This resubmission fixes the WAVECAL = NO parameter for the STIS G140L observations of Sz 115, and updates the correct B band photometry for Sz 114 (in teh target section)
16 Jun 2022
Repeat of 1C was split into AC and AD to facilitate scheduling-470235151----- Attempting Submission 2 (Fri Dec 17 22:00:43 GMT 2021) -----
----- Attempting Submission 3 (Tue Jan 04 21:11:18 GMT 2022) -----
----- Attempting Submission 4 (Tue Mar 08 21:42:48 GMT 2022) -----
----- Attempting Submission 5 (Thu Jun 16 21:10:55 GMT 2022) -----ULLYSES M-Type T Tauri Survey Stars in Lupus III: Part 3The Space Telescope Science Institute (STScI) Director has decided to devote up to 1000 orbits of Director's Discretionary time in observing Cycles 27-29 to a new Hubble Ultraviolet Legacy program focused on star formation and associated stellar physics. This new program, ULLYSES (UV Legacy Library of Young Stars as Essential Standards), will provide a UV spectroscopic reference sample of young (< 10 Myr) high- and low-mass stars. It will target over ~150 OB stars in the Magellanic Clouds and lower metallicity galaxies in the Local Group, and ~40 T Tauri stars and brown dwarfs in the Milky Way. In addition, ULLYSES will monitor 4 typical T Tauri stars over different rotational phases through at least three rotation periods, and over timescales of months to years. The resulting library will provide template spectra of massive stars at metallicities substantially below the well studied, while the low mass sample will cover a wide range of ages, accretion rates, and masses, including objects down to well below 0.5 M_sun. The legacy of this large UV dataset on the first 10 Myr of stellar evolution will be enhanced by complementary datasets obtained by the scientific community. In addition to the core goals of the program related to stellar astrophysics of low and high mass stars, this data will also enable exciting science in the fields of ISM, CGM, jets, and exoplanets. ULLYSES will be modeled after the Frontier Fields program: all data obtained will be non-proprietary. The implementation team at STScI is developing high-level science data products and a sophisticated database and website for disseminating data from the ULLYSES program and ancillary datasets for the ULLYSES target sample from space and ground-based facilities.This proposal includes a subset of the low mass ULLYSES survey stars. Each target will be observed with the COS c1291 + c1589 + c1623 settings, as well as with STIS G230L, G430L, and G750L. All observations will normally be constrained to occur within 1 day.
Signal-to-noise requirements used to determine the desired exposures times were defined as follows:
COS/G130M/c1291: N V 1239 +- 1 A -- S/N=10/6-pix-resel at the peak of the line
COS/G160M/c1589: C IV 1549 +- 1 A -- S/N=20/6-pix-resel at the peak of the line (combined c1589 & c1623)
COS/G160M/c1623: C IV 1549 +- 1 A -- S/N=20/6-pix-resel at the peak of the line (combined c1589 & c1623)
STIS/G230L/52X2: Mg II 2800 +-15 A -- S/N=20/2-pix-resel at the peak of the line
STIS/G430L/52X2: continuum average 4000 +-5 A -- S/N=20/2-pix-resel (2 reads)
STIS/G750L/52X2: continuum average 5700 +-5 A -- S/N=20/2-pix-resel (2 reads)
Additional details about the scientific motivation and technical implementation strategy of the ULLYSES observations can be found at http://www.stsci.edu/stsci-research/research-topics-and-programs/ullyses. The ULLYSES program is based on the recommendations of a working group led by Sally Oey; the full text of that group's report can be found at http://www.stsci.edu/files/live/sites/www/files/home/stsci-research/research-topics-and-programs/ullyses/_documents/HSTUV-report-ULLYSES.pdf.0falseSUPPORTEDSTART TAURI STARPRE-MAIN SEQUENCE STARNOSZ114 : V908 Sco
Region: Lupus III
Simbad: http://simbad.u-strasbg.fr/simbad/sim-id?Ident=sz114&submit=submit+id
Target coordinates are from Gaia DR2.
Spectral type: M4.8 ; A_V: 0.3 ; Distance (pc): 200
M*: 0.21 ; log(dm/dt): -8.96
Input file: lowmass_survey_Input-gaia.csv
sz114_lya2_etc_scaled_pAV0.50.txt
Calculation performed 2021-10-21T02:39:00, v0.8
-------------------------------------------------------------------------------
tstatus; SZ114; P/COS ready for internal review; S/STIS ready for internal review; P/JRD 11/05/21; S/JRD 11/05/21
tcheck; APT/SIMBAD target names: ; OK
tcheck; Target info verification status?; OK
tcheck; Coordinates & P.M. verified, epoch checked?; Yes
tcheck; Adopted SED compared to Observations?; Yes
Flux in the optical template is about 2x flux in the photometryV908-SCOJ2000SpT=M4.8; A_V=0.30; B=15.33; V=14.12; J=10.41START TAURI STARPRE-MAIN SEQUENCE STARNOSZ115
Region: Lupus III
Simbad: http://simbad.u-strasbg.fr/simbad/sim-id?Ident=sz115&submit=submit+id
Target coordinates are from Gaia DR2.
Spectral type: M4.5 ; A_V: 0.5 ; Distance (pc): 200
M*: 0.19 ; log(dm/dt): -9.24
Input file: lowmass_survey_Input-gaia.csv
sz115_lya2_etc_scaled_pAV0.50.txt
Calculation performed 2021-10-21T02:38:50, v0.8
-------------------------------------------------------------------------------
tstatus; SZ115; P/COS ready for internal review; S/STIS ready for internal review; P/JRD 11/05/21; S/JRD 11/05/21
tcheck; APT/SIMBAD target names: ; OK
tcheck; Target info verification status?; OK
tcheck; Coordinates & P.M. verified, epoch checked?; Yes
tcheck; Adopted SED compared to Observations?; Yes
Flux in the optical template is about 3-4x flux in the photometryJ2000SpT=M4.5; A_V=0.50; B=16.88; V=15.48; J=11.33EXT-STARPRE-MAIN SEQUENCE START TAURI STARNOJ2000K2; U = 12.57; B = 11.91Timing link suitability includes constraints ([Group (1C 1S) Within 1.0 days])The scheduling data was generated by CASM 30.1.CASM was run in Phase II mode./private/var/folders/mk/5ss11qnx2hq98tz1y17xc5080001ws/T/OPVisit2383102553658166974.xmlvstatus; 1C; SZ114; P/COS ready for internal review; P/JRD 12/11/21 ; intrev: complete ; P/AH 17/12/21
vcheck; Enter targ name & Inst. & Resp. Sci.; SZ114 ;COS ; JRD
vcheck; ETC numbers entered in APT?; Yes
vcheck; Any screening violations?;No
vcheck; M-dwarf check complete and added to box folder?; Yes
vcheck; S/N ETC calcs done & documented?; YEs
vcheck; Field images checked & saved?; Yes
vcheck; Selected ACQ strategy?; yes
vcheck; Possible ACQ or Sci spoilers?; No
vcheck; Field BOT clear?; Yes
vcheck; Visual BOT check for stars not in catalog?; Yes
vcheck; Orbit packing finalized?; Yes
vcheck; Buffer times optimized?; Yes
vcheck; Verify visit grouping correct; Yes
vcheck; phase constraint for ground based observations added?; N/A
vcheck; BETWEENS for coordinated observations added?; Yes
vcheck; Is visit ready for int. review?; Yes
Allocated COS orbits = 516535672870002.110080864968893(Tic-Visit
:proposal-id 16857
:visit-id "1C"
:proposal-version -1
:trans-version "20211222"
:date "16-Jun-2022 14:08:16.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 5
:saa-model "31"
:si-bright-earth-limb-angle 20.0
:data-volume 278544
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16857
:visit-id "1C"
:obset-id "1C"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16857
:visit-id "1C"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2534
:al-overhead-at-end 0
:internal-dur-at-end 67
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2927
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16857
:visit-id "1C"
:orbit-number 2
:pcs-time 392
:si-vis-utilization 2534
:al-overhead-at-end 0
:internal-dur-at-end 67
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2927
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16857
:visit-id "1C"
:orbit-number 3
:pcs-time 392
:si-vis-utilization 2535
:al-overhead-at-end 0
:internal-dur-at-end 67
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2927
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16857
:visit-id "1C"
:orbit-number 4
:pcs-time 392
:si-vis-utilization 2535
:al-overhead-at-end 0
:internal-dur-at-end 76
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2927
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16857
:visit-id "1C"
:orbit-number 5
:pcs-time 392
:si-vis-utilization 2535
:al-overhead-at-end 0
:internal-dur-at-end 401
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2927
:pcs-gap 0
)true50Sz114 does not pass the M dwarf BOP with PSA and requires BOA, but that makes exptimes prohibitive (Same for spec acq). Doing an offset target acq with nearby (1.7') T Tauri star RX J1608.9-3905 (K2, V = 10.8). This is a weakly accreting star similar to RXJ0438.6+1546 (K2, V = 10.8). We have a template for RXJ0438.6+1546 that was obtained from an observed spectrum of LkCa19 (another similar star, K0, V = 11.12, WTTS) scaled to the V mag of RXJ0438.6+1546. We use this template to clear RX J1608.9-3905 for the BOP (COS.ta.1546173).
For the exposure time, we assume the fainter scenario of a K2 V with E(B-V) = 0.17 normalized to V = 10.88 (see ETC box).
We also confirm the BOP and exptimes with a Kurucz model K0 with no extinction normalized to V = 10.8: COS.ta.1546175
All safe to observe. Pad exptimes by a factor of 2 to be conservative.sz114_lya2_etc_scaled_pAV0.50.txt; cos,fuv,g160m,c1589,psa,mjd#59670; fp-pos=None, segment=None)
Input file: lowmass_survey_Input-gaia.csv
Spectral type: M4.8 ; A_V: 0.3 ; Distance (pc): 200
M*: 0.21 ; log(dm/dt): -8.96
For exptime=1939.5 s, spectral region:
1549.0 +- 1.0 A achieves SNR=20.0 / 6-pix-resel for combined c1589 & c1623
The exptime for this c1589 exposure has been halved because c1589 & c1623 target the same line.
A factor of 2.0 has been applied to the exptime in each exposure.
global countrate (brightest segment): 77.5 cts/s/segment
brightest pixel: 0.005 cts/s/pix at 1446.2 A
Calculation performed 2021-10-21T02:38:56, v0.23
Exptime computed with sz114_lya2_etc_scaled_pAV0.50.txt (extra A_V of 0.5)
Safe with x4 accretion rate (sz114_lya2_x4.00_etc.txt), see COS.sp.1544550 (also buffer time from this template)
Safe under flare M dwarf conditions, see COS.sp.1544551, generated with sz114_flarespec.fits, obtained with Elaine Fraizer's tool with J mag as input. J mag is input instead of V mag due to veiling in the V band (veiling at 710 nm from Alcala+2014 is 5%, more in the V band).sz114_lya2_etc_scaled_pAV0.50.txt; cos,fuv,g160m,c1589,psa,mjd#59670; fp-pos=None, segment=None)
Input file: lowmass_survey_Input-gaia.csv
Spectral type: M4.8 ; A_V: 0.3 ; Distance (pc): 200
M*: 0.21 ; log(dm/dt): -8.96
For exptime=1939.5 s, spectral region:
1549.0 +- 1.0 A achieves SNR=20.0 / 6-pix-resel for combined c1589 & c1623
The exptime for this c1589 exposure has been halved because c1589 & c1623 target the same line.
A factor of 2.0 has been applied to the exptime in each exposure.
global countrate (brightest segment): 77.5 cts/s/segment
brightest pixel: 0.005 cts/s/pix at 1446.2 A
Calculation performed 2021-10-21T02:38:56, v0.23
Exptime computed with sz114_lya2_etc_scaled_pAV0.50.txt (extra A_V of 0.5)
Safe with x4 accretion rate (sz114_lya2_x4.00_etc.txt), see COS.sp.1544550 (also buffer time from this template)
Safe under flare M dwarf conditions, see COS.sp.1544551, generated with sz114_flarespec.fits, obtained with Elaine Fraizer's tool with J mag as input. J mag is input instead of V mag due to veiling in the V band (veiling at 710 nm from Alcala+2014 is 5%, more in the V band).sz114_lya2_etc_scaled_pAV0.50.txt; cos,fuv,g160m,c1623,psa,mjd#59670; fp-pos=None, segment=None)
Input file: lowmass_survey_Input-gaia.csv
Spectral type: M4.8 ; A_V: 0.3 ; Distance (pc): 200
M*: 0.21 ; log(dm/dt): -8.96
For exptime=1984.8 s, spectral region:
1549.0 +- 1.0 A achieves SNR=20.0 / 6-pix-resel for combined c1589 & c1623
The exptime for this c1623 exposure has been halved because c1589 & c1623 target the same line.
A factor of 2.0 has been applied to the exptime in each exposure.
global countrate (brightest segment): 75.2 cts/s/segment
brightest pixel: 0.004 cts/s/pix at 1446.2 A
Calculation performed 2021-10-21T02:38:58, v0.23
Exptime computed with sz114_lya2_etc_scaled_pAV0.50.txt (extra A_V of 0.5)
Safe with x4 accretion rate (sz114_lya2_x4.00_etc.txt), see COS.sp.1544550 (also buffer time from this template)
Safe under flare M dwarf conditions, see COS.sp.1544551, generated with sz114_flarespec.fits, obtained with Elaine Fraizer's tool with J mag as input. J mag is input instead of V mag due to veiling in the V band (veiling at 710 nm from Alcala+2014 is 5%, more in the V band).sz114_lya2_etc_scaled_pAV0.50.txt; cos,fuv,g160m,c1623,psa,mjd#59670; fp-pos=None, segment=None)
Input file: lowmass_survey_Input-gaia.csv
Spectral type: M4.8 ; A_V: 0.3 ; Distance (pc): 200
M*: 0.21 ; log(dm/dt): -8.96
For exptime=1984.8 s, spectral region:
1549.0 +- 1.0 A achieves SNR=20.0 / 6-pix-resel for combined c1589 & c1623
The exptime for this c1623 exposure has been halved because c1589 & c1623 target the same line.
A factor of 2.0 has been applied to the exptime in each exposure.
global countrate (brightest segment): 75.2 cts/s/segment
brightest pixel: 0.004 cts/s/pix at 1446.2 A
Calculation performed 2021-10-21T02:38:58, v0.23
Exptime computed with sz114_lya2_etc_scaled_pAV0.50.txt (extra A_V of 0.5)
Safe with x4 accretion rate (sz114_lya2_x4.00_etc.txt), see COS.sp.1544550 (also buffer time from this template)
Safe under flare M dwarf conditions, see COS.sp.1544551, generated with sz114_flarespec.fits, obtained with Elaine Fraizer's tool with J mag as input. J mag is input instead of V mag due to veiling in the V band (veiling at 710 nm from Alcala+2014 is 5%, more in the V band).sz114_lya2_etc_scaled_pAV0.50.txt; cos,fuv,g130m,c1291,psa,mjd#59670; fp-pos=None, segment=None)
Input file: lowmass_survey_Input-gaia.csv
Spectral type: M4.8 ; A_V: 0.3 ; Distance (pc): 200
M*: 0.21 ; log(dm/dt): -8.96
For exptime=1606.8 s, spectral region:
1239.0 +- 1.0 A achieves SNR=10.0 / 6-pix-resel
A factor of 2.0 has been applied to the exptime in each exposure.
global countrate (brightest segment): 319.0 cts/s/segment
brightest pixel: 0.016 cts/s/pix at 1304.8 A
Calculation performed 2021-10-21T02:39:00, v0.23
Exptime computed with sz114_lya2_etc_scaled_pAV0.50.txt (extra A_V of 0.5)
Safe with x4 accretion rate (sz114_lya2_x4.00_etc.txt), see COS.sp.1544495 (also buffer time from this template)
Safe under flare M dwarf conditions, see COS.sp.1544496, generated with sz114_flarespec.fits, obtained with Elaine Fraizer's tool with J mag as input. J mag is input instead of V mag due to veiling in the V band (veiling at 710 nm from Alcala+2014 is 5%, more in the V band).sz114_lya2_etc_scaled_pAV0.50.txt; cos,fuv,g130m,c1291,psa,mjd#59670; fp-pos=None, segment=None)
Input file: lowmass_survey_Input-gaia.csv
Spectral type: M4.8 ; A_V: 0.3 ; Distance (pc): 200
M*: 0.21 ; log(dm/dt): -8.96
For exptime=1606.8 s, spectral region:
1239.0 +- 1.0 A achieves SNR=10.0 / 6-pix-resel
A factor of 2.0 has been applied to the exptime in each exposure.
global countrate (brightest segment): 319.0 cts/s/segment
brightest pixel: 0.016 cts/s/pix at 1304.8 A
Calculation performed 2021-10-21T02:39:00, v0.23
Exptime computed with sz114_lya2_etc_scaled_pAV0.50.txt (extra A_V of 0.5)
Safe with x4 accretion rate (sz114_lya2_x4.00_etc.txt), see COS.sp.1544495 (also buffer time from this template)
Safe under flare M dwarf conditions, see COS.sp.1544496, generated with sz114_flarespec.fits, obtained with Elaine Fraizer's tool with J mag as input. J mag is input instead of V mag due to veiling in the V band (veiling at 710 nm from Alcala+2014 is 5%, more in the V band).sz114_lya2_etc_scaled_pAV0.50.txt; cos,fuv,g130m,c1291,psa,mjd#59670; fp-pos=None, segment=None)
Input file: lowmass_survey_Input-gaia.csv
Spectral type: M4.8 ; A_V: 0.3 ; Distance (pc): 200
M*: 0.21 ; log(dm/dt): -8.96
For exptime=1606.8 s, spectral region:
1239.0 +- 1.0 A achieves SNR=10.0 / 6-pix-resel
A factor of 2.0 has been applied to the exptime in each exposure.
global countrate (brightest segment): 319.0 cts/s/segment
brightest pixel: 0.016 cts/s/pix at 1304.8 A
Calculation performed 2021-10-21T02:39:00, v0.23
Exptime computed with sz114_lya2_etc_scaled_pAV0.50.txt (extra A_V of 0.5)
Safe with x4 accretion rate (sz114_lya2_x4.00_etc.txt), see COS.sp.1544495 (also buffer time from this template)
Safe under flare M dwarf conditions, see COS.sp.1544496, generated with sz114_flarespec.fits, obtained with Elaine Fraizer's tool with J mag as input. J mag is input instead of V mag due to veiling in the V band (veiling at 710 nm from Alcala+2014 is 5%, more in the V band).Timing link suitability includes constraints ([Group (AC AD AS) Within 1.0 days])The scheduling data was generated by CASM 30.1.CASM was run in Phase II mode./Users/wfischer/Box/ullyses_tech/ullyses_proposals/survey_c29/16857/OP-cache/ULLYSES_16857-vAC.xmlvstatus; AC; SZ114; P/COS ready for internal review; P/JRD 12/11/21 ; intrev: complete ; P/AH 17/12/21
vcheck; Enter targ name & Inst. & Resp. Sci.; SZ114 ;COS ; JRD
vcheck; ETC numbers entered in APT?; Yes
vcheck; Any screening violations?;No
vcheck; M-dwarf check complete and added to box folder?; Yes
vcheck; S/N ETC calcs done & documented?; YEs
vcheck; Field images checked & saved?; Yes
vcheck; Selected ACQ strategy?; yes
vcheck; Possible ACQ or Sci spoilers?; No
vcheck; Field BOT clear?; Yes
vcheck; Visual BOT check for stars not in catalog?; Yes
vcheck; Orbit packing finalized?; Yes
vcheck; Buffer times optimized?; Yes
vcheck; Verify visit grouping correct; Yes
vcheck; phase constraint for ground based observations added?; N/A
vcheck; BETWEENS for coordinated observations added?; Yes
vcheck; Is visit ready for int. review?; Yes
Allocated COS orbits = 5(Tic-Visit
:proposal-id 16857
:visit-id "AC"
:proposal-version -1
:trans-version "20211222"
:date "15-Jun-2022 17:09:25.0"
: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 87104
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16857
:visit-id "AC"
:obset-id "AC"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16857
:visit-id "AC"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2534
:al-overhead-at-end 0
:internal-dur-at-end 67
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2927
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16857
:visit-id "AC"
:orbit-number 2
:pcs-time 392
:si-vis-utilization 2534
:al-overhead-at-end 0
:internal-dur-at-end 363
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2927
:pcs-gap 0
)true20Sz114 does not pass the M dwarf BOP with PSA and requires BOA, but that makes exptimes prohibitive (Same for spec acq). Doing an offset target acq with nearby (1.7') T Tauri star RX J1608.9-3905 (K2, V = 10.8). This is a weakly accreting star similar to RXJ0438.6+1546 (K2, V = 10.8). We have a template for RXJ0438.6+1546 that was obtained from an observed spectrum of LkCa19 (another similar star, K0, V = 11.12, WTTS) scaled to the V mag of RXJ0438.6+1546. We use this template to clear RX J1608.9-3905 for the BOP (COS.ta.1546173).
For the exposure time, we assume the fainter scenario of a K2 V with E(B-V) = 0.17 normalized to V = 10.88 (see ETC box).
We also confirm the BOP and exptimes with a Kurucz model K0 with no extinction normalized to V = 10.8: COS.ta.1546175
All safe to observe. Pad exptimes by a factor of 2 to be conservative.sz114_lya2_etc_scaled_pAV0.50.txt; cos,fuv,g160m,c1589,psa,mjd#59670; fp-pos=None, segment=None)
Input file: lowmass_survey_Input-gaia.csv
Spectral type: M4.8 ; A_V: 0.3 ; Distance (pc): 200
M*: 0.21 ; log(dm/dt): -8.96
For exptime=1939.5 s, spectral region:
1549.0 +- 1.0 A achieves SNR=20.0 / 6-pix-resel for combined c1589 & c1623
The exptime for this c1589 exposure has been halved because c1589 & c1623 target the same line.
A factor of 2.0 has been applied to the exptime in each exposure.
global countrate (brightest segment): 77.5 cts/s/segment
brightest pixel: 0.005 cts/s/pix at 1446.2 A
Calculation performed 2021-10-21T02:38:56, v0.23
Exptime computed with sz114_lya2_etc_scaled_pAV0.50.txt (extra A_V of 0.5)
Safe with x4 accretion rate (sz114_lya2_x4.00_etc.txt), see COS.sp.1544550 (also buffer time from this template)
Safe under flare M dwarf conditions, see COS.sp.1544551, generated with sz114_flarespec.fits, obtained with Elaine Fraizer's tool with J mag as input. J mag is input instead of V mag due to veiling in the V band (veiling at 710 nm from Alcala+2014 is 5%, more in the V band).sz114_lya2_etc_scaled_pAV0.50.txt; cos,fuv,g160m,c1589,psa,mjd#59670; fp-pos=None, segment=None)
Input file: lowmass_survey_Input-gaia.csv
Spectral type: M4.8 ; A_V: 0.3 ; Distance (pc): 200
M*: 0.21 ; log(dm/dt): -8.96
For exptime=1939.5 s, spectral region:
1549.0 +- 1.0 A achieves SNR=20.0 / 6-pix-resel for combined c1589 & c1623
The exptime for this c1589 exposure has been halved because c1589 & c1623 target the same line.
A factor of 2.0 has been applied to the exptime in each exposure.
global countrate (brightest segment): 77.5 cts/s/segment
brightest pixel: 0.005 cts/s/pix at 1446.2 A
Calculation performed 2021-10-21T02:38:56, v0.23
Exptime computed with sz114_lya2_etc_scaled_pAV0.50.txt (extra A_V of 0.5)
Safe with x4 accretion rate (sz114_lya2_x4.00_etc.txt), see COS.sp.1544550 (also buffer time from this template)
Safe under flare M dwarf conditions, see COS.sp.1544551, generated with sz114_flarespec.fits, obtained with Elaine Fraizer's tool with J mag as input. J mag is input instead of V mag due to veiling in the V band (veiling at 710 nm from Alcala+2014 is 5%, more in the V band).Timing link suitability includes constraints ([Group (AC AD AS) Within 1.0 days])The scheduling data was generated by CASM 30.1.CASM was run in Phase II mode./Users/wfischer/Box/ullyses_tech/ullyses_proposals/survey_c29/16857/OP-cache/ULLYSES_16857-vAD.xmlvstatus; AD; SZ114; P/COS ready for internal review; P/JRD 12/11/21 ; intrev: complete ; P/AH 17/12/21
vcheck; Enter targ name & Inst. & Resp. Sci.; SZ114 ;COS ; JRD
vcheck; ETC numbers entered in APT?; Yes
vcheck; Any screening violations?;No
vcheck; M-dwarf check complete and added to box folder?; Yes
vcheck; S/N ETC calcs done & documented?; YEs
vcheck; Field images checked & saved?; Yes
vcheck; Selected ACQ strategy?; yes
vcheck; Possible ACQ or Sci spoilers?; No
vcheck; Field BOT clear?; Yes
vcheck; Visual BOT check for stars not in catalog?; Yes
vcheck; Orbit packing finalized?; Yes
vcheck; Buffer times optimized?; Yes
vcheck; Verify visit grouping correct; Yes
vcheck; phase constraint for ground based observations added?; N/A
vcheck; BETWEENS for coordinated observations added?; Yes
vcheck; Is visit ready for int. review?; Yes
Allocated COS orbits = 5(Tic-Visit
:proposal-id 16857
:visit-id "AD"
:proposal-version -1
:trans-version "20211222"
:date "15-Jun-2022 17:10:10.0"
: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 208912
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16857
:visit-id "AD"
:obset-id "AD"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16857
:visit-id "AD"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2534
:al-overhead-at-end 0
:internal-dur-at-end 67
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2927
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16857
:visit-id "AD"
:orbit-number 2
:pcs-time 392
:si-vis-utilization 2535
:al-overhead-at-end 0
:internal-dur-at-end 76
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2927
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16857
:visit-id "AD"
:orbit-number 3
:pcs-time 392
:si-vis-utilization 2535
:al-overhead-at-end 0
:internal-dur-at-end 401
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2927
:pcs-gap 0
)true30Sz114 does not pass the M dwarf BOP with PSA and requires BOA, but that makes exptimes prohibitive (Same for spec acq). Doing an offset target acq with nearby (1.7') T Tauri star RX J1608.9-3905 (K2, V = 10.8). This is a weakly accreting star similar to RXJ0438.6+1546 (K2, V = 10.8). We have a template for RXJ0438.6+1546 that was obtained from an observed spectrum of LkCa19 (another similar star, K0, V = 11.12, WTTS) scaled to the V mag of RXJ0438.6+1546. We use this template to clear RX J1608.9-3905 for the BOP (COS.ta.1546173).
For the exposure time, we assume the fainter scenario of a K2 V with E(B-V) = 0.17 normalized to V = 10.88 (see ETC box).
We also confirm the BOP and exptimes with a Kurucz model K0 with no extinction normalized to V = 10.8: COS.ta.1546175
All safe to observe. Pad exptimes by a factor of 2 to be conservative.sz114_lya2_etc_scaled_pAV0.50.txt; cos,fuv,g160m,c1623,psa,mjd#59670; fp-pos=None, segment=None)
Input file: lowmass_survey_Input-gaia.csv
Spectral type: M4.8 ; A_V: 0.3 ; Distance (pc): 200
M*: 0.21 ; log(dm/dt): -8.96
For exptime=1984.8 s, spectral region:
1549.0 +- 1.0 A achieves SNR=20.0 / 6-pix-resel for combined c1589 & c1623
The exptime for this c1623 exposure has been halved because c1589 & c1623 target the same line.
A factor of 2.0 has been applied to the exptime in each exposure.
global countrate (brightest segment): 75.2 cts/s/segment
brightest pixel: 0.004 cts/s/pix at 1446.2 A
Calculation performed 2021-10-21T02:38:58, v0.23
Exptime computed with sz114_lya2_etc_scaled_pAV0.50.txt (extra A_V of 0.5)
Safe with x4 accretion rate (sz114_lya2_x4.00_etc.txt), see COS.sp.1544550 (also buffer time from this template)
Safe under flare M dwarf conditions, see COS.sp.1544551, generated with sz114_flarespec.fits, obtained with Elaine Fraizer's tool with J mag as input. J mag is input instead of V mag due to veiling in the V band (veiling at 710 nm from Alcala+2014 is 5%, more in the V band).sz114_lya2_etc_scaled_pAV0.50.txt; cos,fuv,g160m,c1623,psa,mjd#59670; fp-pos=None, segment=None)
Input file: lowmass_survey_Input-gaia.csv
Spectral type: M4.8 ; A_V: 0.3 ; Distance (pc): 200
M*: 0.21 ; log(dm/dt): -8.96
For exptime=1984.8 s, spectral region:
1549.0 +- 1.0 A achieves SNR=20.0 / 6-pix-resel for combined c1589 & c1623
The exptime for this c1623 exposure has been halved because c1589 & c1623 target the same line.
A factor of 2.0 has been applied to the exptime in each exposure.
global countrate (brightest segment): 75.2 cts/s/segment
brightest pixel: 0.004 cts/s/pix at 1446.2 A
Calculation performed 2021-10-21T02:38:58, v0.23
Exptime computed with sz114_lya2_etc_scaled_pAV0.50.txt (extra A_V of 0.5)
Safe with x4 accretion rate (sz114_lya2_x4.00_etc.txt), see COS.sp.1544550 (also buffer time from this template)
Safe under flare M dwarf conditions, see COS.sp.1544551, generated with sz114_flarespec.fits, obtained with Elaine Fraizer's tool with J mag as input. J mag is input instead of V mag due to veiling in the V band (veiling at 710 nm from Alcala+2014 is 5%, more in the V band).sz114_lya2_etc_scaled_pAV0.50.txt; cos,fuv,g130m,c1291,psa,mjd#59670; fp-pos=None, segment=None)
Input file: lowmass_survey_Input-gaia.csv
Spectral type: M4.8 ; A_V: 0.3 ; Distance (pc): 200
M*: 0.21 ; log(dm/dt): -8.96
For exptime=1606.8 s, spectral region:
1239.0 +- 1.0 A achieves SNR=10.0 / 6-pix-resel
A factor of 2.0 has been applied to the exptime in each exposure.
global countrate (brightest segment): 319.0 cts/s/segment
brightest pixel: 0.016 cts/s/pix at 1304.8 A
Calculation performed 2021-10-21T02:39:00, v0.23
Exptime computed with sz114_lya2_etc_scaled_pAV0.50.txt (extra A_V of 0.5)
Safe with x4 accretion rate (sz114_lya2_x4.00_etc.txt), see COS.sp.1544495 (also buffer time from this template)
Safe under flare M dwarf conditions, see COS.sp.1544496, generated with sz114_flarespec.fits, obtained with Elaine Fraizer's tool with J mag as input. J mag is input instead of V mag due to veiling in the V band (veiling at 710 nm from Alcala+2014 is 5%, more in the V band).sz114_lya2_etc_scaled_pAV0.50.txt; cos,fuv,g130m,c1291,psa,mjd#59670; fp-pos=None, segment=None)
Input file: lowmass_survey_Input-gaia.csv
Spectral type: M4.8 ; A_V: 0.3 ; Distance (pc): 200
M*: 0.21 ; log(dm/dt): -8.96
For exptime=1606.8 s, spectral region:
1239.0 +- 1.0 A achieves SNR=10.0 / 6-pix-resel
A factor of 2.0 has been applied to the exptime in each exposure.
global countrate (brightest segment): 319.0 cts/s/segment
brightest pixel: 0.016 cts/s/pix at 1304.8 A
Calculation performed 2021-10-21T02:39:00, v0.23
Exptime computed with sz114_lya2_etc_scaled_pAV0.50.txt (extra A_V of 0.5)
Safe with x4 accretion rate (sz114_lya2_x4.00_etc.txt), see COS.sp.1544495 (also buffer time from this template)
Safe under flare M dwarf conditions, see COS.sp.1544496, generated with sz114_flarespec.fits, obtained with Elaine Fraizer's tool with J mag as input. J mag is input instead of V mag due to veiling in the V band (veiling at 710 nm from Alcala+2014 is 5%, more in the V band).sz114_lya2_etc_scaled_pAV0.50.txt; cos,fuv,g130m,c1291,psa,mjd#59670; fp-pos=None, segment=None)
Input file: lowmass_survey_Input-gaia.csv
Spectral type: M4.8 ; A_V: 0.3 ; Distance (pc): 200
M*: 0.21 ; log(dm/dt): -8.96
For exptime=1606.8 s, spectral region:
1239.0 +- 1.0 A achieves SNR=10.0 / 6-pix-resel
A factor of 2.0 has been applied to the exptime in each exposure.
global countrate (brightest segment): 319.0 cts/s/segment
brightest pixel: 0.016 cts/s/pix at 1304.8 A
Calculation performed 2021-10-21T02:39:00, v0.23
Exptime computed with sz114_lya2_etc_scaled_pAV0.50.txt (extra A_V of 0.5)
Safe with x4 accretion rate (sz114_lya2_x4.00_etc.txt), see COS.sp.1544495 (also buffer time from this template)
Safe under flare M dwarf conditions, see COS.sp.1544496, generated with sz114_flarespec.fits, obtained with Elaine Fraizer's tool with J mag as input. J mag is input instead of V mag due to veiling in the V band (veiling at 710 nm from Alcala+2014 is 5%, more in the V band).Timing link suitability includes constraints ([Group (1C 1S) Within 1.0 days])The scheduling data was generated by CASM 30.1.CASM was run in Phase II mode./private/var/folders/mk/5ss11qnx2hq98tz1y17xc5080001ws/T/OPVisit7529775669720434623.xmlvstatus; 1S; SZ114; S/STIS ready for internal review; S/JRD 12/11/21 ; intrev: complete ; P/AH 17/12/21
vcheck; Enter targ name & Inst. & Resp. Sci.; SZ114; STIS ; JRD
vcheck; ETC numbers entered in APT?; Yes
vcheck; Any screening violations?; No
vcheck; M-dwarf check complete and added to box folder?; Yes
vcheck; S/N ETC calcs done & documented?; Yes
vcheck; Field images checked & saved?; Yes
vcheck; Selected ACQ strategy?; Yes
vcheck; Possible ACQ or Sci spoilers?; no
vcheck; Field BOT clear?; Yes
vcheck; Visual BOT check for stars not in catalog?; Yes
vcheck; Orbit packing finalized?; Yes
vcheck; Buffer times optimized?; Yes
vcheck; Verify visit grouping correct; Yes
vcheck; phase constraint for ground based observations added?; N/A
vcheck; BETWEENS for coordinated observations added?; Yes
vcheck; Is visit ready for int. review?; Yes
Allocated STIS orbits = 2 (constrained in input CSV)16535615730002.203611893986789(Tic-Visit
:proposal-id 16857
:visit-id "1S"
:proposal-version -1
:trans-version "20211222"
:date "16-Jun-2022 14:08:17.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 1
:saa-model "24"
:si-bright-earth-limb-angle 20.0
:data-volume 451424
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16857
:visit-id "1S"
:obset-id "1S"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16857
:visit-id "1S"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2528
:al-overhead-at-end 116
:internal-dur-at-end 1271
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2927
:pcs-gap 0
)true10Time to saturation 1.36s using the x4 accretion rate template: STIS.ta.1546178sz114_lya2_etc_scaled_pAV0.50.txt; stis,nuvmama,g230l,c2376,52x2,mjd#59670
Input file: lowmass_survey_Input-gaia.csv
Spectral type: M4.8 ; A_V: 0.3 ; Distance (pc): 200
M*: 0.21 ; log(dm/dt): -8.96
For exptime=138.1 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): 2381.1 cts/s/segment
brightest pixel: 0.597 cts/s/pix at 2796.8 A
Calculation performed 2021-10-21T02:39:00, v0.23
Safe with x4 accretion rate (sz114_lya2_x4.00_etc.txt, STIS.sp.1546181), BT = 667s
Safe with M dwarf flare (sz114_flarespec.fits, obtained with J mag input): STIS.sp.1546182
padding exptime since template is brighter than photometry at longer wavlengths.sz114_lya2_etc_scaled_pAV0.50.txt; stis,ccd,g430l,c4300,52x2,mjd#59670
WARNING: operating mode = ACCUM
Input file: lowmass_survey_Input-gaia.csv
Spectral type: M4.8 ; A_V: 0.3 ; Distance (pc): 200
M*: 0.21 ; log(dm/dt): -8.96
For exptime=55.4 s, n_reads=2, spectral region:
4000.0 +- 5.0 A achieves SNR=20.0 / 2-pix-resel
A factor of 2.0 has been applied to the exptime in each exposure.
global countrate (brightest segment): 42341.2 cts/s/segment
brightest pixel: 19.506 cts/s/pix at 4560.5 A
Calculation performed 2021-10-21T02:39:00, v0.23
Time to saturation wtih x4 accretion rate = 215s: STIS.sp.1546184. Exptime for each CR split is half of that.
Padding exptimes by a factor of 4 since optical photometry is a factor 2 below the template.sz114_lya2_etc_scaled_pAV0.50.txt; stis,ccd,g750l,c7751,52x2,mjd#59670
WARNING: operating mode = ACCUM
Input file: lowmass_survey_Input-gaia.csv
Spectral type: M4.8 ; A_V: 0.3 ; Distance (pc): 200
M*: 0.21 ; log(dm/dt): -8.96
For exptime=4.8 s, n_reads=2, spectral region:
5700.0 +- 5.0 A achieves SNR=20.0 / 2-pix-resel
A factor of 2.0 has been applied to the exptime in each exposure.
global countrate (brightest segment): 84281.4 cts/s/segment
brightest pixel: 146.061 cts/s/pix at 6563.9 A
Calculation performed 2021-10-21T02:39:00, v0.23
padding exptime by a factor 8 since photometry lies factor 4 below the template at 5700 A.
Time to saturation with x4 accretion rate = 33s (STIS.sp.1546186), more that each CR split exptimeTiming link suitability includes constraints ([Group (AC AD AS) Within 1.0 days])The scheduling data was generated by CASM 30.1.CASM was run in Phase II mode./private/var/folders/mk/5ss11qnx2hq98tz1y17xc5080001ws/T/OPVisit7268332954379902946.xmlvstatus; 1S; SZ114; S/STIS ready for internal review; S/JRD 12/11/21 ; intrev: complete ; P/AH 17/12/21
vcheck; Enter targ name & Inst. & Resp. Sci.; SZ114; STIS ; JRD
vcheck; ETC numbers entered in APT?; Yes
vcheck; Any screening violations?; No
vcheck; M-dwarf check complete and added to box folder?; Yes
vcheck; S/N ETC calcs done & documented?; Yes
vcheck; Field images checked & saved?; Yes
vcheck; Selected ACQ strategy?; Yes
vcheck; Possible ACQ or Sci spoilers?; no
vcheck; Field BOT clear?; Yes
vcheck; Visual BOT check for stars not in catalog?; Yes
vcheck; Orbit packing finalized?; Yes
vcheck; Buffer times optimized?; Yes
vcheck; Verify visit grouping correct; Yes
vcheck; phase constraint for ground based observations added?; N/A
vcheck; BETWEENS for coordinated observations added?; Yes
vcheck; Is visit ready for int. review?; Yes
Allocated STIS orbits = 2 (constrained in input CSV)(Tic-Visit
:proposal-id 16857
:visit-id "AS"
:proposal-version -1
:trans-version "20211222"
:date "16-Jun-2022 14:04:40.0"
: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 451424
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16857
:visit-id "AS"
:obset-id "AS"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16857
:visit-id "AS"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2528
:al-overhead-at-end 116
:internal-dur-at-end 1271
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2927
:pcs-gap 0
)true10Time to saturation 1.36s using the x4 accretion rate template: STIS.ta.1546178sz114_lya2_etc_scaled_pAV0.50.txt; stis,nuvmama,g230l,c2376,52x2,mjd#59670
Input file: lowmass_survey_Input-gaia.csv
Spectral type: M4.8 ; A_V: 0.3 ; Distance (pc): 200
M*: 0.21 ; log(dm/dt): -8.96
For exptime=138.1 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): 2381.1 cts/s/segment
brightest pixel: 0.597 cts/s/pix at 2796.8 A
Calculation performed 2021-10-21T02:39:00, v0.23
Safe with x4 accretion rate (sz114_lya2_x4.00_etc.txt, STIS.sp.1546181), BT = 667s
Safe with M dwarf flare (sz114_flarespec.fits, obtained with J mag input): STIS.sp.1546182
padding exptime since template is brighter than photometry at longer wavlengths.sz114_lya2_etc_scaled_pAV0.50.txt; stis,ccd,g430l,c4300,52x2,mjd#59670
WARNING: operating mode = ACCUM
Input file: lowmass_survey_Input-gaia.csv
Spectral type: M4.8 ; A_V: 0.3 ; Distance (pc): 200
M*: 0.21 ; log(dm/dt): -8.96
For exptime=55.4 s, n_reads=2, spectral region:
4000.0 +- 5.0 A achieves SNR=20.0 / 2-pix-resel
A factor of 2.0 has been applied to the exptime in each exposure.
global countrate (brightest segment): 42341.2 cts/s/segment
brightest pixel: 19.506 cts/s/pix at 4560.5 A
Calculation performed 2021-10-21T02:39:00, v0.23
Time to saturation wtih x4 accretion rate = 215s: STIS.sp.1546184. Exptime for each CR split is half of that.
Padding exptimes by a factor of 4 since optical photometry is a factor 2 below the template.sz114_lya2_etc_scaled_pAV0.50.txt; stis,ccd,g750l,c7751,52x2,mjd#59670
WARNING: operating mode = ACCUM
Input file: lowmass_survey_Input-gaia.csv
Spectral type: M4.8 ; A_V: 0.3 ; Distance (pc): 200
M*: 0.21 ; log(dm/dt): -8.96
For exptime=4.8 s, n_reads=2, spectral region:
5700.0 +- 5.0 A achieves SNR=20.0 / 2-pix-resel
A factor of 2.0 has been applied to the exptime in each exposure.
global countrate (brightest segment): 84281.4 cts/s/segment
brightest pixel: 146.061 cts/s/pix at 6563.9 A
Calculation performed 2021-10-21T02:39:00, v0.23
padding exptime by a factor 8 since photometry lies factor 4 below the template at 5700 A.
Time to saturation with x4 accretion rate = 33s (STIS.sp.1546186), more that each CR split exptimeTiming link suitability includes constraints ([Group (2S 2T 2U) Within 1.5 days])The scheduling data was generated by CASM 30.1.CASM was run in Phase II mode./private/var/folders/mk/5ss11qnx2hq98tz1y17xc5080001ws/T/OPVisit18227932325619235584.xmlvstatus; 2C; SZ115; S/STIS ready for internal review; P/JRD 24/11/21 ; intrev: complete ; P/AH 17/12/21
vcheck; Enter targ name & Inst. & Resp. Sci.; SZ115 ; STIS ; JRD
vcheck; ETC numbers entered in APT?; Yes
vcheck; Any screening violations?; No
vcheck; M-dwarf check complete and added to box folder?; Yes
vcheck; S/N ETC calcs done & documented?; Yes
vcheck; Field images checked & saved?; Yes
vcheck; Selected ACQ strategy?; Yes
vcheck; Possible ACQ or Sci spoilers?; No
vcheck; Field BOT clear?; Yes
vcheck; Visual BOT check for stars not in catalog?; Yes
vcheck; Orbit packing finalized?; Yes
vcheck; Buffer times optimized?; Yes
vcheck; Verify visit grouping correct; Yes
vcheck; phase constraint for ground based observations added?; NA
vcheck; BETWEENS for coordinated observations added?; Yes
vcheck; Is visit ready for int. review?; Yes
Allocated COS orbits = 13 - modified to use STIS/G140L due to inability to safely acquiring the target (M dwarf BOP, no viable offset target)165431576700028.8975990130607(Tic-Visit
:proposal-id 16857
:visit-id "2S"
:proposal-version -1
:trans-version "20211222"
:date "16-Jun-2022 14:08:18.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 3
:saa-model "24"
:si-bright-earth-limb-angle 20.0
:data-volume 470064
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16857
:visit-id "2S"
:obset-id "2S"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16857
:visit-id "2S"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2417
:al-overhead-at-end 0
:internal-dur-at-end 368
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2927
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16857
:visit-id "2S"
:orbit-number 2
:pcs-time 392
:si-vis-utilization 2526
:al-overhead-at-end 0
:internal-dur-at-end 368
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2927
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16857
:visit-id "2S"
:orbit-number 3
:pcs-time 392
:si-vis-utilization 2526
:al-overhead-at-end 0
:internal-dur-at-end 630
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2927
:pcs-gap 0
)true30Exptime run with M6, EBV = 0.3, normalized to V = 15.46 (0.14s, time to saturation 24s)Exptime computed from sz115_lya2_etc_scaled_pAV0.50.txt with factor 2 padding (template scaled by accretion rate, distance, and extinction).
Buffer time computed from x4 accretion rate (sz115_lya2_x4.00_etc.txt), also shows that this target is safe to observe under x4 variability (STIS.sp.1666099)
Target clears BOP under M dwarf flare conditions, see STIS.sp.1666100 computed with sz115_flarespec.fits. This spectrum was itself obtained using Elaine Frazer's M dwarf flare simulator, with V mag of 15.48 input.Exptime computed from sz115_lya2_etc_scaled_pAV0.50.txt with factor 2 padding (template scaled by accretion rate, distance, and extinction).
Buffer time computed from x4 accretion rate (sz115_lya2_x4.00_etc.txt), also shows that this target is safe to observe under x4 variability (STIS.sp.1666099)
Target clears BOP under M dwarf flare conditions, see STIS.sp.16661003 computed with sz115_flarespec.fits. This spectrum was itself obtained using Elaine Frazer's M dwarf flare simulator, with V mag of 15.48 input.Exptime computed from sz115_lya2_etc_scaled_pAV0.50.txt with factor 2 padding (template scaled by accretion rate, distance, and extinction).
Buffer time computed from x4 accretion rate (sz115_lya2_x4.00_etc.txt), also shows that this target is safe to observe under x4 variability (STIS.sp.1666099)
Target clears BOP under M dwarf flare conditions, see STIS.sp.16661003 computed with sz115_flarespec.fits. This spectrum was itself obtained using Elaine Frazer's M dwarf flare simulator, with V mag of 15.48 input.Timing link suitability includes constraints ([Group (2S 2T 2U) Within 1.5 days])The scheduling data was generated by CASM 30.1.CASM was run in Phase II mode./private/var/folders/mk/5ss11qnx2hq98tz1y17xc5080001ws/T/OPVisit13470327500839390808.xmlvstatus; 2C; SZ115; S/STIS ready for internal review; P/JRD 24/11/21 ; intrev: complete ; P/AH 17/12/21
vcheck; Enter targ name & Inst. & Resp. Sci.; SZ115 ; STIS ; JRD
vcheck; ETC numbers entered in APT?; Yes
vcheck; Any screening violations?; No
vcheck; M-dwarf check complete and added to box folder?; Yes
vcheck; S/N ETC calcs done & documented?; Yes
vcheck; Field images checked & saved?; Yes
vcheck; Selected ACQ strategy?; Yes
vcheck; Possible ACQ or Sci spoilers?; No
vcheck; Field BOT clear?; Yes
vcheck; Visual BOT check for stars not in catalog?; Yes
vcheck; Orbit packing finalized?; Yes
vcheck; Buffer times optimized?; Yes
vcheck; Verify visit grouping correct; Yes
vcheck; phase constraint for ground based observations added?; NA
vcheck; BETWEENS for coordinated observations added?; Yes
vcheck; Is visit ready for int. review?; Yes
Allocated COS orbits = 13 - modified to use STIS/G140L due to inability to safely acquiring the target (M dwarf BOP, no viable offset target)165440146700031.700933353129813(Tic-Visit
:proposal-id 16857
:visit-id "2T"
:proposal-version -1
:trans-version "20211222"
:date "16-Jun-2022 14:08:19.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 3
:saa-model "24"
:si-bright-earth-limb-angle 20.0
:data-volume 690928
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16857
:visit-id "2T"
:obset-id "2T"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16857
:visit-id "2T"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2532
:al-overhead-at-end 0
:internal-dur-at-end 368
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2927
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16857
:visit-id "2T"
:orbit-number 2
:pcs-time 392
:si-vis-utilization 2526
:al-overhead-at-end 0
:internal-dur-at-end 368
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2927
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16857
:visit-id "2T"
:orbit-number 3
:pcs-time 392
:si-vis-utilization 2527
:al-overhead-at-end 116
:internal-dur-at-end 1192
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2927
:pcs-gap 0
)true30Exptime run with M6, EBV = 0.3, normalized to V = 15.46 (0.14s, time to saturation 24s)Exptime computed from sz115_lya2_etc_scaled_pAV0.50.txt with factor 2 padding (template scaled by accretion rate, distance, and extinction).
Buffer time computed from x4 accretion rate (sz115_lya2_x4.00_etc.txt), also shows that this target is safe to observe under x4 variability (STIS.sp.1666099)
Target clears BOP under M dwarf flare conditions, see STIS.sp.16661003 computed with sz115_flarespec.fits. This spectrum was itself obtained using Elaine Frazer's M dwarf flare simulator, with V mag of 15.48 input.Exptime computed from sz115_lya2_etc_scaled_pAV0.50.txt with factor 2 padding (template scaled by accretion rate, distance, and extinction).
Buffer time computed from x4 accretion rate (sz115_lya2_x4.00_etc.txt), also shows that this target is safe to observe under x4 variability (STIS.sp.1666099)
Target clears BOP under M dwarf flare conditions, see STIS.sp.16661003 computed with sz115_flarespec.fits. This spectrum was itself obtained using Elaine Frazer's M dwarf flare simulator, with V mag of 15.48 input.Exptime computed from sz115_lya2_etc_scaled_pAV0.50.txt with factor 2 padding (template scaled by accretion rate, distance, and extinction).
Buffer time computed from x4 accretion rate (sz115_lya2_x4.00_etc.txt), also shows that this target is safe to observe under x4 variability (STIS.sp.1666107)
Target clears BOP under M dwarf flare conditions, see STIS.sp.1666108 computed with sz115_flarespec.fits. This spectrum was itself obtained using Elaine Frazer's M dwarf flare simulator, with V mag of 15.48 input.Nominal exptime computed with a Castelli & Kurucz M6 with EBV = 0.3 normalized to V = 15.48, with some padding. Time to saturation is 10ks even without extinction, so not a concern (STIS.sp.1666110)Nominal exptime computed with a Castelli & Kurucz M6 with EBV = 0.3 normalized to V = 15.48, with some padding. Brightest case for saturation computed without extinction (STIS.sp.1666112)
sz115_lya2_etc_scaled_pAV0.50.txt; stis,ccd,g750l,c7751,52x2,mjd#59670
WARNING: operating mode = ACCUM
Input file: lowmass_survey_Input-gaia.csv
Spectral type: M4.5 ; A_V: 0.5 ; Distance (pc): 200
M*: 0.19 ; log(dm/dt): -9.24
For exptime=8.3 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): 66182.1 cts/s/segment
brightest pixel: 95.388 cts/s/pix at 6563.9 A
Calculation performed 2021-10-21T02:38:50, v0.23Timing link suitability includes constraints ([Group (2S 2T 2U) Within 1.5 days])The scheduling data was generated by CASM 30.1.CASM was run in Phase II mode./private/var/folders/mk/5ss11qnx2hq98tz1y17xc5080001ws/T/OPVisit12718738902361494584.xmlvstatus; 2C; SZ115; S/STIS ready for internal review; P/JRD 24/11/21 ; intrev: complete ; P/AH 17/12/21
vcheck; Enter targ name & Inst. & Resp. Sci.; SZ115 ; STIS ; JRD
vcheck; ETC numbers entered in APT?; Yes
vcheck; Any screening violations?; No
vcheck; M-dwarf check complete and added to box folder?; Yes
vcheck; S/N ETC calcs done & documented?; Yes
vcheck; Field images checked & saved?; Yes
vcheck; Selected ACQ strategy?; Yes
vcheck; Possible ACQ or Sci spoilers?; No
vcheck; Field BOT clear?; Yes
vcheck; Visual BOT check for stars not in catalog?; Yes
vcheck; Orbit packing finalized?; Yes
vcheck; Buffer times optimized?; Yes
vcheck; Verify visit grouping correct; Yes
vcheck; phase constraint for ground based observations added?; NA
vcheck; BETWEENS for coordinated observations added?; Yes
vcheck; Is visit ready for int. review?; Yes
Allocated COS orbits = 13 - modified to use STIS/G140L due to inability to safely acquiring the target (M dwarf BOP, no viable offset target)165433290700029.46506161345411(Tic-Visit
:proposal-id 16857
:visit-id "2U"
:proposal-version -1
:trans-version "20211222"
:date "16-Jun-2022 14:08:20.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 3
:saa-model "24"
:si-bright-earth-limb-angle 20.0
:data-volume 470064
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 16857
:visit-id "2U"
:obset-id "2U"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 16857
:visit-id "2U"
:orbit-number 1
:pcs-time 393
:si-vis-utilization 2417
:al-overhead-at-end 0
:internal-dur-at-end 368
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2927
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16857
:visit-id "2U"
:orbit-number 2
:pcs-time 392
:si-vis-utilization 2526
:al-overhead-at-end 0
:internal-dur-at-end 368
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2927
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 16857
:visit-id "2U"
:orbit-number 3
:pcs-time 392
:si-vis-utilization 2526
:al-overhead-at-end 0
:internal-dur-at-end 630
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 2927
:pcs-gap 0
)true30Exptime run with M6, EBV = 0.3, normalized to V = 15.46 (0.14s, time to saturation 24s)Exptime computed from sz115_lya2_etc_scaled_pAV0.50.txt with factor 2 padding (template scaled by accretion rate, distance, and extinction).
Buffer time computed from x4 accretion rate (sz115_lya2_x4.00_etc.txt), also shows that this target is safe to observe under x4 variability (STIS.sp.1666099)
Target clears BOP under M dwarf flare conditions, see STIS.sp.16661003 computed with sz115_flarespec.fits. This spectrum was itself obtained using Elaine Frazer's M dwarf flare simulator, with V mag of 15.48 input.Exptime computed from sz115_lya2_etc_scaled_pAV0.50.txt with factor 2 padding (template scaled by accretion rate, distance, and extinction).
Buffer time computed from x4 accretion rate (sz115_lya2_x4.00_etc.txt), also shows that this target is safe to observe under x4 variability (STIS.sp.1666099)
Target clears BOP under M dwarf flare conditions, see STIS.sp.16661003 computed with sz115_flarespec.fits. This spectrum was itself obtained using Elaine Frazer's M dwarf flare simulator, with V mag of 15.48 input.Exptime computed from sz115_lya2_etc_scaled_pAV0.50.txt with factor 2 padding (template scaled by accretion rate, distance, and extinction).
Buffer time computed from x4 accretion rate (sz115_lya2_x4.00_etc.txt), also shows that this target is safe to observe under x4 variability (STIS.sp.1666099)
Target clears BOP under M dwarf flare conditions, see STIS.sp.16661003 computed with sz115_flarespec.fits. This spectrum was itself obtained using Elaine Frazer's M dwarf flare simulator, with V mag of 15.48 input.