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

<HSTProposal
   Phase1ID="1179"
   Phase2ID="11285"
   Phase="Phase I"
   AptVersion="Version 16.0.2 ">
   <!--**********************************************************************************************************************-->
   <!--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="1"
            SubmissionSuccessCounter="0"
            HasErrors="false"
            Cycle="16"
            IncludeSysInfo="true"
            NotificationAddress="tully@ifa.hawaii.edu"
            AssignedID="1179">
            
            <SystemInformation
               os.arch="sparc"
               os.name="SunOS"
               os.version="5.9"
               java.version="1.5.0_08"
               linux.distribution="not available"
               linux.version="not available" />
            
            <SubmissionComments />
            
            <SubmissionLog>  Assigned ID: 1179
----- Attempting Submission 1 (Thu Feb 08 21:32:25 GMT 2007) -----
</SubmissionLog>
            
            <DiagnosticJustification />
         </SubmissionData>
      </ToolDataItem>
   </ToolData>
   
   <ProposalInformation
      Category="AR"
      PureParallelProposal="false"
      Cycle="16"
      STScIEditNumber="0">
      
      <Title>TRGB Distances from Archived Data</Title>
      
      <Abstract>Accurate distances can be determined to galaxies if the Tip of the 
Red Giant Branch (TRGB) can be resolved.  The methodology was taken
to a new level of refinement with HST/ACS, with distances accurate
to 5% obtained for galaxies at 8 Mpc with single orbit observations.
Given multiple orbit observations, distances can be obtained for galaxies 
as remote as the Virgo Cluster.  There are now a tremendous number of
images in the HST archive that can be used for TRGB measurements.
Many were obtained expressly for this purpose but many more were taken
for other reasons.  While the TRGB method has been demonstrated to give
accurate distances, systematic effects can dominate if the data is not
analyzed in a coherent manner.  The authors of this proposal have
recently developed an end-to-end analysis procedure that they have
been applying to data acquired in the course of their own program.
Now that ACS is not available, there will be less new material entering
the archive.  It is an appropriate time to process all the available
images and recover consistent TRGB measurements and distances for all
nearby galaxies observed with HST.</Abstract>
      
      <PrincipalInvestigator
         Honorific="Dr."
         FirstName="R."
         MiddleInitial="Brent"
         LastName="Tully"
         ESAMember="false"
         UniqueID="2613"
         AddressVerifiedCycle="16">
         
         <Address
            Institution="University of Hawaii"
            USState="HI"
            Country="USA" />
      </PrincipalInvestigator>
      
      <CoInvestigator
         Honorific="Dr."
         FirstName="Luca"
         LastName="Rizzi"
         ESAMember="false"
         UniqueID="6602"
         AdminUSPI="false"
         Contact="false"
         AddressVerifiedCycle="16">
         
         <Address
            Institution="University of Hawaii"
            USState="HI"
            Country="USA" />
      </CoInvestigator>
      
      <CoInvestigator
         Honorific="Dr."
         FirstName="Edward"
         MiddleInitial="J."
         LastName="Shaya"
         ESAMember="false"
         UniqueID="2358"
         AdminUSPI="false"
         Contact="false"
         AddressVerifiedCycle="16">
         
         <Address
            Institution="University of Maryland"
            USState="MD"
            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="/scr1/stcyc16/archive/trgb_ar16.pdf">
         
         <ScientificCategory>COSMOLOGY</ScientificCategory>
         
         <ScientificKeyword1
            Keyword="COSMOLOGICAL PARAMETERS AND DISTANCE SCALE" />
         
         <ScientificKeyword2
            Keyword="DWARF GALAXIES" />
         
         <ScientificKeyword3
            Keyword="LARGE SCALE STRUCTURE AND PECULIAR VELOCITIES" />
         
         <ScientificKeyword4
            Keyword="LOW SURFACE BRIGHTNESS GALAXIES" />
         
         <ScientificKeyword5
            Keyword="RESOLVED STELLAR POPULATIONS" />
         
         <ProprietaryPeriod>12</ProprietaryPeriod>
         
         <Budget>68194</Budget>
         
         <CalibProp>false</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="ACS"
         Number="1"
         NumberOfDatasets="504"
         RetrievalMethod="FTP"
         RetrievalPlan="1/12th of the datasets per month" />
      
      <Dataset
         Instrument="WFPC2"
         Number="2"
         NumberOfDatasets="769"
         RetrievalMethod="FTP"
         RetrievalPlan="1/12th of datasets per month" />
   </Datasets>
   
   <Patterns />
   
   <Visits />
</HSTProposal>


