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<HSTProposal
   Phase1ID="691"
   Phase2ID="10937"
   Phase="Phase I"
   AptVersion="Version 15.0 ">
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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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            AptVersion="Version 15.0 "
            SubmissionCounter="1"
            SubmissionSuccessCounter="0"
            HasErrors="false"
            Cycle="15"
            IncludeSysInfo="true"
            NotificationAddress="bouwens@astro.uco.lick"
            AssignedID="691">
            
            <SystemInformation
               os.arch="ppc"
               os.name="Mac OS X"
               os.version="10.4.4"
               java.version="1.4.2_09"
               linux.distribution="not available"
               linux.version="not available" />
            
            <SubmissionComments />
            
            <SubmissionLog>  Assigned ID: 691
----- Submission 1 (Sat Jan 28 00:54:16 GMT 2006) -----
</SubmissionLog>
            
            <DiagnosticJustification />
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   <ProposalInformation
      Category="AR"
      PureParallelProposal="false"
      Cycle="15">
      
      <Title>Probing the Galaxy Population at z~7-10 Using Archival ACS + NICMOS data</Title>
      
      <Abstract>Recent searches for galaxies at z&gt;=7 have placed a great deal of emphasis on obtaining ultra deep infrared observations to probe down to extremely faint luminosities, either through gravitational lensing or by extremely deep observations with NICMOS.  However, to fully understand the evolution of a galaxy population, it is important to cover significant areas as well, both to probe evolution at the bright end of the luminosity function and to locate objects capable for follow-up in other wavebands.  We propose to complement current deep studies of the high redshift universe by conducting a comprehensive search for z&gt;=7 objects in all HST fields in the archive with deep ACS and NICMOS data.  Particular emphasis will be  given to the NICMOS data over the GOODS fields.  With current data, we expect to more than quadruple the sizes of current z&gt;=7 samples. In addition to the clear science objectives of this search, the legacy of this program will be a homogeneous reduction of all NICMOS data (~1500 orbits) over the two GOODS fields.</Abstract>
      
      <PrincipalInvestigator
         Honorific="Dr."
         FirstName="Rychard"
         LastName="Bouwens"
         ESAMember="false"
         UniqueID="6910"
         AddressVerifiedCycle="15">
         
         <Address
            Institution="University of California - Santa Cruz"
            USState="CA"
            Country="USA" />
      </PrincipalInvestigator>
      
      <CoInvestigator
         Honorific="Prof."
         FirstName="Garth"
         MiddleInitial="D."
         LastName="Illingworth"
         ESAMember="false"
         UniqueID="2955"
         AdminUSPI="false"
         Contact="false"
         AddressVerifiedCycle="15">
         
         <Address
            Institution="University of California - Santa Cruz"
            USState="CA"
            Country="USA" />
      </CoInvestigator>
      
      <CoInvestigator
         Honorific="Dr."
         FirstName="Wei"
         LastName="Zheng"
         ESAMember="false"
         UniqueID="3914"
         AdminUSPI="false"
         Contact="false"
         AddressVerifiedCycle="15">
         
         <Address
            Institution="The Johns Hopkins University"
            USState="MD"
            Country="USA" />
      </CoInvestigator>
      
      <CoInvestigator
         Honorific="Mr."
         FirstName="Daniel"
         MiddleInitial="K."
         LastName="Magee"
         ESAMember="false"
         AdminUSPI="false"
         Contact="false"
         AddressVerifiedCycle="15">
         
         <Address
            Institution="University of California - Santa Cruz"
            USState="CA"
            Country="USA" />
      </CoInvestigator>
      
      <CoInvestigator
         Honorific="Dr."
         FirstName="Marijn"
         LastName="Franx"
         ESAMember="true"
         UniqueID="699"
         AdminUSPI="false"
         Contact="false"
         AddressVerifiedCycle="15">
         
         <Address
            Institution="Universiteit Leiden"
            Country="Netherlands" />
      </CoInvestigator>
      
      <CoInvestigator
         Honorific="Dr."
         FirstName="John"
         MiddleInitial="P."
         LastName="Blakeslee"
         ESAMember="false"
         UniqueID="4820"
         AdminUSPI="false"
         Contact="false"
         AddressVerifiedCycle="15">
         
         <Address
            Institution="Washington State University"
            USState="WA"
            Country="USA" />
      </CoInvestigator>
      
      <Questions>
         
         <Phase2Questions>
            
            <ObservingDescription />
            
            <RealtimeJustification />
            
            <CalibrationJustification />
            
            <AdditionalComments />
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      <Orbits
         ThisCycle2GyroPrimary="1"
         ThisCycle2GyroParallel="0"
         NextCycle2GyroPrimary="0"
         NextCycle2GyroParallel="0"
         AfterNext2GyroPrimary="0"
         AfterNext2GyroParallel="0" />
      
      <Phase1ProposalInformation
         TotalTargets="1"
         Attachment="/Users/magee/rych_prop/phase15-AR.pdf">
         
         <ScientificCategory>COSMOLOGY</ScientificCategory>
         
         <ScientificKeyword1
            Keyword="GALAXY FORMATION AND EVOLUTION" />
         
         <ScientificKeyword2
            Keyword="HIGH REDSHIFT GALAXIES" />
         
         <ScientificKeyword3
            Keyword="HUBBLE DEEP FIELDS" />
         
         <ProprietaryPeriod>12</ProprietaryPeriod>
         
         <Budget>140000.00</Budget>
         
         <CalibProp>false</CalibProp>
         
         <SpitzerHours>0.0</SpitzerHours>
         
         <SpitzerLarge>false</SpitzerLarge>
         
         <Treasury>false</Treasury>
         
         <Legacy>true</Legacy>
         
         <Theory>false</Theory>
         
         <LargeProgram>false</LargeProgram>
      </Phase1ProposalInformation>
      
      <Phase2ProposalInformation
         PCFlag="false">
         
         <Availability>SUPPORTED</Availability>
      </Phase2ProposalInformation>
   </ProposalInformation>
   
   <Targets />
   
   <Observations />
   
   <Patterns />
   
   <Visits />
</HSTProposal>


