<?xml version="1.0" encoding="ISO-8859-1"?>

<HSTProposal
   Phase1ID="1218"
   Phase2ID="11244"
   Phase="Phase I"
   AptVersion="Version 16.0.3 ">
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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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   <ToolData>
      
      <ToolDataItem
         Key="SubmissionData">
         
         <SubmissionData
            AptVersion="Version 16.0.3 "
            SubmissionCounter="1"
            SubmissionSuccessCounter="0"
            HasErrors="false"
            Cycle="16"
            IncludeSysInfo="true"
            NotificationAddress="adolphin@raytheon.com"
            AssignedID="1218">
            
            <SystemInformation
               os.arch="i386"
               os.name="Mac OS X"
               os.version="10.4.8"
               java.version="1.5.0_06"
               linux.distribution="not available"
               linux.version="not available" />
            
            <SubmissionComments />
            
            <SubmissionLog>  Assigned ID: 1218
----- Attempting Submission 1 (Thu Feb 08 22:32:00 MST 2007) -----
</SubmissionLog>
            
            <DiagnosticJustification />
         </SubmissionData>
      </ToolDataItem>
   </ToolData>
   
   <ProposalInformation
      Category="AR"
      PureParallelProposal="false"
      Cycle="16"
      STScIEditNumber="0">
      
      <Title>WFPC2 CTE and Photometric Zero Points</Title>
      
      <Abstract>With charge-transfer efficiency (CTE) losses of several tenths of a magnitude in many current exposures, the accuracy of CTE corrections is a limiting factor in the accuracy of photometry that can be obtained with WFPC2.  However, the CTE corrections in common use are five years old, and thus corrections for CTE loss on current observations are made with the dangerous assumption that CTE loss has continued growing over the past five years at the rate it grew for the instruments first eight years of service.  The uncertainty caused by this assumption implies that the use of these old CTE corrections is the dominant error source in many WFPC2 images, and will become even worse in Cycle 16 as the extrapolation increases.

This proposal seeks to remedy this situation by undertaking an examination of CTE using data of the Omega Cen calibration field obtained over the entire lifetime of WFPC2.  The methodology has been proven to produce accurate CTE corrections (indeed, they are the recommended corrections in the WFPC2 handbook and online CTE calculator).</Abstract>
      
      <PrincipalInvestigator
         Honorific="Dr."
         FirstName="Andrew"
         LastName="Dolphin"
         ESAMember="false"
         AddressVerifiedCycle="16">
         
         <Address
            Institution="Raytheon Company"
            NewInstitution="true"
            />
      </PrincipalInvestigator>
      
      <Questions>
         
         <Phase2Questions>
            
            <ObservingDescription />
            
            <RealtimeJustification />
            
            <CalibrationJustification />
            
            <AdditionalComments />
         </Phase2Questions>
      </Questions>
      
      <Orbits
         ThisCycle2GyroPrimary="1"
         ThisCycle2GyroParallel="0"
         NextCycle2GyroPrimary="0"
         NextCycle2GyroParallel="0"
         AfterNext2GyroPrimary="0"
         AfterNext2GyroParallel="0" />
      
      <Phase1ProposalInformation
         TotalTargets="1"
         Attachment="/Users/andy/HST_C16/archival.pdf">
         
         <ScientificCategory>RESOLVED STELLAR POPULATIONS</ScientificCategory>
         
         <ScientificKeyword1
            Keyword="STELLAR POPULATIONS IN EXTERNAL GALAXIES" />
         
         <ScientificKeyword2
            Keyword="GLOBULAR CLUSTERS" />
         
         <ScientificKeyword3
            Keyword="RESOLVED STELLAR POPULATIONS" />
         
         <ProprietaryPeriod>12</ProprietaryPeriod>
         
         <Budget>90000.00</Budget>
         
         <CalibProp>true</CalibProp>
         
         <SpitzerHours>0.0</SpitzerHours>
         
         <Treasury>false</Treasury>
         
         <Legacy>false</Legacy>
         
         <Theory>false</Theory>
         
         <LargeProgram>false</LargeProgram>
         
         <Spitzer>false</Spitzer>
         
         <Survey>false</Survey>
      </Phase1ProposalInformation>
      
      <Phase2ProposalInformation
         PCFlag="false">
         
         <Availability>SUPPORTED</Availability>
      </Phase2ProposalInformation>
   </ProposalInformation>
   
   <Targets />
   
   <Observations />
   
   <Datasets>
      
      <Dataset
         Instrument="WFPC2"
         Number="1"
         NumberOfDatasets="1412"
         RetrievalMethod="FTP"
         RetrievalPlan="Obtain data by FTP over several weeks." />
   </Datasets>
   
   <Patterns />
   
   <Visits />
</HSTProposal>


