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      <Title>The pristine globular cluster population of the primordial relic galaxy NGC1277</Title>
      
      <Abstract>Galaxy mass assembly is driven dually by in-situ star formation and mergers, though  which modes dominate in galaxies of different mass and at different epochs is poorly understood. These bimodal processes are thought to be mirrored in the formation mechanisms for ancient red and blue globular clusters (GC) present in massive galaxies. Whereas the red GCs are theorized to form in situ together with the core of the massive galaxy, the blue subpopulation is expected to have an external accreted origin. This scenario, however, continues presently
untested. The proposed observations (2 orbits in the g and z filters using the ACS camera) will provide a direct test of this accretion hypothesis by characterizing the GC population of a massive galaxy that has survived untouched since its early assembly at z&gt;2: NGC1277. If the accretion scenario is correct, the GC color distribution of NGC1277 will be unimodal (having only red GCs). This result would provide direct constraints on the early accretion and assembly of massive galaxies in the early universe.</Abstract>
      
      <PrincipalInvestigator
         Honorific="Dr."
         FirstName="Ignacio"
         LastName="Trujillo"
         ESAMember="true"
         Retired="false"
         UniqueID="12688"
         Institution="Instituto de Astrofisica de Canarias"
         Country="ESP"
         Contact="true"
         AdminCoI="CoI: Dr. Mireia Montes " />
      
      <CoInvestigator
         Honorific="Dr."
         FirstName="Michael"
         MiddleInitial="A."
         LastName="Beasley"
         ESAMember="true"
         Retired="false"
         UniqueID="6456"
         Institution="Instituto de Astrofisica de Canarias"
         Country="ESP"
         Contact="false"
         AdminUSPI="false" />
      
      <CoInvestigator
         Honorific="Dr."
         FirstName="Ryan"
         LastName="Leaman"
         ESAMember="true"
         Retired="false"
         UniqueID="12350"
         Institution="Max Planck Institute for Astronomy"
         Country="DEU"
         Contact="false"
         AdminUSPI="false" />
      
      <CoInvestigator
         Honorific="Dr."
         FirstName="Mireia"
         LastName="Montes"
         ESAMember="false"
         Retired="false"
         UniqueID="16744"
         Institution="Yale University"
         Country="USA"
         State="CT"
         Contact="false"
         AdminUSPI="true" />
      
      <Questions>
         
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            <ObservingDescription>Filter choices and photometric depth:

To conduct our observations, we are asking for one orbit each in the ACS F475W (g475) and F850LP (z850) bands to image NGC1277 and its GC system.
Based on its declination, NGC~1277 is visible for 57 minutes in each orbit - with overheads the total integration time on source is ~2400s.  The ACS ETC suggests that with one orbit, we will reach the GC luminosity function turnover magnitude of r~26.3 with S/N~10 - allowing us to obtain the necessary number of GCs, and with sufficient photometric precision to characterize the color distribution.</ObservingDescription>
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         ThisCycle2GyroPrimary="2" />
      
      <Phase1ProposalInformation
         Attachment="C:\Users\bethp\C:\Users\itc\Desktop\phase1-GO.pdf"
         ProposalSize="SMALL">
         
         <ScientificCategory>UNRESOLVED STELLAR POPULATIONS AND GALAXY STRUCTURE</ScientificCategory>
         
         <ScientificKeyword1
            Keyword="Elliptical Galaxies" />
         
         <ScientificKeyword2
            Keyword="Galaxy Formation And Evolution" />
         
         <ScientificKeyword3
            Keyword="Globular Clusters" />
         
         <ScientificKeyword4
            Keyword="High Redshift Galaxies" />
         
         <ScientificKeyword5
            Keyword="Stellar Populations In External Galaxies" />
         
         <ProprietaryPeriod
            Default="true">12</ProprietaryPeriod>
         
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         <UvInit>false</UvInit>
         
         <Treasury>false</Treasury>
         
         <MultiCycleTreasury>false</MultiCycleTreasury>
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         PCFlag="true">
         
         <Availability>SUPPORTED</Availability>
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      <FixedTarget
         Name="NGC-1277"
         Number="1"
         ReferenceFrame="SIMBAD"
         ProvisionalCoordinates="03 19 51.4880 +41 34 24.26">
         
         <PrimaryCategory>GALAXY</PrimaryCategory>
         
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            <Description>ELLIPTICAL</Description>
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         <Extended>YES</Extended>
         
         <Comments>This object was generated by the targetselector and retrieved from the SIMBAD database.</Comments>
         
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               Magnitude="13"
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         TotalOrbits="2"
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         TargetOfOpportunity="No"
         CVZ="false"
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               <Polarimetry>No</Polarimetry>
               
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