16824( 3) - 05-Aug-2022 14:32:51 - [ 1] HUBBLE SPACE TELESCOPE OBSERVING PROGRAM 16824 Version: 3 Check-in Time: 05-Aug-2022 14:32:51 STScI Edit Number: 2 Title ULLYSES LMC Late-O Dwarfs - COS and STIS ------------------------------------------------------------------------------------ Type Cycle GO/DD 29 ------------------------------------------------------------------------------------ Investigators Contact? PI: Dr. Julia Christine Roman-Duval Space Telescope Science Institute Y CoI: Dr. Kenneth Sembach Space Telescope Science Institute N CoI: Dr. TalaWanda R. Monroe Space Telescope Science Institute Y CoI: Joanna Taylor Space Telescope Science Institute N CoI: Dr. Travis C Fischer Space Telescope Science Institute - ESA N CoI: Dr. William J. Fischer Space Telescope Science Institute N CoI: Dr. Alexander W. Fullerton Space Telescope Science Institute Y CoI: Dr. Alessandra Aloisi Space Telescope Science Institute N CoI: Christopher Britt Space Telescope Science Institute N CoI: Dr. Thomas M. Brown Space Telescope Science Institute N CoI: Ivo Busko Space Telescope Science Institute N CoI: Dr. Joleen Carlberg Space Telescope Science Institute N CoI: Dr. Gisella De Rosa Space Telescope Science Institute N CoI: Elaine M Frazer Space Telescope Science Institute N CoI: Dr. Svea S Hernandez Space Telescope Science Institute - ESA - N JWST CoI: Dr. Alec S. Hirschauer Space Telescope Science Institute N CoI: Dr. Bethan Lesley James Space Telescope Science Institute - ESA - N JWST CoI: Robert Jedrzejewski Space Telescope Science Institute N CoI: Sean Lockwood Space Telescope Science Institute N CoI: Dr. Cristina Oliveira Space Telescope Science Institute N CoI: Rachel Plesha Space Telescope Science Institute N CoI: Dr. Charles R. Proffitt Space Telescope Science Institute N CoI: Dr. I. Neill Reid Space Telescope Science Institute N CoI: Dr. Adric R. Riedel Space Telescope Science Institute N CoI: Dr. David J. Sahnow Space Telescope Science Institute N CoI: Dr. Ravi Sankrit Space Telescope Science Institute N CoI: Dr. Richard Shaw Space Telescope Science Institute N CoI: Dr. Linda J. Smith Space Telescope Science Institute N CoI: Dr. Sangmo Tony Sohn Space Telescope Science Institute N CoI: Dr. Debopam Som Space Telescope Science Institute N CoI: Dr. Leonardo Ubeda Space Telescope Science Institute N CoI: Dr. Daniel E. Welty Space Telescope Science Institute N CoI: Dr. W. Van Dyke Dixon Space Telescope Science Institute N ------------------------------------------------------------------------------------ Abstract 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) 16824( 3) - 05-Aug-2022 14:32:51 - [ 2] 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. ------------------------------------------------------------------------------------ Observations Description ------------------------ This proposal includes a subset of the massive ULLYSES stars being observed in the Magellanic clouds. Depending on target brightness, the main FUV spectral range will generally use either the STIS E140M setting or the combination of the COS c1291 + c1611 settings. Sufficiently bright stars without good FUSE data in the archive will also be observed with the COS c1096 setting to provide coverage at shorter wavelengths. Where time permits, stars of type O9 or later will also be observed with STIS E230M/1978, while for supergiants of spectral type B5 or later E230M/2707 may also be included. Where possible, targets of a given spectral type were selected to span both a range in extinction and in rotation rates to support a variety of stellar and ISM studies. Signal-to-noise requirements used to determine the desired exposures times were defined as follows: COS/G130M/c1096: 20 / nine-pixel resel at 1080 A COS/G130M/c1291: 30 / six-pixel resel at 1150 A COS/G160M/c1611: 30 / six-pixel resel at 1590 A COS/G185M/c1953: 30 / three-pixel resel at 1860 A COS/G185M/c1986: 30 / three-pixel resel at 1980 A STIS/E140M/c1425: 20 / two-pixel resel at 1200 A STIS/E230M/c1978: 20 / two-pixel resel at 1800 A STIS/E230M/c2707: 20 / two-pixel resel at 2800 A The actual implemented exposure times may be adjusted to efficiently use HST orbits, but should always provide at least 80% of the desired time as defined by the above requirements. 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 16824( 3) - 05-Aug-2022 14:32:51 - [ 3] http://www.stsci.edu/files/live/sites/www/files/home/stsci-research/research-to pics-and-programs/ullyses/_documents/HSTUV-report-ULLYSES.pdf. ------------------------------------------------------------------------------------ 16824( 3) - 05-Aug-2022 14:32:51 - [ 4] TARGET LIST Fixed Targets ------------------------------------------------------------------------------------------------------------------------------------ Tar| Target | Target | Target |Coord | Radial | Flux data No | Name | Description | Position |Eqnx | Vel. | ------------------------------------------------------------------------------------------------------------------------------------ 16824( 3) - 05-Aug-2022 14:32:51 - [ 5] TARGET LIST Fixed Targets ------------------------------------------------------------------------------------------------------------------------------------ Tar| Target | Target | Target |Coord | Radial | Flux data No | Name | Description | Position |Eqnx | Vel. | ------------------------------------------------------------------------------------------------------------------------------------ 1 N11-ELS-046 STAR, MAIN SEQUENCE O RA=04H56M44.6321S +/- 0", J2000 V = 13.98 SpT=O9.5 V; E(B-V)=0.02; DEC=-66D34'20.88" +/- 0" B=13.74; V=13.98 Reference Frame: ICRS Extended: NO Comments: N11-ELS-046 : [ELS2006] N11 046 Previous name : N11-046 Input file: ULLYSES_Cycle29_MassiveStar_ProgramInput_v5.csv SpT = O9.5 V COS/G130M/c1096 : rn(PoWR-OB-new(PoWR_34000_4.20_m7.00_Z0.50.fits, lmc-ob-i 34-42, Z=0.500 solar, Teff=34000, log_lum=4.58, log_g=4.20, log_mdot=-7.00) (extinction lmcavg=0.020), johnson B mag=13.740 vegamag) Coordinate pedigree: Gaia DR2 Calculation performed 2021-10-25T01:00:53, v0.9 ----------------------------------------------------------- -------------------- tstatus; N11-ELS-046; P/COS approved for submission; S/STIS approved for submission; P/AF 14/07/22; S/TM 12/05/22 tcheck; APT/SIMBAD target names: ; N11-ELS-046 '[ELS2006] N11 046' tcheck; Target info verification status?; OK ... Simbad mags are within ~0.1 mag to those adopted for the phase II (which come from Evans et al. 2006, A&A, 456, 623). tcheck; Coordinates & P.M. verified, epoch checked?; Gaia coords ok, added epoch for DR2 tcheck; Adopted SED compared to Observations?; Limited data available ... No FUV, NUV, or optical spectra available, must rely on optical broadband magnitudes Default mags are within 2 percent of the normalized SED. Only B and V from Evans et al. were supplied in the photo.dat file, but other mags are available through SIMBAD (though their origin is unclear: the reference given by SIMBAD incorrectly attributes the measurements to Evans et al. 2006). Added SIMBAD magintudes to SED plots. Ratios to the SED are within 20% for the U band. Ratios to the SED are within ~0.1 mag for Simbad B and V mags. Although the photometry may carry residual uncertainties, Hunter et al. (2008, A&A, 479, 541) derived (Teff, log g) = (33500 K, 4.25) from model atmosphere fits to optical spectra. Consequently, the underlying PoWR model adopted for ETC calculations (Teff, log g) = (34000 K, 4.20) should be quite reliable. The adopted reddening is extremely small, so any residual photometric uncertainties can only act to increase its value (and decrease the flux of the adopted SED at far-UV wavelengths). Hunter et al. indicate that the star is a binary, but do not provide any details. Epoch of Position RA proper motion (seconds of time/yr) DEC Proper Motion (arcsec/yr) Annual Parallax (arcsec) 2015.5 0.0 0.0 0 16824( 3) - 05-Aug-2022 14:32:51 - [ 6] TARGET LIST Fixed Targets ------------------------------------------------------------------------------------------------------------------------------------ Tar| Target | Target | Target |Coord | Radial | Flux data No | Name | Description | Position |Eqnx | Vel. | ------------------------------------------------------------------------------------------------------------------------------------ ------------------------------------------------------------------------------------------------------------------------------------ 2 N11-ELS-049 STAR, MAIN SEQUENCE O RA=04H56M29.5641S +/- 0", J2000 V = 14.02 SpT=O7.5 V; E(B-V)=0.03; DEC=-66D28'20.98" +/- 0" B=13.78; V=14.02 Reference Frame: ICRS Extended: NO Comments: N11-ELS-049 : [ELS2006] N11 049 Previous name : N11-049 Input file: ULLYSES_Cycle29_MassiveStar_ProgramInput_v5.csv SpT = O7.5 V COS/G130M/c1096 : rn(PoWR-OB-new(PoWR_36000_4.00_m7.00_Z0.50.fits, lmc-ob-i 36-40, Z=0.500 solar, Teff=36000, log_lum=5.00, log_g=4.00, log_mdot=-7.00) (extinction lmcavg=0.030), johnson B mag=13.780 vegamag) Coordinate pedigree: Gaia DR2 Calculation performed 2021-10-25T01:00:42, v0.9 ----------------------------------------------------------- -------------------- tstatus; N11-ELS-049; P/COS approved for submission; S/STIS approved for submission; P/AF 14/07/22; S/TM 12/05/22 tcheck; APT/SIMBAD target names: ; N11-ELS-049 [ELS2006] N11 049 '[L72] LH 9-73' tcheck; Target info verification status?; OK ... Simbad mags are within ~0.05mag of the phase II values tcheck; Coordinates & P.M. verified, epoch checked?; Gaia coords ok, added epoch for DR2 tcheck; Adopted SED compared to Observations?; Limited data available ... No FUV, NUV, or optical spectra available, must rely on optical broadband magnitudes Default mags are within 2 percent of the normalized SED. Only B and V were supplied in the photo.dat file, but other mags are available through SIMBAD (though their origin is unclear). Added SIMBAD magintudes to SED plots. Ratios to the SED are within 25% for the U band. Ratios to the SED are within ~0.05 mag for Simbad B and V mags. The reddening indicated by the photometry and spectral type is very small. The far-UV fluxes of the adopted SED will be near the maximum possible value that isalso consistent with the spectral type (which was used to select the model parameters) and the optical photometry (which was used to normalize the flux distribution). Epoch of Position RA proper motion (seconds of time/yr) DEC Proper Motion (arcsec/yr) Annual Parallax (arcsec) 2015.5 0.0 0.0 0 ------------------------------------------------------------------------------------------------------------------------------------ 16824( 3) - 05-Aug-2022 14:32:51 - [ 7] Visit: 1C (N11-ELS-046-COS) Visit Requirements: SCHED 100% On Hold Comments: Additional Comments: vstatus; 1C; N11-ELS-046; P/COS approved for submission; P/AF 14/07/22 ; intrev started ; P/RS 25/07/22 vcheck; Enter targ name & Inst. & Resp. Sci.; N11-ELS-046 ; COS ; AF vcheck; ETC numbers entered in APT?; Completed vcheck; Any screening violations?; None vcheck; S/N ETC calcs done & documented?; Yes vcheck; Field images checked & saved?; Yes - N11-ELS-046_COS_DSS_BOT.png and N11-ELS-046_COS_gaiaBOT.png vcheck; Selected ACQ strategy?; Dispersed G130M/1291 vcheck; Possible ACQ or Sci spoilers?; None vcheck; Field BOT clear?; Yes - see Comments vcheck; Visual BOT check for stars not in catalog?; Completed using gaiaBOT vcheck; Orbit packing finalized?; 1 orbit, recovered 91% of desired exposure time vcheck; Buffer times optimized?; Done vcheck; Verify visit grouping correct; N/A vcheck; Is visit ready for int. review?; Yes Allocated COS orbits = 1 Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 16824( 3) - 05-Aug-2022 14:32:51 - [ 8] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 1 N11-ELS-046 COS/FUV ACQ/PEA PSA G130M 1291 CENTER=FLUX-WT, NUM-POS=3, 1 0.1 S (0.1 KXD STEP-SIZE=1.3 S) Comments: Bright Object Check (GSCII) PEAKXD (H&S, Science, Safe, Unknown) = (0, 0, 1, 56) The unknown stars can be identified with the following stars in the Gaia DR2 catalog, which are referenced for convenience via their gaiaBOT numbers. gaiBOT also allows their "worst-case, O5 V" V-magnitudes to be estimated (Vest) and compared with the limit of V~14.0. See ~/box/ullyses_tech/ullyses_proposals/c29_mc/1 6924/N11-ELS-046/N11-ELS-046_COS_DSS_BOT.png ~/box/ullyses_tech/ullyses_proposals/c29_mc/1 6924/N11-ELS-046/N11-ELS-046_COS_gaiaBOT.png gBOT# Vest Comment BOA S1IW146161 04 56 42.0099 -66 34 26.50 26 18.68 Safe BOA S1IW146177 04 56 41.9330 -66 34 15.27 29 18.77 Safe BOA S1IW146189 04 56 46.4630 -66 34 11.92 22 18.06 Safe BOA S1IW146208 04 56 44.8737 -66 34 30.37 14 19.52 Safe PSA S1IW112536 04 56 44.5551 -66 34 22.93 ?? none Spurious? The data in the gaiaBOT spreadsheet ~/box/ullyses_tech/ullyses_proposals/c29_mc/1 6824/gaiaBOT/16824_N11_ELS_046_GAIA_DR2_r22ar csec_bot.csv indicates that there is nothing brighter than Vest = 14.00 within the COS macroaperture (radius = 22 arcseconds) of the target. Thus, gaiaBOT indicates that all stars in the field are safe. There are no spoilers in this field. ------------------------------------------------------------------------------------------------------------------------------------ 16824( 3) - 05-Aug-2022 14:32:51 - [ 9] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 2 N11-ELS-046 COS/FUV ACQ/PEA PSA G130M 1291 CENTER=FLUX-WT-FLR, NUM-POS=5, 1 0.1 S (0.1 KD STEP-SIZE=0.9 S) Comments: Bright Object Check (GSCII) PEAKD (H&S, Science, Safe, Unknown) = (0, 0, 1, 6) The unknown stars can be identified with the following stars in the Gaia DR2 catalog, which are referenced for convenience via their gaiaBOT numbers. gaiBOT also allows their "worst-case, O5 V" V-magnitudes to be estimated (Vest) and compared with the limit of V~14.0. See ~/box/ullyses_tech/ullyses_proposals/c29_mc/1 6924/N11-ELS-046/N11-ELS-046_COS_DSS_BOT.png ~/box/ullyses_tech/ullyses_proposals/c29_mc/1 6924/N11-ELS-046/N11-ELS-046_COS_gaiaBOT.png gBOT# Vest Comment BOA S1IW146161 04 56 42.0099 -66 34 26.50 26 18.68 Safe BOA S1IW146177 04 56 41.9330 -66 34 15.27 29 18.77 Safe BOA S1IW146189 04 56 46.4630 -66 34 11.92 22 18.06 Safe BOA S1IW146208 04 56 44.8737 -66 34 30.37 14 19.52 Safe PSA S1IW112536 04 56 44.5551 -66 34 22.93 ?? none Spurious? The data in the gaiaBOT spreadsheet ~/box/ullyses_tech/ullyses_proposals/c29_mc/1 6824/gaiaBOT/16824_N11_ELS_046_GAIA_DR2_r22ar csec_bot.csv indicates that there is nothing brighter than Vest = 14.00 within the COS macroaperture (radius = 22 arcseconds) of the target. Thus, gaiaBOT indicates that all stars in the field are safe. There are no spoilers in this field. ------------------------------------------------------------------------------------------------------------------------------------ 16824( 3) - 05-Aug-2022 14:32:51 - [ 10] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 3 N11-ELS-046 COS/FUV TIME-TA PSA G130M 1096 BUFFER-TIME=141, FP-POS=ALL 1 392 S G (1568 S) Comments: ETC calculations used ~/box/ullyses_tech/ullyses_proposals/c29_mc/1 6824/N11-ELS-046/N11-ELS-046_adopted_sed.fits which is identical to ~/box/ullyses_tech/ullyses_proposals/c29_mc/1 6824/N11-ELS-046/seds/N11-ELS-46_COS_G130M_c1 096_sed.fits This is the PoWR_34000_4.20_m7.00_Z0.50 model, reddened by E(B-V) = 0.02 with the lmcavg law, and normalized to B=13.74. ETC calculation COS.sp.1814898 indicates that SNR=20/resel is obtained at 1080 +/- 0.5 A in 1719.455 s - Warning Issued: count-rate exceeds segment/stripe limit for irregularly-variable source, which is not relevant for current source - There is a factor of 1.7 (0.57 magnitudes) margin before Segment A reaches the 15, 000 count/s limit. This is much larger than the uncertainty in the normalization provided by the optical photometry, so photometric errors should not be a concern Baseline exposure rounded to 1720 s (430 per FP-POS) Count Rate (Total, Segment A, Segment B) = (9083.512, 8874.924, 208.588) Brightest Pixel: 0.115 counts/s at 1216.22 A Buffer-Fill Time = 259s Buffer Time = 2/3 * 259 s = 172 s Optimized = 141 s After orbital packing and buffer time optimization, the exposure time was adjusted to 392 s per FP-POS, which yields 91% the baseline exposure time. The predicted S/N = sqrt(392/967) * 20 = 19.1 per resel. Bright Object Check with GSCII G130M/1096 (H&S, Science, Safe, Unknown) = (0, 0, 1, 5) The unknown stars can be identified with the following stars in the Gaia DR2 catalog, which are referenced for convenience via their gaiaBOT numbers. gaiBOT also allows their "worst-case, O5 V" V-magnitudes to be estimated (Vest) and compared with the limit of V~14.0. See ~/box/ullyses_tech/ullyses_proposals/c29_mc/1 6824/N11-ELS-046/N11-ELS-046_COS_DSS_BOT.png ~/box/ullyses_tech/ullyses_proposals/c29_mc/1 6824/N11-ELS-046/N11-ELS-046_COS_gaiaBOT.png gBOT# Vest Comment BOA S1IW146161 04 56 42.0099 -66 34 26.50 26 18.68 Safe BOA S1IW146177 04 56 41.9330 -66 34 15.27 29 18.77 Safe BOA S1IW146189 04 56 46.4630 -66 34 11.92 22 18.06 Safe BOA S1IW146208 04 56 44.8737 -66 34 30.37 14 19.52 Safe PSA S1IW112536 04 56 44.5551 -66 34 22.93 ?? none Spurious? The data in the gaiaBOT spreadsheet ~/box/ullyses_tech/ullyses_proposals/c29_mc/1 6824/gaiaBOT/16824_N11_ELS_046_GAIA_DR2_r22ar csec_bot.csv indicates that there is nothing brighter than Vest = 14.00 within the COS macroaperture (radius = 22 arcseconds) of the target. Thus, gaiaBOT indicates that all stars in the field are safe. There are no spoilers in this field. 16824( 3) - 05-Aug-2022 14:32:51 - [ 11] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ ------------------------------------------------------------------------------------------------------------------------------------ Sub Exposures ------------------------------------------------------------------------------------------------------------------------------------ Target | Exp |Instr | Oper. | Aper |Spectral|Cent.|Primary |Secondary |Iteration |CR-SPLIT |Orbit |Duration Name | Num |Config | Mode | or FOV |Element |Wave.|Pattern Pos |Pattern Pos |Num |Num |Number | ------------------------------------------------------------------------------------------------------------------------------------ N11-ELS-046 1 COS/FUV ACQ/PEA PSA G130M 1291 none none none none 1 N/A KXD N11-ELS-046 2 COS/FUV ACQ/PEA PSA G130M 1291 none none none none 1 N/A KD N11-ELS-046 3 COS/FUV TIME-TA PSA G130M 1096 none none none 1 1 N/A G N11-ELS-046 3 COS/FUV TIME-TA PSA G130M 1096 none none none 2 1 N/A G N11-ELS-046 3 COS/FUV TIME-TA PSA G130M 1096 none none none 3 1 N/A G N11-ELS-046 3 COS/FUV TIME-TA PSA G130M 1096 none none none 4 1 N/A G 16824( 3) - 05-Aug-2022 14:32:51 - [ 12] Visit: 1S (N11-ELS-046-STIS) Visit Requirements: SCHED 100%; ORIENT 260D TO 280 D; ORIENT 80D TO 100 D; GROUP 1S, 1C WITHIN 30D On Hold Comments: Additional Comments: vstatus; 1S; N11-ELS-046; S/STIS approved for submission; S/TM 12/05/22 ; intrev: complete ; S/DW 04/08/22 vcheck; Enter targ name & Inst. & Resp. Sci.; N11-ELS-046 '[ELS2006] N11 046' ; STIS ; TM vcheck; ETC numbers entered in APT?; completed vcheck; Any screening violations?; none vcheck; S/N ETC calcs done & documented?; Yes ... STIS.sp.1748937 with 7252 sec exptime gives SNR = 16 (or 20 from ETC plots) at 1200A Given the uncertainty in normalization due to no obs. spectra, I did an extreme BOP calculation of 2 times the original SED: STIS.sp.1749888 A padding of 20% more flux is more realistic and was used for the buffer time calculations: STIS.sp.1749887 vcheck; Field images checked & saved?; yes Saved images of DSS, 2MASS, and GALEX. No spoiler stars within 5". 2Mass image has some elongation near the target though. vcheck; Selected ACQ strategy?; STIS F28X50OII 11sec ... Using the OII filter given that the discovered companion at 0.2" may be redder in the F28x50LP filter. STIS.ta.1817373 gives SNR = 50 in 9.75 sec STIS.ta.1817372 Castelli-Kurucz Models O9V model with V=13.98 and E(B-V) = 0.02 gives 9.6235 sec for SNR = 50 Given the uncertainty in normalization and reddening, rounded up to 11 sec. vcheck; Possible ACQ or Sci spoilers?; No ... Checked Simbad and Gaia catalogs for nearby sources. None within 5" There is a red Gaia source at 7", but that's outside the region of interest. Zaritsky catalog has 3 sources - 2 of the target, one offset north of the target with Vmag =19. vcheck; Field BOT clear?; yes ... Only the 1 source appears in GSC2, it's offset from the DSS target and Gaia coordinates. Target is visible in Galex images, but is not returned by the BOT. vcheck; Visual BOT check for stars not in catalog?; ok vcheck; Orbit packing finalized?; yes, 3 orbits vcheck; Buffer times optimized?; yes ... Given no obs. spectra for SED normalization, I scaled the SED by 1.2 in case the source is 20 percent brighter unexpectedly. See STIS.sp.1749887 vcheck; Verify visit grouping correct; yes vcheck; Is visit ready for int. review?; yes Allocated STIS orbits = 3 Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 1 N11-ELS-046 STIS/CCD ACQ F28X50OII MIRROR 1 11 S (11 S) ------------------------------------------------------------------------------------------------------------------------------------ 16824( 3) - 05-Aug-2022 14:32:51 - [ 13] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 2 N11-ELS-046 STIS/FUV TIME-TA 0.2X0.2 E140M 1425 WAVECAL=NO, BUFFER-TIME=380 1 2121 S -MAMA G (2121 S) Comments: rn(PoWR-OB-new(PoWR_34000_4.20_m7.00_Z0.50.fi ts, lmc-ob-i 34-42, Z=0.500 solar, Teff=34000, log_lum=4.58, log_g=4.20, log_mdot=-7.00) (extinction lmcavg=0.020), johnson B mag=13.740 vegamag); stis, fuvmama, e140m, c1425, 0.2x0.2, mjd#59670 From file ULLYSES_Cycle29_MassiveStar_ProgramInput_v5.c sv Spectral type: O9.5 V SED = N11-ELS-46_STIS_E140M_c1425_sed.fits For exptime=7045.7 s, spectral region: 1200.0 +- 0.5 A achieves SNR=20.0/resel global countrate (brightest segment): 3546.1 cts/s/segment brightest pixel: 0.043 cts/s/pix at 1298.0 A Calculation performed 2021-10-25T01:01:02, v0.9 ------------------------------------------------------------------------------------------------------------------------------------ 3 WAVE STIS/FUV ACCUM 0.2X0.2 E140M 1425 1 DEF (0 S) -MAMA ------------------------------------------------------------------------------------------------------------------------------------ 4 N11-ELS-046 STIS/FUV TIME-TA 0.2X0.2 E140M 1425 WAVECAL=NO, BUFFER-TIME=380 1 2548 S -MAMA G (2548 S) Comments: rn(PoWR-OB-new(PoWR_34000_4.20_m7.00_Z0.50.fi ts, lmc-ob-i 34-42, Z=0.500 solar, Teff=34000, log_lum=4.58, log_g=4.20, log_mdot=-7.00) (extinction lmcavg=0.020), johnson B mag=13.740 vegamag); stis, fuvmama, e140m, c1425, 0.2x0.2, mjd#59670 From file ULLYSES_Cycle29_MassiveStar_ProgramInput_v5.c sv Spectral type: O9.5 V SED = N11-ELS-46_STIS_E140M_c1425_sed.fits For exptime=7045.7 s, spectral region: 1200.0 +- 0.5 A achieves SNR=20.0/resel global countrate (brightest segment): 3546.1 cts/s/segment brightest pixel: 0.043 cts/s/pix at 1298.0 A Calculation performed 2021-10-25T01:01:02, v0.9 ------------------------------------------------------------------------------------------------------------------------------------ 16824( 3) - 05-Aug-2022 14:32:51 - [ 14] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 5 WAVE STIS/FUV ACCUM 0.2X0.2 E140M 1425 1 DEF (0 S) -MAMA ------------------------------------------------------------------------------------------------------------------------------------ 6 N11-ELS-046 STIS/FUV TIME-TA 0.2X0.2 E140M 1425 WAVECAL=NO, BUFFER-TIME=380 1 2548 S -MAMA G (2548 S) Comments: rn(PoWR-OB-new(PoWR_34000_4.20_m7.00_Z0.50.fi ts, lmc-ob-i 34-42, Z=0.500 solar, Teff=34000, log_lum=4.58, log_g=4.20, log_mdot=-7.00) (extinction lmcavg=0.020), johnson B mag=13.740 vegamag); stis, fuvmama, e140m, c1425, 0.2x0.2, mjd#59670 From file ULLYSES_Cycle29_MassiveStar_ProgramInput_v5.c sv Spectral type: O9.5 V SED = N11-ELS-46_STIS_E140M_c1425_sed.fits For exptime=7045.7 s, spectral region: 1200.0 +- 0.5 A achieves SNR=20.0/resel global countrate (brightest segment): 3546.1 cts/s/segment brightest pixel: 0.043 cts/s/pix at 1298.0 A Calculation performed 2021-10-25T01:01:02, v0.9 ------------------------------------------------------------------------------------------------------------------------------------ 7 WAVE STIS/FUV ACCUM 0.2X0.2 E140M 1425 1 DEF (0 S) -MAMA ------------------------------------------------------------------------------------------------------------------------------------ Sub Exposures ------------------------------------------------------------------------------------------------------------------------------------ Target | Exp |Instr | Oper. | Aper |Spectral|Cent.|Primary |Secondary |Iteration |CR-SPLIT |Orbit |Duration Name | Num |Config | Mode | or FOV |Element |Wave.|Pattern Pos |Pattern Pos |Num |Num |Number | ------------------------------------------------------------------------------------------------------------------------------------ N11-ELS-046 1 STIS/CCD ACQ F28X50OI MIRROR none none none none 1 N/A I N11-ELS-046 2 STIS/FUV TIME-TA 0.2X0.2 E140M 1425 none none none none 1 N/A -MAMA G WAVE 3 STIS/FUV ACCUM 0.2X0.2 E140M 1425 none none none none 1 N/A -MAMA N11-ELS-046 4 STIS/FUV TIME-TA 0.2X0.2 E140M 1425 none none none none 2 N/A -MAMA G WAVE 5 STIS/FUV ACCUM 0.2X0.2 E140M 1425 none none none none 2 N/A -MAMA N11-ELS-046 6 STIS/FUV TIME-TA 0.2X0.2 E140M 1425 none none none none 3 N/A -MAMA G 16824( 3) - 05-Aug-2022 14:32:51 - [ 15] Sub Exposures ------------------------------------------------------------------------------------------------------------------------------------ Target | Exp |Instr | Oper. | Aper |Spectral|Cent.|Primary |Secondary |Iteration |CR-SPLIT |Orbit |Duration Name | Num |Config | Mode | or FOV |Element |Wave.|Pattern Pos |Pattern Pos |Num |Num |Number | ------------------------------------------------------------------------------------------------------------------------------------ WAVE 7 STIS/FUV ACCUM 0.2X0.2 E140M 1425 none none none none 3 N/A -MAMA 16824( 3) - 05-Aug-2022 14:32:51 - [ 16] Visit: 2C (N11-ELS-049-COS) Visit Requirements: SCHED 100% On Hold Comments: Additional Comments: vstatus; 2C; N11-ELS-049; P/COS approved for submission; P/AF 14/07/22 ; intrev complete ; P/RS 25/07/22 vcheck; Enter targ name & Inst. & Resp. Sci.; N11-ELS-049 ; COS ; AF vcheck; ETC numbers entered in APT?; Completed vcheck; Any screening violations?; None vcheck; S/N ETC calcs done & documented?; Yes vcheck; Field images checked & saved?; Yes - N11-ELS-049_COS_DSS_BOT.png and N11-ELS-049_COS_gaiaBOT.png vcheck; Selected ACQ strategy?; Dispersed G130M/1291 vcheck; Possible ACQ or Sci spoilers?; None vcheck; Field BOT clear?; Yes - see Comments vcheck; Visual BOT check for stars not in catalog?; Completed using gaiaBOT vcheck; Orbit packing finalized?; 1 orbit, recovered 79% of desired exposure time vcheck; Buffer times optimized?; Done vcheck; Verify visit grouping correct; N/A vcheck; Is visit ready for int. review?; Yes Allocated COS orbits = 1 Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 16824( 3) - 05-Aug-2022 14:32:51 - [ 17] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 1 N11-ELS-049 COS/FUV ACQ/PEA PSA G130M 1291 CENTER=FLUX-WT, NUM-POS=3, 1 0.2 S (0.2 KXD STEP-SIZE=1.3 S) Comments: COS.sa.1815097 indicates that S/N = 30 can be achived with texp = 0.1026 s, which was rounded up to 0.2 s. The ETC issued a WARNING that the count-rate exceeds the segment/stripe limit for irregularly variable sources, which is not relevant in this case. Bright Object Check with GSCII PEAKXD (H&S, Science, Safe, Unknown) = (0, 0, 4, 3) The unknown stars can be identified with the following stars in the Gaia DR2 catalog, which are referenced for convenience via their gaiaBOT numbers. gaiBOT also allows their "worst-case, O5 V" V-magnitudes to be estimated (Vest) and compared with the limit of V~14.0. See ~/box/ullyses_tech/ullyses_proposals/c29_mc/1 6924/N11-ELS-049/N11-ELS-049_COS_DSS_BOT.png ~/box/ullyses_tech/ullyses_proposals/c29_mc/1 6924/N11-ELS-049/N11-ELS-049_COS_gaiaBOT.png gBOT# Vest Comment BOA S1IW146778 04 56 27.4896 -66 28 35.57 73, 77 19.4, 19.6 Safe BOA S1IW146813 04 56 26.6290 -66 28 14.86 56 19.0 Safe PSA S1IW113581 04 56 29.5660 -66 28 20.88 This appears to be the target, which is Safe The data in the gaiaBOT spreadsheet ~/box/ullyses_tech/ullyses_proposals/c29_mc/1 6924/gaiaBOT/16824_N11_ELS_049_GAIA_DR2_r22ar csec_bot.csv indicates that there is nothing brighter than Vest = 14.00 within 22 arcseconds of the target. ------------------------------------------------------------------------------------------------------------------------------------ 16824( 3) - 05-Aug-2022 14:32:51 - [ 18] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 2 N11-ELS-049 COS/FUV ACQ/PEA PSA G130M 1291 CENTER=FLUX-WT-FLR, NUM-POS=5, 1 0.2 S (0.2 KD STEP-SIZE=0.9 S) Comments: COS.sa.1815097 indicates that S/N = 30 can be achived with texp = 0.1026 s, which was rounded up to 0.2 s. The ETC issued a WARNING that the count-rate exceeds the segment/stripe limit for irregularly variable sources, which is not relevant in this case. Bright Object Check with GSCII PEAKD (H&S, Science, Safe, Unknown) = (0, 0, 7, 3) The unknown stars can be identified with the following stars in the Gaia DR2 catalog, which are referenced for convenience via their gaiaBOT numbers. gaiBOT also allows their "worst-case, O5 V" V-magnitudes to be estimated (Vest) and compared with the limit of V~14.0. See ~/box/ullyses_tech/ullyses_proposals/c29_mc/1 6924/N11-ELS-049/N11-ELS-049_COS_DSS_BOT.png ~/box/ullyses_tech/ullyses_proposals/c29_mc/1 6924/N11-ELS-049/N11-ELS-049_COS_gaiaBOT.png gBOT# Vest Comment BOA S1IW146778 04 56 27.4896 -66 28 35.57 73, 77 19.4, 19.6 Safe BOA S1IW146813 04 56 26.6290 -66 28 14.86 56 19.0 Safe PSA S1IW113581 04 56 29.5660 -66 28 20.88 This appears to be the target, which is Safe The data in the gaiaBOT spreadsheet ~/box/ullyses_tech/ullyses_proposals/c29_mc/1 6924/gaiaBOT/16824_N11_ELS_049_GAIA_DR2_r22ar csec_bot.csv indicates that there is nothing brighter than Vest = 14.00 within 22 arcseconds of the target. ------------------------------------------------------------------------------------------------------------------------------------ 16824( 3) - 05-Aug-2022 14:32:51 - [ 19] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 3 N11-ELS-049 COS/FUV TIME-TA PSA G130M 1096 BUFFER-TIME=145.0, FP-POS=ALL 1 399 S G (1596 S) Comments: The ETC calculations used ~/box/ullyses_tech/ullyses_proposals/c29_mc/1 6824/N11-ELS-049/N11-ELS-049_adopted_sed.fits which is identical to ~/box/ullyses_tech/ullyses_proposals/c29_mc/1 6824/N11-ELS-049/seds/N11-ELS-49_COS_G130M_c1 096_sed.fits This is the PoWR_36000_4.00_m7.00_Z0.50 model, reddened by E(B-V) = 0.03 with the lmcavg law, and normalized to B=13.78. ETC calculation COS.sp.1815098 indicates that SNR=20/resel is obtained at 1080 +/- 0.5 A in 2013 s - WARNING Issued: count-rate exceeds segment/stripe limit for irregularly-variable source, which is not relevant for current source - There is a factor of 1.8 (0.65 magnitudes) margin before Segment A reaches the 15, 000 count/s limit. This is much larger than the uncertainty in the normalization provided by the optical photometry. The baseline exposure was rounded to 2012 s (503 s per FP-POS) Count Rate (Total, Segment A, Segment B) = (8, 403.289, 8, 215.660, 187.629) Brightest Pixel: 0.118 counts/s at 1216.22 A Buffer-Fill Time = 280 s Buffer Time = 2/3 * 259 s = 187 s Optimized = 131 s After orbital packing, the exposure time was reduced to 399 s per FP-POS with an optimized buffer time of 145 s. The net exposure time is 79.3% of the baseline required to achieve the S/N goal. The predicted S/N = sqrt(399/503) * 20 = 17.8 per resel, which is acceptable. Bright Object Check with GSCII G130M/1096 (H&S, Science, Safe, Unknown) = (0, 0, 4, 3) The 3 unknown stars can be identified with the following stars in the Gaia DR2 catalog, which are referenced for convenience via their gaiaBOT numbers. gaiBOT also allows their "worst-case, O5 V" V-magnitudes to be estimated (Vest) and compared with the limit of V~14.0. See ~/box/ullyses_tech/ullyses_proposals/c29_mc/1 6824/N11-ELS-049/N11-ELS-049_COS_DSS_BOT.png ~/box/ullyses_tech/ullyses_proposals/c29_mc/1 6824/N11-ELS-049/N11-ELS-049_COS_gaiaBOT.png gBOT# Vest Comment BOA S1IW146778 04 56 27.4896 -66 28 35.57 73, 77 19.4, 19.6 Safe BOA S1IW146813 04 56 26.6290 -66 28 14.86 56 19.0 Safe PSA S1IW113581 04 56 29.5660 -66 28 20.88 This appears to be the target, which is Safe The data in the gaiaBOT spreadsheet ~/box/ullyses_tech/ullyses_proposals/c29_mc/1 6824/gaiaBOT/16824_N11_ELS_049_GAIA_DR2_r22ar csec_bot.csv indicates that there is nothing brighter than Vest = 14.00 within the COS macroaperture (radius = 22 arcseconds) of the target. Thus, gaiaBOT indicates that all stars in the field are safe. There are no spoilers in this field. 16824( 3) - 05-Aug-2022 14:32:51 - [ 20] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ ------------------------------------------------------------------------------------------------------------------------------------ Sub Exposures ------------------------------------------------------------------------------------------------------------------------------------ Target | Exp |Instr | Oper. | Aper |Spectral|Cent.|Primary |Secondary |Iteration |CR-SPLIT |Orbit |Duration Name | Num |Config | Mode | or FOV |Element |Wave.|Pattern Pos |Pattern Pos |Num |Num |Number | ------------------------------------------------------------------------------------------------------------------------------------ N11-ELS-049 1 COS/FUV ACQ/PEA PSA G130M 1291 none none none none 1 N/A KXD N11-ELS-049 2 COS/FUV ACQ/PEA PSA G130M 1291 none none none none 1 N/A KD N11-ELS-049 3 COS/FUV TIME-TA PSA G130M 1096 none none none 1 1 N/A G N11-ELS-049 3 COS/FUV TIME-TA PSA G130M 1096 none none none 2 1 N/A G N11-ELS-049 3 COS/FUV TIME-TA PSA G130M 1096 none none none 3 1 N/A G N11-ELS-049 3 COS/FUV TIME-TA PSA G130M 1096 none none none 4 1 N/A G 16824( 3) - 05-Aug-2022 14:32:51 - [ 21] Visit: 2S (N11-ELS-049-STIS) Visit Requirements: SCHED 100%; GROUP 2S, 2C WITHIN 30D On Hold Comments: Additional Comments: vstatus; 2S; N11-ELS-049; S/STIS approved for submission; S/TM 19/05/22 ; intrev: complete ; S/DW 04/08/22 vcheck; Enter targ name & Inst. & Resp. Sci.; N11-ELS-049 [ELS2006] N11 049 '[L72] LH 9-73' ; STIS ; TM vcheck; ETC numbers entered in APT?; yes ... STIS.sp.1749891: Default SED gives SNR = 16.1 in 7252 sec Given uncertainty in the SED normalization, asssumed 20 percent brighter SED for buffer time calcluation STIS.sp.1749892 for buffer time Given the uncertainty in normalization due to no obs. spectra, I did an extreme BOP calculation of 2 times the original SED: STIS.sp.1749893 vcheck; Any screening violations?; None vcheck; S/N ETC calcs done & documented?; Yes ... STIS.sp.1749891: Default SED gives SNR = 16.1 (but 20 on SNR plot) in 7252 sec vcheck; Field images checked & saved?; Yes vcheck; Selected ACQ strategy?; STIS F28X50LP 0.3sec ... PoWR SEDs don't go redward enough for the F28x50LP filter but STIS.ta.1749991 gives SNR = 40 in 0.24 sec, with only partial bandpass coverage STIS.ta.1749995 Castelli-Kurucz Models O7V model with V=14.02 and E(B-V) = 0.03, rounding to 0.3s vcheck; Possible ACQ or Sci spoilers?; none ... Closest Simbad source is 5.9" to the north, with V=19mag, not a concern No red 2MASS sources nearby. No Gaia sources brighter than the target within 5". No Gaia red sources that are concerns either. A red source with g=18.8 mag at 5.8" is no concern. vcheck; Field BOT clear?; yes ... GSC2 only returns the target. Galex returns nothing, and image is a confused mess. Nothing bright in the Zaritsky catalog. vcheck; Visual BOT check for stars not in catalog?; OK vcheck; Orbit packing finalized?; yes, 3 orbits vcheck; Buffer times optimized?; yes ... Given no obs. spectra for SED normalization, I scaled the SED by 1.2 in case the source is 20 percent brighter unexpectedly. See STIS.sp.1749892 vcheck; Verify visit grouping correct; group 30D added vcheck; Is visit ready for int. review?; yes Allocated STIS orbits = 3 Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 1 N11-ELS-049 STIS/CCD ACQ F28X50LP MIRROR 1 0.3 S (0.3 S) Comments: Exposure time not yet calculated. ------------------------------------------------------------------------------------------------------------------------------------ 16824( 3) - 05-Aug-2022 14:32:51 - [ 22] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 2 N11-ELS-049 STIS/FUV TIME-TA 0.2X0.2 E140M 1425 WAVECAL=NO, BUFFER-TIME=406 1 2196 S -MAMA G (2196 S) Comments: rn(PoWR-OB-new(PoWR_36000_4.00_m7.00_Z0.50.fi ts, lmc-ob-i 36-40, Z=0.500 solar, Teff=36000, log_lum=5.00, log_g=4.00, log_mdot=-7.00) (extinction lmcavg=0.030), johnson B mag=13.780 vegamag); stis, fuvmama, e140m, c1425, 0.2x0.2, mjd#59670 From file ULLYSES_Cycle29_MassiveStar_ProgramInput_v5.c sv Spectral type: O7.5 V SED = N11-ELS-49_STIS_E140M_c1425_sed.fits For exptime=7344.0 s, spectral region: 1200.0 +- 0.5 A achieves SNR=20.0/resel global countrate (brightest segment): 3314.9 cts/s/segment brightest pixel: 0.038 cts/s/pix at 1298.0 A Calculation performed 2021-10-25T01:00:52, v0.9 ------------------------------------------------------------------------------------------------------------------------------------ 3 WAVE STIS/FUV ACCUM 0.2X0.2 E140M 1425 1 DEF (0 S) -MAMA ------------------------------------------------------------------------------------------------------------------------------------ 4 N11-ELS-049 STIS/FUV TIME-TA 0.2X0.2 E140M 1425 WAVECAL=NO, BUFFER-TIME=406 1 2548 S -MAMA G (2548 S) Comments: rn(PoWR-OB-new(PoWR_36000_4.00_m7.00_Z0.50.fi ts, lmc-ob-i 36-40, Z=0.500 solar, Teff=36000, log_lum=5.00, log_g=4.00, log_mdot=-7.00) (extinction lmcavg=0.030), johnson B mag=13.780 vegamag); stis, fuvmama, e140m, c1425, 0.2x0.2, mjd#59670 From file ULLYSES_Cycle29_MassiveStar_ProgramInput_v5.c sv Spectral type: O7.5 V SED = N11-ELS-49_STIS_E140M_c1425_sed.fits For exptime=7344.0 s, spectral region: 1200.0 +- 0.5 A achieves SNR=20.0/resel global countrate (brightest segment): 3314.9 cts/s/segment brightest pixel: 0.038 cts/s/pix at 1298.0 A Calculation performed 2021-10-25T01:00:52, v0.9 ------------------------------------------------------------------------------------------------------------------------------------ 16824( 3) - 05-Aug-2022 14:32:51 - [ 23] Exposures ------------------------------------------------------------------------------------------------------------------------------------ Exp | Target | Instr | Oper. | Aper |Spectral|Central| Optional |Num| Time | Special Num | Name | Config | Mode | or FOV |Element |Waveln.| Parameters |Exp| (Total) | Requirements ------------------------------------------------------------------------------------------------------------------------------------ 5 WAVE STIS/FUV ACCUM 0.2X0.2 E140M 1425 1 DEF (0 S) -MAMA ------------------------------------------------------------------------------------------------------------------------------------ 6 N11-ELS-049 STIS/FUV TIME-TA 0.2X0.2 E140M 1425 WAVECAL=NO, BUFFER-TIME=406 1 2548 S -MAMA G (2548 S) Comments: rn(PoWR-OB-new(PoWR_36000_4.00_m7.00_Z0.50.fi ts, lmc-ob-i 36-40, Z=0.500 solar, Teff=36000, log_lum=5.00, log_g=4.00, log_mdot=-7.00) (extinction lmcavg=0.030), johnson B mag=13.780 vegamag); stis, fuvmama, e140m, c1425, 0.2x0.2, mjd#59670 From file ULLYSES_Cycle29_MassiveStar_ProgramInput_v5.c sv Spectral type: O7.5 V SED = N11-ELS-49_STIS_E140M_c1425_sed.fits For exptime=7344.0 s, spectral region: 1200.0 +- 0.5 A achieves SNR=20.0/resel global countrate (brightest segment): 3314.9 cts/s/segment brightest pixel: 0.038 cts/s/pix at 1298.0 A Calculation performed 2021-10-25T01:00:52, v0.9 ------------------------------------------------------------------------------------------------------------------------------------ 7 WAVE STIS/FUV ACCUM 0.2X0.2 E140M 1425 1 DEF (0 S) -MAMA ------------------------------------------------------------------------------------------------------------------------------------ Sub Exposures ------------------------------------------------------------------------------------------------------------------------------------ Target | Exp |Instr | Oper. | Aper |Spectral|Cent.|Primary |Secondary |Iteration |CR-SPLIT |Orbit |Duration Name | Num |Config | Mode | or FOV |Element |Wave.|Pattern Pos |Pattern Pos |Num |Num |Number | ------------------------------------------------------------------------------------------------------------------------------------ N11-ELS-049 1 STIS/CCD ACQ F28X50LP MIRROR none none none none 1 N/A N11-ELS-049 2 STIS/FUV TIME-TA 0.2X0.2 E140M 1425 none none none none 1 N/A -MAMA G WAVE 3 STIS/FUV ACCUM 0.2X0.2 E140M 1425 none none none none 1 N/A -MAMA N11-ELS-049 4 STIS/FUV TIME-TA 0.2X0.2 E140M 1425 none none none none 2 N/A -MAMA G WAVE 5 STIS/FUV ACCUM 0.2X0.2 E140M 1425 none none none none 2 N/A -MAMA N11-ELS-049 6 STIS/FUV TIME-TA 0.2X0.2 E140M 1425 none none none none 3 N/A -MAMA G WAVE 7 STIS/FUV ACCUM 0.2X0.2 E140M 1425 none none none none 3 N/A -MAMA 16824( 3) - 05-Aug-2022 14:32:51 - [ 24] Summary Form for Proposal 16824 Item Used in this proposal ------------------------------------------------------------------------------------------------------------------------------------ Apertures 0.2X0.2, F28X50LP, F28X50OII, PSA ------------------------------------------------------------------------------------------------------------------------------------ Configurations COS/FUV, STIS/CCD, STIS/FUV-MAMA ------------------------------------------------------------------------------------------------------------------------------------ Opmodes ACCUM, ACQ, ACQ/PEAKD, ACQ/PEAKXD, TIME-TAG ------------------------------------------------------------------------------------------------------------------------------------ Optional Parameters BUFFER-TIME=141, BUFFER-TIME=145.0, BUFFER-TIME=380, BUFFER-TIME=406, CENTER=FLUX-WT, CENTER=FLUX-WT-FLR, FP-POS=ALL, NUM-POS=3, NUM-POS=5, STEP-SIZE=0.9, STEP-SIZE=1.3, WAVECAL=NO ------------------------------------------------------------------------------------------------------------------------------------ Special Requirements GROUP 1S, 1C WITHIN 30D, GROUP 2S, 2C WITHIN 30D, ORIENT 260D TO 280 D, ORIENT 80D TO 100 D, SCHED 100% ------------------------------------------------------------------------------------------------------------------------------------ Spectral Elements E140M, G130M, MIRROR ------------------------------------------------------------------------------------------------------------------------------------ Target Names N11-ELS-046, N11-ELS-049, WAVE ------------------------------------------------------------------------------------------------------------------------------------