0 Assigned ID: 357 ----- Attempting Submission 1 (Fri Apr 05 06:32:32 GMT 2019) ----- HST Phase I Proposal 357 (APT_BroadBand_Imaging.apt) successfully submitted. Receipt: # 357-1 ----- Attempting Submission 2 (Fri Apr 05 17:17:39 GMT 2019) ----- The list of Investigators does not match the STScI records for this program. The unique ID for this investigator was not found in the STScI database. 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 corrected the unwanted changes that happened in the last submission and added visits 21 and 22 again -1723077734 ----- Attempting Submission 1 (Thu Jul 25 14:42:02 GMT 2019) ----- HST Phase II Proposal 15939 (phase2_20190624.apt) successfully submitted. Receipt: # 15939-1 ----- Attempting Submission 2 (Thu Aug 01 12:07:34 GMT 2019) ----- HST Phase II Proposal 15939 (phase2_resubmitted.apt) successfully submitted. Receipt: # 15939-2 ----- Attempting Submission 3 (Mon Apr 20 14:54:43 GMT 2020) ----- HST Phase II Proposal 15939 (phase2_resubmitted.apt) successfully submitted. Receipt: # 15939-3 ----- Attempting Submission 4 (Mon Jul 27 20:33:53 GMT 2020) ----- HST Phase II Proposal 15939 successfully submitted. Receipt: # 15939-4 ----- Attempting Submission 5 (Mon Aug 03 16:42:02 GMT 2020) ----- HST Phase II Proposal 15939 successfully submitted. Receipt: # 15939-5 ----- Attempting Submission 7 (Tue Sep 29 17:48:52 GMT 2020) ----- CoI Hamanowicz has recently changed her affiliation The stellar populations of gas-rich absorbing galaxies detected with VLT/MUSE and ALMA: the essential link to the baryon cycle The physical processes by which the gas is accreted onto galaxies, tranformed into stars and then expelled from galaxies are of paramount importance to galaxy evolution studies. Observationally constraining each of these baryon components in the same systems is however extremely challenging. Absorption lines detected against background quasars offer the most compelling way to study the cold gas in the circumgalactic medium (CGM). We have selected a unique sample of 17 VLT/MUSE quasar fields, comprising 40 z<0.85 absorbers and 120 associated galaxies, some of which are also detected in CO with ALMA. These absorbers have measured N(H I), absorption and emission metallicities and reconstructed 3D kinematics. An additional sample of 200 z<1.2 galaxies have MgII coverage from quasar spectroscopy. Only the powerful combination of high spatial resolution and UV coverage offered by HST will permit to characterise the stellar content of these objects. Therefore, we propose a 40-orbit 3-band UVIS and IR WFC3 imaging campaign to measure their stellar mass, dust content, age of their stellar population, constrain their resolved morphology and large-scale environment. Only the proposed observations will allow us to establish a complete census of the condensed baryons in these systems, to characterise the dynamical structure of the galaxy groups and filaments and to quantify the CGM metal enrichment as a function of stellar mass. Together, these data will provide fresh clues on the baryon cycle, a key component of galaxy formation and evolution. We are observing the faint galaxy counterparts to known absorbers towards the bright targeted quasars. We will measure their magnitudes to determine their stellar masses via SED fitting. The orientations of our observations are chosen such that the faint galaxies are not obstructed by the quasar PSF diffraction spikes. Our team has a strong expertise in the processing of HST observations in general and WFC3 data in particular as well as the auxiliary datasets: HST imaging (R. Augustin, V. Kulkarni, G. Kacprzak, A. Fox, M. Hayes, C. Howk), HST spectroscopy (V. Kulkarni, A. Fox, C. Howk), VLT/MUSE 3D spectroscopy (A. Hamanowicz, A. Klitsch, C. Peroux, H. Rahmani, M. Hayes), high-resolution spectroscopy (C. Peroux, V. Kulkarni, D. York, M. Pettini, H. Rahmani) and ALMA observations (M. Zwaan, A. Klitsch, A. Hamanowicz, C. Peroux). The skills required for the data analysis are shared by several co-Is: Spectral Energy Distribution fit using Le Phase (Ilbert et al. 2006) and Beagle (Chevallard et al. 2016) - (R. Augustin, S. Kassin), light profile modelling with the GIM2D software (G. Kacprzak, R. Augustin, V. Kulkarni), covering fraction estimates (G. Kacprzak, C. Peroux, H. Rahmani). The analysis of these data will include a strong simulation component. Our team comprises one of the core member (D. Nelson) of the state-of-the-art cosmological hydrodynamical simulations Illustris TNG (Nelson et al. 2019, Pillepich et al. 2019). We will utilise these models to interpret the physical processes at the origin of our key observables (metal production sites, the complex nature of flow kinematics, the level and distribution of metal enrichment, all as a function of stellar mass and other key galaxy properties). In turn, the results of this observational program will bring new constraints on physical parameters essential to modelling galaxy evolution such as metal distribution in the CGM, mass loading factor and mass inflow rate. The data reduction will be supervised by HST/WFC3 experts (V. Kulkarni, C. Peroux, A. Fox, G. Kacprzak, M. Hayes) aided by PhD students and post-doctoral researchers. The Munich IMPRS graduate program (accessible to proposers at ESO and MPA) offers a reliable avenue to attract additional outstanding students to the project. Additional fundings will come from national space agencies: NASA, German "Deutsche Zentrum fur Luft- und Raumfahr" DLR and French "Centre national d'etudes spatiales" CNES. Lastly, we have a proven track-record of publishing shortly after observations have been taken. 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CASM was run in Phase II mode. /Users/raugustin/WORK/HST2019/OP-cache/phase2_20200929-v01.xml The science goal is to observe the faint galaxies in the quasar field that are connected to two known absorbers at z=0.38 and z=0.78. We choose the orientation such that the closest of those galaxies are not obstructed by the diffraction spikes in the quasar PSF. 1597324253000 255.0 (Tic-Visit :proposal-id 15939 :visit-id "01" :proposal-version -1 :trans-version "20200619" :date "29-Sep-2020 13:23:52.0" :trans-errors '(:WARNINGS 2 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 2 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 2310000 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15939 :visit-id "01" :obset-id "01" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15939 :visit-id "01" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2823 :al-overhead-at-end 116 :internal-dur-at-end 0 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3157 :pcs-gap 0 ) (Tic-Orbit :proposal-id 15939 :visit-id "01" :orbit-number 2 :pcs-time 392 :si-vis-utilization 2855 :al-overhead-at-end 116 :internal-dur-at-end 668 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3157 :pcs-gap 0 ) true 2 2 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. /Users/raugustin/WORK/HST2019/OP-cache/phase2_20200929-v21.xml The science goal is to observe the faint galaxies in the quasar field that are connected to two known absorbers at z=0.38 and z=0.78. We choose the orientation such that the closest of those galaxies are not obstructed by the diffraction spikes in the quasar PSF. (Tic-Visit :proposal-id 15939 :visit-id "21" :proposal-version -1 :trans-version "20200619" :date "29-Sep-2020 13:18:55.0" :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 1154992 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15939 :visit-id "21" :obset-id "21" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15939 :visit-id "21" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2771 :al-overhead-at-end 116 :internal-dur-at-end 668 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3157 :pcs-gap 0 ) true 1 0 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. /private/var/folders/wh/0x5fvqs94vlbcd6sbksx90nh0002dp/T/OPVisit13189858039808226718.xml The science goal is to observe the faint galaxies in the quasar field that are connected to a known absorbers at z=0.63. We choose the orientation such that the closest of those galaxies are not obstructed by the diffraction spikes in the quasar PSF. (Tic-Visit :proposal-id 15939 :visit-id "02" :proposal-version -1 :trans-version "20200619" :date "29-Sep-2020 13:23:52.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 2 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 2310000 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15939 :visit-id "02" :obset-id "02" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15939 :visit-id "02" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2637 :al-overhead-at-end 116 :internal-dur-at-end 0 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3142 :pcs-gap 0 ) (Tic-Orbit :proposal-id 15939 :visit-id "02" :orbit-number 2 :pcs-time 392 :si-vis-utilization 2651 :al-overhead-at-end 116 :internal-dur-at-end 668 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3142 :pcs-gap 0 ) true 2 0 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. /Users/raugustin/WORK/HST2019/OP-cache/phase2_20200929-v03.xml The science goal is to observe the faint galaxies in the quasar field that are connected to three known absorbers at z=0.31, z=0.32 and z=0.19. We choose the orientation such that the closest of those galaxies are not obstructed by the diffraction spikes in the quasar PSF. 1590715605000 115.0 (Tic-Visit :proposal-id 15939 :visit-id "03" :proposal-version -1 :trans-version "20200619" :date "29-Sep-2020 13:23:53.0" :trans-errors '(:WARNINGS 2 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 2 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 2310000 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15939 :visit-id "03" :obset-id "03" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15939 :visit-id "03" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2816 :al-overhead-at-end 121 :internal-dur-at-end 0 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3149 :pcs-gap 0 ) (Tic-Orbit :proposal-id 15939 :visit-id "03" :orbit-number 2 :pcs-time 392 :si-vis-utilization 2848 :al-overhead-at-end 121 :internal-dur-at-end 668 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3149 :pcs-gap 0 ) true 2 2 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. /private/var/folders/wh/0x5fvqs94vlbcd6sbksx90nh0002dp/T/OPVisit12020721005437360791.xml The science goal is to observe the faint galaxies in the quasar field that are connected to two known absorbers at z=0.39 and z=0.63. We choose the orientation such that the closest of those galaxies are not obstructed by the diffraction spikes in the quasar PSF. (Tic-Visit :proposal-id 15939 :visit-id "04" :proposal-version -1 :trans-version "20200619" :date "29-Sep-2020 13:23:54.0" :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 1154992 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15939 :visit-id "04" :obset-id "04" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15939 :visit-id "04" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2637 :al-overhead-at-end 123 :internal-dur-at-end 668 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3149 :pcs-gap 0 ) true 1 0 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. /Users/raugustin/WORK/HST2019/OP-cache/phase2_20200929-v05.xml The science goal is to observe the faint galaxies in the quasar field that are connected to a known absorbers at z=0.39. We choose the orientation such that the closest of those galaxies are not obstructed by the diffraction spikes in the quasar PSF. 1581286937000 310.2232240382564 (Tic-Visit :proposal-id 15939 :visit-id "05" :proposal-version -1 :trans-version "20200619" :date "29-Sep-2020 13:23:54.0" :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 1154992 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15939 :visit-id "05" :obset-id "05" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15939 :visit-id "05" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2809 :al-overhead-at-end 123 :internal-dur-at-end 668 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3142 :pcs-gap 0 ) true 1 1 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. /Users/raugustin/WORK/HST2019/OP-cache/phase2_20200929-v06.xml The science goal is to observe the faint galaxies in the quasar field that are connected to a known absorbers at z=0.43. We choose the orientation such that the closest of those galaxies are not obstructed by the diffraction spikes in the quasar PSF. 1600313281000 86.0 (Tic-Visit :proposal-id 15939 :visit-id "06" :proposal-version -1 :trans-version "20200619" :date "29-Sep-2020 13:23:54.0" :trans-errors '(:WARNINGS 2 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 2 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 2310000 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15939 :visit-id "06" :obset-id "06" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15939 :visit-id "06" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2815 :al-overhead-at-end 116 :internal-dur-at-end 0 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3149 :pcs-gap 0 ) (Tic-Orbit :proposal-id 15939 :visit-id "06" :orbit-number 2 :pcs-time 392 :si-vis-utilization 2847 :al-overhead-at-end 116 :internal-dur-at-end 668 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3149 :pcs-gap 0 ) true 2 2 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. /Users/raugustin/WORK/HST2019/OP-cache/phase2_20200929-v22.xml The science goal is to observe the faint galaxies in the quasar field that are connected to a known absorbers at z=0.43. We choose the orientation such that the closest of those galaxies are not obstructed by the diffraction spikes in the quasar PSF. (Tic-Visit :proposal-id 15939 :visit-id "22" :proposal-version -1 :trans-version "20200619" :date "29-Sep-2020 13:19:25.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 2 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 2310000 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15939 :visit-id "22" :obset-id "22" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15939 :visit-id "22" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2763 :al-overhead-at-end 116 :internal-dur-at-end 0 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3149 :pcs-gap 0 ) (Tic-Orbit :proposal-id 15939 :visit-id "22" :orbit-number 2 :pcs-time 392 :si-vis-utilization 2755 :al-overhead-at-end 116 :internal-dur-at-end 668 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3149 :pcs-gap 0 ) true 2 0 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. The science goal is to observe the faint galaxies in the quasar field that are connected to a known absorbers at z=0.78. We choose the orientation such that the closest of those galaxies are not obstructed by the diffraction spikes in the quasar PSF. (Tic-Visit :proposal-id 15939 :visit-id "07" :proposal-version -1 :trans-version "20200619" :date "03-Aug-2020 12:37:36.0" :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 1154992 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15939 :visit-id "07" :obset-id "07" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15939 :visit-id "07" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2759 :al-overhead-at-end 116 :internal-dur-at-end 668 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3142 :pcs-gap 0 ) true 1 0 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. The science goal is to observe the faint galaxies in the quasar field that are connected to a known absorbers at z=0.78. We choose the orientation such that the closest of those galaxies are not obstructed by the diffraction spikes in the quasar PSF. (Tic-Visit :proposal-id 15939 :visit-id "19" :proposal-version -1 :trans-version "20200619" :date "03-Aug-2020 12:37:04.0" :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 1154992 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15939 :visit-id "19" :obset-id "19" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15939 :visit-id "19" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2756 :al-overhead-at-end 116 :internal-dur-at-end 668 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3142 :pcs-gap 0 ) true 1 0 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. The science goal is to observe the faint galaxies in the quasar field that are connected to a known absorbers at z=0.78. We choose the orientation such that the closest of those galaxies are not obstructed by the diffraction spikes in the quasar PSF. (Tic-Visit :proposal-id 15939 :visit-id "20" :proposal-version -1 :trans-version "20200619" :date "03-Aug-2020 12:38:01.0" :trans-errors '(:WARNINGS 0 :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 974896 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15939 :visit-id "20" :obset-id "20" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15939 :visit-id "20" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2699 :al-overhead-at-end 0 :internal-dur-at-end 481 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3142 :pcs-gap 0 ) true 1 0 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. /private/var/folders/wh/0x5fvqs94vlbcd6sbksx90nh0002dp/T/OPVisit2054079117683781648.xml The science goal is to observe the faint galaxies in the quasar field that are connected to a known absorbers at z=0.48. We choose the orientation such that the closest of those galaxies are not obstructed by the diffraction spikes in the quasar PSF. (Tic-Visit :proposal-id 15939 :visit-id "08" :proposal-version -1 :trans-version "20200619" :date "29-Sep-2020 13:23:56.0" :trans-errors '(:WARNINGS 3 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 3 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 3465008 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15939 :visit-id "08" :obset-id "08" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15939 :visit-id "08" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2808 :al-overhead-at-end 123 :internal-dur-at-end 0 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3142 :pcs-gap 0 ) (Tic-Orbit :proposal-id 15939 :visit-id "08" :orbit-number 2 :pcs-time 392 :si-vis-utilization 2840 :al-overhead-at-end 116 :internal-dur-at-end 0 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3142 :pcs-gap 0 ) (Tic-Orbit :proposal-id 15939 :visit-id "08" :orbit-number 3 :pcs-time 392 :si-vis-utilization 2840 :al-overhead-at-end 116 :internal-dur-at-end 668 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3142 :pcs-gap 0 ) true 3 3 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. /private/var/folders/wh/0x5fvqs94vlbcd6sbksx90nh0002dp/T/OPVisit1985944653165769688.xml The science goal is to observe the faint galaxies in the quasar field that are connected to two known absorbers at z=0.86 and z=1.15. We choose the orientation such that the closest of those galaxies are not obstructed by the diffraction spikes in the quasar PSF. (Tic-Visit :proposal-id 15939 :visit-id "09" :proposal-version -1 :trans-version "20200619" :date "29-Sep-2020 13:23:56.0" :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 1154992 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15939 :visit-id "09" :obset-id "09" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15939 :visit-id "09" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2808 :al-overhead-at-end 116 :internal-dur-at-end 668 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3142 :pcs-gap 0 ) true 1 1 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. /private/var/folders/wh/0x5fvqs94vlbcd6sbksx90nh0002dp/T/OPVisit1511605815478914168.xml The science goal is to observe the faint galaxies in the quasar field that are connected to two known absorbers at z=0.47 and z=0.48. We choose the orientation such that the closest of those galaxies are not obstructed by the diffraction spikes in the quasar PSF. 1581839863000 72.54971311493159 (Tic-Visit :proposal-id 15939 :visit-id "10" :proposal-version -1 :trans-version "20200619" :date "29-Sep-2020 13:23:57.0" :trans-errors '(:WARNINGS 2 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 2 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 2310000 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15939 :visit-id "10" :obset-id "10" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15939 :visit-id "10" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2823 :al-overhead-at-end 116 :internal-dur-at-end 0 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3157 :pcs-gap 0 ) (Tic-Orbit :proposal-id 15939 :visit-id "10" :orbit-number 2 :pcs-time 392 :si-vis-utilization 2855 :al-overhead-at-end 116 :internal-dur-at-end 668 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3157 :pcs-gap 0 ) true 2 2 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. /private/var/folders/wh/0x5fvqs94vlbcd6sbksx90nh0002dp/T/OPVisit6990433174314877516.xml The science goal is to observe the faint galaxies in the quasar field that are connected to a known absorbers at z=0.74. 1590913323000 112.33209109146821 (Tic-Visit :proposal-id 15939 :visit-id "11" :proposal-version -1 :trans-version "20200619" :date "29-Sep-2020 13:23:58.0" :trans-errors '(:WARNINGS 3 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 3 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 3465008 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15939 :visit-id "11" :obset-id "11" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15939 :visit-id "11" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2808 :al-overhead-at-end 123 :internal-dur-at-end 0 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3142 :pcs-gap 0 ) (Tic-Orbit :proposal-id 15939 :visit-id "11" :orbit-number 2 :pcs-time 392 :si-vis-utilization 2840 :al-overhead-at-end 116 :internal-dur-at-end 0 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3142 :pcs-gap 0 ) (Tic-Orbit :proposal-id 15939 :visit-id "11" :orbit-number 3 :pcs-time 392 :si-vis-utilization 2840 :al-overhead-at-end 116 :internal-dur-at-end 668 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3142 :pcs-gap 0 ) true 3 3 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. /private/var/folders/wh/0x5fvqs94vlbcd6sbksx90nh0002dp/T/OPVisit9027113679323406949.xml The science goal is to observe the faint galaxies in the quasar field that are connected to a known absorbers at z=0.74. (Tic-Visit :proposal-id 15939 :visit-id "18" :proposal-version -1 :trans-version "20200619" :date "29-Sep-2020 13:23:59.0" :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 1154992 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15939 :visit-id "18" :obset-id "18" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15939 :visit-id "18" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2758 :al-overhead-at-end 116 :internal-dur-at-end 668 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3142 :pcs-gap 0 ) true 1 0 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. /private/var/folders/wh/0x5fvqs94vlbcd6sbksx90nh0002dp/T/OPVisit2976291322811324685.xml The science goal is to observe the faint galaxies in the quasar field that are connected to a known absorbers at z=0.54. We choose the orientation such that the closest of those galaxies are not obstructed by the diffraction spikes in the quasar PSF. 1589375273000 111.0 (Tic-Visit :proposal-id 15939 :visit-id "12" :proposal-version -1 :trans-version "20200619" :date "29-Sep-2020 13:24:00.0" :trans-errors '(:WARNINGS 3 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 3 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 3465008 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15939 :visit-id "12" :obset-id "12" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15939 :visit-id "12" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2808 :al-overhead-at-end 123 :internal-dur-at-end 0 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3142 :pcs-gap 0 ) (Tic-Orbit :proposal-id 15939 :visit-id "12" :orbit-number 2 :pcs-time 392 :si-vis-utilization 2840 :al-overhead-at-end 116 :internal-dur-at-end 0 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3142 :pcs-gap 0 ) (Tic-Orbit :proposal-id 15939 :visit-id "12" :orbit-number 3 :pcs-time 392 :si-vis-utilization 2840 :al-overhead-at-end 116 :internal-dur-at-end 668 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3142 :pcs-gap 0 ) true 3 3 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. /private/var/folders/wh/0x5fvqs94vlbcd6sbksx90nh0002dp/T/OPVisit11139230297846689368.xml The science goal is to observe the faint galaxies in the quasar field that are connected to a known absorbers at z=0.61. We choose the orientation such that the closest of those galaxies are not obstructed by the diffraction spikes in the quasar PSF. (Tic-Visit :proposal-id 15939 :visit-id "13" :proposal-version -1 :trans-version "20200619" :date "29-Sep-2020 13:24:01.0" :trans-errors '(:WARNINGS 3 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 3 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 3465008 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15939 :visit-id "13" :obset-id "13" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15939 :visit-id "13" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2808 :al-overhead-at-end 123 :internal-dur-at-end 0 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3142 :pcs-gap 0 ) (Tic-Orbit :proposal-id 15939 :visit-id "13" :orbit-number 2 :pcs-time 392 :si-vis-utilization 2840 :al-overhead-at-end 116 :internal-dur-at-end 0 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3142 :pcs-gap 0 ) (Tic-Orbit :proposal-id 15939 :visit-id "13" :orbit-number 3 :pcs-time 392 :si-vis-utilization 2840 :al-overhead-at-end 116 :internal-dur-at-end 668 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3142 :pcs-gap 0 ) true 3 3 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. /private/var/folders/wh/0x5fvqs94vlbcd6sbksx90nh0002dp/T/OPVisit2347597299271242582.xml The science goal is to observe the faint galaxies in the quasar field that are connected to two known absorbers at z=0.61 and z=0.69. We choose the orientation such that the closest of those galaxies are not obstructed by the diffraction spikes in the quasar PSF. 1590771187000 121.0 (Tic-Visit :proposal-id 15939 :visit-id "14" :proposal-version -1 :trans-version "20200619" :date "29-Sep-2020 13:24:02.0" :trans-errors '(:WARNINGS 3 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 3 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 3465008 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15939 :visit-id "14" :obset-id "14" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15939 :visit-id "14" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2808 :al-overhead-at-end 123 :internal-dur-at-end 0 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3142 :pcs-gap 0 ) (Tic-Orbit :proposal-id 15939 :visit-id "14" :orbit-number 2 :pcs-time 392 :si-vis-utilization 2840 :al-overhead-at-end 116 :internal-dur-at-end 0 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3142 :pcs-gap 0 ) (Tic-Orbit :proposal-id 15939 :visit-id "14" :orbit-number 3 :pcs-time 392 :si-vis-utilization 2840 :al-overhead-at-end 116 :internal-dur-at-end 668 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3142 :pcs-gap 0 ) true 3 3 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. /private/var/folders/wh/0x5fvqs94vlbcd6sbksx90nh0002dp/T/OPVisit12118834182371590464.xml The science goal is to observe the faint galaxies in the quasar field that are connected to a known absorbers at z=0.56. 1590862838000 145.13282909378609 (Tic-Visit :proposal-id 15939 :visit-id "15" :proposal-version -1 :trans-version "20200619" :date "29-Sep-2020 13:24:03.0" :trans-errors '(:WARNINGS 3 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 3 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 3465008 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15939 :visit-id "15" :obset-id "15" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15939 :visit-id "15" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2808 :al-overhead-at-end 123 :internal-dur-at-end 0 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3142 :pcs-gap 0 ) (Tic-Orbit :proposal-id 15939 :visit-id "15" :orbit-number 2 :pcs-time 392 :si-vis-utilization 2840 :al-overhead-at-end 116 :internal-dur-at-end 0 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3142 :pcs-gap 0 ) (Tic-Orbit :proposal-id 15939 :visit-id "15" :orbit-number 3 :pcs-time 392 :si-vis-utilization 2840 :al-overhead-at-end 116 :internal-dur-at-end 668 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3142 :pcs-gap 0 ) true 3 3 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. /private/var/folders/wh/0x5fvqs94vlbcd6sbksx90nh0002dp/T/OPVisit3486229626567347368.xml The science goal is to observe the faint galaxies in the quasar field that are connected to a known absorbers at z=0.79. We choose the orientation such that the closest of those galaxies are not obstructed by the diffraction spikes in the quasar PSF. 1584737353000 270.0 (Tic-Visit :proposal-id 15939 :visit-id "16" :proposal-version -1 :trans-version "20200619" :date "29-Sep-2020 13:24:04.0" :trans-errors '(:WARNINGS 2 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 3 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 3284912 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15939 :visit-id "16" :obset-id "16" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15939 :visit-id "16" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2821 :al-overhead-at-end 116 :internal-dur-at-end 0 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3157 :pcs-gap 0 ) (Tic-Orbit :proposal-id 15939 :visit-id "16" :orbit-number 2 :pcs-time 392 :si-vis-utilization 2853 :al-overhead-at-end 116 :internal-dur-at-end 31 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3157 :pcs-gap 0 ) (Tic-Orbit :proposal-id 15939 :visit-id "16" :orbit-number 3 :pcs-time 392 :si-vis-utilization 2699 :al-overhead-at-end 0 :internal-dur-at-end 291 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3157 :pcs-gap 0 ) true 3 2 The scheduling data was generated by CASM 28.2. CASM was run in Phase II mode. /private/var/folders/wh/0x5fvqs94vlbcd6sbksx90nh0002dp/T/OPVisit163765452649446642.xml The science goal is to observe the faint galaxies in the quasar field that are connected to a known absorbers at z=0.60. 1578286706000 66.21557415603391 (Tic-Visit :proposal-id 15939 :visit-id "17" :proposal-version -1 :trans-version "20200619" :date "29-Sep-2020 13:24:05.0" :trans-errors '(:WARNINGS 3 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 3 :saa-model "29" :si-bright-earth-limb-angle 20.0 :data-volume 3465008 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15939 :visit-id "17" :obset-id "17" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15939 :visit-id "17" :orbit-number 1 :pcs-time 383 :si-vis-utilization 2808 :al-overhead-at-end 123 :internal-dur-at-end 0 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3142 :pcs-gap 0 ) (Tic-Orbit :proposal-id 15939 :visit-id "17" :orbit-number 2 :pcs-time 392 :si-vis-utilization 2840 :al-overhead-at-end 116 :internal-dur-at-end 0 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3142 :pcs-gap 0 ) (Tic-Orbit :proposal-id 15939 :visit-id "17" :orbit-number 3 :pcs-time 392 :si-vis-utilization 2840 :al-overhead-at-end 116 :internal-dur-at-end 668 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3142 :pcs-gap 0 ) true 3 3