The previous submission contained a small error in POS TARGs for 8 exposures. ----- Attempting Submission 1 (Mon Sep 26 07:41:41 GMT 2011) ----- HST Phase II Proposal 12332 (12332.apt) successfully submitted. ----- Attempting Submission 2 (Mon Sep 26 17:44:13 GMT 2011) ----- Remaining diagnostic messages are related to the visits that have already been executed. WFC3 imaging of z=6 QSO hosts: Zooming in on the First L>L* Galaxies & their Surroundings This project will study the first massive galaxies and their surroundings at z=6. In WMAP cosmology, there is just enough time (<0.5-0.8 Gyr) since z=10-20 to collapse such a galaxy by z=6. The brightest SDSS QSOs at z=6 may have been hosted by the most massive and luminous galaxies with L>L*. Surprisingly, recent CO studies suggest relatively large masses, and IR-spectra suggest solar Fe/H and significant stellar processing. However, the z=6 host galaxies have not yet been found. We show that this can be done with the WFC3 and careful PSF subtraction. Our program is well beyond the capability of ground-based (AO) facilities. This must be done before HST stops working: 20 WFC3 orbits in J+H will measure the restframe UV-flux of the luminous host galaxies of two SDSS QSOs at z=6. Such galaxies likely have AB~23--24 mag and half-light radii ~0.3-0.5" (~2-3 kpc). WFC3 can detect >60% of the host galaxy flux outside the central peak of the PSF at >20 sigma, and will also detect surrounding fainter structures at z=6. A significant detection of even a few very luminous galaxies at z~6 is critical to constrain: (a) their luminosity & color-profiles, and their physical properties; (b) the process of hierarchical galaxy formation; and (c) the formation history of supermassive black holes.
Two 5-orbit packages, oriented 45 degrees apart, to observe an SDSS z~6 QSO and a nearby star as a PSF model for eventual subtraction. Each 5-orbit package consists of 3 QSO observations and 2 PSF star observations, interleaved to sample both intra-orbit and inter-orbit variations in the PSF (due to spacecraft breathing, etc). COSMOLOGY 0 false 0.0 0 false false false false SUPPORTED GALAXY HIGH REDSHIFT GALAXY QSO This object was generated by the targetselector and retrieved from the SIMBAD database. J2000 J2000 STAR M V-IV This object was generated by the targetselector and retrieved from the SIMBAD database. 2MASS-J12183076+5355181 J2000 J2000 J-Band 16.002 STAR M V-IV This object was generated by the targetselector and retrieved from the SIMBAD database. J2000 J2000 16.27 J mag STAR M V-IV This object was generated by the targetselector and retrieved from the SIMBAD database. J2000 J2000 16.12 J mag GALAXY HIGH REDSHIFT GALAXY QSO This object was generated by the targetselector and retrieved from the NED database. J2000 J 19.87 STAR G V-IV This object was generated by the targetselector and retrieved from the NED database. J2000 SDSS z' (AB) 17.68 NIC2 Imaging Yes No F110W NIC2 Imaging Yes No F160W NIC2 Imaging Yes No F110W NIC2 Imaging Yes No F160W NIC1 Imaging No No F110W NIC1 Imaging No No F160W NIC1 Imaging No No F110W NIC1 Imaging No No F160W ACS/WFC Imaging No No F775W ACS/WFC Imaging No No F850LP ACS/WFC Imaging No No F775W ACS/WFC Imaging No No F850LP NIC2 Imaging Yes No F110W NIC2 Imaging Yes No F160W NIC2 Imaging Yes No F110W NIC2 Imaging Yes No F160W NIC1 Imaging No No F110W NIC1 Imaging No No F160W NIC1 Imaging No No F110W NIC1 Imaging No No F160W ACS/WFC Imaging No No F775W ACS/WFC Imaging No No F850LP ACS/WFC Imaging No No F775W ACS/WFC Imaging No No F850LP Timing link suitability includes constraints ([02 After 01 by 0.1 to 0.1 days]) Same orient constraint links visits (01 03 05) The scheduling data was generated by CASM 19.3. CASM was run in Phase II mode. /Users/mrm/Dropbox/WIP/TTRBLetter/second QSO APT/OP-cache/12332-v01.xml First orbit of QSO observations To ensure maximum thermal stability (and thus PSF stability) for these PSF-sensitive observations, we request one of the following constraints, _if possible and if they do not interfere with the schedulability of other programs_. 1) If our observations occur directly after an SAA transit, that the telescope be slewed to our initial pointing _before_ the SAA transit, allowing thermal settling to occur during the transit. 2) Our observations occur directly after observations on a nearby target (e.g. in the Virgo cluster), to minimize the change in pointing angle (and thus thermal settling time) at the beginning of our observations. 1296485345000 225.0 (Tic-Visit :proposal-id 12332 :visit-id "01" :proposal-version -1 :trans-version "20110811" :date "25-Sep-2011 14:15:40.0" :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 772528 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12332 :visit-id "01" :obset-id "01" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12332 :visit-id "01" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3003 :al-overhead-at-end 0 :internal-dur-at-end 635 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3445 :pcs-gap 0 ) true 1 0 Timing link suitability includes constraints ([02 After 01 by 0.1 to 0.1 days] [03 After 02 by 0.1 to 0.1 days]) The scheduling data was generated by CASM 19.3. 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CASM was run in Phase II mode. /Users/mrm/Dropbox/WIP/TTRBLetter/second QSO APT/OP-cache/12332-v06.xml +45 degrees, First orbit of QSO observations NOTE ON ORIENTATION REQUIREMENT We'd like the second set of 5 orbits to orient exactly 45 degrees from the first set of 5, but this relaxable in the event that we are unschedulable 1291556486000 296.0 (Tic-Visit :proposal-id 12332 :visit-id "06" :proposal-version -1 :trans-version "20110811" :date "25-Sep-2011 14:16:11.0" :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 772528 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12332 :visit-id "06" :obset-id "06" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12332 :visit-id "06" :orbit-number 1 :pcs-time 333 :si-vis-utilization 3003 :al-overhead-at-end 0 :internal-dur-at-end 635 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3445 :pcs-gap 0 ) true 1 0 Timing link suitability includes constraints ([07 After 06 by 0.1 to 0.1 days] [08 After 07 by 0.1 to 0.1 days]) The scheduling data was generated by CASM 19.3. 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CASM was run in Phase II mode. To ensure maximum thermal stability (and thus PSF stability) for these PSF-sensitive observations, we request one of the following constraints, _if possible and if they do not interfere with the schedulability of other programs_. 1) If our observations occur directly after an SAA transit, that the telescope be slewed to our initial pointing _before_ the SAA transit, allowing thermal settling to occur during the transit. 2) Our observations occur directly after observations on a nearby target, to minimize the change in pointing angle (and thus thermal settling time) at the beginning of our observations. 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CASM was run in Phase II mode. (Tic-Visit :proposal-id 12332 :visit-id "14" :proposal-version -1 :trans-version "20110811" :date "26-Sep-2011 10:43:55.0" :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 307216 :tdrss-contact-duration 0 :coron NIL ) (Tic-Obset :proposal-id 12332 :visit-id "14" :obset-id "14" :pcs-mode "FGS" ) (Tic-Orbit :proposal-id 12332 :visit-id "14" :orbit-number 1 :pcs-time 333 :si-vis-utilization 2591 :al-overhead-at-end 0 :internal-dur-at-end 419 :dark-offset NIL :dark-utilization 0 :max-dark-utilization 1920 :low-sky "N" :pcs-visibility 3234 :pcs-gap 0 ) true 1 0 /Users/mrm/Dropbox/WIP/TTRBLetter/second QSO APT/OP-cache/12332-v11.xml Timing link suitability includes constraints ([12 After 11 by 0.3 to 0.3 days]) The scheduling data was generated by CASM 19.3. CASM was run in Phase II mode. To ensure maximum thermal stability (and thus PSF stability) for these PSF-sensitive observations, we request one of the following constraints, _if possible and if they do not interfere with the schedulability of other programs_. 1) If our observations occur directly after an SAA transit, that the telescope be slewed to our initial pointing _before_ the SAA transit, allowing thermal settling to occur during the transit. 2) Our observations occur directly after observations on a nearby target, to minimize the change in pointing angle (and thus thermal settling time) at the beginning of our observations. 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