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<HSTProposal
   Phase1ID="40"
   Phase2ID="10553"
   Phase="Phase II"
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   <!--This file is automatically generated and should not be edited by hand. Editing this file directly is at your own risk.-->
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            NotificationAddress="schmidt@as.arizona.edu">
            
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            <SubmissionComments>Please review that specified orientation ranges AVOID placing spider diffraction spikes along NSEW directions.  
Anticipated bleed/blooming from nearby 12th-magnitude star has been checked and should not affect useability 
of images.</SubmissionComments>
            
            <SubmissionLog>----- Submission 1 (Thu May 05 21:50:11 GMT 2005) -----
</SubmissionLog>
            
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            <SubmissionComments />
            
            <SubmissionLog>        Assigned ID: 40
----- Submission 1 (Wed Jan 19 15:50:02 GMT 2005) -----



</SubmissionLog>
            
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      Category="GO"
      PureParallelProposal="false"
      Cycle="14">
      
      <Title>Bipolar Scattering Structures in AGN</Title>
      
      <Abstract>The Unified Scheme for Seyfert galaxies successfully explains the basic distinctions between Type 1 and Type 2 AGN, including the existence of broad scattered lines in polarized flux spectra of the latter.  However, it fails to account for the strongly polarized broad lines often observed  in Type 1 AGN.  We have discovered an intermediate type red QSO that exhibits polarization properties of both types; indeed it suggests a bipolar scattering geometry similar to that seen in Galactic protoplanetary nebulae.  We request a small allocation with the high-resolution camera on ACS to image the object in two key spectral bands.  The results will allow an unambiguous interpretation of ground-based data, and enable modeling of the inclination and opening angle that illuminates the scattering clouds.  Like NGC 1068, a successful explanation of this object will not only allow further unification of AGN but also aid in unraveling the details of their inner structure.</Abstract>
      
      <PrincipalInvestigator
         Honorific="Dr."
         FirstName="Gary"
         MiddleInitial="D."
         LastName="Schmidt"
         ESAMember="false"
         UniqueID="2291">
         
         <Address
            Institution="University of Arizona"
            USState="AZ"
            Country="USA" />
      </PrincipalInvestigator>
      
      <CoInvestigator
         Honorific="Dr."
         FirstName="Paul"
         LastName="Smith"
         ESAMember="false"
         UniqueID="2426"
         AdminUSPI="false"
         Contact="false">
         
         <Address
            Institution="University of Arizona"
            USState="AZ"
            Country="USA" />
      </CoInvestigator>
      
      <CoInvestigator
         Honorific="Dr."
         FirstName="Dean"
         MiddleInitial="C."
         LastName="Hines"
         ESAMember="false"
         UniqueID="936"
         AdminUSPI="false"
         Contact="false">
         
         <Address
            Institution="Space Science Institute"
            USState="CO"
            Country="USA" />
      </CoInvestigator>
      
      <Questions>
         
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            <ObservingDescription>The observations are straightforward imaging, except for the proximity (7.8 arcsec E) of a V = 12 mag G star that raises concern about possible scattered light. We choose the ACS/HRC, which can yield a PSF approaching 0.03" FWHM in the blue, and the  26" FOV is ample for imaging the QSO. We wish to observe with a roll angle that orients the secondary spider diffraction spikes at least 15 degrees from E-W. Image dithering and drizzle analysis will be used to maximize resolution while removing the cosmic rays. The blue scattered component is well-sampled by the F435W filter. In the red we choose F658N.</ObservingDescription>
            
            <RealtimeJustification />
            
            <CalibrationJustification />
            
            <AdditionalComments />
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         AfterNextParallel="0"
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      <Phase1ProposalInformation
         TotalTargets="1"
         Attachment="/home/schmidt/projects/proposals/hst2m14/agn.pdf">
         
         <ScientificCategory>AGN/QUASARS</ScientificCategory>
         
         <ScientificKeyword1
            Keyword="AGN PHYSICS" />
         
         <ScientificKeyword2
            Keyword="SEYFERT GALAXIES" />
         
         <ScientificKeyword3
            Keyword="IR-LUMINOUS GALAXIES" />
         
         <ScientificKeyword4
            Keyword="RADIO-QUIET QUASARS" />
         
         <ProprietaryPeriod>12</ProprietaryPeriod>
         
         <CalibProp>false</CalibProp>
         
         <SpitzerHours>0.0</SpitzerHours>
         
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         <Treasury>false</Treasury>
         
         <Legacy>false</Legacy>
         
         <Theory>false</Theory>
         
         <LargeProgram>false</LargeProgram>
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         <Availability>SUPPORTED</Availability>
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         CoordinateSource="NED"
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         TargetOfOpportunity="false"
         CVZ="false"
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               <Polarimetry>No</Polarimetry>
               
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