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<HSTProposal
   Phase1ID="453"
   Phase2ID="10662"
   Phase="Phase I"
   AptVersion="Version 14.0 ">
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            Cycle="14"
            IncludeSysInfo="true"
            NotificationAddress="holwerda@stsci.edu">
            
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            <SubmissionLog>  Assigned ID: 453
----- Submission 1 (Fri Jan 21 22:19:58 GMT 2005) -----
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   <ProposalInformation
      Category="AR"
      PureParallelProposal="false"
      Cycle="14">
      
      <Title>An dust extinction map of M51 from counts of distant galaxies</Title>
      
      <Abstract>The number of distant galaxies seen in Heritage Project's ACS images of M51 can be used to probe the extinction in this spiral disk. The ``Synthetic Field Method'' (Gonzalez et al. (1998), Holwerda et al. (2005a)) can be used to calibrate this number for crowding and confusion effects. The Heritage Project observing strategy is very suitable for this kind of work. The total extinction of the disk can be compared to the  disk emission, such as SCUBA sub-mm observations and Spitzer maps and the atomic hydrogen column density (HI). Such comparisons will reveal the role of dust in spiral disk of M51.</Abstract>
      
      <PrincipalInvestigator
         Honorific="Mr."
         FirstName="Benne"
         MiddleInitial="Willem"
         LastName="Holwerda"
         ESAMember="false">
         
         <Address
            Institution="Kapteyn Astronomical Institute"
            Country="Netherlands" />
      </PrincipalInvestigator>
      
      <CoInvestigator
         Honorific="Dr."
         FirstName="Ronald"
         MiddleInitial="J."
         LastName="Allen"
         ESAMember="false"
         UniqueID="3397"
         AdminUSPI="true"
         Contact="false">
         
         <Address
            Institution="Space Telescope Science Institute"
            USState="MD"
            Country="USA" />
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      <Questions>
         
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            <ObservingDescription />
            
            <RealtimeJustification />
            
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            <AdditionalComments />
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      <Orbits
         ThisCyclePrimary="1"
         ThisCycleParallel="0"
         NextCyclePrimary="0"
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      <Phase1ProposalInformation
         TotalTargets="1"
         Attachment="/Users/benneholwerda/Desktop/HST AT proposal/M51 Proposal/M51-AR.pdf">
         
         <ScientificCategory>GALAXIES</ScientificCategory>
         
         <ScientificKeyword1
            Keyword="DUST" />
         
         <ScientificKeyword2
            Keyword="GALAXY DISKS" />
         
         <ScientificKeyword3
            Keyword="GALAXY MORPHOLOGY AND STRUCTURE" />
         
         <ScientificKeyword4
            Keyword="SPIRAL GALAXIES" />
         
         <ScientificKeyword5
            Keyword="MOLECULAR CLOUDS" />
         
         <ProprietaryPeriod>12</ProprietaryPeriod>
         
         <Budget>50000</Budget>
         
         <BudgetExplanation>6 months postdoc salary, incl. overhead.</BudgetExplanation>
         
         <CalibProp>false</CalibProp>
         
         <SpitzerHours>0.0</SpitzerHours>
         
         <SpitzerLarge>false</SpitzerLarge>
         
         <Treasury>false</Treasury>
         
         <Legacy>false</Legacy>
         
         <Theory>false</Theory>
         
         <LargeProgram>false</LargeProgram>
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         <Availability>SUPPORTED</Availability>
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