0 Assigned ID: 149 ----- Attempting Submission 1 (Wed Apr 03 20:05:32 GMT 2019) ----- HST Phase I Proposal 149 (Cstars.apt) successfully submitted. Receipt: # 149-1 ----- Attempting Submission 2 (Fri Apr 05 15:46:54 GMT 2019) ----- ORBITAL VISIBILITY OVERRUN ORBITAL VISIBILITY OVERRUN ORBITAL VISIBILITY OVERRUN ORBITAL VISIBILITY OVERRUN ORBITAL VISIBILITY OVERRUN ORBITAL VISIBILITY OVERRUN ORBITAL VISIBILITY OVERRUN ORBITAL VISIBILITY OVERRUN ORBITAL VISIBILITY OVERRUN ORBITAL VISIBILITY OVERRUN ORBITAL VISIBILITY OVERRUN ORBITAL VISIBILITY OVERRUN ORBITAL VISIBILITY OVERRUN ORBITAL VISIBILITY OVERRUN ORBITAL VISIBILITY OVERRUN ORBITAL VISIBILITY OVERRUN ORBITAL VISIBILITY OVERRUN ORBITAL VISIBILITY OVERRUN ORBITAL VISIBILITY OVERRUN ORBITAL VISIBILITY OVERRUN ORBITAL VISIBILITY OVERRUN ORBITAL VISIBILITY OVERRUN ORBITAL VISIBILITY OVERRUN ORBITAL VISIBILITY OVERRUN ORBITAL VISIBILITY OVERRUN ORBITAL VISIBILITY OVERRUN ORBITAL VISIBILITY OVERRUN ORBITAL VISIBILITY OVERRUN ORBITAL VISIBILITY OVERRUN ORBITAL VISIBILITY OVERRUN ORBITAL VISIBILITY OVERRUN ORBITAL VISIBILITY OVERRUN ORBITAL VISIBILITY OVERRUN ORBITAL VISIBILITY OVERRUN ORBITAL VISIBILITY OVERRUN ORBITAL VISIBILITY OVERRUN ORBITAL VISIBILITY OVERRUN We had to make a slight adjustment to the position of target M33-07 to make sure that it falls within the PHAT coverage no matter what the orientation ends up being. It's only a slight shift in coordinates -- we don't need an exact location, we just need a star field. 7/24/2019: removing orient restrictions 10/17/2019: fixed typo in M33-01 target coordinates. 11/3/2020: Submitting re-observations of failed visits. 1153741827 ----- Attempting Submission 1 (Fri Jul 12 22:43:56 GMT 2019) ----- ----- Attempting Submission 2 (Thu Jul 25 00:42:20 GMT 2019) ----- ----- Attempting Submission 3 (Thu Oct 17 17:08:46 GMT 2019) ----- ----- Attempting Submission 4 (Tue Nov 03 19:58:24 GMT 2020) ----- I think warnings are on the change in the orbit length. PC says it's fine. Theoretical models of Asymptotic Giant Branch (AGB) evolution rely on calibrating observations of the ratio of carbon-rich (C) to oxygen-rich (M) stars and the C star luminosity function (CSLF). Sensitivity and resolution limits previously restricted C/M and CSLF measurements to nearby metal-poor galaxies that are not applicable to metal-rich AGB stars that dominate the near-IR light of massive galaxies. Fortunately, recent studies show that the WFC3/IR medium-band filters can be used to isolate C and M stars out to >5 Mpc. A Cycle 23 program used this technique in M31 to provide the first constraints to metal-rich AGB star models. Those results show an unexpected sharp drop in C/M in M31 that is presumably caused by the high metallicity. To constrain the physical properties that cause this dramatic change in behavior, we propose to image fields in M31 and M33 to target C stars in the metallicity gap between the LMC and M31, where this shift in the C/M slope is expected to appear. Our measurement of C/M will leverage M31/M33's metallicity distributions to also determine the metallicity limit above which C stars cannot form. In addition, our precise measurement of the CSLF will calibrate the efficiency of the 3rd dredge up and the minimum core mass to form a C star, both of which depend strongly on metallicity. The interpretation of these observations is straightforward owing to the ability to leverage data products from the Panchromatic Andromeda/Triangulum Treasury (PHAT) programs. As a result, we can conclusively evaluate AGB evolution models in the metal-rich regime - critical for application of stellar models to the massive galaxies that dominate redshift surveys. Required primary exposure times and photometric depth: In order to detect all AGB stars, we must achieve full photometric completeness at the tip of the red giant branch (TRGB). We can achieve the necessary photometric depth within a single orbit (as demonstrated in GO-14072). After accounting for overheads, this allows for total exposure times of about 800-850 s in each filter, resulting in S/N > 7.3 in F139M (optimal S/N > 9.2) for m_F160W = 23 mag, using a Bruzual template for an K0III star. The S/N is even better in the F127M and F153M filters, owing to a higher throughput. For reference, the TRGB in the F160W filter corresponds to ~19 mag at the distance of M31. For the parallels, we maximize the exposure time in F658N, while also preserving image quality and avoiding buffer dump latency. The remainging available parallel time is filled with F625W for continuum subtraction. Dithering Strategy for primaries: Dithering diminishes errors associated with where a source is placed on a pixel, undersampling of the WFC3/IR channel, and image artifacts such as cosmic rays. We choose a 4-pt dither pattern to acheive Nyquist sampling of the PSF in F127M. The remaining 2 filters will use a 2-pt dither: we will reduce F127M simultaneously to acheive Nyquist sampling for the 2-pt dithers (e.g., PHAT; Dalcanton et al. 2012). We choose this strategy to allow for ACS buffer dumps in parallel. The dither patterns are entered manually in the position offsets, following the WFC3-IR-DITHER-BOX-MIN pattern values listed in the WFC3 handbook in Table C.3. For the parallels, each filter is imaged in two of the dither positions. The PHAT data is Nyquist sampled in F814W, and we will re-reduce that data simultaneously to achieve Nyquist sampling in F625W and F658N. Parallels: We are observing with ACS in parallel for the 7 M33 observations. Our team includes members of multiple Treasury, large GO, and Archival programs of resolved stellar populations in the Local Group and Volume (e.g., PHAT, ANGST, ANGRRR, ANGST-SNAP, GHOSTS). We have observed, reduced, analyzed, and disseminated > 1500 orbits of HST imaging, resulting in publicly released photometry in excess of 100 million stars. All necessary software, analysis, and data dissemination tools are in place and tested, maximizing the efficiency of our scientific program while minimizing the time needed to release high level data products. Our team also includes key members of the Padova modeling group - experts in evolve star evolution. This team obtained similar observations in Cycle 23 (PI Boyer), which produced the surprising results described in the proposal. The current proposal is a follow-up program. Boyer and Williams will lead the data processing. Photometry, images, and SED fits will be released via a database interface developed for PHAT. TP-AGB science will be coordinated by Boyer, including a description of the observation results and modeling efforts. The Padova group (Marigo, Girardi, Chen, Aringer, Pastorelli) will drive the modeling effort. Emission line star science using the parallel fields will be led by Dalcanton, who is leading similar efforts in our Cycle 23 program. Stellar Populations Stellar Physics 6 false false false false false false false SUPPORTED GALAXY DISK SPIRAL This is a star field, with a wide range of V-mags. The brightest star in the optical HST images of M31 from the Panchromatic Hubble Andromeda Treasury (PHAT) is about F475W=18 mag. The stars of interest to this program range from approximately F814W=18-23 mag. J2000 J2000 GALAXY DISK SPIRAL This is a star field, with a wide range of V-mags. The brightest star in the optical HST images of M31 from the Panchromatic Hubble Andromeda Treasury (PHAT) is about F475W=18 mag. The stars of interest to this program range from approximately F814W=18-23 mag. J2000 J2000 GALAXY DISK SPIRAL This is a star field, with a wide range of V-mags. The brightest star in the optical HST images of M31 from the Panchromatic Hubble Andromeda Treasury (PHAT) is about F475W=18 mag. The stars of interest to this program range from approximately F814W=18-23 mag. J2000 J2000 GALAXY DISK SPIRAL This is a star field, with a wide range of V-mags. The brightest star in the optical HST images of M31 from the Panchromatic Hubble Andromeda Treasury (PHAT) is about F475W=18 mag. The stars of interest to this program range from approximately F814W=18-23 mag. J2000 J2000 GALAXY DISK SPIRAL This is a star field, with a wide range of V-mags. The brightest star in the optical HST images of M31 from the Panchromatic Hubble Andromeda Treasury (PHAT) is about F475W=18 mag. The stars of interest to this program range from approximately F814W=18-23 mag. J2000 J2000 GALAXY DISK SPIRAL This is a star field, with a wide range of V-mags. The brightest star in the optical HST images of M31 from the Panchromatic Hubble Andromeda Treasury (PHAT) is about F475W=18 mag. The stars of interest to this program range from approximately F814W=18-23 mag. J2000 J2000 GALAXY DISK SPIRAL This is a star field, with a wide range of V-mags. The brightest star in the optical HST images of M31 from the Panchromatic Hubble Andromeda Treasury (PHAT) is about F475W=18 mag. The stars of interest to this program range from approximately F814W=18-23 mag. J2000 J2000 GALAXY DISK SPIRAL This is a star field, with a wide range of V-mags. The brightest star in the optical HST images of M31 from the Panchromatic Hubble Andromeda Treasury (PHAT) is about F475W=18 mag. The stars of interest to this program range from approximately F814W=18-23 mag. J2000 J2000 GALAXY DISK SPIRAL This is a star field, with a wide range of V-mags. The brightest star in the optical HST images of M31 from the Panchromatic Hubble Andromeda Treasury (PHAT) is about F475W=18 mag. The stars of interest to this program range from approximately F814W=18-23 mag. J2000 J2000 GALAXY DISK SPIRAL This is a star field, with a wide range of V-mags. The brightest star in the optical HST images of M31 from the Panchromatic Hubble Andromeda Treasury (PHAT) is about F475W=18 mag. The stars of interest to this program range from approximately F814W=18-23 mag. J2000 J2000 GALAXY DISK SPIRAL This is a star field, with a wide range of V-mags. The brightest star in the optical HST images of M31 from the Panchromatic Hubble Andromeda Treasury (PHAT) is about F475W=18 mag. The stars of interest to this program range from approximately F814W=18-23 mag. J2000 J2000 GALAXY BULGE SPIRAL This is a star field, with a wide range of V-mags. The brightest star in the optical HST images of M31 from the Panchromatic Hubble Andromeda Treasury (PHAT) is about F475W=18 mag. The stars of interest to this program range from approximately F814W=18-23 mag. J2000 J2000 GALAXY BULGE SPIRAL This is a star field, with a wide range of V-mags. The brightest star in the optical HST images of M31 from the Panchromatic Hubble Andromeda Treasury (PHAT) is about F475W=18 mag. The stars of interest to this program range from approximately F814W=18-23 mag. J2000 J2000 GALAXY BULGE SPIRAL This is a star field, with a wide range of V-mags. The brightest star in the optical HST images of M31 from the Panchromatic Hubble Andromeda Treasury (PHAT) is about F475W=18 mag. The stars of interest to this program range from approximately F814W=18-23 mag. J2000 J2000 GALAXY BULGE SPIRAL This is a star field, with a wide range of V-mags. The brightest star in the optical HST images of M31 from the Panchromatic Hubble Andromeda Treasury (PHAT) is about F475W=18 mag. The stars of interest to this program range from approximately F814W=18-23 mag. J2000 J2000 GALAXY BULGE SPIRAL This is a star field, with a wide range of V-mags. The brightest star in the optical HST images of M31 from the Panchromatic Hubble Andromeda Treasury (PHAT) is about F475W=18 mag. The stars of interest to this program range from approximately F814W=18-23 mag. J2000 J2000 GALAXY BULGE SPIRAL This is a star field, with a wide range of V-mags. The brightest star in the optical HST images of M31 from the Panchromatic Hubble Andromeda Treasury (PHAT) is about F475W=18 mag. The stars of interest to this program range from approximately F814W=18-23 mag. J2000 J2000 GALAXY BULGE SPIRAL This is a star field, with a wide range of V-mags. The brightest star in the optical HST images of M31 from the Panchromatic Hubble Andromeda Treasury (PHAT) is about F475W=18 mag. The stars of interest to this program range from approximately F814W=18-23 mag. J2000 J2000 GALAXY BULGE SPIRAL This is a star field, with a wide range of V-mags. The brightest star in the optical HST images of M31 from the Panchromatic Hubble Andromeda Treasury (PHAT) is about F475W=18 mag. The stars of interest to this program range from approximately F814W=18-23 mag. J2000 J2000 GALAXY BULGE SPIRAL This is a star field, with a wide range of V-mags. The brightest star in the optical HST images of M31 from the Panchromatic Hubble Andromeda Treasury (PHAT) is about F475W=18 mag. The stars of interest to this program range from approximately F814W=18-23 mag. J2000 J2000 GALAXY BULGE SPIRAL This is a star field, with a wide range of V-mags. The brightest star in the optical HST images of M31 from the Panchromatic Hubble Andromeda Treasury (PHAT) is about F475W=18 mag. The stars of interest to this program range from approximately F814W=18-23 mag. J2000 J2000 GALAXY BULGE SPIRAL This is a star field, with a wide range of V-mags. The brightest star in the optical HST images of M31 from the Panchromatic Hubble Andromeda Treasury (PHAT) is about F475W=18 mag. The stars of interest to this program range from approximately F814W=18-23 mag. J2000 J2000 GALAXY BULGE SPIRAL This is a star field, with a wide range of V-mags. The brightest star in the optical HST images of M31 from the Panchromatic Hubble Andromeda Treasury (PHAT) is about F475W=18 mag. The stars of interest to this program range from approximately F814W=18-23 mag. J2000 J2000 GALAXY BULGE SPIRAL This is a star field, with a wide range of V-mags. The brightest star in the optical HST images of M31 from the Panchromatic Hubble Andromeda Treasury (PHAT) is about F475W=18 mag. The stars of interest to this program range from approximately F814W=18-23 mag. J2000 J2000 GALAXY BULGE SPIRAL This is a star field, with a wide range of V-mags. The brightest star in the optical HST images of M31 from the Panchromatic Hubble Andromeda Treasury (PHAT) is about F475W=18 mag. The stars of interest to this program range from approximately F814W=18-23 mag. J2000 J2000 GALAXY BULGE SPIRAL This is a star field, with a wide range of V-mags. The brightest star in the optical HST images of M31 from the Panchromatic Hubble Andromeda Treasury (PHAT) is about F475W=18 mag. The stars of interest to this program range from approximately F814W=18-23 mag. J2000 J2000 GALAXY SPIRAL This is a star field, with a wide range of V-mags. The brightest star in the optical HST images of M33 from the Panchromatic Hubble Andromeda Treasury (PHAT) is about F475W=18 mag. The stars of interest to this program range from approximately F814W=18-23 mag. J2000 J2000 GALAXY SPIRAL This is a star field, with a wide range of V-mags. The brightest star in the optical HST images of M33 from the Panchromatic Hubble Andromeda Treasury (PHAT) is about F475W=18 mag. The stars of interest to this program range from approximately F814W=18-23 mag. J2000 J2000 GALAXY SPIRAL This is a star field, with a wide range of V-mags. The brightest star in the optical HST images of M33 from the Panchromatic Hubble Andromeda Treasury (PHAT) is about F475W=18 mag. The stars of interest to this program range from approximately F814W=18-23 mag. J2000 J2000 GALAXY SPIRAL This is a star field, with a wide range of V-mags. The brightest star in the optical HST images of M33 from the Panchromatic Hubble Andromeda Treasury (PHAT) is about F475W=18 mag. The stars of interest to this program range from approximately F814W=18-23 mag. J2000 J2000 GALAXY SPIRAL This is a star field, with a wide range of V-mags. The brightest star in the optical HST images of M33 from the Panchromatic Hubble Andromeda Treasury (PHAT) is about F475W=18 mag. The stars of interest to this program range from approximately F814W=18-23 mag. J2000 J2000 GALAXY SPIRAL This is a star field, with a wide range of V-mags. The brightest star in the optical HST images of M33 from the Panchromatic Hubble Andromeda Treasury (PHAT) is about F475W=18 mag. The stars of interest to this program range from approximately F814W=18-23 mag. J2000 J2000 GALAXY SPIRAL This is a star field, with a wide range of V-mags. The brightest star in the optical HST images of M33 from the Panchromatic Hubble Andromeda Treasury (PHAT) is about F475W=18 mag. The stars of interest to this program range from approximately F814W=18-23 mag. J2000 J2000 WFC3/IR Imaging No No F127M WFC3/IR Imaging No No F139M WFC3/IR Imaging No No F153M WFC3/IR Imaging No No F127M WFC3/IR Imaging No No F139M WFC3/IR Imaging No No F153M WFC3/IR Imaging No No F127M WFC3/IR Imaging No No F139M WFC3/IR Imaging No No F153M WFC3/IR Imaging No No F127M WFC3/IR Imaging No No F139M WFC3/IR Imaging No No F153M WFC3/IR Imaging No No F127M WFC3/IR Imaging No No F139M WFC3/IR Imaging No No F153M WFC3/IR Imaging No No F127M WFC3/IR Imaging No No F139M WFC3/IR Imaging No No F153M WFC3/IR Imaging No No F127M WFC3/IR Imaging No No F139M WFC3/IR Imaging No No F153M WFC3/IR Imaging No No F127M WFC3/IR Imaging No No F139M WFC3/IR Imaging No No F153M WFC3/IR Imaging No No F127M WFC3/IR Imaging No No F139M WFC3/IR Imaging No No F153M WFC3/IR Imaging No No F127M WFC3/IR Imaging No No F139M WFC3/IR Imaging No No F153M WFC3/IR Imaging No No F127M WFC3/IR Imaging No No F139M WFC3/IR Imaging No No F153M WFC3/IR Imaging No No F127M WFC3/IR Imaging No No F139M WFC3/IR Imaging No No F153M WFC3/IR Imaging No No F127M WFC3/IR Imaging No No F139M WFC3/IR Imaging No No F153M WFC3/IR Imaging No No F127M WFC3/IR Imaging No No F139M WFC3/IR Imaging No No F153M WFC3/IR Imaging No No F127M WFC3/IR Imaging No No F139M WFC3/IR Imaging No No F153M WFC3/IR Imaging No No F127M WFC3/IR Imaging No No F139M WFC3/IR Imaging No No F153M WFC3/IR Imaging No No F127M WFC3/IR Imaging No No F139M WFC3/IR Imaging No No F153M WFC3/IR Imaging No No F127M WFC3/IR Imaging No No F139M WFC3/IR Imaging No No F153M WFC3/IR Imaging No No F127M WFC3/IR Imaging No No F139M WFC3/IR Imaging No No F153M WFC3/IR Imaging No No F127M WFC3/IR Imaging No No F139M WFC3/IR Imaging No No F153M WFC3/IR Imaging No No F127M WFC3/IR Imaging No No F139M WFC3/IR Imaging No No F153M WFC3/IR Imaging No No F127M WFC3/IR Imaging No No F139M WFC3/IR Imaging No No F153M WFC3/IR Imaging No No F127M WFC3/IR Imaging No No F139M WFC3/IR Imaging No No F153M WFC3/IR Imaging No No F127M WFC3/IR Imaging No No F139M WFC3/IR Imaging No No F153M WFC3/IR Imaging No No F127M WFC3/IR Imaging No No F139M WFC3/IR Imaging No No F153M WFC3/IR Imaging No No F127M WFC3/IR Imaging No No F139M WFC3/IR Imaging No No F153M WFC3/IR Imaging No No F127M WFC3/IR Imaging No No F139M WFC3/IR Imaging No No F153M WFC3/IR Imaging No No F127M WFC3/IR Imaging No No F139M WFC3/IR Imaging No No F153M WFC3/IR Imaging No No F127M WFC3/IR Imaging No No F139M WFC3/IR Imaging No No F153M WFC3/IR Imaging No No F127M WFC3/IR Imaging No No F139M WFC3/IR Imaging No No F153M WFC3/IR Imaging No No F127M WFC3/IR Imaging No No F139M WFC3/IR Imaging No No F153M WFC3/IR Imaging No No F127M WFC3/IR Imaging No No F139M WFC3/IR Imaging No No F153M WFC3/IR Imaging No No F127M WFC3/IR Imaging No No F139M WFC3/IR Imaging No No F153M ACS/WFC Imaging No No F658N ACS/WFC Imaging No No F625W ACS/WFC Imaging No No F658N ACS/WFC Imaging No No F625W ACS/WFC Imaging No No F658N ACS/WFC Imaging No No F625W ACS/WFC Imaging No No F658N ACS/WFC Imaging No No F625W ACS/WFC Imaging No No F658N ACS/WFC Imaging No No F625W ACS/WFC Imaging No No F658N ACS/WFC Imaging No No F625W ACS/WFC Imaging No No F658N ACS/WFC Imaging No No F625W 1604433064513 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. /private/var/folders/r0/xqryfdg13cb439h_rxxbkwf0000113/T/OPVisit6322859123787562587.xml Using a 4pt dither for F127M, and a 2pt dither for F139M and F153M. Nyquist sampling will be recovered in two redder filters by leveraging the dithers in the blue filter - all filters will be reduced simultaneously. This strategy follows that used by GO-14072, which this program is an extension of. 1600371475000 202.49028706550678 (Tic-Visit :proposal-id 15932 :visit-id "01" :proposal-version -1 :trans-version "20200619" :date "03-Nov-2020 14:51:04.0" :trans-errors '(:WARNINGS 1 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "30" :si-bright-earth-limb-angle 20.0 :data-volume 1723472 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15932 :visit-id "01" :obset-id "01" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15932 :visit-id "01" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2882 :al-overhead-at-end 0 :internal-dur-at-end 709 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3238 :pcs-gap 0 ) true 1 1 1604433065434 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. /private/var/folders/r0/xqryfdg13cb439h_rxxbkwf0000113/T/OPVisit17601399562240898952.xml Using a 4pt dither for F127M, and a 2pt dither for F139M and F153M. Nyquist sampling will be recovered in two redder filters by leveraging the dithers in the blue filter - all filters will be reduced simultaneously. This strategy follows that used by GO-14072, which this program is an extension of. 1600531607000 200.43061977607022 (Tic-Visit :proposal-id 15932 :visit-id "02" :proposal-version -1 :trans-version "20200619" :date "03-Nov-2020 14:51:05.0" :trans-errors '(:WARNINGS 1 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "30" :si-bright-earth-limb-angle 20.0 :data-volume 1723472 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15932 :visit-id "02" :obset-id "02" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15932 :visit-id "02" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2882 :al-overhead-at-end 0 :internal-dur-at-end 709 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3238 :pcs-gap 0 ) true 1 1 1604433066303 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. /private/var/folders/r0/xqryfdg13cb439h_rxxbkwf0000113/T/OPVisit169245654787751351.xml Using a 4pt dither for F127M, and a 2pt dither for F139M and F153M. Nyquist sampling will be recovered in two redder filters by leveraging the dithers in the blue filter - all filters will be reduced simultaneously. This strategy follows that used by GO-14072, which this program is an extension of. 1600537326000 200.40344964091594 (Tic-Visit :proposal-id 15932 :visit-id "03" :proposal-version -1 :trans-version "20200619" :date "03-Nov-2020 14:51:06.0" :trans-errors '(:WARNINGS 1 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "30" :si-bright-earth-limb-angle 20.0 :data-volume 1723472 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15932 :visit-id "03" :obset-id "03" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15932 :visit-id "03" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2882 :al-overhead-at-end 0 :internal-dur-at-end 709 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3238 :pcs-gap 0 ) true 1 1 1604433067147 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. /private/var/folders/r0/xqryfdg13cb439h_rxxbkwf0000113/T/OPVisit17551023710246551889.xml Using a 4pt dither for F127M, and a 2pt dither for F139M and F153M. Nyquist sampling will be recovered in two redder filters by leveraging the dithers in the blue filter - all filters will be reduced simultaneously. This strategy follows that used by GO-14072, which this program is an extension of. 1600617390000 199.55294067708292 (Tic-Visit :proposal-id 15932 :visit-id "04" :proposal-version -1 :trans-version "20200619" :date "03-Nov-2020 14:51:06.0" :trans-errors '(:WARNINGS 1 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "30" :si-bright-earth-limb-angle 20.0 :data-volume 1723472 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15932 :visit-id "04" :obset-id "04" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15932 :visit-id "04" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2882 :al-overhead-at-end 0 :internal-dur-at-end 709 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3238 :pcs-gap 0 ) true 1 1 1604433067979 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. /private/var/folders/r0/xqryfdg13cb439h_rxxbkwf0000113/T/OPVisit14080291799010561789.xml Using a 4pt dither for F127M, and a 2pt dither for F139M and F153M. Nyquist sampling will be recovered in two redder filters by leveraging the dithers in the blue filter - all filters will be reduced simultaneously. This strategy follows that used by GO-14072, which this program is an extension of. 1600623109000 199.5481636825143 (Tic-Visit :proposal-id 15932 :visit-id "05" :proposal-version -1 :trans-version "20200619" :date "03-Nov-2020 14:51:07.0" :trans-errors '(:WARNINGS 1 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "30" :si-bright-earth-limb-angle 20.0 :data-volume 1723472 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15932 :visit-id "05" :obset-id "05" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15932 :visit-id "05" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2882 :al-overhead-at-end 0 :internal-dur-at-end 709 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3238 :pcs-gap 0 ) true 1 1 1604433068811 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. /private/var/folders/r0/xqryfdg13cb439h_rxxbkwf0000113/T/OPVisit4433502527691117808.xml Using a 4pt dither for F127M, and a 2pt dither for F139M and F153M. Nyquist sampling will be recovered in two redder filters by leveraging the dithers in the blue filter - all filters will be reduced simultaneously. This strategy follows that used by GO-14072, which this program is an extension of. 1600697468000 198.6294827360282 (Tic-Visit :proposal-id 15932 :visit-id "06" :proposal-version -1 :trans-version "20200619" :date "03-Nov-2020 14:51:08.0" :trans-errors '(:WARNINGS 1 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "30" :si-bright-earth-limb-angle 20.0 :data-volume 1723472 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15932 :visit-id "06" :obset-id "06" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15932 :visit-id "06" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2882 :al-overhead-at-end 0 :internal-dur-at-end 709 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3238 :pcs-gap 0 ) true 1 1 1604433069620 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. /private/var/folders/r0/xqryfdg13cb439h_rxxbkwf0000113/T/OPVisit10123035129451775996.xml Using a 4pt dither for F127M, and a 2pt dither for F139M and F153M. Nyquist sampling will be recovered in two redder filters by leveraging the dithers in the blue filter - all filters will be reduced simultaneously. This strategy follows that used by GO-14072, which this program is an extension of. 1600703190000 198.58635427073398 (Tic-Visit :proposal-id 15932 :visit-id "07" :proposal-version -1 :trans-version "20200619" :date "03-Nov-2020 14:51:09.0" :trans-errors '(:WARNINGS 1 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "30" :si-bright-earth-limb-angle 20.0 :data-volume 1723472 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15932 :visit-id "07" :obset-id "07" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15932 :visit-id "07" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2882 :al-overhead-at-end 0 :internal-dur-at-end 709 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3238 :pcs-gap 0 ) true 1 1 1604433070455 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. /private/var/folders/r0/xqryfdg13cb439h_rxxbkwf0000113/T/OPVisit6770219508241124870.xml Using a 4pt dither for F127M, and a 2pt dither for F139M and F153M. Nyquist sampling will be recovered in two redder filters by leveraging the dithers in the blue filter - all filters will be reduced simultaneously. This strategy follows that used by GO-14072, which this program is an extension of. 1600686024000 198.652363605919 (Tic-Visit :proposal-id 15932 :visit-id "08" :proposal-version -1 :trans-version "20200619" :date "03-Nov-2020 14:51:10.0" :trans-errors '(:WARNINGS 1 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "30" :si-bright-earth-limb-angle 20.0 :data-volume 1723472 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15932 :visit-id "08" :obset-id "08" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15932 :visit-id "08" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2882 :al-overhead-at-end 0 :internal-dur-at-end 709 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3238 :pcs-gap 0 ) true 1 1 1604433071307 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. /private/var/folders/r0/xqryfdg13cb439h_rxxbkwf0000113/T/OPVisit6992239392350160744.xml Using a 4pt dither for F127M, and a 2pt dither for F139M and F153M. Nyquist sampling will be recovered in two redder filters by leveraging the dithers in the blue filter - all filters will be reduced simultaneously. This strategy follows that used by GO-14072, which this program is an extension of. 1600708909000 198.37770233086383 (Tic-Visit :proposal-id 15932 :visit-id "09" :proposal-version -1 :trans-version "20200619" :date "03-Nov-2020 14:51:11.0" :trans-errors '(:WARNINGS 1 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "30" :si-bright-earth-limb-angle 20.0 :data-volume 1723472 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15932 :visit-id "09" :obset-id "09" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15932 :visit-id "09" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2882 :al-overhead-at-end 0 :internal-dur-at-end 709 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3238 :pcs-gap 0 ) true 1 1 1604433072212 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. /private/var/folders/r0/xqryfdg13cb439h_rxxbkwf0000113/T/OPVisit11330249104451834927.xml Using a 4pt dither for F127M, and a 2pt dither for F139M and F153M. Nyquist sampling will be recovered in two redder filters by leveraging the dithers in the blue filter - all filters will be reduced simultaneously. This strategy follows that used by GO-14072, which this program is an extension of. 1600691747000 198.6269957847187 (Tic-Visit :proposal-id 15932 :visit-id "10" :proposal-version -1 :trans-version "20200619" :date "03-Nov-2020 14:51:11.0" :trans-errors '(:WARNINGS 1 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "30" :si-bright-earth-limb-angle 20.0 :data-volume 1723472 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15932 :visit-id "10" :obset-id "10" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15932 :visit-id "10" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2882 :al-overhead-at-end 0 :internal-dur-at-end 709 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3238 :pcs-gap 0 ) true 1 1 1604433073049 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. /private/var/folders/r0/xqryfdg13cb439h_rxxbkwf0000113/T/OPVisit16017289650100822313.xml Using a 4pt dither for F127M, and a 2pt dither for F139M and F153M. Nyquist sampling will be recovered in two redder filters by leveraging the dithers in the blue filter - all filters will be reduced simultaneously. This strategy follows that used by GO-14072, which this program is an extension of. 1600674582000 198.74436018807756 (Tic-Visit :proposal-id 15932 :visit-id "11" :proposal-version -1 :trans-version "20200619" :date "03-Nov-2020 14:51:12.0" :trans-errors '(:WARNINGS 1 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "30" :si-bright-earth-limb-angle 20.0 :data-volume 1723472 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15932 :visit-id "11" :obset-id "11" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15932 :visit-id "11" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2882 :al-overhead-at-end 0 :internal-dur-at-end 709 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3238 :pcs-gap 0 ) true 1 1 1604433073902 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. /private/var/folders/r0/xqryfdg13cb439h_rxxbkwf0000113/T/OPVisit11023955677698227018.xml Using a 4pt dither for F127M, and a 2pt dither for F139M and F153M. Nyquist sampling will be recovered in two redder filters by leveraging the dithers in the blue filter - all filters will be reduced simultaneously. This strategy follows that used by GO-14072, which this program is an extension of. 1600680279000 207.22429124722748 (Tic-Visit :proposal-id 15932 :visit-id "12" :proposal-version -1 :trans-version "20200619" :date "03-Nov-2020 14:51:13.0" :trans-errors '(:WARNINGS 1 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "30" :si-bright-earth-limb-angle 20.0 :data-volume 1723472 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15932 :visit-id "12" :obset-id "12" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15932 :visit-id "12" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2882 :al-overhead-at-end 0 :internal-dur-at-end 709 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3238 :pcs-gap 0 ) true 1 1 1604433075137 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. /private/var/folders/r0/xqryfdg13cb439h_rxxbkwf0000113/T/OPVisit17342807383075807070.xml Using a 4pt dither for F127M, and a 2pt dither for F139M and F153M. Nyquist sampling will be recovered in two redder filters by leveraging the dithers in the blue filter - all filters will be reduced simultaneously. This strategy follows that used by GO-14072, which this program is an extension of. 1603448002000 155.0 (Tic-Visit :proposal-id 15932 :visit-id "13" :proposal-version -1 :trans-version "20200619" :date "03-Nov-2020 14:51:14.0" :trans-errors '(:WARNINGS 1 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "30" :si-bright-earth-limb-angle 20.0 :data-volume 1723472 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15932 :visit-id "13" :obset-id "13" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15932 :visit-id "13" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2882 :al-overhead-at-end 0 :internal-dur-at-end 709 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3238 :pcs-gap 0 ) true 1 1 1604433076013 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. /private/var/folders/r0/xqryfdg13cb439h_rxxbkwf0000113/T/OPVisit13796843836206524058.xml Using a 4pt dither for F127M, and a 2pt dither for F139M and F153M. Nyquist sampling will be recovered in two redder filters by leveraging the dithers in the blue filter - all filters will be reduced simultaneously. This strategy follows that used by GO-14072, which this program is an extension of. 1603533763000 144.0 (Tic-Visit :proposal-id 15932 :visit-id "14" :proposal-version -1 :trans-version "20200619" :date "03-Nov-2020 14:51:15.0" :trans-errors '(:WARNINGS 1 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "30" :si-bright-earth-limb-angle 20.0 :data-volume 1723472 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15932 :visit-id "14" :obset-id "14" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15932 :visit-id "14" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2882 :al-overhead-at-end 0 :internal-dur-at-end 709 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3238 :pcs-gap 0 ) true 1 1 1604433076872 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. /private/var/folders/r0/xqryfdg13cb439h_rxxbkwf0000113/T/OPVisit13522481061077387471.xml Using a 4pt dither for F127M, and a 2pt dither for F139M and F153M. Nyquist sampling will be recovered in two redder filters by leveraging the dithers in the blue filter - all filters will be reduced simultaneously. This strategy follows that used by GO-14072, which this program is an extension of. 1603453719000 155.0 (Tic-Visit :proposal-id 15932 :visit-id "15" :proposal-version -1 :trans-version "20200619" :date "03-Nov-2020 14:51:16.0" :trans-errors '(:WARNINGS 1 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "30" :si-bright-earth-limb-angle 20.0 :data-volume 1723472 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15932 :visit-id "15" :obset-id "15" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15932 :visit-id "15" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2882 :al-overhead-at-end 0 :internal-dur-at-end 709 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3238 :pcs-gap 0 ) true 1 1 1604433077745 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. /private/var/folders/r0/xqryfdg13cb439h_rxxbkwf0000113/T/OPVisit15312935836200148653.xml Using a 4pt dither for F127M, and a 2pt dither for F139M and F153M. Nyquist sampling will be recovered in two redder filters by leveraging the dithers in the blue filter - all filters will be reduced simultaneously. This strategy follows that used by GO-14072, which this program is an extension of. 1603539479000 145.92105981286358 (Tic-Visit :proposal-id 15932 :visit-id "16" :proposal-version -1 :trans-version "20200619" :date "03-Nov-2020 14:51:17.0" :trans-errors '(:WARNINGS 1 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "30" :si-bright-earth-limb-angle 20.0 :data-volume 1723472 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15932 :visit-id "16" :obset-id "16" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15932 :visit-id "16" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2882 :al-overhead-at-end 0 :internal-dur-at-end 709 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3238 :pcs-gap 0 ) true 1 1 1604433078615 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. /private/var/folders/r0/xqryfdg13cb439h_rxxbkwf0000113/T/OPVisit13482343422115958476.xml Using a 4pt dither for F127M, and a 2pt dither for F139M and F153M. Nyquist sampling will be recovered in two redder filters by leveraging the dithers in the blue filter - all filters will be reduced simultaneously. This strategy follows that used by GO-14072, which this program is an extension of. 1603705285000 142.67090675769532 (Tic-Visit :proposal-id 15932 :visit-id "17" :proposal-version -1 :trans-version "20200619" :date "03-Nov-2020 14:51:18.0" :trans-errors '(:WARNINGS 1 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "30" :si-bright-earth-limb-angle 20.0 :data-volume 1723472 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15932 :visit-id "17" :obset-id "17" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15932 :visit-id "17" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2882 :al-overhead-at-end 0 :internal-dur-at-end 709 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3238 :pcs-gap 0 ) true 1 1 1604433079473 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. /private/var/folders/r0/xqryfdg13cb439h_rxxbkwf0000113/T/OPVisit13027702758706985330.xml Using a 4pt dither for F127M, and a 2pt dither for F139M and F153M. Nyquist sampling will be recovered in two redder filters by leveraging the dithers in the blue filter - all filters will be reduced simultaneously. This strategy follows that used by GO-14072, which this program is an extension of. 1603619524000 144.371414881517 (Tic-Visit :proposal-id 15932 :visit-id "18" :proposal-version -1 :trans-version "20200619" :date "03-Nov-2020 14:51:19.0" :trans-errors '(:WARNINGS 1 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "30" :si-bright-earth-limb-angle 20.0 :data-volume 1723472 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15932 :visit-id "18" :obset-id "18" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15932 :visit-id "18" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2882 :al-overhead-at-end 0 :internal-dur-at-end 709 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3238 :pcs-gap 0 ) true 1 1 1604433080305 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. /private/var/folders/r0/xqryfdg13cb439h_rxxbkwf0000113/T/OPVisit5880969178886916761.xml Using a 4pt dither for F127M, and a 2pt dither for F139M and F153M. Nyquist sampling will be recovered in two redder filters by leveraging the dithers in the blue filter - all filters will be reduced simultaneously. This strategy follows that used by GO-14072, which this program is an extension of. 1603625242000 144.169572639178 (Tic-Visit :proposal-id 15932 :visit-id "19" :proposal-version -1 :trans-version "20200619" :date "03-Nov-2020 14:51:20.0" :trans-errors '(:WARNINGS 1 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "30" :si-bright-earth-limb-angle 20.0 :data-volume 1723472 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15932 :visit-id "19" :obset-id "19" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15932 :visit-id "19" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2882 :al-overhead-at-end 0 :internal-dur-at-end 709 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3238 :pcs-gap 0 ) true 1 1 1604433081149 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. /private/var/folders/r0/xqryfdg13cb439h_rxxbkwf0000113/T/OPVisit6943050374626930048.xml Using a 4pt dither for F127M, and a 2pt dither for F139M and F153M. Nyquist sampling will be recovered in two redder filters by leveraging the dithers in the blue filter - all filters will be reduced simultaneously. This strategy follows that used by GO-14072, which this program is an extension of. Duplicate of visit 19, which failed. (Tic-Visit :proposal-id 15932 :visit-id "72" :proposal-version -1 :trans-version "20200619" :date "03-Nov-2020 14:51:20.0" :trans-errors '(:WARNINGS 1 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "30" :si-bright-earth-limb-angle 20.0 :data-volume 1723472 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15932 :visit-id "72" :obset-id "72" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15932 :visit-id "72" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2882 :al-overhead-at-end 0 :internal-dur-at-end 709 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3238 :pcs-gap 0 ) true 1 1 1604433081997 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. /private/var/folders/r0/xqryfdg13cb439h_rxxbkwf0000113/T/OPVisit3345532942340567813.xml Using a 4pt dither for F127M, and a 2pt dither for F139M and F153M. Nyquist sampling will be recovered in two redder filters by leveraging the dithers in the blue filter - all filters will be reduced simultaneously. This strategy follows that used by GO-14072, which this program is an extension of. 1604248533000 123.0 (Tic-Visit :proposal-id 15932 :visit-id "20" :proposal-version -1 :trans-version "20200619" :date "03-Nov-2020 14:51:21.0" :trans-errors '(:WARNINGS 1 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "30" :si-bright-earth-limb-angle 20.0 :data-volume 1723472 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15932 :visit-id "20" :obset-id "20" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15932 :visit-id "20" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2882 :al-overhead-at-end 0 :internal-dur-at-end 709 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3238 :pcs-gap 0 ) true 1 1 1604433082844 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. /private/var/folders/r0/xqryfdg13cb439h_rxxbkwf0000113/T/OPVisit1677676934327245946.xml Using a 4pt dither for F127M, and a 2pt dither for F139M and F153M. Nyquist sampling will be recovered in two redder filters by leveraging the dithers in the blue filter - all filters will be reduced simultaneously. This strategy follows that used by GO-14072, which this program is an extension of. Duplicate of visit 20, which failed (Tic-Visit :proposal-id 15932 :visit-id "73" :proposal-version -1 :trans-version "20200619" :date "03-Nov-2020 14:51:22.0" :trans-errors '(:WARNINGS 1 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "30" :si-bright-earth-limb-angle 20.0 :data-volume 1723472 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15932 :visit-id "73" :obset-id "73" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15932 :visit-id "73" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2882 :al-overhead-at-end 0 :internal-dur-at-end 709 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3238 :pcs-gap 0 ) true 1 1 1604433083771 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. /private/var/folders/r0/xqryfdg13cb439h_rxxbkwf0000113/T/OPVisit15332434194773240129.xml Using a 4pt dither for F127M, and a 2pt dither for F139M and F153M. Nyquist sampling will be recovered in two redder filters by leveraging the dithers in the blue filter - all filters will be reduced simultaneously. This strategy follows that used by GO-14072, which this program is an extension of. 1603110674000 164.0 (Tic-Visit :proposal-id 15932 :visit-id "21" :proposal-version -1 :trans-version "20200619" :date "03-Nov-2020 14:51:23.0" :trans-errors '(:WARNINGS 1 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "30" :si-bright-earth-limb-angle 20.0 :data-volume 1723472 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15932 :visit-id "21" :obset-id "21" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15932 :visit-id "21" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2882 :al-overhead-at-end 0 :internal-dur-at-end 709 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3238 :pcs-gap 0 ) true 1 1 1604433084602 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. /private/var/folders/r0/xqryfdg13cb439h_rxxbkwf0000113/T/OPVisit9521895183111643292.xml Using a 4pt dither for F127M, and a 2pt dither for F139M and F153M. Nyquist sampling will be recovered in two redder filters by leveraging the dithers in the blue filter - all filters will be reduced simultaneously. This strategy follows that used by GO-14072, which this program is an extension of. Duplicate of visit 21, which failed (Tic-Visit :proposal-id 15932 :visit-id "71" :proposal-version -1 :trans-version "20200619" :date "03-Nov-2020 14:51:24.0" :trans-errors '(:WARNINGS 1 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "30" :si-bright-earth-limb-angle 20.0 :data-volume 1723472 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15932 :visit-id "71" :obset-id "71" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15932 :visit-id "71" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2882 :al-overhead-at-end 0 :internal-dur-at-end 709 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3238 :pcs-gap 0 ) true 1 1 1604433085809 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. /private/var/folders/r0/xqryfdg13cb439h_rxxbkwf0000113/T/OPVisit3460370687903104880.xml Using a 4pt dither for F127M, and a 2pt dither for F139M and F153M. Nyquist sampling will be recovered in two redder filters by leveraging the dithers in the blue filter - all filters will be reduced simultaneously. This strategy follows that used by GO-14072, which this program is an extension of. 1603876813000 138.90831403722188 (Tic-Visit :proposal-id 15932 :visit-id "22" :proposal-version -1 :trans-version "20200619" :date "03-Nov-2020 14:51:25.0" :trans-errors '(:WARNINGS 1 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "30" :si-bright-earth-limb-angle 20.0 :data-volume 1723472 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15932 :visit-id "22" :obset-id "22" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15932 :visit-id "22" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2882 :al-overhead-at-end 0 :internal-dur-at-end 709 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3238 :pcs-gap 0 ) true 1 1 1604433086661 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. /private/var/folders/r0/xqryfdg13cb439h_rxxbkwf0000113/T/OPVisit12802222502449253181.xml Using a 4pt dither for F127M, and a 2pt dither for F139M and F153M. Nyquist sampling will be recovered in two redder filters by leveraging the dithers in the blue filter - all filters will be reduced simultaneously. This strategy follows that used by GO-14072, which this program is an extension of. 1604500305000 126.68761890303739 (Tic-Visit :proposal-id 15932 :visit-id "23" :proposal-version -1 :trans-version "20200619" :date "03-Nov-2020 14:51:26.0" :trans-errors '(:WARNINGS 1 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "30" :si-bright-earth-limb-angle 20.0 :data-volume 1723472 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15932 :visit-id "23" :obset-id "23" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15932 :visit-id "23" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2882 :al-overhead-at-end 0 :internal-dur-at-end 709 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3238 :pcs-gap 0 ) true 1 1 1604433087501 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. /private/var/folders/r0/xqryfdg13cb439h_rxxbkwf0000113/T/OPVisit12299888298543659434.xml Using a 4pt dither for F127M, and a 2pt dither for F139M and F153M. Nyquist sampling will be recovered in two redder filters by leveraging the dithers in the blue filter - all filters will be reduced simultaneously. This strategy follows that used by GO-14072, which this program is an extension of. 1604134141000 133.68065205825093 (Tic-Visit :proposal-id 15932 :visit-id "24" :proposal-version -1 :trans-version "20200619" :date "03-Nov-2020 14:51:27.0" :trans-errors '(:WARNINGS 1 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "30" :si-bright-earth-limb-angle 20.0 :data-volume 1723472 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15932 :visit-id "24" :obset-id "24" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15932 :visit-id "24" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2882 :al-overhead-at-end 0 :internal-dur-at-end 709 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3238 :pcs-gap 0 ) true 1 1 1604433088373 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. /private/var/folders/r0/xqryfdg13cb439h_rxxbkwf0000113/T/OPVisit9678724447141332744.xml Using a 4pt dither for F127M, and a 2pt dither for F139M and F153M. Nyquist sampling will be recovered in two redder filters by leveraging the dithers in the blue filter - all filters will be reduced simultaneously. This strategy follows that used by GO-14072, which this program is an extension of. Duplicate of visit 24, which failed. (Tic-Visit :proposal-id 15932 :visit-id "74" :proposal-version -1 :trans-version "20200619" :date "03-Nov-2020 14:51:28.0" :trans-errors '(:WARNINGS 1 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "30" :si-bright-earth-limb-angle 20.0 :data-volume 1723472 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15932 :visit-id "74" :obset-id "74" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15932 :visit-id "74" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2882 :al-overhead-at-end 0 :internal-dur-at-end 709 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3238 :pcs-gap 0 ) true 1 1 1604433089227 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. /private/var/folders/r0/xqryfdg13cb439h_rxxbkwf0000113/T/OPVisit7634038563597829194.xml Using a 4pt dither for F127M, and a 2pt dither for F139M and F153M. Nyquist sampling will be recovered in two redder filters by leveraging the dithers in the blue filter - all filters will be reduced simultaneously. This strategy follows that used by GO-14072, which this program is an extension of. 1604506030000 118.67334071309028 (Tic-Visit :proposal-id 15932 :visit-id "25" :proposal-version -1 :trans-version "20200619" :date "03-Nov-2020 14:51:29.0" :trans-errors '(:WARNINGS 1 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "30" :si-bright-earth-limb-angle 20.0 :data-volume 1723472 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15932 :visit-id "25" :obset-id "25" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15932 :visit-id "25" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2882 :al-overhead-at-end 0 :internal-dur-at-end 709 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3238 :pcs-gap 0 ) true 1 1 1604433090056 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. /private/var/folders/r0/xqryfdg13cb439h_rxxbkwf0000113/T/OPVisit5355722972837381312.xml Using a 4pt dither for F127M, and a 2pt dither for F139M and F153M. Nyquist sampling will be recovered in two redder filters by leveraging the dithers in the blue filter - all filters will be reduced simultaneously. This strategy follows that used by GO-14072, which this program is an extension of. 1603373677000 156.0 (Tic-Visit :proposal-id 15932 :visit-id "26" :proposal-version -1 :trans-version "20200619" :date "03-Nov-2020 14:51:29.0" :trans-errors '(:WARNINGS 1 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "30" :si-bright-earth-limb-angle 20.0 :data-volume 1723472 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15932 :visit-id "26" :obset-id "26" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15932 :visit-id "26" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2882 :al-overhead-at-end 0 :internal-dur-at-end 709 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3238 :pcs-gap 0 ) true 1 1 1604433091270 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. /private/var/folders/r0/xqryfdg13cb439h_rxxbkwf0000113/T/OPVisit15025695333094587934.xml Using a 4pt dither for F127M, and a 2pt dither for F139M and F153M. Nyquist sampling will be recovered in two redder filters by leveraging the dithers in the blue filter - all filters will be reduced simultaneously. This strategy follows that used by GO-14072, which this program is an extension of. 1594313771000 250.0 (Tic-Visit :proposal-id 15932 :visit-id "27" :proposal-version -1 :trans-version "20200619" :date "03-Nov-2020 14:51:30.0" :trans-errors '(:WARNINGS 1 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "30" :si-bright-earth-limb-angle 20.0 :data-volume 2268464 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15932 :visit-id "27" :obset-id "27" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15932 :visit-id "27" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2814 :al-overhead-at-end 0 :internal-dur-at-end 1075 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3180 :pcs-gap 0 ) true 1 1 1604433092481 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. /private/var/folders/r0/xqryfdg13cb439h_rxxbkwf0000113/T/OPVisit14099807840251107766.xml Using a 4pt dither for F127M, and a 2pt dither for F139M and F153M. Nyquist sampling will be recovered in two redder filters by leveraging the dithers in the blue filter - all filters will be reduced simultaneously. This strategy follows that used by GO-14072, which this program is an extension of. 1603711324000 158.0 (Tic-Visit :proposal-id 15932 :visit-id "28" :proposal-version -1 :trans-version "20200619" :date "03-Nov-2020 14:51:32.0" :trans-errors '(:WARNINGS 1 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "30" :si-bright-earth-limb-angle 20.0 :data-volume 2268464 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15932 :visit-id "28" :obset-id "28" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15932 :visit-id "28" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2814 :al-overhead-at-end 0 :internal-dur-at-end 1075 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3180 :pcs-gap 0 ) true 1 1 1604433093639 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. /private/var/folders/r0/xqryfdg13cb439h_rxxbkwf0000113/T/OPVisit5677438450403937282.xml Using a 4pt dither for F127M, and a 2pt dither for F139M and F153M. Nyquist sampling will be recovered in two redder filters by leveraging the dithers in the blue filter - all filters will be reduced simultaneously. This strategy follows that used by GO-14072, which this program is an extension of. 1600543155000 222.87746292364733 (Tic-Visit :proposal-id 15932 :visit-id "29" :proposal-version -1 :trans-version "20200619" :date "03-Nov-2020 14:51:33.0" :trans-errors '(:WARNINGS 1 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "30" :si-bright-earth-limb-angle 20.0 :data-volume 2268464 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15932 :visit-id "29" :obset-id "29" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15932 :visit-id "29" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2814 :al-overhead-at-end 0 :internal-dur-at-end 1075 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3180 :pcs-gap 0 ) true 1 1 1604433094854 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. /private/var/folders/r0/xqryfdg13cb439h_rxxbkwf0000113/T/OPVisit15709804726864352767.xml Using a 4pt dither for F127M, and a 2pt dither for F139M and F153M. Nyquist sampling will be recovered in two redder filters by leveraging the dithers in the blue filter - all filters will be reduced simultaneously. This strategy follows that used by GO-14072, which this program is an extension of. 1594262306000 250.0 (Tic-Visit :proposal-id 15932 :visit-id "30" :proposal-version -1 :trans-version "20200619" :date "03-Nov-2020 14:51:34.0" :trans-errors '(:WARNINGS 1 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "30" :si-bright-earth-limb-angle 20.0 :data-volume 2268464 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15932 :visit-id "30" :obset-id "30" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15932 :visit-id "30" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2814 :al-overhead-at-end 0 :internal-dur-at-end 1075 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3180 :pcs-gap 0 ) true 1 1 1604433096361 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. /private/var/folders/r0/xqryfdg13cb439h_rxxbkwf0000113/T/OPVisit11827762746136347495.xml Using a 4pt dither for F127M, and a 2pt dither for F139M and F153M. Nyquist sampling will be recovered in two redder filters by leveraging the dithers in the blue filter - all filters will be reduced simultaneously. This strategy follows that used by GO-14072, which this program is an extension of. 1595120416000 249.48943292014445 (Tic-Visit :proposal-id 15932 :visit-id "31" :proposal-version -1 :trans-version "20200619" :date "03-Nov-2020 14:51:36.0" :trans-errors '(:WARNINGS 1 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "30" :si-bright-earth-limb-angle 20.0 :data-volume 2268464 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15932 :visit-id "31" :obset-id "31" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15932 :visit-id "31" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2814 :al-overhead-at-end 0 :internal-dur-at-end 1075 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3180 :pcs-gap 0 ) true 1 1 1604433097507 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. /private/var/folders/r0/xqryfdg13cb439h_rxxbkwf0000113/T/OPVisit4756291552177941281.xml Using a 4pt dither for F127M, and a 2pt dither for F139M and F153M. Nyquist sampling will be recovered in two redder filters by leveraging the dithers in the blue filter - all filters will be reduced simultaneously. This strategy follows that used by GO-14072, which this program is an extension of. 1603797105000 133.0 (Tic-Visit :proposal-id 15932 :visit-id "32" :proposal-version -1 :trans-version "20200619" :date "03-Nov-2020 14:51:37.0" :trans-errors '(:WARNINGS 1 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "30" :si-bright-earth-limb-angle 20.0 :data-volume 2268464 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15932 :visit-id "32" :obset-id "32" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15932 :visit-id "32" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2814 :al-overhead-at-end 0 :internal-dur-at-end 1075 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3180 :pcs-gap 0 ) true 1 1 1604433098655 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. /private/var/folders/r0/xqryfdg13cb439h_rxxbkwf0000113/T/OPVisit15691368770912347830.xml Using a 4pt dither for F127M, and a 2pt dither for F139M and F153M. Nyquist sampling will be recovered in two redder filters by leveraging the dithers in the blue filter - all filters will be reduced simultaneously. This strategy follows that used by GO-14072, which this program is an extension of. 1595801523000 247.00390572882094 (Tic-Visit :proposal-id 15932 :visit-id "33" :proposal-version -1 :trans-version "20200619" :date "03-Nov-2020 14:51:38.0" :trans-errors '(:WARNINGS 1 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "30" :si-bright-earth-limb-angle 20.0 :data-volume 2268464 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15932 :visit-id "33" :obset-id "33" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15932 :visit-id "33" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2814 :al-overhead-at-end 0 :internal-dur-at-end 1075 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3180 :pcs-gap 0 ) true 1 1