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<HSTProposal
   Phase1ID="2131"
   Phase2ID="16601"
   Phase="Phase I"
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   <!--APT Version: Version 2021.2  JWST PRD: PRDOPSSOC-037 -->
   <!--Date: Wed Jun 30 16:49:02 GMT 2021-->
   
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            <SubmissionLog>Assigned ID: 2131

----- Attempting Submission 1 (Fri Apr 09 19:11:58 GMT 2021) -----</SubmissionLog>
            
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   <ProposalInformation
      Category="AR"
      SnapPriority="Normal Priority"
      PureParallelProposal="false"
      Cycle="29"
      STScIEditNumber="0">
      
      <Title>Measuring the contribution of quasar outflows to AGN feedback</Title>
      
      <Abstract>There has been major progress recently in the study of quasar absorption outflows and their potential contribution for AGN feedback. HST spectral observations of the 500A-1050A  rest-frame (hereafter, EUV500) in medium redshift objects (z~1)  uncovered a rich phenomenology of absorption troughs. The quality and quantity of EUV500 diagnostic troughs allow us to probe the very high ionization phase, which carries 90%  or more of the outflowing material, as well as  determine the distance of most outflows from the central source (R). The first objective is impossible to achieve with the thousands of available ground-based spectra, and R can be measured in only ~1% of them. The EUV500 effort yielded the most energetic outflows measured to date with enough kinetic luminosity to be major agents of AGN feedback processes.

The HST spectral UV archive includes observations of more than 800 quasars.  These observations were taken for studying intervening absorption systems, and quasar outflows detected in these spectra were rarely analyzed. WE PROPOSE an archive program to study the EUV500 outflows found in these spectra.   Based on previous studies, we expect to find 20-30 very high ionization outflows (tripling the existing sample), and 10-15 outflows with measurable distance (doubling the existing sample).</Abstract>
      
      <PrincipalInvestigator
         Honorific="Dr."
         FirstName="Nahum"
         LastName="Arav"
         ESAMember="false"
         CSAMember="false"
         Retired="false"
         UniqueID="2921"
         Institution="Virginia Polytechnic Institute and State University"
         Country="USA"
         State="VA"
         Contact="true" />
      
      <CoInvestigator
         Honorific="Dr."
         FirstName="Gerard"
         MiddleInitial="A."
         LastName="Kriss"
         ESAMember="false"
         CSAMember="false"
         Retired="false"
         UniqueID="1160"
         Institution="Space Telescope Science Institute"
         Country="USA"
         State="MD"
         Contact="false"
         AdminUSPI="false" />
      
      <CoInvestigator
         Honorific="Dr."
         FirstName="Xinfeng"
         LastName="Xu"
         ESAMember="false"
         CSAMember="false"
         Retired="false"
         UniqueID="19011"
         Institution="The Johns Hopkins University"
         Country="USA"
         State="MD"
         Contact="false"
         AdminUSPI="false" />
      
      <CoInvestigator
         Honorific="Prof."
         FirstName="Kirk"
         MiddleInitial="T."
         LastName="Korista"
         ESAMember="false"
         CSAMember="false"
         Retired="false"
         UniqueID="1148"
         Institution="Western Michigan University"
         Country="USA"
         State="MI"
         Contact="false"
         AdminUSPI="false" />
      
      <Questions>
         
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      <TeamExpertise>PI Dr. Arav published several refereed papers on analyzing COS data of quasar outflows, including on a
similar quasar outflow:
Arav et al. 2013 MNRAS, 436, 3286
Quasar outflows and AGN feedback in the extreme UV:
HST/COS observations of HE 0238-1904

The Co-I team has substantial expertise in both the data and science of this proposal.

Dr Jerry Kriss: An expert on COS data and in the analysis of AGN outflows based on COS data.

Dr. Korista is an AGN expert, with several publications on quasar and Seyfert outflows involving HST 
UV spectral observations.

Dr Xinfeng Xu: who published 3 papers analyzing COS data of quasar outflows</TeamExpertise>
      
      <Phase1ProposalInformation
         Attachment="/System/Volumes/Data/solaris/user1/williamj/HST-C29/TAC/C:\Users\arav\Desktop\galileo\arav\HST propsals\HST29\Archive_EUV500\EUV500-AR2021_NEW.pdf">
         
         <ScientificCategory>Supermassive Black Holes and Active Galaxies</ScientificCategory>
         
         <ScientificKeyword1
            Keyword="AGN Host Galaxies" />
         
         <ScientificKeyword2
            Keyword="Broad-Absorption Line Quasar" />
         
         <ScientificKeyword3
            Keyword="Galaxy Winds" />
         
         <ScientificKeyword4
            Keyword="Quasars" />
         
         <ProprietaryPeriod
            Default="true">0</ProprietaryPeriod>
         
         <Budget>Regular</Budget>
         
         <CalibProp>false</CalibProp>
         
         <FundamentalPhysics>false</FundamentalPhysics>
         
         <UvInit>true</UvInit>
         
         <Theory>false</Theory>
         
         <CloudComputing>false</CloudComputing>
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