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<HSTProposal
   Phase1ID="96"
   Phase2ID="11255"
   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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   <ToolData>
      
      <ToolDataItem
         Key="SubmissionData">
         
         <SubmissionData
            AptVersion="Version 16.0.2 "
            SubmissionCounter="5"
            SubmissionSuccessCounter="4"
            HasErrors="true"
            Cycle="16"
            IncludeSysInfo="true"
            NotificationAddress="fabio@astro.washington.edu"
            AssignedID="96">
            
            <SystemInformation
               os.arch="i386"
               os.name="Linux"
               os.version="2.6.9-42.0.3.ELsmp"
               java.version="1.5.0_08"
               linux.distribution="Red Hat Enterprise"
               linux.version="4 " />
            
            <SubmissionComments>No need for dataset entry. Theory Proposal.</SubmissionComments>
            
            <SubmissionLog>    Assigned ID: 96
----- Attempting Submission 1 (Thu Jan 25 02:34:40 GMT 2007) -----
  Phase I Proposal 96 (FGHST07b) successfully submitted.

----- Attempting Submission 5 (Fri Jan 26 20:06:43 GMT 2007) -----
</SubmissionLog>
            
            <DiagnosticJustification>No need for dataset entry. Theory Proposal.</DiagnosticJustification>
         </SubmissionData>
      </ToolDataItem>
   </ToolData>
   
   <ProposalInformation
      Category="AR"
      PureParallelProposal="false"
      Cycle="16"
      STScIEditNumber="0">
      
      <Title>Simulating the Evolution of the Galaxy Luminosity Function from z=6 to the Present.</Title>
      
      <Abstract>Using hydrodynamical simulations of galaxy formation we will provide (1) updated predictions for the luminosity function of galaxies in HST and Spitzer bands from z ~ 6 to the present and (2) study the physical mechanism that drives its evolution.

Particular emphasis will be on providing results easily comparable with the real observations: Using the code Sunrise (developed by P.Jonsson, UCSC) we will produce artificial images at kpc resolution for thousand of galaxies to obtain individual magnitudes and light profiles in HST and Spitzer bands that keep into account the detailed geometry of each galaxy and a self consistent treatment of dust reprocessing of light sources.


The simulations will consists of a large, 800 million particles SPH simulation of a 50 Mpc cosmological volume and of several very high resolution simulations of individual galaxies in a cosmological context. While the large volume will provide us with a large statistical sample, the high resolution simulations will allow us to identify the physical mechanisms (cold flows, energy feedback, mergers) that drive the evolution of the galaxy Luminosity Function at different masses and cosmic times.  This double approach will allow us to properly evaluate any numerical effects present in the simulations.</Abstract>
      
      <PrincipalInvestigator
         Honorific="Prof."
         FirstName="Fabio"
         LastName="Governato"
         ESAMember="false"
         UniqueID="7155"
         AddressVerifiedCycle="16">
         
         <Address
            Institution="University of Washington"
            USState="WA"
            Country="USA" />
      </PrincipalInvestigator>
      
      <CoInvestigator
         Honorific="Dr."
         FirstName="Chris"
         LastName="Brook"
         ESAMember="false"
         AdminUSPI="false"
         Contact="false"
         AddressVerifiedCycle="16">
         
         <Address
            Institution="University of Washington"
            USState="WA"
            Country="USA" />
      </CoInvestigator>
      
      <CoInvestigator
         Honorific="Dr."
         FirstName="Beth"
         LastName="Willman"
         ESAMember="false"
         AdminUSPI="false"
         Contact="false"
         AddressVerifiedCycle="16">
         
         <Address
            Institution="Harvard University"
            USState="MA"
            Country="USA" />
      </CoInvestigator>
      
      <CoInvestigator
         Honorific="Prof."
         FirstName="Thomas"
         LastName="Quinn"
         ESAMember="false"
         UniqueID="7156"
         AdminUSPI="false"
         Contact="false"
         AddressVerifiedCycle="16">
         
         <Address
            Institution="University of Washington"
            USState="WA"
            Country="USA" />
      </CoInvestigator>
      
      <CoInvestigator
         Honorific="Ms."
         FirstName="Alyson"
         LastName="Brooks"
         ESAMember="false"
         AdminUSPI="false"
         Contact="false"
         AddressVerifiedCycle="16">
         
         <Address
            Institution="University of Washington"
            USState="WA"
            Country="USA" />
      </CoInvestigator>
      
      <CoInvestigator
         Honorific="Mr."
         FirstName="Gregory"
         LastName="Stinson"
         ESAMember="false"
         UniqueID="7159"
         AdminUSPI="false"
         Contact="false"
         AddressVerifiedCycle="16">
         
         <Address
            Institution="University of Washington"
            USState="WA"
            Country="USA" />
      </CoInvestigator>
      
      <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="/astro/users/fabio/testi/Grants/HST07b/HST07b.pdf">
         
         <ScientificCategory>UNRESOLVED STELLAR POPULATIONS</ScientificCategory>
         
         <ScientificKeyword1
            Keyword="EVOLUTION" />
         
         <ScientificKeyword2
            Keyword="GALAXY DISKS" />
         
         <ScientificKeyword3
            Keyword="GALAXY BULGES" />
         
         <ScientificKeyword4
            Keyword="GALAXY FORMATION AND EVOLUTION" />
         
         <ScientificKeyword5
            Keyword="GALAXY MORPHOLOGY AND STRUCTURE" />
         
         <ProprietaryPeriod>12</ProprietaryPeriod>
         
         <Budget>48000</Budget>
         
         <BudgetExplanation>See page 8 for details.</BudgetExplanation>
         
         <CalibProp>false</CalibProp>
         
         <SpitzerHours>0.0</SpitzerHours>
         
         <Treasury>false</Treasury>
         
         <Legacy>false</Legacy>
         
         <Theory>true</Theory>
         
         <LargeProgram>false</LargeProgram>
         
         <Spitzer>false</Spitzer>
         
         <Survey>false</Survey>
      </Phase1ProposalInformation>
      
      <Phase2ProposalInformation
         PCFlag="false">
         
         <Availability>SUPPORTED</Availability>
      </Phase2ProposalInformation>
   </ProposalInformation>
   
   <Targets />
   
   <Observations />
   
   <Datasets>
      
      <Dataset
         Number="1"
         NumberOfDatasets="0" />
   </Datasets>
   
   <Patterns />
   
   <Visits />
</HSTProposal>


