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<HSTProposal
   Phase1ID="306"
   Phase2ID="11262"
   Phase="Phase I"
   AptVersion="Version 16.0.2 ">
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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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         <SubmissionData
            AptVersion="Version 16.0.2 "
            SubmissionCounter="3"
            SubmissionSuccessCounter="2"
            HasErrors="false"
            Cycle="16"
            IncludeSysInfo="true"
            NotificationAddress="koekemoe@stsci.edu"
            AssignedID="306">
            
            <SystemInformation
               os.arch="x86"
               os.name="Windows 2000"
               os.version="5.0"
               java.version="1.5.0_08"
               linux.distribution="not available"
               linux.version="not available" />
            
            <SubmissionComments />
            
            <SubmissionLog>  Assigned ID: 306
----- Attempting Submission 1 (Fri Jan 26 18:00:35 GMT 2007) -----
  Phase I Proposal 306 (prop1) successfully submitted.
----- Attempting Submission 3 (Sat Jan 27 00:30:02 GMT 2007) -----
</SubmissionLog>
            
            <DiagnosticJustification />
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   <ProposalInformation
      Category="AR"
      PureParallelProposal="false"
      Cycle="16"
      STScIEditNumber="0">
      
      <Title>Deepening the Hubble UDF - Constraining the High-z Galaxy Luminosity Function Faint End Slope and Reionization</Title>
      
      <Abstract>We propose to significantly improve the depth of the Hubble Ultra Deep Field (UDF) by ~0.4-0.5 magnitudes (equivalent to doubling the exposure time of the original UDF), through recalibrating and reprocessing the original UDF ACS data with improved reference files and new techniques to remove a variety of electronic instrumental signatures from the images. Since ACS has now been in operation for almost 5 years, this provides an opportunity to improve significantly upon the original calibration which had been performed using the best available information 18 months after the installation of ACS. Our team has the demonstrated expertise to carry out this recalibration and reprocessing, and we also have the demonstrated ability to release such products to the commmunity on a timely basis. We propose this as an Archival Legacy program because the resulting dataset, as well as the techniques that we are using, will be of great value to the community and should enable significant new science to be obtained from this unique dataset. In addition, the resulting improvements on the number counts of redshift ~6 dropout sources will significantly improve the current uncertainties in this field regarding the faint end slope and normalization of the luminosity function of the redshift ~6 population, and ultimately the role played by these sources in reionizing the universe.</Abstract>
      
      <PrincipalInvestigator
         Honorific="Dr."
         FirstName="Anton"
         MiddleInitial="M."
         LastName="Koekemoer"
         ESAMember="false"
         UniqueID="3952"
         AddressVerifiedCycle="16">
         
         <Address
            Institution="Space Telescope Science Institute"
            USState="MD"
            Country="USA" />
      </PrincipalInvestigator>
      
      <CoInvestigator
         Honorific="Dr."
         FirstName="Massimo"
         LastName="Stiavelli"
         ESAMember="false"
         UniqueID="2484"
         AdminUSPI="false"
         Contact="false"
         AddressVerifiedCycle="16">
         
         <Address
            Institution="Space Telescope Science Institute"
            USState="MD"
            Country="USA" />
      </CoInvestigator>
      
      <CoInvestigator
         Honorific="Mr."
         FirstName="Louis"
         LastName="Bergeron"
         ESAMember="false"
         UniqueID="3435"
         AdminUSPI="false"
         Contact="false"
         AddressVerifiedCycle="16">
         
         <Address
            Institution="Space Telescope Science Institute"
            USState="MD"
            Country="USA" />
      </CoInvestigator>
      
      <CoInvestigator
         Honorific="Dr."
         FirstName="Steven"
         LastName="Beckwith"
         ESAMember="false"
         UniqueID="157"
         AdminUSPI="false"
         Contact="false"
         AddressVerifiedCycle="16">
         
         <Address
            Institution="Space Telescope Science Institute"
            USState="MD"
            Country="USA" />
      </CoInvestigator>
      
      <Questions>
         
         <Phase2Questions>
            
            <ObservingDescription />
            
            <RealtimeJustification />
            
            <CalibrationJustification />
            
            <AdditionalComments />
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      </Questions>
      
      <Orbits
         ThisCycle2GyroPrimary="1"
         ThisCycle2GyroParallel="0"
         NextCycle2GyroPrimary="0"
         NextCycle2GyroParallel="0"
         AfterNext2GyroPrimary="0"
         AfterNext2GyroParallel="0" />
      
      <Phase1ProposalInformation
         TotalTargets="1"
         Attachment="C:\apt - proposals\Cycle 16 - 2007a - UDF AR Legacy\prop_final.pdf">
         
         <ScientificCategory>COSMOLOGY</ScientificCategory>
         
         <ScientificKeyword1
            Keyword="GALAXY FORMATION AND EVOLUTION" />
         
         <ScientificKeyword2
            Keyword="GALAXY MORPHOLOGY AND STRUCTURE" />
         
         <ScientificKeyword3
            Keyword="HIGH REDSHIFT GALAXIES" />
         
         <ScientificKeyword4
            Keyword="HUBBLE DEEP FIELDS" />
         
         <ProprietaryPeriod>12</ProprietaryPeriod>
         
         <Budget>62000</Budget>
         
         <CalibProp>false</CalibProp>
         
         <SpitzerHours>0.0</SpitzerHours>
         
         <Treasury>false</Treasury>
         
         <Legacy>true</Legacy>
         
         <Theory>false</Theory>
         
         <LargeProgram>false</LargeProgram>
         
         <Spitzer>false</Spitzer>
         
         <Survey>false</Survey>
      </Phase1ProposalInformation>
      
      <Phase2ProposalInformation
         PCFlag="true">
         
         <Availability>SUPPORTED</Availability>
      </Phase2ProposalInformation>
   </ProposalInformation>
   
   <Targets />
   
   <Observations />
   
   <Datasets>
      
      <Dataset
         Instrument="ACS"
         Number="1"
         NumberOfDatasets="400"
         RetrievalMethod="FTP"
         RetrievalPlan="All ACS/WFC data from Prop. 9978 (PI: Beckwith)" />
   </Datasets>
   
   <Patterns />
   
   <Visits />
</HSTProposal>


