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<HSTProposal
   Phase1ID="1913"
   Phase2ID="16600"
   Phase="Phase I"
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   <!--APT Version: Version 2021.2  JWST PRD: PRDOPSSOC-037 -->
   <!--Date: Wed Jun 30 16:31:45 GMT 2021-->
   
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----- Attempting Submission 1 (Fri Apr 09 13:34:41 GMT 2021) -----</SubmissionLog>
            
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   <ProposalInformation
      Category="AR"
      SnapPriority="Normal Priority"
      PureParallelProposal="false"
      Cycle="29"
      STScIEditNumber="0">
      
      <Title>A new paradigm for Seyfert outflows and their connection to AGN feedback</Title>
      
      <Abstract>AGN outflows play an important role in feedback processes that control galaxy evolution and the growth of central black holes. Over the past few years a paradigm shift regarding the physical parameters and picture of Seyfert outflows has occurred. In particular, monitoring variability of the outflow absorption troughs in NGC 5548 yielded the first comprehensive,yet simple, model that can explain the physical characteristics of AGN outflows. Compared with previous analyses, the new results are different by a factor of 10 in the distance of the outflow from the central source (R), two orders of magnitude in total outflowing column density (NH), and ascribe trough variability to changes in the photoionization of a constant NH absorber, in contrast with the previous picture of changing NH. Similar results were obtained for the outflow observed in NGC 7469.

WE PROPOSE to apply this new paradigm in reanalyzing most of the large multi-epoch archival HST data of Seyfert outflows (~500ks total) to:
1) Fundamentally revise our NH, R, ionization parameter, mass flow rate and kinetic luminosity estimates in the 10 best-observed Seyfert outflows.
2) Study the newly discovered obscurer phenomenon in these objects.
3) Use the new reliable parameters to perform a comparative study of Seyfert outflows: try to determine the relationship between the velocity, distance, mass flux and energetics of the outflows to the luminosity, BH mass, Eddington ratio, and orientation of their AGN.</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="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" />
      
      <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" />
      
      <Questions>
         
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      <TeamExpertise>PI Dr. Arav published several refereed papers on analyzing COS and STIS data of Seyfert outflows, including
the main paper, which this proposal is based on:
Arav, N.; Chamberlain, C.; Kriss, G. A.; Kaastra, J. S.; et al.,
Anatomy of the AGN in NGC 5548. II. The spatial, temporal, and
physical nature of the outflow from HST/COS Observations
2015, A&amp;A, 577A, 37

The Co-I team: is also experienced in analyzing HST UV data of AGN outflows:

Dr Jerry Kriss: An expert on COS data and in the analysis of AGN outflows based on COS data.
He published many papers analyzing HST UV spectra and X-ray data of Seyfert outflows, e.g.,
Kriss, G. A.; Mehdipour, M.; Kaastra, J. S.; Arav, N. et al.
HST/COS observations of the newly discovered obscuring outflow in NGC 3783
2019, A&amp;A, 621A, 12

Dr. Korista is an AGN expert, with several publications on quasar and Seyfert outflows involving HST UV
spectral observations.

Dr Xinfeng Xu:  who published papers analyzing spectral data of quasar outflows.</TeamExpertise>
      
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         <ScientificCategory>Supermassive Black Holes and Active Galaxies</ScientificCategory>
         
         <SecondaryScientificCategory>Supermassive Black Holes and Active Galaxies</SecondaryScientificCategory>
         
         <ScientificKeyword1
            Keyword="Galaxy Winds" />
         
         <ScientificKeyword2
            Keyword="Seyfert Galaxies" />
         
         <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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