0 Assigned ID: 4591 ----- Attempting Submission 1 (Wed May 24 20:21:41 GMT 2023) ----- HST Phase I Proposal 4591 successfully submitted. Receipt: # 4591-1 ----- Attempting Submission 2 (Wed May 24 20:33:49 GMT 2023) ----- HST Phase I Proposal 4591 successfully submitted. Receipt: # 4591-2 ----- Attempting Submission 3 (Wed May 24 20:34:22 GMT 2023) ----- HST Phase I Proposal 4591 successfully submitted. Receipt: # 4591-3 ----- Attempting Submission 4 (Wed May 24 20:50:11 GMT 2023) ----- Shifted Visit 13 to try and find second guide star. 1241111210 ----- Attempting Submission 1 (Thu Sep 14 15:10:41 GMT 2023) ----- ----- Attempting Submission 2 (Thu Jun 20 14:04:08 GMT 2024) ----- Your proposal could not be saved. Submission aborted. ----- Attempting Submission 3 (Fri Jun 21 14:38:14 GMT 2024) ----- Winging the SMC: 3D Structure of the Interstellar Medium in the Tidally Distrupted Wing of the SMC We propose to use resolved stellar populations to constrain the dynamical state of the interstellar medium (ISM) in star-forming regions N83/N84 of the Small Magellanic Cloud (SMC). Our proposal will use 15 orbits and 12 hours of HST and JWST time to cover a 12.5'x7.5' area of the SMC in 6 broad-band filters from near ultra-violet (NUV) to the near-infrared (NIR). By fitting the spectral energy distributions (SED) of resolved stars with broad wavelength coverage, we can simultaneously probe distance and line-of-sight extinction, enabling us to constrain distances to diffuse gas structures. The broadband SEDs will provide stellar and dust extinction physical parameters to complement existing observations of molecular gas (ALMA), ionized gas (Spitzer-IRS), and atomic hydrogen (GASKAP) in the region. With these results, we can map the 3D gas distribution in the region to see whether gas flows are colliding or diverging. These results will help us understand how tidal interactions between interacting galaxies are capable of fostering bursts of star formation. We aim to achieve the following objectives: (1) measure the definitive distance to the ISM in the SMC wing, providing vital model constraints for understanding the collision history between the SMC and LMC; (2) determine the relative distance between molecular clouds to gain insight into the dynamical state of the ISM in the region; (3) investigate the correlation between extinction and various phases of the ISM in low-metallicity environments. We will obtain high-resolution UV-optical imaging using HST/ACS for F475W and F814W, and WFC3/UVIS for F336W and F275W. To complete the coverage in the IR, we will obtain F115W and F160W imaging from JWST/NIRCam, which are comparable to HST WFC3 F110W and F160W. We design our pointings to cover a total area of 72 square arcmin. By using ACS and WFC3/UVIS in parallel, we can obtain NUV and optical imaging simultaneously. In a single orbit visit, ACS/WFC will obtain F475W and F814W data while WFC3/UVIS obtains F336W and F275W data in a parallel field. Effective exposure times are 720s in F275W, 700s in F336W, 679s in F475W, and 700s in F814W, including short guard exposures in F475W (5s) to avoid saturation of bright sources. Our dithering will include a half-pixel along the diagonal, allowing us to recover as much spatial resolution as possible. To efficiently image the 6x12 arcmin region with NIRCam, we use a mosaic of 1x6 tiles with 10% overlap. Each tile uses the FULLBOX dither type with 4TIGHT primary and subpixel dithers to provide approximately uniform depth covering the gaps between the two modules and the 4 short wavelength detectors. This results in at least 4 exposures over a large fraction of the mosaic, with some regions having more and a few regions with less exposures. For the detector setup, we use the BRIGHT2 readout pattern with NGROUPS=4. This results in an exposure time of 300s and using the JWST ETC this provides a S/N of over 50 in both F115W and F150W for a source that has 22 vegamag in WFC3/F160W. Setting this up in APT gives a total time of 12.09~hours after running smart accounting. While primary science is focused on the F115W and F150W filters, we simultaneously use the F330M and F300M filters in the long wavelength NIRCam channel to obtain measurements of the 3.3 micron emission. Since this proposal uses both ACS and WFC3 wavelength coverage and relies upon 180-degree flips, we expect that Reduced-Gyro Mode will increase our number of required orbits by 50% to achieve similar observations, according to the reduced-gyro mode presentations made to the Space Telescope Users Committee in May 2019. Team: Christina W. Lindberg, Claire Murray, Karl Gordon, Benjamin Williams, L. Cliff Johnson, Julia Roman-Duval, Karin Sandstrom, Karoline Gilbert, Martha Boyer, Caroline Bot, Joshua Peek, Kristen McQuinn, Petia Yanuchlova Merica-Jones, Christopher Clark, Alec Hirschauer, Roger Cohen, Steve Goldman, Yumi Choi, Elizabeth Tarantino, Catherine Zucker PI Lindberg has been a key contributor to the HST programs Scylla, a 500-orbit HST imaging program (PIDs 15891, 16235, 16786) in parallel with ULLYSES to survey dust in the Magellanic Clouds, and is experienced in conducting research with other resolved stellar population surveys such as the Panchromatic Hubble Andromeda Treasury. PI Lindberg will lead the observations, and oversee data reduction and analysis. The team includes experts on the gas (Murray, Roman-Duval), dust (Gordon, Sandstrom, Bot, Johnson, Hirschauer), ISM structure (Yanchulova Merica-Jones, Lindberg), and stellar populations (Gilbert, Williams, Boyer, Cohen, McQuinn) of galaxies in the Local Group. This includes science analysis (star formation histories, rare stellar types, star formation feedback, dust production and destruction) as well as technical execution of HST observations. Most of the team members are part of the Scylla survey, which will provide excellent comparison for this study. Further descriptions of expertise are listed below. Co-I Murray is an expert in the multiphase interstellar medium traced by radio spectral lines and resolved stellar populations. As the PI of Scylla, Murray has extensive experience with planning, executing and analyzing multi-wavelength resolved stellar photometry from HST. Co-I Williams is an expert in HST and JWST photometry, as well as resolved stellar populations and spectral energy distribution fitting. Williams has a full decade of experience with these tasks for virtually all multi-wavelength HST surveys of resolved stellar populations in the Local Group, including PHAT, PHATTER, SMIDGE, METAL and Scylla (PIDs 12581, 13659, 14675, 15891, 16235, 16786). Co-I L. Clifton Johnson is a stellar populations expert who is experienced in SED fitting of young stars in SMC star forming regions and is PI for the N83/N84 ALMA ACA program (ALMA-2018.1.01319.S) and a similar HST program targeting SMC molecular clouds (HST-GO-15912). Co-I Roman-Duval, is an expert in COS data reduction and interstellar medium research, particularly dust properties and interstellar depletions (Roman-Duval+2010, 2014, 2017). She is the PI of the METAL (GO-14675) and METAL-Z (GO-15880) large HST programs (Roman-Duval+2019, 2021, 2022a, b, Hamanowicz+2022) to obtain chemical abundances and depletions in nearby low-metallicity galaxies. Co-I Sandstrom is an expert on topics related to SMC, particularly on the abundance of polycyclic aromatic hydrocarbons. They are also a co-PI of NIRCam imaging for the Cycle 1 PHANGS Treasury, and led SMIDGE, which was similar multi-band HST imaging for the SW Bar. Co-I Gilbert is an expert in studying resolved stellar populations of galaxies in the Local Group and is co-PI of the LUVIT program (PI of GO-15275), which is using UV through NIR observations of resolved stars in galaxies in the Local Group and Local Volume to characterize and study the recent star formation, dust properties, and evolved stars of the most metal-poor star forming galaxies. Co-I Bot is an expert on the Small Magellanic Cloud, a galaxy on which she has worked since 2003, as well as on dust properties in galaxies. Co-I Yanchulova Merica-Jones has expertise in studying SMC dust extinction properties. Co-I Cohen is an expert on precision photometry of stellar populations in the Local Group, and has led multiple HST GO programs. Co-I Goldman is a BEAST developer, an expert in evolved stellar populations, SED-fitting of evolved stars, and the dusty evolved stellar population in the SMC. Co-I Choi is an expert in resolved stellar populations and stellar structures of the Magellanic Clouds. Co-I Tarantino is a postdoctoral fellow at the Space Telescope Science Institute studying the ISM properties of low metallicity dwarf galaxies. She is also an expert in CO observations in the Magellanic Clouds. Co-I Zucker is a Hubble Fellow at the Space Telescope Science Institute with expertise in 3D dust mapping, stellar modeling, star formation, the evolution of supernova remnants, and the structure and dynamics of the Milky Way. Stellar Populations and the Interstellar Medium Galaxies 6 false true false false false false false SUPPORTED EXT-MEDIUM HII REGION MOLECULAR CLOUD STAR FORMING REGION J2000 J2000 EXT-MEDIUM HII REGION MOLECULAR CLOUD STAR FORMING REGION J2000 J2000 EXT-MEDIUM HII REGION MOLECULAR CLOUD STAR FORMING REGION J2000 J2000 EXT-MEDIUM HII REGION MOLECULAR CLOUD STAR FORMING REGION J2000 J2000 EXT-MEDIUM HII REGION MOLECULAR CLOUD STAR FORMING REGION J2000 J2000 EXT-MEDIUM HII REGION MOLECULAR CLOUD STAR FORMING REGION J2000 J2000 EXT-MEDIUM HII REGION MOLECULAR CLOUD STAR FORMING REGION J2000 J2000 EXT-MEDIUM HII REGION MOLECULAR CLOUD STAR FORMING REGION J2000 J2000 EXT-MEDIUM HII REGION MOLECULAR CLOUD STAR FORMING REGION J2000 J2000 EXT-MEDIUM HII REGION MOLECULAR CLOUD STAR FORMING REGION J2000 J2000 EXT-MEDIUM HII REGION MOLECULAR CLOUD STAR FORMING REGION J2000 J2000 EXT-MEDIUM HII REGION MOLECULAR CLOUD STAR FORMING REGION J2000 J2000 EXT-MEDIUM HII REGION MOLECULAR CLOUD STAR FORMING REGION J2000 J2000 EXT-MEDIUM HII REGION MOLECULAR CLOUD STAR FORMING REGION J2000 J2000 EXT-MEDIUM HII REGION MOLECULAR CLOUD STAR FORMING REGION J2000 J2000 EXT-MEDIUM HII REGION MOLECULAR CLOUD STAR FORMING REGION J2000 J2000 EXT-MEDIUM HII REGION MOLECULAR CLOUD STAR FORMING REGION J2000 J2000 EXT-MEDIUM HII REGION MOLECULAR CLOUD STAR FORMING REGION J2000 J2000 EXT-MEDIUM HII REGION MOLECULAR CLOUD STAR FORMING REGION J2000 J2000 EXT-MEDIUM HII REGION MOLECULAR CLOUD STAR FORMING REGION J2000 J2000 EXT-MEDIUM HII REGION MOLECULAR CLOUD STAR FORMING REGION J2000 J2000 EXT-MEDIUM HII REGION MOLECULAR CLOUD STAR FORMING REGION J2000 J2000 EXT-MEDIUM HII REGION MOLECULAR CLOUD STAR FORMING REGION J2000 J2000 EXT-MEDIUM HII REGION MOLECULAR CLOUD STAR FORMING REGION J2000 J2000 EXT-MEDIUM HII REGION MOLECULAR CLOUD STAR FORMING REGION J2000 J2000 EXT-MEDIUM HII REGION MOLECULAR CLOUD STAR FORMING REGION J2000 J2000 EXT-MEDIUM HII REGION MOLECULAR CLOUD STAR FORMING REGION J2000 J2000 EXT-MEDIUM HII REGION MOLECULAR CLOUD STAR FORMING REGION J2000 J2000 EXT-MEDIUM HII REGION MOLECULAR CLOUD STAR FORMING REGION J2000 J2000 EXT-MEDIUM HII REGION MOLECULAR CLOUD STAR FORMING REGION J2000 J2000 ACS/WFC Imaging No No F475W ACS/WFC Imaging No No F814W WFC3/UVIS Imaging No No F275W WFC3/UVIS Imaging No No F336W ACS/WFC Imaging No No F475W ACS/WFC Imaging No No F814W WFC3/UVIS Imaging No No F275W WFC3/UVIS Imaging No No F336W ACS/WFC Imaging No No F475W ACS/WFC Imaging No No F814W WFC3/UVIS Imaging No No F275W WFC3/UVIS Imaging No No F336W ACS/WFC Imaging No No F475W ACS/WFC Imaging No No F814W WFC3/UVIS Imaging No No F275W WFC3/UVIS Imaging No No F336W ACS/WFC Imaging No No F475W ACS/WFC Imaging No No F814W WFC3/UVIS Imaging No No F275W WFC3/UVIS Imaging No No F336W ACS/WFC Imaging No No F475W ACS/WFC Imaging No No F814W WFC3/UVIS Imaging No No F275W WFC3/UVIS Imaging No No F336W ACS/WFC Imaging No No F475W ACS/WFC Imaging No No F814W WFC3/UVIS Imaging No No F275W WFC3/UVIS Imaging No No F336W ACS/WFC Imaging No No F475W ACS/WFC Imaging No No F814W WFC3/UVIS Imaging No No F275W WFC3/UVIS Imaging No No F336W ACS/WFC Imaging No No F475W ACS/WFC Imaging No No F814W WFC3/UVIS Imaging No No F275W WFC3/UVIS Imaging No No F336W ACS/WFC Imaging No No F475W ACS/WFC Imaging No No F814W WFC3/UVIS Imaging No No F275W WFC3/UVIS Imaging No No F336W ACS/WFC Imaging No No F475W ACS/WFC Imaging No No F814W WFC3/UVIS Imaging No No F275W WFC3/UVIS Imaging No No F336W ACS/WFC Imaging No No F475W ACS/WFC Imaging No No F814W WFC3/UVIS Imaging No No F275W WFC3/UVIS Imaging No No F336W ACS/WFC Imaging No No F475W ACS/WFC Imaging No No F814W WFC3/UVIS Imaging No No F275W WFC3/UVIS Imaging No No F336W ACS/WFC Imaging No No F475W ACS/WFC Imaging No No F814W WFC3/UVIS Imaging No No F275W WFC3/UVIS Imaging No No F336W ACS/WFC Imaging No No F475W ACS/WFC Imaging No No F814W WFC3/UVIS Imaging No No F275W WFC3/UVIS Imaging No No F336W The scheduling data was generated by CASM 32.1. CASM was run in Phase II mode. 1737400554000 100.0 (Tic-Visit :proposal-id 17509 :visit-id "01" :proposal-version -1 :trans-version "20240604" :date "21-Jun-2024 10:29:13.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 2291888 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 17509 :visit-id "01" :obset-id "01" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 17509 :visit-id "01" :orbit-number 1 :pcs-time 380 :si-vis-utilization 2582 :al-overhead-at-end 118 :internal-dur-at-end 1015 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2965 :pcs-gap 0 ) true 1 0 The scheduling data was generated by CASM 32.1. CASM was run in Phase II mode. 1737406200000 100.0 (Tic-Visit :proposal-id 17509 :visit-id "02" :proposal-version -1 :trans-version "20240604" :date "21-Jun-2024 10:29:14.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 2291888 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 17509 :visit-id "02" :obset-id "02" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 17509 :visit-id "02" :orbit-number 1 :pcs-time 380 :si-vis-utilization 2546 :al-overhead-at-end 125 :internal-dur-at-end 1015 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2965 :pcs-gap 0 ) true 1 0 The scheduling data was generated by CASM 32.1. CASM was run in Phase II mode. 1737411845000 100.0 (Tic-Visit :proposal-id 17509 :visit-id "03" :proposal-version -1 :trans-version "20240604" :date "21-Jun-2024 10:29:15.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 2291888 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 17509 :visit-id "03" :obset-id "03" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 17509 :visit-id "03" :orbit-number 1 :pcs-time 380 :si-vis-utilization 2546 :al-overhead-at-end 125 :internal-dur-at-end 1015 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2965 :pcs-gap 0 ) true 1 0 The scheduling data was generated by CASM 32.1. CASM was run in Phase II mode. 1719918164000 280.0 (Tic-Visit :proposal-id 17509 :visit-id "04" :proposal-version -1 :trans-version "20240604" :date "21-Jun-2024 10:29:16.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 2291888 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 17509 :visit-id "04" :obset-id "04" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 17509 :visit-id "04" :orbit-number 1 :pcs-time 380 :si-vis-utilization 2546 :al-overhead-at-end 125 :internal-dur-at-end 1015 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2965 :pcs-gap 0 ) true 1 0 The scheduling data was generated by CASM 32.1. CASM was run in Phase II mode. 1719963620000 280.0 (Tic-Visit :proposal-id 17509 :visit-id "05" :proposal-version -1 :trans-version "20240604" :date "21-Jun-2024 10:29:18.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 2291888 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 17509 :visit-id "05" :obset-id "05" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 17509 :visit-id "05" :orbit-number 1 :pcs-time 380 :si-vis-utilization 2546 :al-overhead-at-end 125 :internal-dur-at-end 1015 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2965 :pcs-gap 0 ) true 1 0 The scheduling data was generated by CASM 32.1. CASM was run in Phase II mode. 1737479789000 100.0 (Tic-Visit :proposal-id 17509 :visit-id "06" :proposal-version -1 :trans-version "20240604" :date "21-Jun-2024 10:29:19.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 2291888 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 17509 :visit-id "06" :obset-id "06" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 17509 :visit-id "06" :orbit-number 1 :pcs-time 380 :si-vis-utilization 2546 :al-overhead-at-end 125 :internal-dur-at-end 1015 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2965 :pcs-gap 0 ) true 1 0 The scheduling data was generated by CASM 32.1. CASM was run in Phase II mode. 1737485459000 100.0 (Tic-Visit :proposal-id 17509 :visit-id "07" :proposal-version -1 :trans-version "20240604" :date "21-Jun-2024 10:29:20.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 2291888 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 17509 :visit-id "07" :obset-id "07" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 17509 :visit-id "07" :orbit-number 1 :pcs-time 380 :si-vis-utilization 2546 :al-overhead-at-end 125 :internal-dur-at-end 1015 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2965 :pcs-gap 0 ) true 1 0 The scheduling data was generated by CASM 32.1. CASM was run in Phase II mode. 1737491129000 100.0 (Tic-Visit :proposal-id 17509 :visit-id "08" :proposal-version -1 :trans-version "20240604" :date "21-Jun-2024 10:29:21.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 2291888 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 17509 :visit-id "08" :obset-id "08" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 17509 :visit-id "08" :orbit-number 1 :pcs-time 380 :si-vis-utilization 2546 :al-overhead-at-end 125 :internal-dur-at-end 1015 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2965 :pcs-gap 0 ) true 1 0 The scheduling data was generated by CASM 32.1. CASM was run in Phase II mode. 1719992035000 280.0 (Tic-Visit :proposal-id 17509 :visit-id "09" :proposal-version -1 :trans-version "20240604" :date "21-Jun-2024 10:29:23.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 2291888 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 17509 :visit-id "09" :obset-id "09" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 17509 :visit-id "09" :orbit-number 1 :pcs-time 380 :si-vis-utilization 2546 :al-overhead-at-end 125 :internal-dur-at-end 1015 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2965 :pcs-gap 0 ) true 1 0 The scheduling data was generated by CASM 32.1. CASM was run in Phase II mode. 1720122656000 280.0 (Tic-Visit :proposal-id 17509 :visit-id "10" :proposal-version -1 :trans-version "20240604" :date "21-Jun-2024 10:29:24.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 2291888 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 17509 :visit-id "10" :obset-id "10" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 17509 :visit-id "10" :orbit-number 1 :pcs-time 380 :si-vis-utilization 2546 :al-overhead-at-end 125 :internal-dur-at-end 1015 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2965 :pcs-gap 0 ) true 1 0 The scheduling data was generated by CASM 32.1. CASM was run in Phase II mode. 1737496800000 100.0 (Tic-Visit :proposal-id 17509 :visit-id "11" :proposal-version -1 :trans-version "20240604" :date "21-Jun-2024 10:29:25.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 2291888 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 17509 :visit-id "11" :obset-id "11" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 17509 :visit-id "11" :orbit-number 1 :pcs-time 380 :si-vis-utilization 2546 :al-overhead-at-end 125 :internal-dur-at-end 1015 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2965 :pcs-gap 0 ) true 1 0 The scheduling data was generated by CASM 32.1. CASM was run in Phase II mode. 1737502470000 100.0 (Tic-Visit :proposal-id 17509 :visit-id "12" :proposal-version -1 :trans-version "20240604" :date "21-Jun-2024 10:29:26.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 2291888 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 17509 :visit-id "12" :obset-id "12" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 17509 :visit-id "12" :orbit-number 1 :pcs-time 380 :si-vis-utilization 2546 :al-overhead-at-end 125 :internal-dur-at-end 1015 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2965 :pcs-gap 0 ) true 1 0 The scheduling data was generated by CASM 32.1. CASM was run in Phase II mode. 1737508140000 100.0 (Tic-Visit :proposal-id 17509 :visit-id "13" :proposal-version -1 :trans-version "20240604" :date "21-Jun-2024 10:29:27.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 2291888 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 17509 :visit-id "13" :obset-id "13" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 17509 :visit-id "13" :orbit-number 1 :pcs-time 380 :si-vis-utilization 2546 :al-overhead-at-end 125 :internal-dur-at-end 1015 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2965 :pcs-gap 0 ) true 1 0 The scheduling data was generated by CASM 33.0. CASM was run in Phase II mode. /System/Volumes/Data/solaris/user1/royle/OP-cache/17509-v63.xml This visit will repeat visit 13 which failed. 1769145969000 100.0 (Tic-Visit :proposal-id 17509 :visit-id "63" :proposal-version -1 :trans-version "20241217" :date "18-Feb-2025 11:22:34.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 2291888 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 17509 :visit-id "63" :obset-id "63" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 17509 :visit-id "63" :orbit-number 1 :pcs-time 380 :si-vis-utilization 2546 :al-overhead-at-end 125 :internal-dur-at-end 1015 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2965 :pcs-gap 0 ) true 1 0 The scheduling data was generated by CASM 34.0. CASM was run in Phase II mode. /System/Volumes/Data/solaris/user1/royle/OP-cache/17509-vA3.xml This visit will repeat visit 63 which failed. (Tic-Visit :proposal-id 17509 :visit-id "A3" :proposal-version -1 :trans-version "20250929" :date "11-Feb-2026 15:14:32.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 1154976 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 17509 :visit-id "A3" :obset-id "A3" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 17509 :visit-id "A3" :orbit-number 1 :pcs-time 380 :si-vis-utilization 2500 :al-overhead-at-end 126 :internal-dur-at-end 668 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2907 :pcs-gap 0 ) true 1 0 The scheduling data was generated by CASM 32.1. CASM was run in Phase II mode. 1720338420000 280.0 (Tic-Visit :proposal-id 17509 :visit-id "14" :proposal-version -1 :trans-version "20240604" :date "21-Jun-2024 10:29:28.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 2291888 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 17509 :visit-id "14" :obset-id "14" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 17509 :visit-id "14" :orbit-number 1 :pcs-time 380 :si-vis-utilization 2546 :al-overhead-at-end 125 :internal-dur-at-end 1015 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2965 :pcs-gap 0 ) true 1 0 The scheduling data was generated by CASM 32.1. CASM was run in Phase II mode. 1720389575000 280.0 (Tic-Visit :proposal-id 17509 :visit-id "15" :proposal-version -1 :trans-version "20240604" :date "21-Jun-2024 10:29:30.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 2291888 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 17509 :visit-id "15" :obset-id "15" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 17509 :visit-id "15" :orbit-number 1 :pcs-time 380 :si-vis-utilization 2546 :al-overhead-at-end 125 :internal-dur-at-end 1015 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 2965 :pcs-gap 0 ) true 1 0