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<HSTProposal
   Phase1ID="255"
   Phase2ID="10963"
   Phase="Phase I"
   AptVersion="Version 15.0 ">
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            Cycle="15"
            IncludeSysInfo="true"
            NotificationAddress="martins@stsci.edu"
            AssignedID="255">
            
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            <SubmissionLog>  Assigned ID: 255
----- Submission 1 (Fri Jan 27 16:30:17 GMT 2006) -----
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   <ProposalInformation
      Category="AR"
      PureParallelProposal="false"
      Cycle="15">
      
      <Title>A High Resolution alpha-enhanced Stellar Library for Evolutionary Population Synthesis</Title>
      
      <Abstract>Libraries of stellar spectra are fundamental tools for the study of stellar populations. We propose to create a high-resolution stellar library with alpha-enhanced compositions, computed with the latest improvements in stellar atmospheres, ranging from near-UV to the near-IR. The library will span all stellar types that are relevant for evolutionary models. The atomic and molecular line list will be calibrated  with unprecedented accuracy by using the new NGSL, an empirical stellar library created with STIS HST observations. The library will be implemented on evolutionary synthesis codes to create for the first time an appropriate tool to study and model stellar systems that have undergone different star formation histories than that of our local universe.</Abstract>
      
      <PrincipalInvestigator
         Honorific="Dr."
         FirstName="Lucimara"
         LastName="Martins"
         ESAMember="false"
         UniqueID="5429"
         AddressVerifiedCycle="15">
         
         <Address
            Institution="Space Telescope Science Institute"
            USState="MD"
            Country="USA" />
      </PrincipalInvestigator>
      
      <CoInvestigator
         Honorific="Dr."
         FirstName="Paula"
         LastName="Coelho"
         ESAMember="false"
         AdminUSPI="false"
         Contact="false"
         AddressVerifiedCycle="15">
         
         <Address
            Institution="Instituto de Astronomia, Geofísica e Ciências Atmosféricas - USP"
            NewInstitution="true"
            />
      </CoInvestigator>
      
      <CoInvestigator
         Honorific="Dr."
         FirstName="Duilia"
         MiddleInitial="F."
         LastName="de Mello"
         ESAMember="false"
         UniqueID="4733"
         AdminUSPI="false"
         Contact="false"
         AddressVerifiedCycle="15">
         
         <Address
            Institution="Catholic University of America"
            USState="DC"
            Country="USA" />
      </CoInvestigator>
      
      <Questions>
         
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            <ObservingDescription />
            
            <RealtimeJustification />
            
            <CalibrationJustification />
            
            <AdditionalComments />
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         NextCycle2GyroPrimary="0"
         NextCycle2GyroParallel="0"
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         AfterNext2GyroParallel="0" />
      
      <Phase1ProposalInformation
         TotalTargets="1"
         Attachment="C:\Documents and Settings\martins\Desktop\Proposals\hubble06.pdf">
         
         <ScientificCategory>UNRESOLVED STELLAR POPULATIONS</ScientificCategory>
         
         <ScientificKeyword1
            Keyword="CHEMICAL ABUNDANCES" />
         
         <ScientificKeyword2
            Keyword="STELLAR POPULATIONS IN EXTERNAL GALAXIES" />
         
         <ScientificKeyword3
            Keyword="RESOLVED STELLAR POPULATIONS" />
         
         <ProprietaryPeriod>12</ProprietaryPeriod>
         
         <Budget>60598</Budget>
         
         <CalibProp>false</CalibProp>
         
         <SpitzerHours>0.0</SpitzerHours>
         
         <SpitzerLarge>false</SpitzerLarge>
         
         <Treasury>false</Treasury>
         
         <Legacy>false</Legacy>
         
         <Theory>true</Theory>
         
         <LargeProgram>false</LargeProgram>
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         PCFlag="false">
         
         <Availability>SUPPORTED</Availability>
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