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            <SubmissionComments>Revised the ORIENTS according to Sylvia's suggestions</SubmissionComments>
            
            <SubmissionLog>----- Attempting Submission 1 (Wed Sep 29 01:28:32 GMT 2010) -----
----- Attempting Submission 2 (Mon Nov 01 18:16:52 GMT 2010) -----</SubmissionLog>
            
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      Cycle="18"
      STScIEditNumber="0">
      
      <Title>AGN heating and cooling in the most luminous group cool core</Title>
      
      <Abstract>Outbursts of SMBHs have significant impact on structure formation and evolution. Their imprint on ICM (e.g., shocks, cavities, elevated entropy) provides an historical chronicle of the SMBH activity. Because of the expected bigger impact of AGN heating on the group gas than the cluster gas, group cool cores are ideal places to study SMBH outbursts. We propose an 89 ks observation of the most X-ray luminous group cool core at z&lt;0.05 (also the second brightest one) that only has 7 ks Chandra data. It also hosts one of the most spectacular Ha filaments in nearby groups. The requested ACIS data, in combination with the joint VLA and HST observations, will be used to examine cavities, shocks, the relation between gas in different phases and star formation, and the AGN activity history.</Abstract>
      
      <PrincipalInvestigator
         Honorific="Dr."
         FirstName="Ming"
         LastName="Sun"
         ESAMember="false"
         UniqueID="8572"
         AddressVerifiedCycle="18">
         
         <Address
            Institution="The University of Virginia"
            USState="VA"
            Country="USA" />
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      <CoInvestigator
         Honorific="Dr."
         FirstName="Paul"
         LastName="Nulson"
         ESAMember="false"
         AdminUSPI="false"
         Contact="false"
         AddressVerifiedCycle="18">
         
         <Address
            Institution="Smithsonian Institution Astrophysical Observatory"
            USState="MA"
            Country="USA" />
      </CoInvestigator>
      
      <CoInvestigator
         Honorific="Dr."
         FirstName="Tracy"
         LastName="Clarke"
         ESAMember="false"
         AdminUSPI="false"
         Contact="false"
         AddressVerifiedCycle="18">
         
         <Address
            Institution="Naval Research Laboratory"
            USState="DC"
            Country="USA" />
      </CoInvestigator>
      
      <CoInvestigator
         Honorific="Dr."
         FirstName="William"
         MiddleInitial="R."
         LastName="Forman"
         ESAMember="false"
         UniqueID="4975"
         AdminUSPI="false"
         Contact="false"
         AddressVerifiedCycle="18">
         
         <Address
            Institution="Smithsonian Institution Astrophysical Observatory"
            USState="MA"
            Country="USA" />
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      <CoInvestigator
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         FirstName="Craig"
         MiddleInitial="L."
         LastName="Sarazin"
         ESAMember="false"
         UniqueID="2267"
         AdminUSPI="false"
         Contact="false"
         AddressVerifiedCycle="18">
         
         <Address
            Institution="The University of Virginia"
            USState="VA"
            Country="USA" />
      </CoInvestigator>
      
      <CoInvestigator
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         FirstName="Robert"
         MiddleInitial="W."
         LastName="O'Connell"
         ESAMember="false"
         UniqueID="1960"
         AdminUSPI="false"
         Contact="false"
         AddressVerifiedCycle="18">
         
         <Address
            Institution="The University of Virginia"
            USState="VA"
            Country="USA" />
      </CoInvestigator>
      
      <Questions>
         
         <Phase2Questions>
            
            <ObservingDescription>We will use WFC3/UVIS and ACS to study star formation in the cool core of
A3581. We plan deep exposures in the F336W (U) band and supporting
exposures on the F475W and F814W with ACS.</ObservingDescription>
            
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            <CalibrationJustification />
            
            <AdditionalComments />
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         Attachment="/Users/blacker/Desktop/HST/PDFs/12800410_msun_f.pdf">
         
         <ScientificCategory />
         
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         <Legacy>false</Legacy>
         
         <Theory>false</Theory>
         
         <LargeProgram>false</LargeProgram>
         
         <Spitzer>false</Spitzer>
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         PCFlag="false">
         
         <Availability>SUPPORTED</Availability>
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            <Description>ELLIPTICAL</Description>
            
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