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<HSTProposal
   Phase1ID="597"
   Phase2ID="12496"
   Phase="Phase II"
   AptVersion="Version 20.0.2 ">
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   <!--This file is automatically generated and should not be edited by hand. Editing this file directly is at your own risk.-->
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   <!--APT Version: Version 20.0.2 -->
   <!--Date: Wed Feb 15 14:09:26 GMT 2012-->
   
   <ToolData />
   
   <ProposalInformation
      Category="GO"
      PureParallelProposal="false"
      Cycle="19"
      STScIEditNumber="2">
      
      <Title>A Quasar-Starburst Merger System at z=6.2 ?</Title>
      
      <Abstract>Observations of high-redshift quasars probe the growth of supermassive black holes and their connections to galaxy formation at the earliest epoch. We have been carrying out a systematic survey of the star formation and ISM properties in the host galaxies of z~6 quasars using millimeter dust continuum and molecular CO emission. In this survey, we recently discovered the first z~6 quasar-starburst merger system: radio-loud quasar CFHQS J1429+5447 (z=6.2) is detected as a bright 3.4 mJy source in millimeter continuum; high resolution EVLA imaging of CO(2-1) transition reveals two distinct peaks separated by 1.2" (6.9 kpc), and ~50 km/s in velocity space, strongly suggesting that this is a merging system with two intense star forming components, only one of which is in the active quasar phase. We propose deep HST WFC3/F105W, F140W observations to confirm the merger nature, and measure the size, morphology, UV-based star formation rate, and constrain the UV continuum slope of both the quasar host galaxy and its merging companion galaxy. Comparison of our HST and mm/CO observations  with detailed cosmological simulations of high-redshift quasar formation will place this unique system in the evolutionary sequence of SMBH/galaxy coevolution, and test models of quasar formation. The proposed observation of CFHQS J1429+5447 also provides an important test case for the future high-z quasar host galaxy imaging with HST/JWST and ALMA.</Abstract>
      
      <PrincipalInvestigator
         Honorific="Dr."
         FirstName="Ran"
         LastName="Wang"
         ESAMember="false"
         UniqueID="11873"
         Institution="University of Arizona"
         Country="USA"
         State="AZ" />
      
      <CoInvestigator
         Honorific="Dr."
         FirstName="Chris"
         MiddleInitial="J."
         LastName="Willott"
         ESAMember="false"
         UniqueID="5817"
         Institution="Dominion Astrophysical Observatory"
         Country="CAN"
         State="BC"
         AdminUSPI="false"
         Contact="false" />
      
      <CoInvestigator
         Honorific="Prof."
         FirstName="Xiaohui"
         LastName="Fan"
         ESAMember="false"
         UniqueID="5750"
         Institution="University of Arizona"
         Country="USA"
         State="AZ"
         AdminUSPI="false"
         Contact="false" />
      
      <CoInvestigator
         Honorific="Prof."
         FirstName="Alain"
         LastName="Omont"
         ESAMember="true"
         UniqueID="1980"
         Institution="CNRS, Institut d'Astrophysique de Paris"
         Country="FRA"
         AdminUSPI="false"
         Contact="false" />
      
      <CoInvestigator
         Honorific="Dr."
         FirstName="Chris"
         LastName="Carilli"
         ESAMember="false"
         UniqueID="6477"
         Institution="Associated Universities, Inc."
         Country="USA"
         State="VA"
         AdminUSPI="false"
         Contact="false" />
      
      <CoInvestigator
         Honorific="Dr."
         FirstName="John"
         LastName="Hutchings"
         ESAMember="false"
         UniqueID="992"
         Institution="Dominion Astrophysical Observatory"
         Country="CAN"
         State="BC"
         AdminUSPI="false"
         Contact="false" />
      
      <CoInvestigator
         Honorific="Dr."
         FirstName="Linhua"
         LastName="Jiang"
         ESAMember="false"
         UniqueID="8933"
         Institution="Arizona State University"
         Country="USA"
         State="AZ"
         AdminUSPI="false"
         Contact="false" />
      
      <CoInvestigator
         Honorific="Dr."
         FirstName="Yuexing"
         LastName="Li"
         ESAMember="false"
         UniqueID="11874"
         Institution="The Pennsylvania State University"
         Country="USA"
         State="PA"
         AdminUSPI="false"
         Contact="false" />
      
      <Questions>
         
         <Phase2Questions>
            
            <ObservingDescription>The observations include 5-orbit observations of an CFHQS z=6.2 quasars with WFC3/IR F105W and F140W, and 1-orbit observation of a nearby star to measure the PSF with WFC3/IR F105W and F140W. 
For the observations of the science target, we plan to do the 3-orbits observation with F140W first. Then if possible, please hold the observation for about 10~20 days to let us check the data and decide if we want to continue to do F105W or use the remaining 2 orbits in F140W to improve the S/N.</ObservingDescription>
            
            <RealtimeJustification />
            
            <CalibrationJustification />
            
            <AdditionalComments />
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         AfterNext2GyroParallel="0" />
      
      <Phase1ProposalInformation
         TotalTargets="1"
         Attachment="/Users/astrocat/catwork/proposals/nic11/J1429hst.pdf">
         
         <ScientificCategory>AGN/QUASARS</ScientificCategory>
         
         <ScientificKeyword1
            Keyword="Clusters Of Galaxies" />
         
         <ScientificKeyword2
            Keyword="High Redshift Galaxies" />
         
         <ScientificKeyword3
            Keyword="Interacting And Merging Galaxies" />
         
         <ScientificKeyword4
            Keyword="Radio-Loud Quasars" />
         
         <ScientificKeyword5
            Keyword="Star Formation" />
         
         <ProprietaryPeriod>12</ProprietaryPeriod>
         
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         <MultiCycleTreasury>false</MultiCycleTreasury>
         
         <Theory>false</Theory>
         
         <LargeProgram>false</LargeProgram>
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      <Phase2ProposalInformation
         PCFlag="true">
         
         <Availability>SUPPORTED</Availability>
      </Phase2ProposalInformation>
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         Name="CFHQSJ1429+5447"
         Number="1"
         ReferenceFrame="ICRS"
         Redshift="6.183"
         ProvisionalCoordinates="14 29 52.1700 +54 47 17.60">
         
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         <PrimaryDescription>
            
            <Description>HIGH REDSHIFT GALAXY</Description>
            
            <Description>QSO</Description>
            
            <Description>STARBURST</Description>
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         <Comments>Science target</Comments>
         
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         <PrimaryDescription>
            
            <Description>M III-I</Description>
            
            <Description>M V-IV</Description>
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         <Comments>a star for PSF</Comments>
         
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            <AlternateName>2MASS-J14282482+5443207</AlternateName>
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            <OtherFluxes>J=16.37, H=15.92, Ks=15.25</OtherFluxes>
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         <Comments>3-orbit observations of CFHQSJ1429+5447 with F140W. 
According to BOT, there are four bright 2MASS source J=13 to 16 in the field. We have defined a series of orient ranges. The goal is to avoid contaminations from spikes of the bright stars in the field.</Comments>
         
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                     <StConstraintSchedulingWindows
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                     <AncillaryData
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                        <String>The scheduling data was generated by CASM 19.3.</String>
                        
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         <Comments>2-orbit observations of CFHQSJ1429+5447 with WFC3/IR F105W. 
According to BOT, there are four bright 2MASS source J=13 to 16 in the field. We have defined a series of orient ranges. The goal is to avoid contaminations from spikes of the bright stars in the field.

we plan to do the 3-orbits observation with F140W first. Then if possible, please hold the observation for about 10~20 days to let us check the data and decide if we want to continue to do F105W or use the remaining 2 orbits in F140W to improve the S/N.</Comments>
         
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               Degrees="110" />
            
            <To
               Degrees="175" />
         </Orient>
         
         <Orient>
            
            <From
               Degrees="206" />
            
            <To
               Degrees="255" />
         </Orient>
         
         <Orient>
            
            <From
               Degrees="296" />
            
            <To
               Degrees="336" />
         </Orient>
         
         <AfterVisit
            Visit="01">
            
            <From
               Days="30" />
            
            <To
               Days="40" />
         </AfterVisit>
         
         <SeqWithin>
            
            <VisitList />
         </SeqWithin>
         
         <OnHoldComments />
         
         <ExposureGroup
            Type="Pattern"
            Pattern="1">
            
            <Exposure
               Number="1"
               Label="QSO-exp1-f105w"
               TargetName="CFHQSJ1429+5447"
               Config="WFC3/IR"
               Opmode="MULTIACCUM"
               Aperture="IR"
               SpElement="F105W"
               NumberOfIterations="4"
               WasRunThroughBot="true"
               TimePerExposure="DEF"
               RealtimeAnalysis="false"
               RequiresUplink="false"
               Expand="false"
               LowSky="false"
               Shadow="false"
               NewAlignment="false"
               NewObset="false"
               NewObsetFullAcq="false"
               SpecialCommand="false">
               
               <MaxDur />
               
               <MinDur />
               
               <Comments />
               
               <InstrumentParameters
                  SAMP-SEQ="STEP50"
                  NSAMP="12" />
               
               <SubExposures>
                  
                  <SubExposure
                     PrimaryPatternPosition="1"
                     CopyNumber="1"
                     OrbitNumber="1" />
                  
                  <SubExposure
                     PrimaryPatternPosition="1"
                     CopyNumber="2"
                     OrbitNumber="1" />
                  
                  <SubExposure
                     PrimaryPatternPosition="1"
                     CopyNumber="3"
                     OrbitNumber="1" />
                  
                  <SubExposure
                     PrimaryPatternPosition="1"
                     CopyNumber="4"
                     OrbitNumber="1" />
                  
                  <SubExposure
                     PrimaryPatternPosition="2"
                     CopyNumber="1"
                     OrbitNumber="1" />
                  
                  <SubExposure
                     PrimaryPatternPosition="2"
                     CopyNumber="2"
                     OrbitNumber="1" />
                  
                  <SubExposure
                     PrimaryPatternPosition="2"
                     CopyNumber="3"
                     OrbitNumber="1" />
                  
                  <SubExposure
                     PrimaryPatternPosition="2"
                     CopyNumber="4"
                     OrbitNumber="1" />
                  
                  <SubExposure
                     PrimaryPatternPosition="3"
                     CopyNumber="1"
                     OrbitNumber="2" />
                  
                  <SubExposure
                     PrimaryPatternPosition="3"
                     CopyNumber="2"
                     OrbitNumber="2" />
                  
                  <SubExposure
                     PrimaryPatternPosition="3"
                     CopyNumber="3"
                     OrbitNumber="2" />
                  
                  <SubExposure
                     PrimaryPatternPosition="3"
                     CopyNumber="4"
                     OrbitNumber="2" />
                  
                  <SubExposure
                     PrimaryPatternPosition="4"
                     CopyNumber="1"
                     OrbitNumber="2" />
                  
                  <SubExposure
                     PrimaryPatternPosition="4"
                     CopyNumber="2"
                     OrbitNumber="2" />
                  
                  <SubExposure
                     PrimaryPatternPosition="4"
                     CopyNumber="3"
                     OrbitNumber="2" />
                  
                  <SubExposure
                     PrimaryPatternPosition="4"
                     CopyNumber="4"
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               </SubExposures>
            </Exposure>
         </ExposureGroup>
      </Visit>
      
      <Visit
         Number="03"
         Status="implementation"
         After=""
         Before="">
         
         <ToolData>
            
            <ToolDataItem
               Key="Visit Planner">
               
               <VpVisitData>
                  
                  <StVisitSchedulingWindows
                     Binary="true"
                     UpToDate="true"
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                     <StConstraintSchedulingWindows
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                     <StConstraintSchedulingWindows
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                     <StConstraintSchedulingWindows
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                     <AncillaryData
                        Title="Comments"
                        Label="Comments">
                        
                        <String>The scheduling data was generated by CASM 19.3.</String>
                        
                        <String>CASM was run in Phase II mode.</String>
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                  <AncillaryData
                     Title="Roll Ranges Report"
                     Label="Roll Ranges Report"
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         <Comments>Observations of the PSF star WFC3/IR F105W F140W. 
According to BOT, there are two bright 2MASS source J=13 to 15 close to the edge of the field. We have defined a series of orient ranges. The goal is to avoid contaminations from spikes of the bright stars in the field.</Comments>
         
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