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<HSTProposal
   Phase1ID="346"
   Phase2ID="11746"
   Phase="Phase I"
   AptVersion="Version 17.0 ">
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   <!--APT Version: Version 17.0 -->
   <!--Date: Fri Mar 07 15:01:21 GMT 2008-->
   
   <ToolData>
      
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         <SubmissionData
            AptVersion="Version 17.0 "
            SubmissionCounter="1"
            SubmissionSuccessCounter="0"
            HasErrors="false"
            Cycle="17"
            IncludeSysInfo="true"
            NotificationAddress="fritz@astro.as.utexas.edu"
            AssignedID="346">
            
            <SystemInformation
               os.arch="i386"
               os.name="Mac OS X"
               os.version="10.4.11"
               java.version="1.5.0_13"
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            <SubmissionComments>First of two.</SubmissionComments>
            
            <SubmissionLog>Assigned ID: 346
----- Attempting Submission 1 (Fri Mar 07 15:01:21 GMT 2008) -----</SubmissionLog>
            
            <DiagnosticJustification />
         </SubmissionData>
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   <ProposalInformation
      Category="AR"
      PureParallelProposal="false"
      Cycle="17"
      STScIEditNumber="0">
      
      <Title>A Definitive HST/FGS Parallax for the Hyades</Title>
      
      <Abstract>We propose to obtain from the archive the forty orbits of GTO FGS fringe tracking data secured by the HST Astrometry Science team using FGS 3. These data contain FGS observations of a total of 7 science targets (confirmed members of the Hyades open cluster) and 36 reference stars. These data were previously analyzed and resulted in a parallax for the Hyades published in 1997. Since that time Benedict, McArthur, and Harrison have significantly changed and improved the processing pipeline and the methodology employed to derive parallaxes from HST FGS data. Our expected parallax precision will be nearly three times better than what was previously obtained. These should yield single star absolute magnitudes with errors of 0.04 mag or better, aiding studies of cluster shape and intrinsic main sequence width.

Given the importance of the Hyades as a rung in the distance scale ladder, it would be valuable to obtain a definitive, independent parallax for the Hyades and confirm that HIPPARCOS got that one right. A weighted average of the HIPPARCOS and HST parallaxes could provide a valuable test metric for upcoming space astrometry missions such as SIM and/or GAIA.</Abstract>
      
      <PrincipalInvestigator
         Honorific="Dr."
         FirstName="George"
         MiddleInitial="Fritz"
         LastName="Benedict"
         ESAMember="false"
         UniqueID="173"
         AddressVerifiedCycle="17">
         
         <Address
            Institution="University of Texas at Austin"
            USState="TX"
            Country="USA" />
      </PrincipalInvestigator>
      
      <CoInvestigator
         Honorific="Ms."
         FirstName="Barbara"
         LastName="McArthur"
         ESAMember="false"
         UniqueID="4137"
         AdminUSPI="false"
         Contact="false"
         AddressVerifiedCycle="17">
         
         <Address
            Institution="University of Texas at Austin"
            USState="TX"
            Country="USA" />
      </CoInvestigator>
      
      <CoInvestigator
         Honorific="Dr."
         FirstName="William"
         MiddleInitial="F."
         LastName="van Altena"
         ESAMember="false"
         UniqueID="2636"
         AdminUSPI="false"
         Contact="false"
         AddressVerifiedCycle="17">
         
         <Address
            Institution="Yale University"
            USState="CT"
            Country="USA" />
      </CoInvestigator>
      
      <CoInvestigator
         Honorific="Dr."
         FirstName="Thomas"
         LastName="Harrison"
         ESAMember="false"
         UniqueID="3839"
         AdminUSPI="false"
         Contact="false"
         AddressVerifiedCycle="17">
         
         <Address
            Institution="New Mexico State University"
            USState="NM"
            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="/Volumes/RoadWarrior II/Active/HST Proposals/C17/Hyades AR/HyadesC17-AR.pdf">
         
         <ScientificCategory>COOL STARS</ScientificCategory>
         
         <ScientificKeyword1
            Keyword="Astrometry" />
         
         <ScientificKeyword2
            Keyword="Cosmological Parameters And Distance Scale" />
         
         <ScientificKeyword3
            Keyword="Galactic Structure" />
         
         <ScientificKeyword4
            Keyword="Main Sequence Stars" />
         
         <ScientificKeyword5
            Keyword="Open and Globular Star Clusters" />
         
         <ProprietaryPeriod>12</ProprietaryPeriod>
         
         <Budget>80000</Budget>
         
         <BudgetExplanation>See Scientific Justification</BudgetExplanation>
         
         <CalibProp>false</CalibProp>
         
         <ChandraCoord>0.0</ChandraCoord>
         
         <NOAONights>0.0</NOAONights>
         
         <Treasury>false</Treasury>
         
         <Legacy>false</Legacy>
         
         <Theory>false</Theory>
         
         <LargeProgram>false</LargeProgram>
         
         <Survey>false</Survey>
      </Phase1ProposalInformation>
      
      <Phase2ProposalInformation
         PCFlag="false">
         
         <Availability>SUPPORTED</Availability>
      </Phase2ProposalInformation>
   </ProposalInformation>
   
   <Targets />
   
   <Observations />
   
   <Datasets>
      
      <Dataset
         Instrument="FGS"
         Number="1"
         NumberOfDatasets="400"
         RetrievalMethod="FTP"
         RetrievalPlan="Retrieve data in July 2008." />
   </Datasets>
   
   <Patterns />
   
   <Visits />
</HSTProposal>


