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<HSTProposal
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   Phase2ID="10560"
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            NotificationAddress="debes@astro.psu.edu">
            
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            <SubmissionLog>      ----- Submission 1 (Tue May 10 21:26:14 GMT 2005) -----



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            <SubmissionLog>                      Assigned ID: 243
----- Submission 1 (Fri Jan 21 17:16:39 GMT 2005) -----
  Phase I Proposal 243 (wd1620) successfully submitted.










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   <ProposalInformation
      Category="GO"
      PureParallelProposal="false"
      Cycle="14">
      
      <Title>Confirming Planetary Candidates in the Stellar Graveyard with NICMOS</Title>
      
      <Abstract>We propose to follow up planetary candidates imaged near the white dwarf WD 1620-391 with second epoch images from NICMOS.  This white dwarf was imaged during Cycle 12 as part of a campaign to detect massive planetary companions to nearby white dwarfs with photospheric metal line absorption.  While at a low galactic latitude, a puzzling excess of objects are present &lt; 4", suggesting the possiblity of objects physically associated with the white dwarf.  With second epoch information we can test these candidates for common proper motion, a test for physical association.  If any of these candidates are confirmed, they will be consistent with 6-10 M$_{Jup}$ companions at projected orbital separations of between 25-50 AU.</Abstract>
      
      <PrincipalInvestigator
         Honorific="Mr."
         FirstName="John"
         MiddleInitial="Henry"
         LastName="Debes"
         ESAMember="false"
         UniqueID="6865"
         AddressVerifiedCycle="15">
         
         <Address
            Institution="The Pennsylvania State University"
            USState="PA"
            Country="USA" />
      </PrincipalInvestigator>
      
      <CoInvestigator
         Honorific="Dr."
         FirstName="Steinn"
         LastName="Sigurdsson"
         ESAMember="false"
         UniqueID="2384"
         AdminUSPI="false"
         Contact="false"
         AddressVerifiedCycle="15">
         
         <Address
            Institution="The Pennsylvania State University"
            USState="PA"
            Country="USA" />
      </CoInvestigator>
      
      <Questions>
         
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            <ObservingDescription>In 2 Gyro mode, two orbits will be used to observe WD 1620-391.  This target will be observed behind the NIC2 coronagraphic spot at one orientation in the first orbit, and then in the very next orbit will be observed at a different spacecraft roll, preferably at a difference of ~10-30 degrees.</ObservingDescription>
            
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            <AdditionalComments />
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         ThisCycle2GyroParallel="0"
         NextCycle2GyroPrimary="0"
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         AfterNext2GyroPrimary="0"
         AfterNext2GyroParallel="0" />
      
      <Phase1ProposalInformation
         TotalTargets="1"
         Attachment="/Users/grog/PROPOSALS/HST05/WD1620/proposal.pdf">
         
         <ScientificCategory>ISM AND CIRCUMSTELLAR MATTER</ScientificCategory>
         
         <ScientificKeyword1
            Keyword="EXTRA-SOLAR PLANETS" />
         
         <ScientificKeyword2
            Keyword="IMAGING" />
         
         <ScientificKeyword3
            Keyword="WHITE DWARFS" />
         
         <ProprietaryPeriod>12</ProprietaryPeriod>
         
         <CalibProp>false</CalibProp>
         
         <SpitzerHours>0.0</SpitzerHours>
         
         <SpitzerLarge>false</SpitzerLarge>
         
         <Treasury>false</Treasury>
         
         <Legacy>false</Legacy>
         
         <Theory>false</Theory>
         
         <LargeProgram>false</LargeProgram>
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      <Phase2ProposalInformation
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         <Availability>SUPPORTED</Availability>
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         Name="WD-1620-391"
         Number="1"
         CoordinateSource="GSC_SURVEY_PLATE"
         ReferenceFrame="GSC1"
         RAPM="0.0050"
         DecPM="0.0"
         Epoch="1987.385"
         AnnualParallax="0.068">
         
         <PrimaryCategory>STAR</PrimaryCategory>
         
         <PrimaryDescription>
            
            <Description>DA</Description>
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         <Comments />
         
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            <BroadBandMagnitude
               Band="V"
               Magnitude="11.16"
               MagnitudeUnc="0.37" />
            
            <OtherFluxes>H=11.708</OtherFluxes>
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               Hrs="16"
               Mins="23"
               Secs="33.7500" />
            
            <RAUnc
               Arcsec="0.1" />
            
            <DEC
               Degrees="-39"
               Arcmin="13"
               Arcsec="46.00" />
            
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            <Equinox>J2000</Equinox>
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         <ProvisionalRA>16 23 33.8367</ProvisionalRA>
         
         <ProvisionalDEC>-39 13 46.16</ProvisionalDEC>
         
         <Equinox>J2000</Equinox>
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         NumberOfOrbits="2"
         NumberOfIterations="2"
         TotalOrbits="4"
         PureParallel="false"
         CoordinatedParallel="false"
         TargetOfOpportunity="false"
         CVZ="false"
         Duplication="false">
         
         <Configurations>
            
            <Configuration>
               
               <Config>NIC2</Config>
               
               <ScienceMode>Imaging</ScienceMode>
               
               <Coronography>Yes</Coronography>
               
               <Polarimetry>No</Polarimetry>
               
               <SpectralElement>F160W</SpectralElement>
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         <OrbitalVisibility>
            
            <Time
               Mins="46.0" />
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         <ObservationRequirements
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            DaysLow="0"
            Visibility=""
            OrbitsPerDay="0"
            ObservationRequirements="NOCONSTRAINTS" />
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         <Comments>First coronagraphic observations, with acquisition and direct observing behind the spot.  To be used if 2 Gyro mode is active.  Orientation restrictions are in place to ensure that two candidate planetary companions with separations of ~3.6 and 3.9 arcseconds at pointing angles (East of North) of 27 degrees and 279 degrees are still
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