0 Assigned ID: 913 ----- Attempting Submission 1 (Fri Mar 06 23:08:59 GMT 2020) ----- FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. 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See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser FLASH level may be too high for this exposure or a long subexposure. See extended explanation in the diagnostic browser Thank you VERY much for your help, Amber and Sylvia. This version uses Jay Anderson's recommended 6 point dither with shorter exposures (to prevent saturation on the AGN PSF) and the 1k x 1k subarray to improve efficiency. We do sacrifice some total time-on-target to gain the added dither points, but I think this is a reasonable tradeoff. 1517919588 ----- Attempting Submission 1 (Tue Jun 30 20:24:58 GMT 2020) ----- HST Phase II Proposal 16173 successfully submitted. Receipt: # 16173-1 ----- Attempting Submission 2 (Fri Jul 03 12:19:11 GMT 2020) ----- HST Phase II Proposal 16173 successfully submitted. Receipt: # 16173-2 ----- Attempting Submission 3 (Fri Dec 04 22:50:52 GMT 2020) ----- Dr. Leitherer approved this change today (6/30/2020) Dear Dr. Tremblay, I approve adding these co-investigators to HST program 16173 who had inadvertently been omitted in the Phase 1 submission: Dr. Rebecca Nevin, Smithsonian Institution Astrophysical Observatory, rebecca.nevin@cfa.harvard.edu Dr. Christopher P. O’Dea, University of Manitoba, odeac@umanitoba.ca Dr. Ralph Kraft, Smithsonian Institution Astrophysical Observatory, rkraft@cfa.harvard.edu Dr. Alexey Vikhlinin, Smithsonian Institution Astrophysical Observatory, avikhlinin@cfa.harvard.edu Dr. Mojegan Azadi, Smithsonian Institution Astrophysical Observatory, mojegan.azadi@cfa.harvard.edu Prof. Vardha N. Bennert, Cal Poly Corporation, Sponsored Programs Department, vbennert@calpoly.edu Dr. Svetlana Starikova, Smithsonian Institution Astrophysical Observatory, svetlana.starikova@cfa.harvard.edu Thank you, Claus Leitherer The Close AGN Reference Survey (CARS; www.cars-survey.org) has assembled a rich, hyperdimensional dataset for 33 nearby Type 1 AGN, anchored by VLT/MUSE IFU datacubes for every target, along with pan-chromatic complementary datasets including ALMA for a large subset of the sample. We now propose an orders-of-magnitude increase in the spatial and temporal resolution of young stars and their ages (respectively) for the entire sample. The proposed WFC3/UVIS UV imaging will map sites of very recent star formation along multiphase quasar-driven outflows, instability-driven gas inflows, and merger-driven tidal interactions, testing whether each might lead to the suppression or even triggering of star formation. It is, therefore, a direct test of both negative and positive black hole feedback models. We have adopted the recommended WFC3/UVIS 6 point dither pattern (from Table 6 of Instrument Science Report WFC3 2020-07) to improve PSF sampling and mitigate against defects. Because the galaxies do not (nearly) fill the WFC3 FoV, and to reduce readout overhead as well as manage CTE, we have opted to use the 1k by 1k subarray. We also apply FLASH=20 to every ~110sec exposure (as recommended by WFC3 ISR 2020-08). Given that we cannot risk saturating any sub-exposure on the bright nuclear PSF, the 6-point dither allows for shorter exposures than we initially listed in our Phase 1 proposal (where we suggsted ~300 sec exposures). At each of the six POS-TARG dither points, we will observe for ~110-120 sec (each visit varies slightly to optimally pack the orbit) with both the F225W and F336W filters, for a total of ~660-720 seconds per filter, per target. Each orbit is efficient, with minimal detector-related overheads and less than ~6 seconds of unused visibiliy. Dr. Grant Tremblay is an Astrophysicist and Deputy Lead for the Lynx X-ray Observatory at the Center for Astrophysics | Harvard & Smithsonian. He was previously a NASA Einstein Fellow at Yale University, a European Southern Observatory (ESO) Fellow, and a Fellow Astronomer at ESO's Very Large Telescope in Chile. A major fraction of his PhD thesis work was done while he was a graduate student at the Space Telescope Science Institute. Dr. Tremblay has expertise in HST data reduction and analysis for WFPC2, ACS, WFC3, STIS, NICMOS, and COS (e.g., Tremblay et al. 2006; 2009; 2010; 2012a,b; 2015, 2018), including direct experience with the type of data we propose to obtain here. He is an author on more than 60 refereed publications in the scientific literature, many of which include data from HST. This program will be conducted in close and direct collaboration with the highly qualified members of the Close AGN Reference Survey (CARS; www.cars-survey.org), which is filled with a number of HST experts including Dr. Bernd Husemann, Dr. Tanya Urrutia. Dr. Timothy Davis, Drs. Meg Urry, Chris O'Dea, and Stefi Baum (all of whom were HST scientists at STScI for many years), as well as 12 other observational astrophysicists across the U.S., Europe, and Australia. Taken together, the expertise of all members of the CARS collaboration spans the wide breadth of galaxy evolution, AGN phenomenology, multiphase gas flows in galaxies, etc., including highly successful theorists (like Dr. Massimo Gaspari, Dr. Jason Dexter, etc.). The team has a demonstrated track record of rapid, high quality, and numerous publications. The proposed HST data will play a keystone role in a highly multiwavelength analysis, demonstrating the combined power of HST with, e.g., powerful ground-based facilities like ALMA and MUSE. Supermassive Black Holes and Active Galaxies Galaxies 6 false false true false false false false false SUPPORTED GALAXY SEYFERT Target parameters verified by G. Tremblay and the CARS Team. GALEX NUVmag 18.04922 J2000 J2000 GALEX NUVmag 18.04922 GALAXY SEYFERT Target parameters verified by G. Tremblay and the CARS Team GALEX NUVmag 19.18688 J2000 J2000 GALEX NUVmag 19.18688 GALAXY SEYFERT Target parameters verified by G. Tremblay and the CARS Team. GALEX NUVmag 16.3434 J2000 J2000 GALEX NUVmag 16.3434 GALAXY SEYFERT Target parameters verified by G. Tremblay and the CARS Team. GALEX NUVmag 17.75873 J2000 J2000 GALEX NUVmag 17.75873 GALAXY SEYFERT Target parameters verified by G. Tremblay and the CARS Team J2000 J2000 GALEX NUVmag 16.83709 GALAXY SEYFERT Target parameters verified by G. Tremblay and the CARS Team J2000 J2000 GALEX NUVmag 15.94877 GALAXY SEYFERT Target parameters verified by G. Tremblay and the CARS Team J2000 J2000 GALEX NUVm,ag 16.46274 GALAXY SEYFERT Target parameters verified by G. Tremblay and the CARS Team J2000 J2000 GALEX NUVmag 17.86037 GALAXY SEYFERT Target parameters verified by G. Tremblay and the CARS Team J2000 J2000 GALEX NUVmag 15.10552 GALAXY SEYFERT Target parameters verified by G. Tremblay and the CARS Team J2000 J2000 GALEX NUVmag 14.88734 GALAXY SEYFERT Target parameters verified by G. Tremblay and the CARS Team J2000 J2000 GALEX NUVmag 17.97991 GALAXY SEYFERT Target parameters verified by G. Tremblay and the CARS Team J2000 J2000 GALAXY SEYFERT Target parameters verified by G. Tremblay and the CARS Team J2000 J2000 GALAXY SEYFERT Target parameters verified by G. Tremblay and the CARS Team J2000 J2000 GALEX NUVmag 17.85951 GALAXY SEYFERT Target parameters verified by G. Tremblay and the CARS Team J2000 J2000 GALAXY SEYFERT Target parameters verified by G. Tremblay and the CARS Team J2000 J2000 GALEX NUVmag 15.87399 GALAXY SEYFERT Target parameters verified by G. Tremblay and the CARS Team J2000 J2000 GALAXY SEYFERT Target parameters verified by G. Tremblay and the CARS Team J2000 J2000 GALAXY SEYFERT Target parameters verified by G. Tremblay and the CARS Team J2000 J2000 GALEX NUVmag 16.96109 GALAXY SEYFERT Target parameters verified by G. Tremblay and the CARS Team J2000 J2000 GALEX NUVmag 15.82247 GALAXY SEYFERT Target parameters verified by G. Tremblay and the CARS Team J2000 J2000 GALAXY SEYFERT Target parameters verified by G. Tremblay and the CARS Team J2000 J2000 GALEX NUVmag 15.73376 GALAXY SEYFERT Target parameters verified by G. Tremblay and the CARS Team J2000 J2000 GALEX NUVmag 16.95734 GALAXY SEYFERT Target parameters verified by G. Tremblay and the CARS Team J2000 J2000 GALAXY SEYFERT Target parameters verified by G. Tremblay and the CARS Team J2000 J2000 GALAXY SEYFERT Target parameters verified by G. Tremblay and the CARS Team J2000 J2000 GALAXY SEYFERT Target parameters verified by G. Tremblay and the CARS Team J2000 J2000 GALAXY SEYFERT Target parameters verified by G. Tremblay and the CARS Team J2000 J2000 GALAXY SEYFERT Target parameters verified by G. Tremblay and the CARS Team J2000 J2000 GALAXY SEYFERT Target parameters verified by G. Tremblay and the CARS Team J2000 J2000 GALAXY SEYFERT Target parameters verified by G. Tremblay and the CARS Team J2000 J2000 GALAXY SEYFERT Target parameters verified by G. Tremblay and the CARS Team MRK1253 J2000 J2000 GALAXY SEYFERT Target parameters verified by G. Tremblay and the CARS Team J2000 J2000 WFC3/UVIS Imaging No No F225W WFC3/UVIS Imaging No No F336W WFC3/UVIS Imaging No No F225W WFC3/UVIS Imaging No No F336W WFC3/UVIS Imaging No No F225W WFC3/UVIS Imaging No No F336W WFC3/UVIS Imaging No No F225W WFC3/UVIS Imaging No No F336W WFC3/UVIS Imaging No No F225W WFC3/UVIS Imaging No No F336W WFC3/UVIS Imaging No No F225W WFC3/UVIS Imaging No No F336W WFC3/UVIS Imaging No No F225W WFC3/UVIS Imaging No No F336W WFC3/UVIS Imaging No No F225W WFC3/UVIS Imaging No No F336W WFC3/UVIS Imaging No No F225W WFC3/UVIS Imaging No No F336W WFC3/UVIS Imaging No No F225W WFC3/UVIS Imaging No No F336W WFC3/UVIS Imaging No No F225W WFC3/UVIS Imaging No No F336W WFC3/UVIS Imaging No No F225W WFC3/UVIS Imaging No No F336W WFC3/UVIS Imaging No No F225W WFC3/UVIS Imaging No No F336W WFC3/UVIS Imaging No No F225W WFC3/UVIS Imaging No No F336W WFC3/UVIS Imaging No No F225W WFC3/UVIS Imaging No No F336W WFC3/UVIS Imaging No No F225W WFC3/UVIS Imaging No No F336W WFC3/UVIS Imaging No No F225W WFC3/UVIS Imaging No No F336W WFC3/UVIS Imaging No No F225W WFC3/UVIS Imaging No No F336W WFC3/UVIS Imaging No No F225W WFC3/UVIS Imaging No No F336W WFC3/UVIS Imaging No No F225W WFC3/UVIS Imaging No No F336W WFC3/UVIS Imaging No No F225W WFC3/UVIS Imaging No No F336W WFC3/UVIS Imaging No No F225W WFC3/UVIS Imaging No No F336W WFC3/UVIS Imaging No No F225W WFC3/UVIS Imaging No No F336W WFC3/UVIS Imaging No No F225W WFC3/UVIS Imaging No No F336W WFC3/UVIS Imaging No No F225W WFC3/UVIS Imaging No No F336W WFC3/UVIS Imaging No No F225W WFC3/UVIS Imaging No No F336W WFC3/UVIS Imaging No No F225W WFC3/UVIS Imaging No No F336W WFC3/UVIS Imaging No No F225W WFC3/UVIS Imaging No No F336W WFC3/UVIS Imaging No No F225W WFC3/UVIS Imaging No No F336W WFC3/UVIS Imaging No No F225W WFC3/UVIS Imaging No No F336W WFC3/UVIS Imaging No No F225W WFC3/UVIS Imaging No No F336W WFC3/UVIS Imaging No No F225W WFC3/UVIS Imaging No No F336W WFC3/UVIS Imaging No No F225W WFC3/UVIS Imaging No No F336W 1607111970410 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. All visits in this program implent Jay Anderson's recommended WFC3/UVIS 6-point dither pattern as shown in Table 6 of Instrument Science Report WFC3 2020-07. 1626656393000 255.15957772687062 (Tic-Visit :proposal-id 16173 :visit-id "01" :proposal-version -1 :trans-version "20200619" :date "04-Dec-2020 14:59:30.0" :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 213904 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16173 :visit-id "01" :obset-id "01" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16173 :visit-id "01" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2767 :al-overhead-at-end 87 :internal-dur-at-end 270 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3156 :pcs-gap 0 ) true 1 0 1607112134524 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. All visits in this program implent Jay Anderson's recommended WFC3/UVIS 6-point dither pattern as shown in Table 6 of Instrument Science Report WFC3 2020-07. (Tic-Visit :proposal-id 16173 :visit-id "02" :proposal-version -1 :trans-version "20200619" :date "04-Dec-2020 15:02:14.0" :trans-errors '(:WARNINGS 1 :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 213904 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16173 :visit-id "02" :obset-id "02" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16173 :visit-id "02" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2767 :al-overhead-at-end 87 :internal-dur-at-end 270 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3149 :pcs-gap 0 ) false 1 1 1607112281323 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. All visits in this program implent Jay Anderson's recommended WFC3/UVIS 6-point dither pattern as shown in Table 6 of Instrument Science Report WFC3 2020-07. (Tic-Visit :proposal-id 16173 :visit-id "03" :proposal-version -1 :trans-version "20200619" :date "04-Dec-2020 15:04:41.0" :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 213904 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16173 :visit-id "03" :obset-id "03" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16173 :visit-id "03" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2899 :al-overhead-at-end 87 :internal-dur-at-end 270 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3285 :pcs-gap 0 ) true 1 0 1607112362584 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. All visits in this program implent Jay Anderson's recommended WFC3/UVIS 6-point dither pattern as shown in Table 6 of Instrument Science Report WFC3 2020-07. (Tic-Visit :proposal-id 16173 :visit-id "04" :proposal-version -1 :trans-version "20200619" :date "04-Dec-2020 15:06:02.0" :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 213904 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16173 :visit-id "04" :obset-id "04" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16173 :visit-id "04" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2755 :al-overhead-at-end 87 :internal-dur-at-end 270 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3142 :pcs-gap 0 ) true 1 0 1607112520597 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. All visits in this program implent Jay Anderson's recommended WFC3/UVIS 6-point dither pattern as shown in Table 6 of Instrument Science Report WFC3 2020-07. 1623300805000 239.0 (Tic-Visit :proposal-id 16173 :visit-id "05" :proposal-version -1 :trans-version "20200619" :date "04-Dec-2020 15:08:40.0" :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 213904 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16173 :visit-id "05" :obset-id "05" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16173 :visit-id "05" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2755 :al-overhead-at-end 87 :internal-dur-at-end 270 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3142 :pcs-gap 0 ) true 1 0 1607112572362 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. All visits in this program implent Jay Anderson's recommended WFC3/UVIS 6-point dither pattern as shown in Table 6 of Instrument Science Report WFC3 2020-07. 1627565847000 251.21498086401465 (Tic-Visit :proposal-id 16173 :visit-id "06" :proposal-version -1 :trans-version "20200619" :date "04-Dec-2020 15:09:32.0" :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 213904 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16173 :visit-id "06" :obset-id "06" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16173 :visit-id "06" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2755 :al-overhead-at-end 87 :internal-dur-at-end 270 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3142 :pcs-gap 0 ) true 1 0 1607112618224 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. All visits in this program implent Jay Anderson's recommended WFC3/UVIS 6-point dither pattern as shown in Table 6 of Instrument Science Report WFC3 2020-07. 1628322889000 253.31768958124354 (Tic-Visit :proposal-id 16173 :visit-id "07" :proposal-version -1 :trans-version "20200619" :date "04-Dec-2020 15:10:18.0" :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 213904 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16173 :visit-id "07" :obset-id "07" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16173 :visit-id "07" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2755 :al-overhead-at-end 87 :internal-dur-at-end 270 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3142 :pcs-gap 0 ) true 1 0 1607112721874 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. All visits in this program implent Jay Anderson's recommended WFC3/UVIS 6-point dither pattern as shown in Table 6 of Instrument Science Report WFC3 2020-07. 1629076482000 267.5 (Tic-Visit :proposal-id 16173 :visit-id "08" :proposal-version -1 :trans-version "20200619" :date "04-Dec-2020 15:12:01.0" :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 213904 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16173 :visit-id "08" :obset-id "08" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16173 :visit-id "08" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2779 :al-overhead-at-end 87 :internal-dur-at-end 270 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3165 :pcs-gap 0 ) true 1 0 1607117672104 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. All visits in this program implent Jay Anderson's recommended WFC3/UVIS 6-point dither pattern as shown in Table 6 of Instrument Science Report WFC3 2020-07. (Tic-Visit :proposal-id 16173 :visit-id "09" :proposal-version -1 :trans-version "20200619" :date "04-Dec-2020 16:34:32.0" :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 213904 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16173 :visit-id "09" :obset-id "09" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16173 :visit-id "09" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2755 :al-overhead-at-end 87 :internal-dur-at-end 270 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3145 :pcs-gap 0 ) true 1 0 1607112819432 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. All visits in this program implent Jay Anderson's recommended WFC3/UVIS 6-point dither pattern as shown in Table 6 of Instrument Science Report WFC3 2020-07. 1629647457000 251.8456211931325 (Tic-Visit :proposal-id 16173 :visit-id "10" :proposal-version -1 :trans-version "20200619" :date "04-Dec-2020 15:13:39.0" :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 213904 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16173 :visit-id "10" :obset-id "10" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16173 :visit-id "10" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2755 :al-overhead-at-end 87 :internal-dur-at-end 270 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3145 :pcs-gap 0 ) true 1 0 1607112910913 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. All visits in this program implent Jay Anderson's recommended WFC3/UVIS 6-point dither pattern as shown in Table 6 of Instrument Science Report WFC3 2020-07. (Tic-Visit :proposal-id 16173 :visit-id "11" :proposal-version -1 :trans-version "20200619" :date "04-Dec-2020 15:15:10.0" :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 213904 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16173 :visit-id "11" :obset-id "11" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16173 :visit-id "11" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2767 :al-overhead-at-end 87 :internal-dur-at-end 270 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3156 :pcs-gap 0 ) true 1 0 1607112968499 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. All visits in this program implent Jay Anderson's recommended WFC3/UVIS 6-point dither pattern as shown in Table 6 of Instrument Science Report WFC3 2020-07. 1627619115000 250.93469148010882 (Tic-Visit :proposal-id 16173 :visit-id "12" :proposal-version -1 :trans-version "20200619" :date "04-Dec-2020 15:16:08.0" :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 213904 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16173 :visit-id "12" :obset-id "12" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16173 :visit-id "12" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2755 :al-overhead-at-end 87 :internal-dur-at-end 270 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3142 :pcs-gap 0 ) true 1 0 1607113073688 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. All visits in this program implent Jay Anderson's recommended WFC3/UVIS 6-point dither pattern as shown in Table 6 of Instrument Science Report WFC3 2020-07. 1627864745000 252.23588567557096 (Tic-Visit :proposal-id 16173 :visit-id "13" :proposal-version -1 :trans-version "20200619" :date "04-Dec-2020 15:17:53.0" :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 213904 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16173 :visit-id "13" :obset-id "13" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16173 :visit-id "13" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2755 :al-overhead-at-end 87 :internal-dur-at-end 270 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3142 :pcs-gap 0 ) true 1 0 1607113183120 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. All visits in this program implent Jay Anderson's recommended WFC3/UVIS 6-point dither pattern as shown in Table 6 of Instrument Science Report WFC3 2020-07. 1629144635000 256.5 (Tic-Visit :proposal-id 16173 :visit-id "14" :proposal-version -1 :trans-version "20200619" :date "04-Dec-2020 15:19:43.0" :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 213904 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16173 :visit-id "14" :obset-id "14" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16173 :visit-id "14" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2755 :al-overhead-at-end 87 :internal-dur-at-end 270 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3145 :pcs-gap 0 ) true 1 0 1607113247343 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. All visits in this program implent Jay Anderson's recommended WFC3/UVIS 6-point dither pattern as shown in Table 6 of Instrument Science Report WFC3 2020-07. 1627796470000 247.0 (Tic-Visit :proposal-id 16173 :visit-id "15" :proposal-version -1 :trans-version "20200619" :date "04-Dec-2020 15:20:47.0" :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 213904 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16173 :visit-id "15" :obset-id "15" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16173 :visit-id "15" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2755 :al-overhead-at-end 87 :internal-dur-at-end 270 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3142 :pcs-gap 0 ) true 1 0 1607113351030 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. All visits in this program implent Jay Anderson's recommended WFC3/UVIS 6-point dither pattern as shown in Table 6 of Instrument Science Report WFC3 2020-07. 1628978866000 251.60000000000002 (Tic-Visit :proposal-id 16173 :visit-id "16" :proposal-version -1 :trans-version "20200619" :date "04-Dec-2020 15:22:30.0" :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 213904 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16173 :visit-id "16" :obset-id "16" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16173 :visit-id "16" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2755 :al-overhead-at-end 87 :internal-dur-at-end 270 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3149 :pcs-gap 0 ) true 1 0 1607113418056 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. All visits in this program implent Jay Anderson's recommended WFC3/UVIS 6-point dither pattern as shown in Table 6 of Instrument Science Report WFC3 2020-07. 1617748534000 98.0423451225638 (Tic-Visit :proposal-id 16173 :visit-id "17" :proposal-version -1 :trans-version "20200619" :date "04-Dec-2020 15:23:37.0" :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 213904 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16173 :visit-id "17" :obset-id "17" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16173 :visit-id "17" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2755 :al-overhead-at-end 87 :internal-dur-at-end 270 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3142 :pcs-gap 0 ) true 1 0 1607113512448 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. All visits in this program implent Jay Anderson's recommended WFC3/UVIS 6-point dither pattern as shown in Table 6 of Instrument Science Report WFC3 2020-07. 1617971719000 100.2387513832183 (Tic-Visit :proposal-id 16173 :visit-id "18" :proposal-version -1 :trans-version "20200619" :date "04-Dec-2020 15:25:12.0" :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 213904 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16173 :visit-id "18" :obset-id "18" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16173 :visit-id "18" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2755 :al-overhead-at-end 87 :internal-dur-at-end 270 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3142 :pcs-gap 0 ) true 1 0 1607113603756 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. All visits in this program implent Jay Anderson's recommended WFC3/UVIS 6-point dither pattern as shown in Table 6 of Instrument Science Report WFC3 2020-07. (Tic-Visit :proposal-id 16173 :visit-id "19" :proposal-version -1 :trans-version "20200619" :date "04-Dec-2020 15:26:43.0" :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 213904 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16173 :visit-id "19" :obset-id "19" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16173 :visit-id "19" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2767 :al-overhead-at-end 87 :internal-dur-at-end 270 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3156 :pcs-gap 0 ) true 1 0 1607113743700 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. All visits in this program implent Jay Anderson's recommended WFC3/UVIS 6-point dither pattern as shown in Table 6 of Instrument Science Report WFC3 2020-07. 1617812155000 91.5 (Tic-Visit :proposal-id 16173 :visit-id "20" :proposal-version -1 :trans-version "20200619" :date "04-Dec-2020 15:29:03.0" :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 213904 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16173 :visit-id "20" :obset-id "20" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16173 :visit-id "20" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2755 :al-overhead-at-end 87 :internal-dur-at-end 270 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3145 :pcs-gap 0 ) true 1 0 1607113947335 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. All visits in this program implent Jay Anderson's recommended WFC3/UVIS 6-point dither pattern as shown in Table 6 of Instrument Science Report WFC3 2020-07. 1619241677000 96.17684893922961 (Tic-Visit :proposal-id 16173 :visit-id "21" :proposal-version -1 :trans-version "20200619" :date "04-Dec-2020 15:32:27.0" :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 213904 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16173 :visit-id "21" :obset-id "21" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16173 :visit-id "21" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2779 :al-overhead-at-end 87 :internal-dur-at-end 270 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3165 :pcs-gap 0 ) true 1 0 1607114068543 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. All visits in this program implent Jay Anderson's recommended WFC3/UVIS 6-point dither pattern as shown in Table 6 of Instrument Science Report WFC3 2020-07. 1617983649000 77.5 (Tic-Visit :proposal-id 16173 :visit-id "22" :proposal-version -1 :trans-version "20200619" :date "04-Dec-2020 15:34:27.0" :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 213904 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16173 :visit-id "22" :obset-id "22" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16173 :visit-id "22" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2755 :al-overhead-at-end 87 :internal-dur-at-end 270 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3142 :pcs-gap 0 ) true 1 0 1607114132979 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. All visits in this program implent Jay Anderson's recommended WFC3/UVIS 6-point dither pattern as shown in Table 6 of Instrument Science Report WFC3 2020-07. 1618241067000 62.25467130444389 (Tic-Visit :proposal-id 16173 :visit-id "23" :proposal-version -1 :trans-version "20200619" :date "04-Dec-2020 15:35:32.0" :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 213904 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16173 :visit-id "23" :obset-id "23" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16173 :visit-id "23" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2755 :al-overhead-at-end 87 :internal-dur-at-end 270 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3149 :pcs-gap 0 ) true 1 0 1607114182378 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. All visits in this program implent Jay Anderson's recommended WFC3/UVIS 6-point dither pattern as shown in Table 6 of Instrument Science Report WFC3 2020-07. 1621438319000 95.34588869545468 (Tic-Visit :proposal-id 16173 :visit-id "24" :proposal-version -1 :trans-version "20200619" :date "04-Dec-2020 15:36:21.0" :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 213904 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16173 :visit-id "24" :obset-id "24" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16173 :visit-id "24" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2767 :al-overhead-at-end 87 :internal-dur-at-end 270 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3156 :pcs-gap 0 ) true 1 0 1607114246425 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. All visits in this program implent Jay Anderson's recommended WFC3/UVIS 6-point dither pattern as shown in Table 6 of Instrument Science Report WFC3 2020-07. 1621432740000 119.33591189380832 (Tic-Visit :proposal-id 16173 :visit-id "25" :proposal-version -1 :trans-version "20200619" :date "04-Dec-2020 15:37:26.0" :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 213904 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16173 :visit-id "25" :obset-id "25" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16173 :visit-id "25" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2755 :al-overhead-at-end 87 :internal-dur-at-end 270 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3145 :pcs-gap 0 ) true 1 0 1607114307303 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. All visits in this program implent Jay Anderson's recommended WFC3/UVIS 6-point dither pattern as shown in Table 6 of Instrument Science Report WFC3 2020-07. 1618078516000 258.93070247083625 (Tic-Visit :proposal-id 16173 :visit-id "26" :proposal-version -1 :trans-version "20200619" :date "04-Dec-2020 15:38:27.0" :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 213904 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16173 :visit-id "26" :obset-id "26" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16173 :visit-id "26" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2755 :al-overhead-at-end 87 :internal-dur-at-end 270 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3142 :pcs-gap 0 ) true 1 0 1607114354997 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. All visits in this program implent Jay Anderson's recommended WFC3/UVIS 6-point dither pattern as shown in Table 6 of Instrument Science Report WFC3 2020-07. 1618157842000 232.87070844305504 (Tic-Visit :proposal-id 16173 :visit-id "27" :proposal-version -1 :trans-version "20200619" :date "04-Dec-2020 15:39:14.0" :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 213904 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16173 :visit-id "27" :obset-id "27" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16173 :visit-id "27" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2815 :al-overhead-at-end 87 :internal-dur-at-end 270 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3200 :pcs-gap 0 ) true 1 0 1607114405948 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. All visits in this program implent Jay Anderson's recommended WFC3/UVIS 6-point dither pattern as shown in Table 6 of Instrument Science Report WFC3 2020-07. 1619278665000 254.34150917803584 (Tic-Visit :proposal-id 16173 :visit-id "28" :proposal-version -1 :trans-version "20200619" :date "04-Dec-2020 15:40:05.0" :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 213904 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16173 :visit-id "28" :obset-id "28" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16173 :visit-id "28" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2755 :al-overhead-at-end 87 :internal-dur-at-end 270 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3142 :pcs-gap 0 ) true 1 0 1607114482093 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. All visits in this program implent Jay Anderson's recommended WFC3/UVIS 6-point dither pattern as shown in Table 6 of Instrument Science Report WFC3 2020-07. 1622578362000 269.1 (Tic-Visit :proposal-id 16173 :visit-id "29" :proposal-version -1 :trans-version "20200619" :date "04-Dec-2020 15:41:22.0" :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 213904 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16173 :visit-id "29" :obset-id "29" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16173 :visit-id "29" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2755 :al-overhead-at-end 87 :internal-dur-at-end 270 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3142 :pcs-gap 0 ) true 1 0 1607114576275 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. All visits in this program implent Jay Anderson's recommended WFC3/UVIS 6-point dither pattern as shown in Table 6 of Instrument Science Report WFC3 2020-07. 1623505316000 264.60323617123686 (Tic-Visit :proposal-id 16173 :visit-id "30" :proposal-version -1 :trans-version "20200619" :date "04-Dec-2020 15:42:56.0" :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 213904 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16173 :visit-id "30" :obset-id "30" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16173 :visit-id "30" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2755 :al-overhead-at-end 87 :internal-dur-at-end 270 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3145 :pcs-gap 0 ) true 1 0 1607114624735 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. All visits in this program implent Jay Anderson's recommended WFC3/UVIS 6-point dither pattern as shown in Table 6 of Instrument Science Report WFC3 2020-07. 1618028993000 104.19999999999999 (Tic-Visit :proposal-id 16173 :visit-id "31" :proposal-version -1 :trans-version "20200619" :date "04-Dec-2020 15:43:44.0" :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 213904 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16173 :visit-id "31" :obset-id "31" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16173 :visit-id "31" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2755 :al-overhead-at-end 87 :internal-dur-at-end 270 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3142 :pcs-gap 0 ) true 1 0 1607114695859 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. All visits in this program implent Jay Anderson's recommended WFC3/UVIS 6-point dither pattern as shown in Table 6 of Instrument Science Report WFC3 2020-07. 1618057609000 98.10039881891629 (Tic-Visit :proposal-id 16173 :visit-id "32" :proposal-version -1 :trans-version "20200619" :date "04-Dec-2020 15:44:55.0" :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 213904 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16173 :visit-id "32" :obset-id "32" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16173 :visit-id "32" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2755 :al-overhead-at-end 87 :internal-dur-at-end 270 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3142 :pcs-gap 0 ) true 1 0 1607114756788 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. All visits in this program implent Jay Anderson's recommended WFC3/UVIS 6-point dither pattern as shown in Table 6 of Instrument Science Report WFC3 2020-07. 1619762728000 108.56679690684967 (Tic-Visit :proposal-id 16173 :visit-id "33" :proposal-version -1 :trans-version "20200619" :date "04-Dec-2020 15:45:56.0" :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 213904 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 16173 :visit-id "33" :obset-id "33" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 16173 :visit-id "33" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2755 :al-overhead-at-end 87 :internal-dur-at-end 270 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3149 :pcs-gap 0 ) true 1 0