Re-submission of 16805. Repeat visit approved via HOPR 92314. -1199240308 ----- Attempting Submission 1 (Wed Mar 30 22:20:19 GMT 2022) ----- HST Phase II Proposal 16805 successfully submitted. Receipt: # 16805-1 ----- Attempting Submission 2 (Mon Aug 29 15:06:44 GMT 2022) ----- One co-I Alyssa Riley has left and one co-I Van Dixon has joined the ULLYSES team 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 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 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 SUPERGIANT O OF NO NGC346-MPG-435 : Cl* NGC 346 W 1 Previous name : NGC346-1 Input file: ULLYSES_Cycle29_MassiveStar_ProgramInput_v5.csv SpT = O4 If + O5-6 Coordinate pedigree: Gaia DR2 Calculation performed 2021-10-25T00:53:53, v0.9 ------------------------------------------------------------------------------- tstatus; NGC346-MPG-435; P/STIS approved for submission; S/STIS not started; P/LS 12/11/21; S/xx DD/MM/YY tcheck; APT/SIMBAD target names: ; NGC-346-MPG-435 'Cl* NGC 346 SSN 7' tcheck; Target info verification status?; OK ... Spectral type is from Dufton et al. (2019) O4If+O4-6 and this is given in SIMBAD tcheck; Coordinates & P.M. verified, epoch checked?; yes - used coords and PMs given in SNAP 16230 for epoch 2015.5... Van Dixon noticed that I had the units of the PM wrong - Derck does not use the default. I have corrected this. tcheck; Adopted SED compared to Observations?; OK - FUSE and NUV match good... Target observed by PID 7437 using STIS echelle but peak-up failed. ACQ was done using offset. PID 16230 acquired target directly so used their coords and PMs. NGC-346-W-1 J2000 SpT=O4 If + O5-6; E(B-V)=0.06; U=11.20; B=12.21; V=12.43; F1160=1.600e-12; F1360=1.400e-12; F1700=9.700e-13; F2200=6.000e-13 1648678617109 /Users/lsmith/Box/ullyses_tech/ullyses_proposals/c29_mc/16805/OP-cache/ULLYSES_16805-v1S.xml The scheduling data was generated by CASM 30.1. CASM was run in Phase II mode. vstatus; 1S; NGC346-MPG-435; P/STIS approved for submission; P/LS 07/12/21 ; intrev: complete ; P/AF 15/03/22 vcheck; Enter targ name & Inst. & Resp. Sci.; NGC-346-MPG-435 'Cl* NGC 346 SSN 7' ; STIS ; LS vcheck; ETC numbers entered in APT?; Completed vcheck; Any screening violations?; None vcheck; S/N ETC calcs done & documented?; Y ...S/N = 14.8 (ETC number) and 18 in ETC S/N plot - may be lower than 20 at 1200 A vcheck; Field images checked & saved?; Yes NGC-346-MPG-435-ACSF555W.png, NGC-346-MPG-435-2MASS.png... GSC2 has no coverage in area of NGC 346 vcheck; Selected ACQ strategy?; STIS F28X50LP, 1 s vcheck; Possible ACQ or Sci spoilers?; No - brightest star at F220W (HRC)... See ACQ image in folder "ACQ images from.." for oec604yxq.png (ID 16230) vcheck; Field BOT clear?; Y... No GSC2 or GALEX availble. Target is brightest source in HRC F220W - see png HRC-F220W.png with 2".5 radius circle vcheck; Visual BOT check for stars not in catalog?; OK ...but see above vcheck; Orbit packing finalized?; 1 orbit vcheck; Buffer times optimized?; Done vcheck; Verify visit grouping correct; N/A vcheck; Is visit ready for int. review?; YES Allocated STIS orbits = 1 1659919706000 296.99604839966 (Tic-Visit :proposal-id 16805 :visit-id "1S" :proposal-version -1 :trans-version "20211222" :date "30-Mar-2022 18:16:56.0" :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 852816 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16805 :visit-id "1S" :obset-id "1S" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16805 :visit-id "1S" :orbit-number 1 :pcs-time 393 :si-vis-utilization 2595 :al-overhead-at-end 0 :internal-dur-at-end 578 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2989 :pcs-gap 0 ) true 1 0 rn(PoWR-OB-new(PoWR_40000_3.80_m6.79_Z0.14.fits, smc-ob-i 40-38, Z=0.140 solar, Teff=40000, log_lum=5.62, log_g=3.80, log_mdot=-6.79) (extinction smcbar=0.060), flux1360 +- 2.0A flux=1.4e-12 Flam); stis,fuvmama,e140m,c1425,0.2x0.2,mjd#59670 From file ULLYSES_Cycle29_MassiveStar_ProgramInput_v5.csv Spectral type: O4 If + O5-6 SED = NGC346-MPG-435_STIS_E140M_c1425_sed.fits For exptime=2619.3 s, spectral region: 1200.0 +- 0.5 A achieves SNR=20.0/resel global countrate (brightest segment): 8074.1 cts/s/segment brightest pixel: 0.100 cts/s/pix at 1243.5 A Calculation performed 2021-10-25T00:54:02, v0.9 *Note: max exposure time for 1 orbit is 2200 s. This gives a S/N of 14.8 at 1200 Ang and 18 on plot. 1661338577412 /Users/lsmith/Box/ullyses_tech/ullyses_proposals/c29_mc/16805/OP-cache/ULLYSES_16805-vAS.xml vstatus; AS; NGC346-MPG-435; P/STIS approved for submission; P/LS 07/12/21 ; intrev: complete ; P/AF 15/03/22 vcheck; Enter targ name & Inst. & Resp. Sci.; NGC-346-MPG-435 'Cl* NGC 346 SSN 7' ; STIS ; LS vcheck; ETC numbers entered in APT?; Completed vcheck; Any screening violations?; None vcheck; S/N ETC calcs done & documented?; Y ...S/N = 14.8 (ETC number) and 18 in ETC S/N plot - may be lower than 20 at 1200 A vcheck; Field images checked & saved?; Yes NGC-346-MPG-435-ACSF555W.png, NGC-346-MPG-435-2MASS.png... GSC2 has no coverage in area of NGC 346 vcheck; Selected ACQ strategy?; STIS F28X50LP, 1 s vcheck; Possible ACQ or Sci spoilers?; No - brightest star at F220W (HRC)... See ACQ image in folder "ACQ images from.." for oec604yxq.png (ID 16230) vcheck; Field BOT clear?; Y... No GSC2 or GALEX availble. Target is brightest source in HRC F220W - see png HRC-F220W.png with 2".5 radius circle vcheck; Visual BOT check for stars not in catalog?; OK ...but see above vcheck; Orbit packing finalized?; 1 orbit vcheck; Buffer times optimized?; Done vcheck; Verify visit grouping correct; N/A vcheck; Is visit ready for int. review?; YES Allocated STIS orbits = 1 (Tic-Visit :proposal-id 16805 :visit-id "AS" :proposal-version -1 :trans-version "20220516" :date "24-Aug-2022 11:56:16.0" :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 852816 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16805 :visit-id "AS" :obset-id "AS" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16805 :visit-id "AS" :orbit-number 1 :pcs-time 393 :si-vis-utilization 2595 :al-overhead-at-end 0 :internal-dur-at-end 578 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2989 :pcs-gap 0 ) true 1 0 rn(PoWR-OB-new(PoWR_40000_3.80_m6.79_Z0.14.fits, smc-ob-i 40-38, Z=0.140 solar, Teff=40000, log_lum=5.62, log_g=3.80, log_mdot=-6.79) (extinction smcbar=0.060), flux1360 +- 2.0A flux=1.4e-12 Flam); stis,fuvmama,e140m,c1425,0.2x0.2,mjd#59670 From file ULLYSES_Cycle29_MassiveStar_ProgramInput_v5.csv Spectral type: O4 If + O5-6 SED = NGC346-MPG-435_STIS_E140M_c1425_sed.fits For exptime=2619.3 s, spectral region: 1200.0 +- 0.5 A achieves SNR=20.0/resel global countrate (brightest segment): 8074.1 cts/s/segment brightest pixel: 0.100 cts/s/pix at 1243.5 A Calculation performed 2021-10-25T00:54:02, v0.9 *Note: max exposure time for 1 orbit is 2200 s. This gives a S/N of 14.8 at 1200 Ang and 18 on plot.