The list of Investigators does not match the STScI records for this program. The number of orbits used exceeds the number allocated 0 ----- Attempting Submission 1 (Fri Jul 30 16:00:27 GMT 2021) ----- The orbit allocation for this program needs to be increased to 8 obrits. The 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. 0 false SUPPORTED STAR T TAURI STAR PRE-MAIN SEQUENCE STAR NO RECX-5 : EK Cha, J08422710-7857479 Region: eta Cha Simbad: https://simbad.u-strasbg.fr/simbad/sim-id?Ident=RECX+5&NbIdent=1&Radius=2&Radius.unit=arcmin&submit=submit+id Target coordinates are from Gaia EDR3. Spectral type: M4.5 ; A_V: 0.0 ; Distance (pc): 94 M*: 0.15 ; log(dm/dt): -9.89 Input file: targets_up_to_May30-2022.csv recx5_lya2_etc.txt Calculation performed 2021-06-18T15:04:33, 0.24 ------------------------------------------------------------------------------- tstatus; RECX-5; P/COS ready for internal review; S/STIS ready for internal review ; P/JRD 09/07/21; S/JRD 09/07/21 tcheck; APT/SIMBAD target names: ; Yes tcheck; Target info verification status?; Yes tcheck; Coordinates & P.M. verified, epoch checked?; Yes tcheck; Adopted SED compared to Observations?; Yes (recx5_photometry.png). Flarespec spectrum uploaded on box (recx5_flarespec.fits) was generated with A_V = 0 and a floor N(HI) = 19.3 cm-2 using Elaine's code. The log N(H) = 19.3 floor is estimated from the N(HI) of nearby stars with no reddening from McJunkin+2014. (cleartargets.py on ullyses_tech repo) EK-CHA J08422710-7857479 J2000 SpT=M4.5; A_V=0.00; U=16.0; V=15.2 STAR T TAURI STAR PRE-MAIN SEQUENCE STAR NO RECX-9 : EN Cha, J08441637-7859080 Region: eta Cha Simbad: https://simbad.u-strasbg.fr/simbad/sim-id?Ident=RECX+9&NbIdent=1&Radius=2&Radius.unit=arcmin&submit=submit+id Target coordinates are from Gaia EDR3. Spectral type: M4.5 ; A_V: 0.0 ; Distance (pc): 94 M*: 0.15 ; log(dm/dt): -9.92 Input file: targets_up_to_May30-2022.csv recx9_lya2_etc.txt Calculation performed 2021-06-18T15:04:42, 0.24 ------------------------------------------------------------------------------- tstatus; RECX-9; P/COS ready for internal review; S/STIS ready for internal review; P/JRD 09/07/21; S/JRD 09/07/21 tcheck; APT/SIMBAD target names: ; Yes tcheck; Target info verification status?; Yes tcheck; Coordinates & P.M. verified, epoch checked?; Yes tcheck; Adopted SED compared to Observations?; Yes (recx9_photometry.png). Flarespec spectrum uploaded on box (recx9_flarespec.fits) was generated with A_V = 0 and a floor N(HI) = 19.3 cm-2 using Elaine's code (cleartargets.py on ullyses_tech repo). The log N(H) = 19.3 floor is estimated from the N(HI) of nearby stars with no reddening from McJunkin+2014. EN-CHA J08441637-7859080 J2000 SpT=M4.5; A_V=0.00; U=15.8; V=15.0 1627659999620 Timing link suitability includes constraints ([Group (1C 1S) Within 1.0 days]) The scheduling data was generated by CASM 29.2. CASM was run in Phase II mode. /Users/duval/Documents/ULLYSES/CTTS_phaseIIs/16595/APT/OP-cache/ULLYSES_16595-v1C.xml vstatus; 1C; RECX-5; P/COS ready for submission; P/JRD 12/07/21 ; intrev complete ; P/CP 27/07/21 vcheck; Enter targ name & Inst. & Resp. Sci.; RECX-5 ; 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?; Yes 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 = 2 (Tic-Visit :proposal-id 16595 :visit-id "1C" :proposal-version -1 :trans-version "20210514" :date "30-Jul-2021 11:46:39.0" :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 374144 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16595 :visit-id "1C" :obset-id "1C" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16595 :visit-id "1C" :orbit-number 1 :pcs-time 393 :si-vis-utilization 2615 :al-overhead-at-end 0 :internal-dur-at-end 105 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3008 :pcs-gap 0 ) (Tic-Orbit :proposal-id 16595 :visit-id "1C" :orbit-number 2 :pcs-time 392 :si-vis-utilization 2604 :al-overhead-at-end 0 :internal-dur-at-end 344 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3008 :pcs-gap 0 ) true 2 0 Exposure time padded to account for flux uncertainties and variability (500s instead of 360s computed with the recx5_lya2_etc template) TA with BOA/MIRRORA is safe under M dwarf flare conditions, see COS.ta.1523551 using recx5_flarespec.fits for which V mag is input (max lcr = 39 cts/pix/s, global = 1543 cts/s) This configuration is also safe for the high end of accretion variability (recx5_lya2_x4.00_etc.txt), see COS.ta.1523556 Excluding field star for which no photometry is available when the PSA is in the field. recx5_lya2_etc.txt; cos,fuv,g130m,c1222,psa,mjd#59670; fp-pos=None, segment=None) Input file: targets_up_to_May30-2022.csv Spectral type: M4.5 ; A_V: 0.0 ; Distance (pc): 94 M*: 0.15 ; log(dm/dt): -9.89 For exptime=1094.7 s, spectral region: 1239.0 +- 1.0 A achieves SNR=20.0 / 6-pix-resel A factor of 2.0 has been applied to the exptime in each exposure. global countrate (brightest segment): 289.6 cts/s/segment brightest pixel: 0.089 cts/s/pix at 1304.8 A Calculation performed 2021-06-18T15:04:32, v0.24 Exptime verified using recx5_lya2_etc.txt, padded to account for flux uncertainty and variability since photometry for this target stops at 4500A and templates aren't very accurate for late M stars. Configuration is safe under M dwarf flare conditions (recx5_flarespec.fits, uses V mag as input), see COS.sp.1523524 Also safe with high range of accretion variability: COS.sp.1523526 (uses recx5_lya2_x4.00_etc) recx5_lya2_etc.txt; cos,fuv,g130m,c1222,psa,mjd#59670; fp-pos=None, segment=None) Input file: targets_up_to_May30-2022.csv Spectral type: M4.5 ; A_V: 0.0 ; Distance (pc): 94 M*: 0.15 ; log(dm/dt): -9.89 For exptime=1094.7 s, spectral region: 1239.0 +- 1.0 A achieves SNR=20.0 / 6-pix-resel A factor of 2.0 has been applied to the exptime in each exposure. global countrate (brightest segment): 289.6 cts/s/segment brightest pixel: 0.089 cts/s/pix at 1304.8 A Calculation performed 2021-06-18T15:04:32, v0.24 Exptime verified using recx5_lya2_etc.txt, padded to account for flux uncertainty and variability since photometry for this target stops at 4500A and templates aren't very accurate for late M stars. Configuration is safe under M dwarf flare conditions (recx5_flarespec.fits, uses V mag as input), see COS.sp.1523524 Also safe with high range of accretion variability: COS.sp.1523526 (uses recx5_lya2_x4.00_etc) recx5_lya2_etc.txt; cos,fuv,g130m,c1222,psa,mjd#59670; fp-pos=None, segment=None) Input file: targets_up_to_May30-2022.csv Spectral type: M4.5 ; A_V: 0.0 ; Distance (pc): 94 M*: 0.15 ; log(dm/dt): -9.89 For exptime=1094.7 s, spectral region: 1239.0 +- 1.0 A achieves SNR=20.0 / 6-pix-resel A factor of 2.0 has been applied to the exptime in each exposure. global countrate (brightest segment): 289.6 cts/s/segment brightest pixel: 0.089 cts/s/pix at 1304.8 A Calculation performed 2021-06-18T15:04:32, v0.24 Exptime verified using recx5_lya2_etc.txt, padded to account for flux uncertainty and variability since photometry for this target stops at 4500A and templates aren't very accurate for late M stars. Configuration is safe under M dwarf flare conditions (recx5_flarespec.fits, uses V mag as input), see COS.sp.1523524 Also safe with high range of accretion variability: COS.sp.1523526 (uses recx5_lya2_x4.00_etc) recx5_lya2_etc.txt; cos,fuv,g130m,c1222,psa,mjd#59670; fp-pos=None, segment=None) Input file: targets_up_to_May30-2022.csv Spectral type: M4.5 ; A_V: 0.0 ; Distance (pc): 94 M*: 0.15 ; log(dm/dt): -9.89 For exptime=1094.7 s, spectral region: 1239.0 +- 1.0 A achieves SNR=20.0 / 6-pix-resel A factor of 2.0 has been applied to the exptime in each exposure. global countrate (brightest segment): 289.6 cts/s/segment brightest pixel: 0.089 cts/s/pix at 1304.8 A Calculation performed 2021-06-18T15:04:32, v0.24 Exptime verified using recx5_lya2_etc.txt, padded to account for flux uncertainty and variability since photometry for this target stops at 4500A and templates aren't very accurate for late M stars. Configuration is safe under M dwarf flare conditions (recx5_flarespec.fits, uses V mag as input), see COS.sp.1523524 Also safe with high range of accretion variability: COS.sp.1523526 (uses recx5_lya2_x4.00_etc) 1627567901489 Timing link suitability includes constraints ([Group (1C 1S) Within 1.0 days]) The scheduling data was generated by CASM 29.2. CASM was run in Phase II mode. /Users/duval/Documents/ULLYSES/CTTS_phaseIIs/16595/APT/OP-cache/ULLYSES_16595-v1S.xml vstatus; 1S; RECX-5; S/STIS ready for submission; S/JRD 12/07/21 ; intrev: complete ; S/DW 30/07/21 vcheck; Enter targ name & Inst. & Resp. Sci.; RECX-5 ;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 (Tic-Visit :proposal-id 16595 :visit-id "1S" :proposal-version -1 :trans-version "20210514" :date "29-Jul-2021 10:11:41.0" :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 1021440 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16595 :visit-id "1S" :obset-id "1S" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16595 :visit-id "1S" :orbit-number 1 :pcs-time 393 :si-vis-utilization 2615 :al-overhead-at-end 0 :internal-dur-at-end 2407 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3008 :pcs-gap 0 ) (Tic-Orbit :proposal-id 16595 :visit-id "1S" :orbit-number 2 :pcs-time 392 :si-vis-utilization 2616 :al-overhead-at-end 116 :internal-dur-at-end 1251 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3008 :pcs-gap 0 ) true 2 0 Exposure time calculated using interpolated spectrum based on optical photometry (recx5_interp.dat). The photometry VOT file was obtained from Vizier. TIme to saturation is 10s, so plenty of margin. recx5_lya2_etc.txt; stis,fuvmama,g140l,c1425,52x2,mjd#59670 Input file: targets_up_to_May30-2022.csv Spectral type: M4.5 ; A_V: 0.0 ; Distance (pc): 94 M*: 0.15 ; log(dm/dt): -9.89 For exptime=193.3 s, spectral region: 1549.0 +- 2.0 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): 973.6 cts/s/segment brightest pixel: 3.889 cts/s/pix at 1304.7 A Calculation performed 2021-06-18T15:04:30, v0.24 Exposure time computed using recx5_lya2_etc.txt, and padded heavily to account for flux uncertainty in this late M star. Configuration is safe for flaring M dwarf - STIS.sp.1523512 (uses recx5_flarespec.fits, which has V mag input) Also safe for high range of accretion (recx5_lya2_x4.00_etc.txt) - STIS.sp.1523521 recx5_lya2_etc.txt; stis,nuvmama,g230l,c2376,52x2,mjd#59670 Input file: targets_up_to_May30-2022.csv Spectral type: M4.5 ; A_V: 0.0 ; Distance (pc): 94 M*: 0.15 ; log(dm/dt): -9.89 For exptime=33.2 s, spectral region: 2800.0 +- 15.0 A achieves SNR=20.0 / 2-pix-resel A factor of 2.0 has been applied to the exptime in each exposure. global countrate (brightest segment): 2526.4 cts/s/segment brightest pixel: 2.442 cts/s/pix at 2796.8 A Calculation performed 2021-06-18T15:04:32, v0.24 Exposure time computed using recx5_lya2_etc.txt, and padded heavily to account for flux uncertainty in this late M star. Configuration is safe for flaring M dwarf - STIS.sp.1523559 (uses recx5_flarespec.fits, which has V mag input) . Note that FSW (not ETC) bright limits apply for flaring M dwarfs. Also safe for high range of accretion (recx5_lya2_x4.00_etc.txt) - STIS.sp.1523561 recx5_lya2_etc.txt; stis,ccd,g430l,c4300,52x2,mjd#59670 WARNING: operating mode = ACCUM Input file: targets_up_to_May30-2022.csv Spectral type: M4.5 ; A_V: 0.0 ; Distance (pc): 94 M*: 0.15 ; log(dm/dt): -9.89 For exptime=13.9 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): 71014.0 cts/s/segment brightest pixel: 68.817 cts/s/pix at 4560.5 A Calculation performed 2021-06-18T15:04:32, v0.24 Exposure time computed from interpolated photometry (recx5_interp.dat), which is just an interpolation of the photometry from Vizier. Exptime is padded by factor 2 to account for variability.Saturation not an issue. recx5_lya2_etc.txt; stis,ccd,g750l,c7751,52x2,mjd#59670 WARNING: operating mode = ACCUM Input file: targets_up_to_May30-2022.csv Spectral type: M4.5 ; A_V: 0.0 ; Distance (pc): 94 M*: 0.15 ; log(dm/dt): -9.89 For exptime=1.6 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): 213776.0 cts/s/segment brightest pixel: 548.575 cts/s/pix at 6563.9 A Calculation performed 2021-06-18T15:04:33, v0.24 Exposure time computed from interpolated photometry (recx5_interp.dat), which is just an interpolation of the photometry from Vizier. Exptime is padded by factor 2 to account for variability.Saturation not an issue. 1627660000933 Timing link suitability includes constraints ([Group (2C 2S) Within 1.0 days]) The scheduling data was generated by CASM 29.2. CASM was run in Phase II mode. /Users/duval/Documents/ULLYSES/CTTS_phaseIIs/16595/APT/OP-cache/ULLYSES_16595-v2C.xml vstatus; 2C; RECX-9; P/COS ready for submission; P/JRD 12/07/21 ; intrev complete ; P/CP 27/07/21 vcheck; Enter targ name & Inst. & Resp. Sci.; RECX-9 ; 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 = 2 (Tic-Visit :proposal-id 16595 :visit-id "2C" :proposal-version -1 :trans-version "20210514" :date "30-Jul-2021 11:46:40.0" :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 374160 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16595 :visit-id "2C" :obset-id "2C" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16595 :visit-id "2C" :orbit-number 1 :pcs-time 393 :si-vis-utilization 2615 :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 3008 :pcs-gap 0 ) (Tic-Orbit :proposal-id 16595 :visit-id "2C" :orbit-number 2 :pcs-time 392 :si-vis-utilization 2604 :al-overhead-at-end 0 :internal-dur-at-end 344 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3008 :pcs-gap 0 ) true 2 0 Exptime based on recx9_lya2_etc.txt, with x2 padding to account for flux uncertainties and variability Configuration safe under M dwarf flare conditions (recx9_flarespec.fits, generated with input V mag), see COS.sa.1523583 . The flarespec was computed using the SpT and V mag as input (zero extinction). Also safe assuming x4 accretion increase, see COS.sa.1523614 generated from recx9_lya2_x4.00_etc.txt Exptime based on recx9_lya2_etc.txt, with x2 padding to account for flux uncertainties and variability Configuration safe under M dwarf flare conditions (recx9_flarespec.fits, generated with input V mag), see COS.sa.1523583. The flarespec was computed using the SpT and V mag as input (zero extinction). Also safe assuming x4 accretion increase, see COS.sa.1523614 generated from recx9_lya2_x4.00_etc.txt recx9_lya2_etc.txt; cos,fuv,g130m,c1222,psa,mjd#59670; fp-pos=None, segment=None) Input file: targets_up_to_May30-2022.csv Spectral type: M4.5 ; A_V: 0.0 ; Distance (pc): 94 M*: 0.15 ; log(dm/dt): -9.92 For exptime=1172.6 s, spectral region: 1239.0 +- 1.0 A achieves SNR=20.0 / 6-pix-resel A factor of 2.0 has been applied to the exptime in each exposure. global countrate (brightest segment): 274.4 cts/s/segment brightest pixel: 0.083 cts/s/pix at 1304.8 A Calculation performed 2021-06-18T15:04:42, v0.24 Exptime computed from recx9_lya2_etc.txt, with extra padding (x8) to account for large uncertainty in flux for this weakly accreting star. Configuration safe under M dwarf flaring conditions, see COS.sp.1523616 generated from recx9_flarespec.fits. The flarespec was computed using the SpT and V mag as input (zero extinction). Configuration is safe for x4 accretion variability, see COS.sp.1523619 generated from recx9_lya2_x4.00_etc. recx9_lya2_etc.txt; cos,fuv,g130m,c1222,psa,mjd#59670; fp-pos=None, segment=None) Input file: targets_up_to_May30-2022.csv Spectral type: M4.5 ; A_V: 0.0 ; Distance (pc): 94 M*: 0.15 ; log(dm/dt): -9.92 For exptime=1172.6 s, spectral region: 1239.0 +- 1.0 A achieves SNR=20.0 / 6-pix-resel A factor of 2.0 has been applied to the exptime in each exposure. global countrate (brightest segment): 274.4 cts/s/segment brightest pixel: 0.083 cts/s/pix at 1304.8 A Calculation performed 2021-06-18T15:04:42, v0.24 Exptime computed from recx9_lya2_etc.txt, with extra padding (x8) to account for large uncertainty in flux for this weakly accreting star. Configuration safe under M dwarf flaring conditions, see COS.sp.1523616 generated from recx9_flarespec.fits. The flarespec was computed using the SpT and V mag as input (zero extinction). Configuration is safe for x4 accretion variability, see COS.sp.1523619 generated from recx9_lya2_x4.00_etc. recx9_lya2_etc.txt; cos,fuv,g130m,c1222,psa,mjd#59670; fp-pos=None, segment=None) Input file: targets_up_to_May30-2022.csv Spectral type: M4.5 ; A_V: 0.0 ; Distance (pc): 94 M*: 0.15 ; log(dm/dt): -9.92 For exptime=1172.6 s, spectral region: 1239.0 +- 1.0 A achieves SNR=20.0 / 6-pix-resel A factor of 2.0 has been applied to the exptime in each exposure. global countrate (brightest segment): 274.4 cts/s/segment brightest pixel: 0.083 cts/s/pix at 1304.8 A Calculation performed 2021-06-18T15:04:42, v0.24 Exptime computed from recx9_lya2_etc.txt, with extra padding (x8) to account for large uncertainty in flux for this weakly accreting star. Configuration safe under M dwarf flaring conditions, see COS.sp.1523616 generated from recx9_flarespec.fits. The flarespec was computed using the SpT and V mag as input (zero extinction). Configuration is safe for x4 accretion variability, see COS.sp.1523619 generated from recx9_lya2_x4.00_etc. recx9_lya2_etc.txt; cos,fuv,g130m,c1222,psa,mjd#59670; fp-pos=None, segment=None) Input file: targets_up_to_May30-2022.csv Spectral type: M4.5 ; A_V: 0.0 ; Distance (pc): 94 M*: 0.15 ; log(dm/dt): -9.92 For exptime=1172.6 s, spectral region: 1239.0 +- 1.0 A achieves SNR=20.0 / 6-pix-resel A factor of 2.0 has been applied to the exptime in each exposure. global countrate (brightest segment): 274.4 cts/s/segment brightest pixel: 0.083 cts/s/pix at 1304.8 A Calculation performed 2021-06-18T15:04:42, v0.24 Exptime computed from recx9_lya2_etc.txt, with extra padding (x8) to account for large uncertainty in flux for this weakly accreting star. Configuration safe under M dwarf flaring conditions, see COS.sp.1523616 generated from recx9_flarespec.fits. The flarespec was computed using the SpT and V mag as input (zero extinction). Configuration is safe for x4 accretion variability, see COS.sp.1523619 generated from recx9_lya2_x4.00_etc. 1627660002477 Timing link suitability includes constraints ([Group (2C 2S) Within 1.0 days]) The scheduling data was generated by CASM 29.2. CASM was run in Phase II mode. /Users/duval/Documents/ULLYSES/CTTS_phaseIIs/16595/APT/OP-cache/ULLYSES_16595-v2S.xml vstatus; 2S; RECX-9; S/STIS ready for submission; S/JRD 15/07/21 ; intrev: complete ; S/DW 30/07/21 vcheck; Enter targ name & Inst. & Resp. Sci.; RECX-9 ; 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 (Tic-Visit :proposal-id 16595 :visit-id "2S" :proposal-version -1 :trans-version "20210514" :date "30-Jul-2021 11:46:42.0" :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 743104 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16595 :visit-id "2S" :obset-id "2S" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16595 :visit-id "2S" :orbit-number 1 :pcs-time 393 :si-vis-utilization 2615 :al-overhead-at-end 0 :internal-dur-at-end 2407 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3008 :pcs-gap 0 ) (Tic-Orbit :proposal-id 16595 :visit-id "2S" :orbit-number 2 :pcs-time 392 :si-vis-utilization 2615 :al-overhead-at-end 116 :internal-dur-at-end 1251 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3008 :pcs-gap 0 ) true 2 0 Exptime calculated from interpolation of photometry obtained from Vizier (recx9_interp.dat). Saturation in 10s, so not an issue. recx9_lya2_etc.txt; stis,fuvmama,g140l,c1425,52x2,mjd#59670 Input file: targets_up_to_May30-2022.csv Spectral type: M4.5 ; A_V: 0.0 ; Distance (pc): 94 M*: 0.15 ; log(dm/dt): -9.92 For exptime=203.7 s, spectral region: 1549.0 +- 2.0 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): 960.2 cts/s/segment brightest pixel: 3.626 cts/s/pix at 1304.7 A Calculation performed 2021-06-18T15:04:40, v0.24 Exptime computed from recx9_lya2_etc.txt, padded by factor 2 to account for flux uncertainties Configuration safe under M dwarf flare conditions, see STIS.sp.1523628, generated with recx9_flarespec.fits. The flarespec is computed using V mag and SpT as inputs (no extinction). Also safe with x4 accretion variability, see STIS.sp.1523626 generated from recx9_lya2_x4.00_etc recx9_lya2_etc.txt; stis,nuvmama,g230l,c2376,52x2,mjd#59670 Input file: targets_up_to_May30-2022.csv Spectral type: M4.5 ; A_V: 0.0 ; Distance (pc): 94 M*: 0.15 ; log(dm/dt): -9.92 For exptime=34.9 s, spectral region: 2800.0 +- 15.0 A achieves SNR=20.0 / 2-pix-resel A factor of 2.0 has been applied to the exptime in each exposure. global countrate (brightest segment): 2514.3 cts/s/segment brightest pixel: 2.325 cts/s/pix at 2796.8 A Calculation performed 2021-06-18T15:04:42, v0.24 Exptime computed from recx9_lya2_etc, padded by factor 6 since flux is very uncertain for mid-late M stars. Configuration is safe under M dwarf flare conditions, see STIS.sp.1523630 generated from recx9_flarespec.fits (with V mag and SpT input, no extinction). Note that FSW limits are used, not ETC screening limits, for Mdwarf BOP clearing. COnfiguration also safe with x4 accretion variability, see STIS.sp.1523631 generated from recx9_lya2_x4.00_etc recx9_lya2_etc.txt; stis,ccd,g430l,c4300,52x2,mjd#59670 WARNING: operating mode = ACCUM Input file: targets_up_to_May30-2022.csv Spectral type: M4.5 ; A_V: 0.0 ; Distance (pc): 94 M*: 0.15 ; log(dm/dt): -9.92 For exptime=14.5 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): 69374.2 cts/s/segment brightest pixel: 66.074 cts/s/pix at 4560.5 A Calculation performed 2021-06-18T15:04:42, v0.24 Exptime computed using interpolated photometry from Vizier (recx9_interp.dat), padded by 250s. Long saturation time (>5000s) so not an issue. recx9_lya2_etc.txt; stis,ccd,g750l,c7751,52x2,mjd#59670 WARNING: operating mode = ACCUM Input file: targets_up_to_May30-2022.csv Spectral type: M4.5 ; A_V: 0.0 ; Distance (pc): 94 M*: 0.15 ; log(dm/dt): -9.92 For exptime=1.7 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): 208232.1 cts/s/segment brightest pixel: 532.289 cts/s/pix at 6563.9 A Calculation performed 2021-06-18T15:04:42, v0.24 Exptime computed from photometry from Vizier interpolated (recx9_interp.dat). Exptime padded by factor 2.