : COS.sp.1460431
cvso58_lya2_etc.txt; cos,fuv,g130m,c1291,psa,mjd#59305; fp-pos=None, segment=None)
Input file: combined_todo_survey_tess_sort_v2_Gaia_J_CP_edit.csv
Spectral type: K7 ; A_V: 0.12 ; Distance (pc): 440
M*: 0.78 ; log(dm/dt): -8.35
For exptime=2636.9 s, spectral region:
1239.0 +- 1.0 A achieves SNR=15.0 / 6-pix-resel
A factor of 2.0 has been applied to the exptime in each exposure.
global countrate (brightest segment): 316.2 cts/s/segment
brightest pixel: 0.005 cts/s/pix at 1304.9 A
Calculation performed 2020-07-30T14:21:50, v0.94x BOP spectrum cvso58_lya2_x4.00_etc.txt; COS.sp.1460428; B.P.= 0.030 cnts/pix/s
Nominal S/N calculation COS.sp.1460429
cvso58_lya2_etc.txt; cos,fuv,g160m,c1611,psa,mjd#59305; fp-pos=None, segment=None)
Input file: combined_todo_survey_tess_sort_v2_Gaia_J_CP_edit.csv
Spectral type: K7 ; A_V: 0.12 ; Distance (pc): 440
M*: 0.78 ; log(dm/dt): -8.35
For exptime=2952.6 s, spectral region:
1549.0 +- 1.0 A achieves SNR=30.0 / 6-pix-resel
A factor of 2.0 has been applied to the exptime in each exposure.
global countrate (brightest segment): 83.1 cts/s/segment
brightest pixel: 0.008 cts/s/pix at 1548.4 A
Calculation performed 2020-07-30T14:21:47, v0.94x BOP spectrum cvso58_lya2_x4.00_etc.txt; COS.sp.1460428; B.P.= 0.030 cnts/pix/s
Nominal S/N calculation COS.sp.1460429
cvso58_lya2_etc.txt; cos,fuv,g160m,c1611,psa,mjd#59305; fp-pos=None, segment=None)
Input file: combined_todo_survey_tess_sort_v2_Gaia_J_CP_edit.csv
Spectral type: K7 ; A_V: 0.12 ; Distance (pc): 440
M*: 0.78 ; log(dm/dt): -8.35
For exptime=2952.6 s, spectral region:
1549.0 +- 1.0 A achieves SNR=30.0 / 6-pix-resel
A factor of 2.0 has been applied to the exptime in each exposure.
global countrate (brightest segment): 83.1 cts/s/segment
brightest pixel: 0.008 cts/s/pix at 1548.4 A
Calculation performed 2020-07-30T14:21:47, v0.94x BOP spectrum cvso58_lya2_x4.00_etc.txt; COS.sp.1460428; B.P.= 0.030 cnts/pix/s
Nominal S/N calculation COS.sp.1460429
cvso58_lya2_etc.txt; cos,fuv,g160m,c1611,psa,mjd#59305; fp-pos=None, segment=None)
Input file: combined_todo_survey_tess_sort_v2_Gaia_J_CP_edit.csv
Spectral type: K7 ; A_V: 0.12 ; Distance (pc): 440
M*: 0.78 ; log(dm/dt): -8.35
For exptime=2952.6 s, spectral region:
1549.0 +- 1.0 A achieves SNR=30.0 / 6-pix-resel
A factor of 2.0 has been applied to the exptime in each exposure.
global countrate (brightest segment): 83.1 cts/s/segment
brightest pixel: 0.008 cts/s/pix at 1548.4 A
Calculation performed 2020-07-30T14:21:47, v0.94x BOP spectrum cvso58_lya2_x4.00_etc.txt; COS.sp.1460428; B.P.= 0.030 cnts/pix/s
Nominal S/N calculation COS.sp.1460429
cvso58_lya2_etc.txt; cos,fuv,g160m,c1611,psa,mjd#59305; fp-pos=None, segment=None)
Input file: combined_todo_survey_tess_sort_v2_Gaia_J_CP_edit.csv
Spectral type: K7 ; A_V: 0.12 ; Distance (pc): 440
M*: 0.78 ; log(dm/dt): -8.35
For exptime=2952.6 s, spectral region:
1549.0 +- 1.0 A achieves SNR=30.0 / 6-pix-resel
A factor of 2.0 has been applied to the exptime in each exposure.
global countrate (brightest segment): 83.1 cts/s/segment
brightest pixel: 0.008 cts/s/pix at 1548.4 A
Calculation performed 2020-07-30T14:21:47, v0.9Timing link suitability includes constraints ([Group (3C 3D 3S) Within 1.0 days])The scheduling data was generated by CASM 28.2.CASM was run in Phase II mode./Users/proffitt/Box/ullyses_tech/ullyses_proposals/survey/16114/OP-cache/ULLYSES_16114-v3D.xmlvstatus; 3C; CVSO-58; P/COS approved for submission; P/CP 02/09/20; internal review complete ; C/DS 16/09/20
vcheck; Enter targ name & Inst. & Resp. Sci.; CVSO-58 ; COS ; CP
vcheck; ETC numbers entered in APT?; Yes
vcheck; Any screening violations?; No
vcheck; M-dwarf check complete and added to box folder?; N/A
vcheck; S/N ETC calcs done & documented?; yes
vcheck; Field images checked & saved?; ------
vcheck; Selected ACQ strategy?; PSA, MIRROB, S/N=40 requires texp=163.4s
vcheck; Possible ACQ or Sci spoilers?;None
vcheck; Field BOT clear?; yes
vcheck; Visual BOT check for stars not in catalog?; all clear
vcheck; Orbit packing finalized?; ------
vcheck; Buffer times optimized?; ------
vcheck; Verify visit grouping correct; ------
vcheck; phase constraint for ground based observations added?; -------
vcheck; BETWEENS for coordinated observations added?; -------
vcheck; Is visit ready for int. review?; ------
Allocated COS orbits = 5(Tic-Visit
:proposal-id 16114
:visit-id "3D"
:proposal-version -1
:trans-version "20200619"
:date "27-Oct-2020 12:02:29.0"
: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 226336
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16114
:visit-id "3D"
:obset-id "3D"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16114
:visit-id "3D"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2525
: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 2918
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16114
:visit-id "3D"
:orbit-number 2
:pcs-time 392
:si-vis-utilization 2526
:al-overhead-at-end 0
:internal-dur-at-end 331
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2918
:pcs-gap 0
)true20Baseline calc CVSO-58_sed.fits, S/N=40, COS.ta.1460423, B.P. = 1.374 cnts/pix/s, exptime=163.4s
BOP calc COS.ta.1460424, B.P. = 5.4774X BOP check: COS.sp.1460432, BP is lyman-alpha geo-coronal
Nominal S/N calculation : COS.sp.1460431
cvso58_lya2_etc.txt; cos,fuv,g130m,c1291,psa,mjd#59305; fp-pos=None, segment=None)
Input file: combined_todo_survey_tess_sort_v2_Gaia_J_CP_edit.csv
Spectral type: K7 ; A_V: 0.12 ; Distance (pc): 440
M*: 0.78 ; log(dm/dt): -8.35
For exptime=2636.9 s, spectral region:
1239.0 +- 1.0 A achieves SNR=15.0 / 6-pix-resel
A factor of 2.0 has been applied to the exptime in each exposure.
global countrate (brightest segment): 316.2 cts/s/segment
brightest pixel: 0.005 cts/s/pix at 1304.9 A
Calculation performed 2020-07-30T14:21:50, v0.94X BOP check: COS.sp.1460432, BP is lyman-alpha geo-coronal
Nominal S/N calculation : COS.sp.1460431
cvso58_lya2_etc.txt; cos,fuv,g130m,c1291,psa,mjd#59305; fp-pos=None, segment=None)
Input file: combined_todo_survey_tess_sort_v2_Gaia_J_CP_edit.csv
Spectral type: K7 ; A_V: 0.12 ; Distance (pc): 440
M*: 0.78 ; log(dm/dt): -8.35
For exptime=2636.9 s, spectral region:
1239.0 +- 1.0 A achieves SNR=15.0 / 6-pix-resel
A factor of 2.0 has been applied to the exptime in each exposure.
global countrate (brightest segment): 316.2 cts/s/segment
brightest pixel: 0.005 cts/s/pix at 1304.9 A
Calculation performed 2020-07-30T14:21:50, v0.94X BOP check: COS.sp.1460432, BP is lyman-alpha geo-coronal
Nominal S/N calculation : COS.sp.1460431
cvso58_lya2_etc.txt; cos,fuv,g130m,c1291,psa,mjd#59305; fp-pos=None, segment=None)
Input file: combined_todo_survey_tess_sort_v2_Gaia_J_CP_edit.csv
Spectral type: K7 ; A_V: 0.12 ; Distance (pc): 440
M*: 0.78 ; log(dm/dt): -8.35
For exptime=2636.9 s, spectral region:
1239.0 +- 1.0 A achieves SNR=15.0 / 6-pix-resel
A factor of 2.0 has been applied to the exptime in each exposure.
global countrate (brightest segment): 316.2 cts/s/segment
brightest pixel: 0.005 cts/s/pix at 1304.9 A
Calculation performed 2020-07-30T14:21:50, v0.94x BOP spectrum cvso58_lya2_x4.00_etc.txt; COS.sp.1460428; B.P.= 0.030 cnts/pix/s
Nominal S/N calculation COS.sp.1460429
cvso58_lya2_etc.txt; cos,fuv,g160m,c1611,psa,mjd#59305; fp-pos=None, segment=None)
Input file: combined_todo_survey_tess_sort_v2_Gaia_J_CP_edit.csv
Spectral type: K7 ; A_V: 0.12 ; Distance (pc): 440
M*: 0.78 ; log(dm/dt): -8.35
For exptime=2952.6 s, spectral region:
1549.0 +- 1.0 A achieves SNR=30.0 / 6-pix-resel
A factor of 2.0 has been applied to the exptime in each exposure.
global countrate (brightest segment): 83.1 cts/s/segment
brightest pixel: 0.008 cts/s/pix at 1548.4 A
Calculation performed 2020-07-30T14:21:47, v0.9/private/var/folders/c1/kkl4zqqs11g637_3q3f43f2m000400/T/OPVisit9604482717348055535.xmlTiming link suitability includes constraints ([Group (3C 3D 3S) Within 1.0 days])The scheduling data was generated by CASM 28.2.CASM was run in Phase II mode.vstatus; 3S; CVSO-58; S/STIS approved for submission; P/CP 12/08/20 ; internal review complete ; S/DW 11/09/20
vcheck; Enter targ name & Inst. & Resp. Sci.; CVSO-58 ; STIS ; CP
vcheck; ETC numbers entered in APT?; Yes
vcheck; Any screening violations?; No
vcheck; M-dwarf check complete and added to box folder?; N/A
vcheck; S/N ETC calcs done & documented?; Yes
vcheck; Field images checked & saved?; yes
vcheck; Selected ACQ strategy?; F28X50LP with S/N=80 (2x normal requirement)
vcheck; Possible ACQ or Sci spoilers?; none
vcheck; Field BOT clear?; yes
vcheck; Visual BOT check for stars not in catalog?; clear
vcheck; Orbit packing finalized?; yes
vcheck; Buffer times optimized?; yes
vcheck; Verify visit grouping correct; SEQ 3S, 3C, 3D within 1 orbit
vcheck; phase constraint for ground based observations added?; yes
vcheck; BETWEENS for coordinated observations added?; Yes
vcheck; Is visit ready for int. review?; yes
Allocated STIS orbits = 1(Tic-Visit
:proposal-id 16114
:visit-id "3S"
:proposal-version -1
:trans-version "20200619"
:date "27-Oct-2020 12:53:48.0"
: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 341008
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16114
:visit-id "3S"
:obset-id "3S"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16114
:visit-id "3S"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2525
:al-overhead-at-end 116
:internal-dur-at-end 958
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2918
:pcs-gap 0
)true10Used baseline spectrum, but with S/N=80 to allow for fainter than expected target STIS.ta.1460500baseline calculation STIS.sp.1460503 requires 167s, with B.P.=0.494
with actual exposure time STIS.sp.1460504 gives S/N=40 at peak of Mg II
4X BOP calculation STIS.sp.1460505 gives B.P. = 1.971 cnts/pix/s
cvso58_lya2_etc.txt; stis,nuvmama,g230l,c2376,52x2,mjd#59305
Input file: combined_todo_survey_tess_sort_v2_Gaia_J_CP_edit.csv
Spectral type: K7 ; A_V: 0.12 ; Distance (pc): 440
M*: 0.78 ; log(dm/dt): -8.35
For exptime=167.3 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): 2433.3 cts/s/segment
brightest pixel: 0.494 cts/s/pix at 2790.4 A
Calculation performed 2020-07-30T14:21:50, v0.9
cited ETC used Lya x 4 -- with brightest 1.971, global 2793baseline calculation STIS.sp.1460502, requires 228.9s, so double to 457.8s
Using just the K star spectrum gives STIS.sp.1463454 for 226s, so all is good!
cvso58_lya2_etc.txt; stis,ccd,g430l,c4300,52x2,mjd#59305
WARNING: operating mode = ACCUM
Input file: combined_todo_survey_tess_sort_v2_Gaia_J_CP_edit.csv
Spectral type: K7 ; A_V: 0.12 ; Distance (pc): 440
M*: 0.78 ; log(dm/dt): -8.35
For exptime=93.8 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): 35983.6 cts/s/segment
brightest pixel: 10.940 cts/s/pix at 4871.0 A
Calculation performed 2020-07-30T14:21:50, v0.9
cited ETC used sed, with brightest, global rates as given abovebaseline calculation STIS.sp.1460501, requires 25.6s, so double to 51.2s
cvso58_lya2_etc.txt; stis,ccd,g750l,c7751,52x2,mjd#59305
WARNING: operating mode = ACCUM
Input file: combined_todo_survey_tess_sort_v2_Gaia_J_CP_edit.csv
Spectral type: K7 ; A_V: 0.12 ; Distance (pc): 440
M*: 0.78 ; log(dm/dt): -8.35
For exptime=10.9 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): 54309.6 cts/s/segment
brightest pixel: 73.144 cts/s/pix at 6563.9 A
Calculation performed 2020-07-30T14:21:50, v0.9
cited ETC used sed, with brightest, global rates as given abovecvso58_lya2_etc.txt; stis,ccd,g750l,c7751,52x2,mjd#59305
WARNING: operating mode = ACCUM
Input file: combined_todo_survey_tess_sort_v2_Gaia_J_CP_edit.csv
Spectral type: K7 ; A_V: 0.12 ; Distance (pc): 440
M*: 0.78 ; log(dm/dt): -8.35
For exptime=10.9 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): 54309.6 cts/s/segment
brightest pixel: 73.144 cts/s/pix at 6563.9 A
Calculation performed 2020-07-30T14:21:50, v0.9cvso58_lya2_etc.txt; stis,ccd,g750l,c7751,52x2,mjd#59305
WARNING: operating mode = ACCUM
Input file: combined_todo_survey_tess_sort_v2_Gaia_J_CP_edit.csv
Spectral type: K7 ; A_V: 0.12 ; Distance (pc): 440
M*: 0.78 ; log(dm/dt): -8.35
For exptime=10.9 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): 54309.6 cts/s/segment
brightest pixel: 73.144 cts/s/pix at 6563.9 A
Calculation performed 2020-07-30T14:21:50, v0.9Timing link suitability includes constraints ([Group (4C 4S) Within 1.0 days])The scheduling data was generated by CASM 28.2.CASM was run in Phase II mode./Users/proffitt/Box/ullyses_tech/ullyses_proposals/survey/16114/OP-cache/ULLYSES_16114-v4C.xmlvstatus; 4C; CVSO-90; P/COS approved for submission; P/CP 02/09/20 ; internal review complete ; C/DS 16/09/20
vcheck; Enter targ name & Inst. & Resp. Sci.; CVSO-90 ; COS ; CP
vcheck; ETC numbers entered in APT?; yes
vcheck; Any screening violations?; no
vcheck; M-dwarf check complete and added to box folder?; N/A
vcheck; S/N ETC calcs done & documented?; yes
vcheck; Field images checked & saved?; yes
vcheck; Selected ACQ strategy?; PSA, MIRRORB, S/N=40
vcheck; Possible ACQ or Sci spoilers?; None
vcheck; Field BOT clear?; yes
vcheck; Visual BOT check for stars not in catalog?; OK
vcheck; Orbit packing finalized?; yes ...
obtained 151.5% of requested c1611 and 154.1% of c1291
vcheck; Buffer times optimized?; Yes
vcheck; Verify visit grouping correct; Group 4C,4S within 1 Day
vcheck; phase constraint for ground based observations added?; yes
vcheck; BETWEENS for coordinated observations added?; Yes
vcheck; Is visit ready for int. review?; yes
Allocated COS orbits = 2(Tic-Visit
:proposal-id 16114
:visit-id "4C"
:proposal-version -1
:trans-version "20200619"
:date "27-Oct-2020 12:02:33.0"
: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 591648
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16114
:visit-id "4C"
:obset-id "4C"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16114
:visit-id "4C"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2523
: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 2918
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16114
:visit-id "4C"
:orbit-number 2
:pcs-time 392
:si-vis-utilization 2524
:al-overhead-at-end 0
:internal-dur-at-end 341
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2918
:pcs-gap 0
)true20Baseline calc COS.ta.1460511 at S/N=40 requires 39.5 s with B.P. = 5.643
BOP calc COS.ta.1460512 has B.P. = 22.5 cnts/pix/s4x BOP ETC calc COS.sp.1460515, P.B.=0.109 cnts/pix/s
baseline S/N ETC calc COS.sp.1460517
cvso90_lya2_etc.txt; cos,fuv,g160m,c1611,psa,mjd#59305; fp-pos=None, segment=None)
Input file: combined_todo_survey_tess_sort_v2_Gaia_J_CP_edit.csv
Spectral type: K7 ; A_V: 0.0 ; Distance (pc): 440
M*: 0.79 ; log(dm/dt): -7.75
For exptime=814.6 s, spectral region:
1549.0 +- 1.0 A achieves SNR=30.0 / 6-pix-resel
A factor of 2.0 has been applied to the exptime in each exposure.
global countrate (brightest segment): 115.2 cts/s/segment
brightest pixel: 0.027 cts/s/pix at 1548.4 A
Calculation performed 2020-07-30T14:20:23, v0.94X BOP ETC calc COS.sp.1460519, gives B.P. 0.432
Would have to scale to U=13.1 (COS.sp.1460521) to get close to local limit in Lyman alpha line
(may need to consider ISM geocoronal absorbption if brighter than this?)
Baseline S/N ETC calc COS.sp.1460518
cvso90_lya2_etc.txt; cos,fuv,g130m,c1291,psa,mjd#59305; fp-pos=None, segment=None)
Input file: combined_todo_survey_tess_sort_v2_Gaia_J_CP_edit.csv
Spectral type: K7 ; A_V: 0.0 ; Distance (pc): 440
M*: 0.79 ; log(dm/dt): -7.75
For exptime=484.1 s, spectral region:
1239.0 +- 1.0 A achieves SNR=15.0 / 6-pix-resel
A factor of 2.0 has been applied to the exptime in each exposure.
global countrate (brightest segment): 573.7 cts/s/segment
brightest pixel: 0.108 cts/s/pix at 1214.2 A
Calculation performed 2020-07-30T14:20:25, v0.9cvso90_lya2_etc.txt; cos,fuv,g130m,c1291,psa,mjd#59305; fp-pos=None, segment=None)
Input file: combined_todo_survey_tess_sort_v2_Gaia_J_CP_edit.csv
Spectral type: K7 ; A_V: 0.0 ; Distance (pc): 440
M*: 0.79 ; log(dm/dt): -7.75
For exptime=484.1 s, spectral region:
1239.0 +- 1.0 A achieves SNR=15.0 / 6-pix-resel
A factor of 2.0 has been applied to the exptime in each exposure.
global countrate (brightest segment): 573.7 cts/s/segment
brightest pixel: 0.108 cts/s/pix at 1214.2 A
Calculation performed 2020-07-30T14:20:25, v0.9/private/var/folders/c1/kkl4zqqs11g637_3q3f43f2m000400/T/OPVisit18322564454345776242.xmlTiming link suitability includes constraints ([Group (4C 4S) Within 1.0 days])The scheduling data was generated by CASM 28.2.CASM was run in Phase II mode.vstatus; 4S; CVSO-90; S/STIS approved for submission; P/CP 12/08/20 ; internal review complete ; S/DW 11/09/20
vcheck; Enter targ name & Inst. & Resp. Sci.; CVSO-90 ; STIS ; CP
vcheck; ETC numbers entered in APT?; Yes
vcheck; Any screening violations?; No
vcheck; M-dwarf check complete and added to box folder?; N/A
vcheck; S/N ETC calcs done & documented?;Yes
vcheck; Field images checked & saved?; yes, field completely clear except for target
vcheck; Selected ACQ strategy?; F28X50LP with S/N=80 for baseline spectrum
vcheck; Possible ACQ or Sci spoilers?; None
vcheck; Field BOT clear?; yes
vcheck; Visual BOT check for stars not in catalog?;OK
vcheck; Orbit packing finalized?; Yes
vcheck; Buffer times optimized?; Yes
vcheck; Verify visit grouping correct; Seq 4S, 4C within 1 orbit
vcheck; phase constraint for ground based observations added?; yes
vcheck; BETWEENS for coordinated observations added?; Done
vcheck; Is visit ready for int. review?; yes
Allocated STIS orbits = 1(Tic-Visit
:proposal-id 16114
:visit-id "4S"
:proposal-version -1
:trans-version "20200619"
:date "27-Oct-2020 12:53:50.0"
: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 410592
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16114
:visit-id "4S"
:obset-id "4S"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16114
:visit-id "4S"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2525
:al-overhead-at-end 116
:internal-dur-at-end 958
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2918
:pcs-gap 0
)true10STIS.ta.1460530 suggests 0.2s for S/N=804X BOP ETC calc
Baseline S/N calc STIS.sp.1460528, B.P. = 7.4 cnts/pix/s
cvso90_lya2_etc.txt; stis,nuvmama,g230l,c2376,52x2,mjd#59305
Input file: combined_todo_survey_tess_sort_v2_Gaia_J_CP_edit.csv
Spectral type: K7 ; A_V: 0.0 ; Distance (pc): 440
M*: 0.79 ; log(dm/dt): -7.75
For exptime=43.7 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): 2799.2 cts/s/segment
brightest pixel: 1.860 cts/s/pix at 2788.8 A
Calculation performed 2020-07-30T14:20:25, v0.9
cited ETC used Lya sed x 4 -- with brightest 7.432, global 4257Baseline ETC calc STIS.sp.1460527 requies 88.6s for S/N=20, so would normally request 177.2s
However, if we instead normalize a K7 star to the observed V mag, we get STIS.sp.1463450, which requires 155.4s -> So let's adopt 310s.
cvso90_lya2_etc.txt; stis,ccd,g430l,c4300,52x2,mjd#59305
WARNING: operating mode = ACCUM
Input file: combined_todo_survey_tess_sort_v2_Gaia_J_CP_edit.csv
Spectral type: K7 ; A_V: 0.0 ; Distance (pc): 440
M*: 0.79 ; log(dm/dt): -7.75
For exptime=35.5 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): 46743.9 cts/s/segment
brightest pixel: 27.378 cts/s/pix at 4871.0 A
Calculation performed 2020-07-30T14:20:25, v0.9
cited ETC used K7sed for CVSO-165 ?Baseline ETC calc STIS.sp.1460526 requies 10.4s for S/N=20, so request 20.8s
cvso90_lya2_etc.txt; stis,ccd,g750l,c7751,52x2,mjd#59305
WARNING: operating mode = ACCUM
Input file: combined_todo_survey_tess_sort_v2_Gaia_J_CP_edit.csv
Spectral type: K7 ; A_V: 0.0 ; Distance (pc): 440
M*: 0.79 ; log(dm/dt): -7.75
For exptime=4.4 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): 78694.2 cts/s/segment
brightest pixel: 143.618 cts/s/pix at 6563.9 A
Calculation performed 2020-07-30T14:20:25, v0.9cvso90_lya2_etc.txt; stis,ccd,g750l,c7751,52x2,mjd#59305
WARNING: operating mode = ACCUM
Input file: combined_todo_survey_tess_sort_v2_Gaia_J_CP_edit.csv
Spectral type: K7 ; A_V: 0.0 ; Distance (pc): 440
M*: 0.79 ; log(dm/dt): -7.75
For exptime=4.4 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): 78694.2 cts/s/segment
brightest pixel: 143.618 cts/s/pix at 6563.9 A
Calculation performed 2020-07-30T14:20:25, v0.9cvso90_lya2_etc.txt; stis,ccd,g750l,c7751,52x2,mjd#59305
WARNING: operating mode = ACCUM
Input file: combined_todo_survey_tess_sort_v2_Gaia_J_CP_edit.csv
Spectral type: K7 ; A_V: 0.0 ; Distance (pc): 440
M*: 0.79 ; log(dm/dt): -7.75
For exptime=4.4 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): 78694.2 cts/s/segment
brightest pixel: 143.618 cts/s/pix at 6563.9 A
Calculation performed 2020-07-30T14:20:25, v0.9