Resubmission with repeat COS and STIS visits (AC and AS, respectiviely) allowed by HOPR #91993 because the original visits (1C and 1S, respectively) failed.
The hard BETWEEN on AC and AS is 12 MAY 2021 00:00 to 10 JUL 2021 23:59 to ensure effective ground based coordination
However, coordination with TESS in sector 30 requires the following BETWEENs:
27 MAY 2021 07:00 to 09 JUN 2021 05:35 and 10 JUN 2021 09:10 - 24 JUN 2021 00:55 for AC
27 MAY 2021 07:00 to 09 JUN 2021 07:10 and 10 JUN 2021 09:10 - 24 JUN 2021 02:30 for AS
AC and AS are grouped within 1 day
---------
Resubmission with updates to the BETWEEN windows for coordination with TESS
---------
Resubmission after removing RECX-7 observations: RECX-7 turns out to be a binary, we can’t clear the apparent M dwarf against flares, and the scientific motivation also becomes dubious.
Title revised to reflect the current observations
---------
Resubmitting after a correcting a G160M cenwave setting error in Exposure 5 of Visit 1C. The cevwave was set to 1611 my mistake and in this submission it is now switched to 1623.
Minor updates: Updated the exposure level comments in Visits 1C, 2C and 2D with the appropriate ETC IDs
---------
Resubmitting to replace c1611 with 1589 (FP 3 and 4) + 1623 (FP 1 and 2) to avoid dropping an important molecular feature in the hole between the segments.
---------
Final implementation done - program ready for CS review
Added a Co-I
Added one orbit in visit 2S
---------
Placeholder submission comments: ----
This is a placeholder with a total of 10 orbits on ECHA J0844.2-7833, and RECX 7. All targets have the same TESS windows (sector 37).
We've restricted the timing to the TESS windows, taking into account the gap in the middle of the sector coverage.
We've also included the "GROUP WITHIN 1 DAY" for each of our targets.
We still have some questions about the FUV exposure times, so its possible we'll come back and add more orbits to some targets, but for now we're giving you our best available
estimate.
----------1470676021----- Attempting Submission 1 (Fri Dec 11 22:28:20 GMT 2020) -----
HST Phase II Proposal 16480 successfully submitted.
Receipt: # 16480-1
----- Attempting Submission 2 (Wed Feb 10 00:34:36 GMT 2021) -----
----- Attempting Submission 3 (Wed Feb 10 19:02:49 GMT 2021) -----
HST Phase II Proposal 16480 successfully submitted.
Receipt: # 16480-3
----- Attempting Submission 4 (Tue Feb 23 15:23:42 GMT 2021) -----
HST Phase II Proposal 16480 successfully submitted.
Receipt: # 16480-4
----- Attempting Submission 5 (Thu Feb 25 17:51:21 GMT 2021) -----
HST Phase II Proposal 16480 successfully submitted.
Receipt: # 16480-5
----- Attempting Submission 6 (Thu Mar 18 15:26:55 GMT 2021) -----
----- Attempting Submission 7 (Wed May 12 01:13:28 GMT 2021) -----ULLYSES T Tauri Survey Star ECHA J0844-7833 in eta ChaThe 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 is a placeholder visit to allow determination of LRP schedulability. Detailed implementaton, including ETC calculations, BOP checks and detailed justification has yet to be done. There may be significant changes in the final flight version.
Intent is to coordinate the objects in this program with TESS, which should observe them during TESS sector 37.
current ESTIMATE for BETWEENs to ensure this are:
02 APR 2021 19:45 - 14 APR 2021 08:55
15 APR 2021 14:25 - 27 APR 2021 22:05
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.0falseSUPPORTEDSTART TAURI STARPRE-MAIN SEQUENCE STARNOECHA J0844.2-7833 : RECX 16, J08440914-7833457
Region: eta Cha
Simbad: https://simbad.u-strasbg.fr/simbad/sim-id?Ident=2MASS+J08440914-7833457&submit=submit+id
Target coordinates are from Gaia DR2.
Spectral type: M6.0 ; A_V: 0.0 ; Distance (pc): 94
M*: 0.052000000000000005 ; log(dm/dt): -10.18
Input file: spring-survey-todo-crp06dec20.csv
echaj08442-7833_lya2_etc.txt
Calculation performed 2020-12-08T03:53:58, v0.4
-------------------------------------------------------------------------------
tstatus; ECHA-J0844.2-7833; P/COS approved for submission; S/STIS approved for submission; P/DS 09/02/21; S/DS 09/02/21
tcheck; APT/SIMBAD target names: ; ECHA-J0844.2-7833 ...
Default SIMBAD name is DENIS J084409.1-783345, aka 2MASS J08440915-7833457, RECX 16
tcheck; Target info verification status?; OK ...
Flam(B) = 3e-16 at 4444 Angstroms and Flam(V) = 5.3e-16 at 5540 Angstroms from Vizier photometry viewer linked from SIMBAD page. R = 17.36 from NOMAD
tcheck; Coordinates & P.M. verified, epoch checked?; Yes
tcheck; Adopted SED compared to Observations?; YesRECX-16J08440914-7833457J2000SpT=M6.0; A_V=0.00; U=19.3; V=18.4; J=12.5; G=16.3; R=17.36Timing link suitability includes constraints ([Group (1C 1S) Within 1.0 days])The scheduling data was generated by CASM 29.0.CASM was run in Phase II mode./private/var/folders/1f/4k5qyrdd0_74wvf4yzrhnqcc0002hj/T/OPVisit9518674078168535863.xmlvstatus; 1C; ECHA-J0844.2-7833; P/COS approved for submission; P/DS 09/02/21 ; intrev: completed ; P/CP 08/02/21
vcheck; Enter targ name & Inst. & Resp. Sci.; ECHA-J0844.2-7833 ; COS ; DS
vcheck; ETC numbers entered in APT?; Yes
vcheck; Any screening violations?; NO
vcheck; M-dwarf check complete and added to box folder?; Yes ...
located at: box/ullyses_tech/ullyses_proposals/survey/revised-mstar-bop.xls
vcheck; S/N ETC calcs done & documented?; Yes
vcheck; Field images checked & saved?; Yes ...
located at: box/ullyses_tech/ullyses_proposals/survey/16480/recx16/
vcheck; Selected ACQ strategy?; PSA, MIRRORB, S/N=40
vcheck; Possible ACQ or Sci spoilers?; No
vcheck; Field BOT clear?; Yes
vcheck; Visual BOT check for stars not in catalog?; Good
vcheck; Orbit packing finalized?; Yes ...
obtained 102% of requested G160M and 103% of c1291
vcheck; Buffer times optimized?; Yes
vcheck; Verify visit grouping correct; Yes ...
STIS visit has GROUP 1S,1C WITHIN 1D
vcheck; phase constraint for ground based observations added?; Yes
vcheck; BETWEENS for coordinated observations added?; Yes ...
02 APR 2021 18:15 to 14 APR 2021 08:25 and 15 APR 2021 12:55 - 27 APR 2021 21:35
vcheck; Is visit ready for int. review?; Yes
Allocated COS orbits = 3161913645400076.0(Tic-Visit
:proposal-id 16480
:visit-id "1C"
:proposal-version -1
:trans-version "20200619"
:date "11-May-2021 19:11:41.0"
: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 139392
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16480
:visit-id "1C"
:obset-id "1C"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16480
:visit-id "1C"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2614
:al-overhead-at-end 0
:internal-dur-at-end 57
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3008
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16480
:visit-id "1C"
:orbit-number 2
:pcs-time 392
:si-vis-utilization 2543
: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 3008
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16480
:visit-id "1C"
:orbit-number 3
:pcs-time 392
:si-vis-utilization 2615
: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 3008
:pcs-gap 0
)true30BOP check with 4X spectrum COS.ta.1476476, B.P. = 7.608
Baseline SED with S/N=40 COS.ta.1476475 requires 114s, B.P. = 1.9644X BOP check: COS.sp.1476478, B.P. = 0.098
Baseline S/N calc: COS.sp.1476477, B.P. = 0.096
echaj08442-7833_lya2_etc.txt; cos,fuv,g130m,c1291,psa,mjd#59305; fp-pos=None, segment=None)
Input file: spring-survey-todo-crp06dec20.csv
Spectral type: M6.0 ; A_V: 0.0 ; Distance (pc): 94
M*: 0.052000000000000005 ; log(dm/dt): -10.18
For exptime=946.5 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): 425.5 cts/s/segment
brightest pixel: 0.047 cts/s/pix at 1304.8 A
Calculation performed 2020-12-08T03:53:58, v0.124X BOP check: COS.sp.1476478, B.P. = 0.098
Baseline S/N calc: COS.sp.1476477, B.P. = 0.096
echaj08442-7833_lya2_etc.txt; cos,fuv,g130m,c1291,psa,mjd#59305; fp-pos=None, segment=None)
Input file: spring-survey-todo-crp06dec20.csv
Spectral type: M6.0 ; A_V: 0.0 ; Distance (pc): 94
M*: 0.052000000000000005 ; log(dm/dt): -10.18
For exptime=946.5 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): 425.5 cts/s/segment
brightest pixel: 0.047 cts/s/pix at 1304.8 A
Calculation performed 2020-12-08T03:53:58, v0.124X BOP calculation: COS.sp.1477098, B.P. = 0.042
echaj08442-7833_lya2_etc.txt; cos,fuv,g160m,c1611,psa,mjd#59305; fp-pos=None, segment=None)
Input file: spring-survey-todo-crp06dec20.csv
Spectral type: M6.0 ; A_V: 0.0 ; Distance (pc): 94
M*: 0.052000000000000005 ; log(dm/dt): -10.18
For exptime=2358.8 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): 107.6 cts/s/segment
brightest pixel: 0.013 cts/s/pix at 1640.5 A
Calculation performed 2020-12-08T03:53:56, v0.124X BOP calculation: COS.sp.1477098, B.P. = 0.042
echaj08442-7833_lya2_etc.txt; cos,fuv,g160m,c1611,psa,mjd#59305; fp-pos=None, segment=None)
Input file: spring-survey-todo-crp06dec20.csv
Spectral type: M6.0 ; A_V: 0.0 ; Distance (pc): 94
M*: 0.052000000000000005 ; log(dm/dt): -10.18
For exptime=2358.8 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): 107.6 cts/s/segment
brightest pixel: 0.013 cts/s/pix at 1640.5 A
Calculation performed 2020-12-08T03:53:56, v0.124X BOP calculation: COS.sp.1477097, B.P. = 0.044
echaj08442-7833_lya2_etc.txt; cos,fuv,g160m,c1611,psa,mjd#59305; fp-pos=None, segment=None)
Input file: spring-survey-todo-crp06dec20.csv
Spectral type: M6.0 ; A_V: 0.0 ; Distance (pc): 94
M*: 0.052000000000000005 ; log(dm/dt): -10.18
For exptime=2358.8 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): 107.6 cts/s/segment
brightest pixel: 0.013 cts/s/pix at 1640.5 A
Calculation performed 2020-12-08T03:53:56, v0.124X BOP calculation: COS.sp.1477097, B.P. = 0.044
echaj08442-7833_lya2_etc.txt; cos,fuv,g160m,c1611,psa,mjd#59305; fp-pos=None, segment=None)
Input file: spring-survey-todo-crp06dec20.csv
Spectral type: M6.0 ; A_V: 0.0 ; Distance (pc): 94
M*: 0.052000000000000005 ; log(dm/dt): -10.18
For exptime=2358.8 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): 107.6 cts/s/segment
brightest pixel: 0.013 cts/s/pix at 1640.5 A
Calculation performed 2020-12-08T03:53:56, v0.12Timing link suitability includes constraints ([Group (1C 1S) Within 1.0 days])The scheduling data was generated by CASM 29.0.CASM was run in Phase II mode./private/var/folders/1f/4k5qyrdd0_74wvf4yzrhnqcc0002hj/T/OPVisit2896559798357702767.xmlvstatus; 1S; ECHA-J0844.2-7833; P/STIS approved for submission; P/DS 09/02/21 ; intrev: completed ; P/CP 08/02/21
vcheck; Enter targ name & Inst. & Resp. Sci.; ECHA-J0844.2-7833 ; STIS ; DS
vcheck; ETC numbers entered in APT?; Yes
vcheck; Any screening violations?; No
vcheck; M-dwarf check complete and added to box folder?; Yes ...
located at: box/ullyses_tech/ullyses_proposals/survey/revised-mstar-bop.xls
vcheck; S/N ETC calcs done & documented?; Yes
vcheck; Field images checked & saved?; Yes ...
located at: box/ullyses_tech/ullyses_proposals/survey/16480/recx16/
vcheck; Selected ACQ strategy?; S/N=80 using R mag with F28X50LP
vcheck; Possible ACQ or Sci spoilers?; No
vcheck; Field BOT clear?; Yes
vcheck; Visual BOT check for stars not in catalog?; Good
vcheck; Orbit packing finalized?; Yes
vcheck; Buffer times optimized?; Yes
vcheck; Verify visit grouping correct; Yes ...
STIS visit has GROUP 1S,1C WITHIN 1D
vcheck; phase constraint for ground based observations added?; Yes
vcheck; BETWEENS for coordinated observations added?; Yes ...
02 APR 2021 18:15 to 14 APR 2021 10:00 and 15 APR 2021 12:55 - 27 APR 2021 23:10
vcheck; Is visit ready for int. review?; Yes
Allocated STIS orbits = 2
We require both the STIS orbits within the same visit to avoid any chance of extra offset between G430L and G230L observations for this highly variable target. For the majority of the ULLYSES T Tauri targets all STIS observations are attempted within a single orbit.161922090000083.21744082110058(Tic-Visit
:proposal-id 16480
:visit-id "1S"
:proposal-version -1
:trans-version "20200619"
:date "11-May-2021 19:11:43.0"
: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 451440
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16480
:visit-id "1S"
:obset-id "1S"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16480
:visit-id "1S"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2614
: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 3008
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16480
:visit-id "1S"
:orbit-number 2
:pcs-time 392
:si-vis-utilization 2558
: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 3008
:pcs-gap 0
)true204 X BOP check: STIS.ta.1476537, B.P. = 369.197
Baseline SED (Castelli-Kurucz M6V 3500 5.0 spectrum renormalized to Johnson R=16.36 vegamag) with S/N=80: STIS.ta.1476535 requires 11s, B.P. = 212.483BOP check with 4X spectrum: STIS.sp.1476540, B.P. = 6.094
Baseline ETC calc with spectrum: STIS.sp.1476539, B.P. = 1.525
echaj08442-7833_lya2_etc.txt; stis,nuvmama,g230l,c2376,52x2,mjd#59305
Input file: spring-survey-todo-crp06dec20.csv
Spectral type: M6.0 ; A_V: 0.0 ; Distance (pc): 94
M*: 0.052000000000000005 ; log(dm/dt): -10.18
For exptime=53.1 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): 2435.1 cts/s/segment
brightest pixel: 1.531 cts/s/pix at 2796.8 A
Calculation performed 2020-12-08T03:53:58, v0.12BOP check with echaj08442-7833_lya2_x4.00_etc.txt (4X sed spectrum): STIS.sp.1476607, B.P. = 1639.951
Baseline ETC calc (Castelli-Kurucz M6V 3500 5.0 spectrum renormalized to Flam = 5.3e-16 in Johnson V): STIS.sp.1476606, B.P. = 2.858
echaj08442-7833_lya2_etc.txt; stis,ccd,g750l,c7751,52x2,mjd#59305
WARNING: operating mode = ACCUM
Input file: spring-survey-todo-crp06dec20.csv
Spectral type: M6.0 ; A_V: 0.0 ; Distance (pc): 94
M*: 0.052000000000000005 ; log(dm/dt): -10.18
For exptime=2.5 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): 166402.4 cts/s/segment
brightest pixel: 411.806 cts/s/pix at 6563.9 A
Calculation performed 2020-12-08T03:53:58, v0.12echaj08442-7833_lya2_etc.txt; stis,ccd,g750l,c7751,52x2,mjd#59305
WARNING: operating mode = ACCUM
Input file: spring-survey-todo-crp06dec20.csv
Spectral type: M6.0 ; A_V: 0.0 ; Distance (pc): 94
M*: 0.052000000000000005 ; log(dm/dt): -10.18
For exptime=2.5 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): 166402.4 cts/s/segment
brightest pixel: 411.806 cts/s/pix at 6563.9 A
Calculation performed 2020-12-08T03:53:58, v0.12echaj08442-7833_lya2_etc.txt; stis,ccd,g750l,c7751,52x2,mjd#59305
WARNING: operating mode = ACCUM
Input file: spring-survey-todo-crp06dec20.csv
Spectral type: M6.0 ; A_V: 0.0 ; Distance (pc): 94
M*: 0.052000000000000005 ; log(dm/dt): -10.18
For exptime=2.5 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): 166402.4 cts/s/segment
brightest pixel: 411.806 cts/s/pix at 6563.9 A
Calculation performed 2020-12-08T03:53:58, v0.12echaj08442-7833_lya2_etc.txt; stis,ccd,g750l,c7751,52x2,mjd#59305
WARNING: operating mode = ACCUM
Input file: spring-survey-todo-crp06dec20.csv
Spectral type: M6.0 ; A_V: 0.0 ; Distance (pc): 94
M*: 0.052000000000000005 ; log(dm/dt): -10.18
For exptime=2.5 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): 166402.4 cts/s/segment
brightest pixel: 411.806 cts/s/pix at 6563.9 A
Calculation performed 2020-12-08T03:53:58, v0.12BOP check with echaj08442-7833_lya2_x4.00_etc.txt (4X sed spectrum): STIS.sp.1476605, B.P. = 185.710
Baseline ETC calc (Castelli-Kurucz M6V 3500 5.0 spectrum renormalized to Flam = 3.0e-16 in Johnson B)): STIS.sp.1476604, B.P. = 0.773
echaj08442-7833_lya2_etc.txt; stis,ccd,g430l,c4300,52x2,mjd#59305
WARNING: operating mode = ACCUM
Input file: spring-survey-todo-crp06dec20.csv
Spectral type: M6.0 ; A_V: 0.0 ; Distance (pc): 94
M*: 0.052000000000000005 ; log(dm/dt): -10.18
For exptime=21.9 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): 56669.0 cts/s/segment
brightest pixel: 46.428 cts/s/pix at 4560.5 A
Calculation performed 2020-12-08T03:53:58, v0.12Timing link suitability includes constraints ([Group (AC AS) Within 1.0 days])The scheduling data was generated by CASM 29.0.CASM was run in Phase II mode./private/var/folders/1f/4k5qyrdd0_74wvf4yzrhnqcc0002hj/T/OPVisit9087255803477500490.xmlvstatus; AC; ECHA-J0844.2-7833; P/COS approved for submission; P/DS 09/02/21 ; intrev: completed ; P/CP 08/02/21
vcheck; Enter targ name & Inst. & Resp. Sci.; ECHA-J0844.2-7833 ; COS ; DS
vcheck; ETC numbers entered in APT?; Yes
vcheck; Any screening violations?; NO
vcheck; M-dwarf check complete and added to box folder?; Yes ...
located at: box/ullyses_tech/ullyses_proposals/survey/revised-mstar-bop.xls
vcheck; S/N ETC calcs done & documented?; Yes
vcheck; Field images checked & saved?; Yes ...
located at: box/ullyses_tech/ullyses_proposals/survey/16480/recx16/
vcheck; Selected ACQ strategy?; PSA, MIRRORB, S/N=40
vcheck; Possible ACQ or Sci spoilers?; No
vcheck; Field BOT clear?; Yes
vcheck; Visual BOT check for stars not in catalog?; Good
vcheck; Orbit packing finalized?; Yes ...
obtained 102% of requested G160M and 103% of c1291
vcheck; Buffer times optimized?; Yes
vcheck; Verify visit grouping correct; Yes ...
STIS visit has GROUP AS,AC WITHIN 1D
vcheck; phase constraint for ground based observations added?; Yes
vcheck; BETWEENS for coordinated observations added?; Yes ...
12 MAY 2021 00:00 to 10 JUL 2021 23:59 to ensure ground based coordination
However, coordination with TESS in sector 39 requires the following BETWEENS:
27 MAY 2021 07:00 to 09 JUN 2021 05:35 and 10 JUN 2021 09:10 - 24 JUN 2021 00:55
vcheck; Is visit ready for int. review?; Yes
Allocated COS orbits = 3(Tic-Visit
:proposal-id 16480
:visit-id "AC"
:proposal-version -1
:trans-version "20200619"
:date "11-May-2021 19:11:44.0"
: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 139392
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16480
:visit-id "AC"
:obset-id "AC"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16480
:visit-id "AC"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2614
:al-overhead-at-end 0
:internal-dur-at-end 57
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3008
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16480
:visit-id "AC"
:orbit-number 2
:pcs-time 392
:si-vis-utilization 2543
: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 3008
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16480
:visit-id "AC"
:orbit-number 3
:pcs-time 392
:si-vis-utilization 2615
: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 3008
:pcs-gap 0
)true30BOP check with 4X spectrum COS.ta.1476476, B.P. = 7.608
Baseline SED with S/N=40 COS.ta.1476475 requires 114s, B.P. = 1.9644X BOP check: COS.sp.1476478, B.P. = 0.098
Baseline S/N calc: COS.sp.1476477, B.P. = 0.096
echaj08442-7833_lya2_etc.txt; cos,fuv,g130m,c1291,psa,mjd#59305; fp-pos=None, segment=None)
Input file: spring-survey-todo-crp06dec20.csv
Spectral type: M6.0 ; A_V: 0.0 ; Distance (pc): 94
M*: 0.052000000000000005 ; log(dm/dt): -10.18
For exptime=946.5 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): 425.5 cts/s/segment
brightest pixel: 0.047 cts/s/pix at 1304.8 A
Calculation performed 2020-12-08T03:53:58, v0.124X BOP check: COS.sp.1476478, B.P. = 0.098
Baseline S/N calc: COS.sp.1476477, B.P. = 0.096
echaj08442-7833_lya2_etc.txt; cos,fuv,g130m,c1291,psa,mjd#59305; fp-pos=None, segment=None)
Input file: spring-survey-todo-crp06dec20.csv
Spectral type: M6.0 ; A_V: 0.0 ; Distance (pc): 94
M*: 0.052000000000000005 ; log(dm/dt): -10.18
For exptime=946.5 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): 425.5 cts/s/segment
brightest pixel: 0.047 cts/s/pix at 1304.8 A
Calculation performed 2020-12-08T03:53:58, v0.124X BOP calculation: COS.sp.1477098, B.P. = 0.042
echaj08442-7833_lya2_etc.txt; cos,fuv,g160m,c1611,psa,mjd#59305; fp-pos=None, segment=None)
Input file: spring-survey-todo-crp06dec20.csv
Spectral type: M6.0 ; A_V: 0.0 ; Distance (pc): 94
M*: 0.052000000000000005 ; log(dm/dt): -10.18
For exptime=2358.8 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): 107.6 cts/s/segment
brightest pixel: 0.013 cts/s/pix at 1640.5 A
Calculation performed 2020-12-08T03:53:56, v0.124X BOP calculation: COS.sp.1477098, B.P. = 0.042
echaj08442-7833_lya2_etc.txt; cos,fuv,g160m,c1611,psa,mjd#59305; fp-pos=None, segment=None)
Input file: spring-survey-todo-crp06dec20.csv
Spectral type: M6.0 ; A_V: 0.0 ; Distance (pc): 94
M*: 0.052000000000000005 ; log(dm/dt): -10.18
For exptime=2358.8 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): 107.6 cts/s/segment
brightest pixel: 0.013 cts/s/pix at 1640.5 A
Calculation performed 2020-12-08T03:53:56, v0.124X BOP calculation: COS.sp.1477097, B.P. = 0.044
echaj08442-7833_lya2_etc.txt; cos,fuv,g160m,c1611,psa,mjd#59305; fp-pos=None, segment=None)
Input file: spring-survey-todo-crp06dec20.csv
Spectral type: M6.0 ; A_V: 0.0 ; Distance (pc): 94
M*: 0.052000000000000005 ; log(dm/dt): -10.18
For exptime=2358.8 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): 107.6 cts/s/segment
brightest pixel: 0.013 cts/s/pix at 1640.5 A
Calculation performed 2020-12-08T03:53:56, v0.124X BOP calculation: COS.sp.1477097, B.P. = 0.044
echaj08442-7833_lya2_etc.txt; cos,fuv,g160m,c1611,psa,mjd#59305; fp-pos=None, segment=None)
Input file: spring-survey-todo-crp06dec20.csv
Spectral type: M6.0 ; A_V: 0.0 ; Distance (pc): 94
M*: 0.052000000000000005 ; log(dm/dt): -10.18
For exptime=2358.8 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): 107.6 cts/s/segment
brightest pixel: 0.013 cts/s/pix at 1640.5 A
Calculation performed 2020-12-08T03:53:56, v0.12Timing link suitability includes constraints ([Group (AC AS) Within 1.0 days])The scheduling data was generated by CASM 29.0.CASM was run in Phase II mode./private/var/folders/1f/4k5qyrdd0_74wvf4yzrhnqcc0002hj/T/OPVisit7911125873147770492.xmlvstatus; AS; ECHA-J0844.2-7833; P/STIS approved for submission; P/DS 09/02/21 ; intrev: completed ; P/CP 08/02/21
vcheck; Enter targ name & Inst. & Resp. Sci.; ECHA-J0844.2-7833 ; STIS ; DS
vcheck; ETC numbers entered in APT?; Yes
vcheck; Any screening violations?; No
vcheck; M-dwarf check complete and added to box folder?; Yes ...
located at: box/ullyses_tech/ullyses_proposals/survey/revised-mstar-bop.xls
vcheck; S/N ETC calcs done & documented?; Yes
vcheck; Field images checked & saved?; Yes ...
located at: box/ullyses_tech/ullyses_proposals/survey/16480/recx16/
vcheck; Selected ACQ strategy?; S/N=80 using R mag with F28X50LP
vcheck; Possible ACQ or Sci spoilers?; No
vcheck; Field BOT clear?; Yes
vcheck; Visual BOT check for stars not in catalog?; Good
vcheck; Orbit packing finalized?; Yes
vcheck; Buffer times optimized?; Yes
vcheck; Verify visit grouping correct; Yes ...
STIS visit has GROUP AS, AC WITHIN 1D
vcheck; phase constraint for ground based observations added?; Yes
vcheck; BETWEENS for coordinated observations added?; Yes ...
12 MAY 2021 00:00 to 10 JUL 2021 23:59 to ensure ground based coordination
However, coordination with TESS in sector 39 requires the following BETWEENS:
27 MAY 2021 07:00 to 09 JUN 2021 07:10 and 10 JUN 2021 09:10 - 24 JUN 2021 02:30
vcheck; Is visit ready for int. review?; Yes
Allocated STIS orbits = 2
We require both the STIS orbits within the same visit to avoid any chance of extra offset between G430L and G230L observations for this highly variable target. For the majority of the ULLYSES T Tauri targets all STIS observations are attempted within a single orbit.(Tic-Visit
:proposal-id 16480
:visit-id "AS"
:proposal-version -1
:trans-version "20200619"
:date "11-May-2021 19:11:45.0"
: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 451440
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16480
:visit-id "AS"
:obset-id "AS"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16480
:visit-id "AS"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2614
: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 3008
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16480
:visit-id "AS"
:orbit-number 2
:pcs-time 392
:si-vis-utilization 2558
: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 3008
:pcs-gap 0
)true204 X BOP check: STIS.ta.1476537, B.P. = 369.197
Baseline SED (Castelli-Kurucz M6V 3500 5.0 spectrum renormalized to Johnson R=16.36 vegamag) with S/N=80: STIS.ta.1476535 requires 11s, B.P. = 212.483BOP check with 4X spectrum: STIS.sp.1476540, B.P. = 6.094
Baseline ETC calc with spectrum: STIS.sp.1476539, B.P. = 1.525
echaj08442-7833_lya2_etc.txt; stis,nuvmama,g230l,c2376,52x2,mjd#59305
Input file: spring-survey-todo-crp06dec20.csv
Spectral type: M6.0 ; A_V: 0.0 ; Distance (pc): 94
M*: 0.052000000000000005 ; log(dm/dt): -10.18
For exptime=53.1 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): 2435.1 cts/s/segment
brightest pixel: 1.531 cts/s/pix at 2796.8 A
Calculation performed 2020-12-08T03:53:58, v0.12BOP check with echaj08442-7833_lya2_x4.00_etc.txt (4X sed spectrum): STIS.sp.1476607, B.P. = 1639.951
Baseline ETC calc (Castelli-Kurucz M6V 3500 5.0 spectrum renormalized to Flam = 5.3e-16 in Johnson V): STIS.sp.1476606, B.P. = 2.858
echaj08442-7833_lya2_etc.txt; stis,ccd,g750l,c7751,52x2,mjd#59305
WARNING: operating mode = ACCUM
Input file: spring-survey-todo-crp06dec20.csv
Spectral type: M6.0 ; A_V: 0.0 ; Distance (pc): 94
M*: 0.052000000000000005 ; log(dm/dt): -10.18
For exptime=2.5 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): 166402.4 cts/s/segment
brightest pixel: 411.806 cts/s/pix at 6563.9 A
Calculation performed 2020-12-08T03:53:58, v0.12echaj08442-7833_lya2_etc.txt; stis,ccd,g750l,c7751,52x2,mjd#59305
WARNING: operating mode = ACCUM
Input file: spring-survey-todo-crp06dec20.csv
Spectral type: M6.0 ; A_V: 0.0 ; Distance (pc): 94
M*: 0.052000000000000005 ; log(dm/dt): -10.18
For exptime=2.5 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): 166402.4 cts/s/segment
brightest pixel: 411.806 cts/s/pix at 6563.9 A
Calculation performed 2020-12-08T03:53:58, v0.12echaj08442-7833_lya2_etc.txt; stis,ccd,g750l,c7751,52x2,mjd#59305
WARNING: operating mode = ACCUM
Input file: spring-survey-todo-crp06dec20.csv
Spectral type: M6.0 ; A_V: 0.0 ; Distance (pc): 94
M*: 0.052000000000000005 ; log(dm/dt): -10.18
For exptime=2.5 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): 166402.4 cts/s/segment
brightest pixel: 411.806 cts/s/pix at 6563.9 A
Calculation performed 2020-12-08T03:53:58, v0.12echaj08442-7833_lya2_etc.txt; stis,ccd,g750l,c7751,52x2,mjd#59305
WARNING: operating mode = ACCUM
Input file: spring-survey-todo-crp06dec20.csv
Spectral type: M6.0 ; A_V: 0.0 ; Distance (pc): 94
M*: 0.052000000000000005 ; log(dm/dt): -10.18
For exptime=2.5 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): 166402.4 cts/s/segment
brightest pixel: 411.806 cts/s/pix at 6563.9 A
Calculation performed 2020-12-08T03:53:58, v0.12BOP check with echaj08442-7833_lya2_x4.00_etc.txt (4X sed spectrum): STIS.sp.1476605, B.P. = 185.710
Baseline ETC calc (Castelli-Kurucz M6V 3500 5.0 spectrum renormalized to Flam = 3.0e-16 in Johnson B)): STIS.sp.1476604, B.P. = 0.773
echaj08442-7833_lya2_etc.txt; stis,ccd,g430l,c4300,52x2,mjd#59305
WARNING: operating mode = ACCUM
Input file: spring-survey-todo-crp06dec20.csv
Spectral type: M6.0 ; A_V: 0.0 ; Distance (pc): 94
M*: 0.052000000000000005 ; log(dm/dt): -10.18
For exptime=21.9 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): 56669.0 cts/s/segment
brightest pixel: 46.428 cts/s/pix at 4560.5 A
Calculation performed 2020-12-08T03:53:58, v0.12