0 Assigned ID: 230 ----- Attempting Submission 1 (Thu Apr 06 15:05:39 GMT 2017) ----- HST Phase I Proposal 230 (new.apt) successfully submitted. Receipt: # 230-1 ----- Attempting Submission 2 (Fri Apr 07 09:06:17 GMT 2017) ----- HST Phase I Proposal 230 (new.apt) successfully submitted. Receipt: # 230-2 ----- Attempting Submission 3 (Fri Apr 07 10:36:26 GMT 2017) ----- HST Phase I Proposal 230 (new.apt) successfully submitted. Receipt: # 230-3 I hope that this is a straightforward program. It is intended to obtain three dithered exposures in F814W of the fields of thirteen different quasars. The quasars are put at the central WFC aperture position. There are three exposures per orbit to allow CR rejection even in the chip gap area. Exposure times are tweaked to fill the orbits. -1427997924 ----- Attempting Submission 1 (Fri Jun 30 10:50:29 GMT 2017) ----- Transport of magnetic fields into the circumgalactic medium Supernova-driven winds are known to play a major role in galaxy evolution, and to drive metal-enriched material far out into the circum-galactic medium. We have demonstrated that magnetic fields in these winds are detectably modifying the polarization properties of background radio quasars with intervening MgII 2799 absorption in their spectra, through Faraday Rotation. We have obtained estimates of the disordered fields within these Faraday screens and wish to map how these vary around galaxies, e.g. whether they are maximal above the poles of the galaxies as we would expect for biconical outflows. We also want to compare our estimates quantitatively with magnetohydrodynamical models that we have been developing. For both investigations, we need to know where the lines of sight pass, relative to the galaxies. For this we need HST resolution images of the host galaxies to establish the orientation and inclination of the disks, and the general morphologies of the galaxies. We have in hand images for 17/30 quasars, and request here images for the remaining 13 sources. This is straightforward imaging of 13 quasar fields using the ACS Galaxies and the IGM 6 false false false false false false SUPPORTED GALAXY QUASAR This object was generated by the targetselector and retrieved from the SIMBAD database. J2000 J2000 GALAXY QUASAR This object was generated by the targetselector and retrieved from the SIMBAD database. J2000 J2000 GALAXY QUASAR This object was generated by the targetselector and retrieved from the SIMBAD database. J2000 J2000 GALAXY QUASAR This object was generated by the targetselector and retrieved from the SIMBAD database. J2000 J2000 GALAXY QUASAR This object was generated by the targetselector and retrieved from the SIMBAD database. J2000 J2000 GALAXY QUASAR This object was generated by the targetselector and retrieved from the SIMBAD database. J2000 J2000 GALAXY QUASAR This object was generated by the targetselector and retrieved from the SIMBAD database. J2000 J2000 GALAXY QUASAR This object was generated by the targetselector and retrieved from the SIMBAD database. J2000 J2000 GALAXY QUASAR This object was generated by the targetselector and retrieved from the SIMBAD database. J2000 J2000 GALAXY QUASAR This object was generated by the targetselector and retrieved from the SIMBAD database. J2000 J2000 GALAXY QUASAR This object was generated by the targetselector and retrieved from the SIMBAD database. J2000 J2000 GALAXY QUASAR This object was generated by the targetselector and retrieved from the SIMBAD database. J2000 J2000 GALAXY QUASAR This object was generated by the targetselector and retrieved from the SIMBAD database. J2000 J2000 ACS/WFC Imaging No No F814W ACS/WFC Imaging No No F814W ACS/WFC Imaging No No F814W ACS/WFC Imaging No No F814W ACS/WFC Imaging No No F814W ACS/WFC Imaging No No F814W ACS/WFC Imaging No No F814W ACS/WFC Imaging No No F814W ACS/WFC Imaging No No F814W ACS/WFC Imaging No No F814W ACS/WFC Imaging No No F814W ACS/WFC Imaging No No F814W ACS/WFC Imaging No No F814W POS-TARG DITHER 3.034 This should be the default 3-point dither to cover the gap and allow CR rejection in the gap. LINE false false 3 85.29 ACS-WFC-DITHER-LINE 1 false /Users/lilly/Other_Science/Project Magnetic Fields/HST_2017/OP-cache/new-v01.xml The scheduling data was generated by CASM 25.2. CASM was run in Phase II mode. 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(Tic-Visit :proposal-id 15282 :visit-id "08" :proposal-version -1 :trans-version "20170613" :date "28-Jun-2017 12:47:17.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "27" :si-bright-earth-limb-angle 20.0 :data-volume 852672 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15282 :visit-id "08" :obset-id "08" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15282 :visit-id "08" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2881 :al-overhead-at-end 0 :internal-dur-at-end 347 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3216 :pcs-gap 0 ) true 1 0 /Users/lilly/Other_Science/Project Magnetic Fields/HST_2017/OP-cache/new-v09.xml The scheduling data was generated by CASM 25.2. CASM was run in Phase II mode. 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(Tic-Visit :proposal-id 15282 :visit-id "12" :proposal-version -1 :trans-version "20170613" :date "28-Jun-2017 12:47:21.0" :trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0 :FATAL-ERRORS 0 :CONTINUABLE-FATALS 0) :number-of-orbits 1 :saa-model "27" :si-bright-earth-limb-angle 20.0 :data-volume 852672 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 15282 :visit-id "12" :obset-id "12" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 15282 :visit-id "12" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2881 :al-overhead-at-end 0 :internal-dur-at-end 347 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3216 :pcs-gap 0 ) true 1 0 /Users/lilly/Other_Science/Project Magnetic Fields/HST_2017/OP-cache/new-v13.xml The scheduling data was generated by CASM 25.2. CASM was run in Phase II mode. 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