The GOGREEN Survey: The Relationship between Quenching, Morphological Transformation and Size Growth of Satellite Galaxies

0 Assigned ID: 714 ----- Attempting Submission 1 (Fri Apr 07 18:28:33 GMT 2017) ----- HST Phase I Proposal 714 (apt.v5.apt) successfully submitted. Receipt: # 714-1 ----- Attempting Submission 2 (Fri Apr 07 22:07:44 GMT 2017) ----- HST Phase I Proposal 714 (apt.v6.pdf.apt) successfully submitted. Receipt: # 714-2 ----- Attempting Submission 3 (Fri Apr 07 23:58:31 GMT 2017) ----- 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 #18th Dec 2018 We updated the visit ("J1051 Reorient (27)") with an ORIENT of 137+-3 deg. The center is offset slightly to optimize the number of spectroscopically confirmed cluster members within the field of view. #14th Dec 2018 We were informed by Patricia Royle on Dec 7th 2018 that there were new rules for guide star selection and the visit ("J1051 Visit B") need to be revised. We have created a new source and a new visit ("J1051 Reorient (27)") with ORIENT 270 degree and a constrain of +-20. The center is offset slightly from J1051 to optimize the number of spectroscopically confirmed cluster members within the field of view. #16th Nov 2018 Following approval for HOPR 91300, as requested by Patricia Royle, we have added a new visit ("J0035 Revisit (26)") with a modified pointing RA and DEC. We have also removed the ORIENT constraint. Each cluster will be imaged in a 2x1 mapping. The visit is designed to begin by pointing to the cluster center and then exposure 1-4 will be offset with POS TARG Y-offset: +55.25 arcsec, exposure 5-8 will be offset with POS TARG Y-offset: -55.25 arcsec. Please be aware of the size of the offset and the direction when selecting guide stars to avoid losing acquisition time. Some of the visits have significant (185s) unused orbital visibility. Do you advise employing an additional shorter exposure to fill up the orbit? -483777426 ----- Attempting Submission 1 (Thu Jul 20 20:26:53 GMT 2017) ----- ----- Attempting Submission 2 (Fri Nov 16 23:50:00 GMT 2018) ----- ----- Attempting Submission 3 (Sat Dec 15 03:51:38 GMT 2018) ----- HST Phase II Proposal 15294 (APT_afterdelete.apt) successfully submitted. Receipt: # 15294-3 ----- Attempting Submission 4 (Tue Dec 18 18:58:58 GMT 2018) ----- We have already run the Orbit and Visit planner, but this warning keeps popping up when we try to resubmit. The GOGREEN Survey: The Relationship between Quenching, Morphological Transformation and Size Growth of Satellite Galaxies Despite a dramatic build-up in the number of quenched galaxies at z < 2, it is still entirely unclear how this quenching comes about. Potential quenching mechanisms fall into two categories: processes that act on "centrals" and those that act on "satellites". While both hydrodynamic and semi-analytic models do a good job of predicting the quenched fraction of centrals, they overpredict the fraction of quenched satellite galaxies, reflecting our much greater uncertainty about how "environmental" quenching occurs. Our 55-night Gemini Observatory "Large and Long Program" GOGREEN survey is obtaining optical spectroscopy for an unprecedentedly large sample of > 1000 members of 12 Coma- and Virgo-mass progenitor clusters at 1 < z < 1.5 (and > 600 field galaxies). Here, we propose for WFC3/F160W imaging of the GOGREEN sample to 1) measure the relative timing of star-formation quenching and morphological transformation, 2) make the first high-z measurement of satellite quenching by controlling for intrinsic quenching, and 3) constrain the dominant driver of size growth in the early-type population. Our team has the modeling framework to interpret the trends and to place unrivaled constraints on the physical processes that underlie environmental quenching and morphological transformation from late- to early-type galaxies. Because of Gemini Observatory's huge investment in the GOGREEN program, this survey will return the premier high-redshift cluster spectroscopic dataset for the foreseeable future. All reduced images, spectra and catalogs will be made publicly available, including catalogs from the F160W observations proposed here. 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(Tic-Visit :proposal-id 15294 :visit-id "23" :proposal-version -1 :trans-version "20181130" :date "18-Dec-2018 10:58:23.0" :trans-errors '(:WARNINGS 2 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 2 :saa-model "30" :si-bright-earth-limb-angle 20.0 :data-volume 2228336 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15294 :visit-id "23" :obset-id "23" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15294 :visit-id "23" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3042 :al-overhead-at-end 0 :internal-dur-at-end 0 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3333 :pcs-gap 0 ) (Tic-Orbit :proposal-id 15294 :visit-id "23" :orbit-number 2 :pcs-time 302 :si-vis-utilization 3042 :al-overhead-at-end 0 :internal-dur-at-end 538 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3333 :pcs-gap 0 ) true 2 2 1545159505305 The scheduling data was generated by CASM 26.2.2. CASM was run in Phase II mode. /private/var/folders/6l/095d9s414c374r_b8ztgw4gr0000gn/T/OPVisit4338378155071239469.xml Exposure 1-8 are for pointing A (POS TARG Y-offset: +55.25) (8 dithers) Exposure 9-16 are for pointing B (POS TARG Y-offset: -55.25) (8 dithers) Exposure 1-8 used NSAMP=15 instead 14 to fill in the unused orbital visibility. 1522148519000 232.67414419964945 (Tic-Visit :proposal-id 15294 :visit-id "24" :proposal-version -1 :trans-version "20181130" :date "18-Dec-2018 10:58:25.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 2 :saa-model "30" :si-bright-earth-limb-angle 20.0 :data-volume 2228336 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15294 :visit-id "24" :obset-id "24" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15294 :visit-id "24" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3042 :al-overhead-at-end 0 :internal-dur-at-end 0 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3389 :pcs-gap 0 ) (Tic-Orbit :proposal-id 15294 :visit-id "24" :orbit-number 2 :pcs-time 302 :si-vis-utilization 3042 :al-overhead-at-end 0 :internal-dur-at-end 538 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3389 :pcs-gap 0 ) true 2 0 1545159507435 The scheduling data was generated by CASM 26.2.2. CASM was run in Phase II mode. /private/var/folders/6l/095d9s414c374r_b8ztgw4gr0000gn/T/OPVisit541847264910844477.xml Exposure 1-8 are for pointing A (POS TARG Y-offset: +55.25) (8 dithers) Exposure 9-16 are for pointing B (POS TARG Y-offset: -55.25) (8 dithers) Exposure 1-8 used NSAMP=15 instead 14 to fill in the unused orbital visibility. 1532317781000 245.0 (Tic-Visit :proposal-id 15294 :visit-id "25" :proposal-version -1 :trans-version "20181130" :date "18-Dec-2018 10:58:27.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 2 :saa-model "30" :si-bright-earth-limb-angle 20.0 :data-volume 2228336 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15294 :visit-id "25" :obset-id "25" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15294 :visit-id "25" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3042 :al-overhead-at-end 0 :internal-dur-at-end 0 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3389 :pcs-gap 0 ) (Tic-Orbit :proposal-id 15294 :visit-id "25" :orbit-number 2 :pcs-time 302 :si-vis-utilization 3042 :al-overhead-at-end 0 :internal-dur-at-end 538 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3389 :pcs-gap 0 ) true 2 0