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<HSTProposal
   Phase1ID="1112"
   Phase2ID="11546"
   Phase="Phase II"
   AptVersion="Version 17.2 ">
   <!--**********************************************************************************************************************-->
   <!--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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   <!--APT Version: Version 17.2 -->
   <!--Date: Tue Jun 03 17:55:04 GMT 2008-->
   
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            AssignedID="11546">
            
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            <SubmissionComments>I'm resubmitting because I've but in a dither pattern for the SBC exposures. I've also 
changed the number of exposures to 4 and increased the exposure time for each exposure.
Thank you.</SubmissionComments>
            
            <SubmissionLog>----- Attempting Submission 1 (Wed Apr 23 20:00:48 GMT 2008) -----
  Phase II Proposal 11546 (M31_RV_ph2.apt) successfully submitted.
----- Attempting Submission 2 (Tue Jun 03 17:55:04 GMT 2008) -----</SubmissionLog>
            
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            <SubmissionComments>This proposal was previously submitted with Proposal ID# 313.</SubmissionComments>
            
            <SubmissionLog>Assigned ID: 1112
----- Attempting Submission 1 (Wed Feb 07 12:04:04 EST 2007) -----
  Phase I Proposal 1112 (M31_RV) successfully submitted.</SubmissionLog>
            
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   <ProposalInformation
      Category="GO"
      PureParallelProposal="false"
      Cycle="16"
      STScIEditNumber="0">
      
      <Title>Ultra-Luminous Red Novae or Mergebursts? A Definitive HST Test</Title>
      
      <Abstract>V838 Mon and M31-RV are extraordinarily luminous (10**6 Lsun) and cool (~1000 K) eruptive variables. Their red colors and cool spectra have prompted claims that these objects are not classical novae, but instead represent a new class of astrophysical object: "MERGEBURSTS". Mergebursts are (hypothetical) mergers of close binary stars, predicted to rival the brightest classical novae in luminosity, but to always be much cooler and redder than novae. This prediction allows a definitive test of the mergeburst hypothesis for M31-RV as follows.
We have found a very bright, BLUE object within 0.4 arcsec of M31-RV in 10-year old archival WFPC2 images...consistent with an old nova, and not a mergeburst. We propose new ACS/SBC UV and WFPC2 visible images that will definitively show if this object is still as hot as nova theory predicts ( &gt;100,000 Kelvin), and if it is fading like an old nova.  This would eliminate the strongest candidate for a mergeburst.</Abstract>
      
      <PrincipalInvestigator
         Honorific="Dr."
         FirstName="Michael"
         LastName="Shara"
         ESAMember="false"
         UniqueID="2879"
         AddressVerifiedCycle="17">
         
         <Address
            Institution="American Museum of Natural History"
            USState="NY"
            Country="USA" />
      </PrincipalInvestigator>
      
      <CoInvestigator
         Honorific="Dr."
         FirstName="David"
         MiddleInitial="R."
         LastName="Zurek"
         ESAMember="false"
         UniqueID="4017"
         AdminUSPI="false"
         Contact="false"
         AddressVerifiedCycle="17">
         
         <Address
            Institution="American Museum of Natural History"
            USState="NY"
            Country="USA" />
      </CoInvestigator>
      
      <CoInvestigator
         Honorific="Dr."
         FirstName="Dina"
         LastName="Prialnik"
         ESAMember="false"
         UniqueID="3285"
         AdminUSPI="false"
         Contact="false"
         AddressVerifiedCycle="17">
         
         <Address
            Institution="Tel Aviv University - Wise Observatory"
            Country="Israel" />
      </CoInvestigator>
      
      <CoInvestigator
         Honorific="Dr."
         FirstName="Ofer"
         LastName="Yaron"
         ESAMember="false"
         AdminUSPI="false"
         Contact="false"
         AddressVerifiedCycle="17">
         
         <Address
            Institution="Tel Aviv University - Wise Observatory"
            Country="Israel" />
      </CoInvestigator>
      
      <Questions>
         
         <Phase2Questions>
            
            <ObservingDescription>We will use the ACS/SBC with the F140LP filter for one orbit to image the Far Ultraviolet flux of the source(s) at the postion
of the M31-RV. We will also image the position of M31-RV with WFPC2 for a total of 4 orbits. We will use F300W (4x600 seconds), F439W (4x400 seconds), F555W (4x200 seconds) and F814W (4x600 seconds). These observations will be deep enough to detect M31-RV if it is a very blue (nova) remnant, or a very red mergeburst.</ObservingDescription>
            
            <RealtimeJustification />
            
            <CalibrationJustification />
            
            <AdditionalComments />
         </Phase2Questions>
      </Questions>
      
      <Orbits
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         ThisCycle2GyroParallel="0"
         NextCycle2GyroPrimary="0"
         NextCycle2GyroParallel="0"
         AfterNext2GyroPrimary="0"
         AfterNext2GyroParallel="0" />
      
      <Phase1ProposalInformation
         TotalTargets="1"
         Attachment="/Users/dzurek/hst_cycle16/M31_RV.pdf">
         
         <ScientificCategory>HOT STARS</ScientificCategory>
         
         <ScientificKeyword1
            Keyword="Eruptive Binary Stars And Cataclysmic Variables" />
         
         <ScientificKeyword2
            Keyword="Novae" />
         
         <ScientificKeyword3
            Keyword="Variability" />
         
         <ScientificKeyword4
            Keyword="UV-Bright Stars" />
         
         <ProprietaryPeriod>12</ProprietaryPeriod>
         
         <CalibProp>false</CalibProp>
         
         <ChandraCoord>0.0</ChandraCoord>
         
         <NOAONights>0.0</NOAONights>
         
         <Treasury>false</Treasury>
         
         <Legacy>false</Legacy>
         
         <Theory>false</Theory>
         
         <LargeProgram>false</LargeProgram>
         
         <Survey>false</Survey>
      </Phase1ProposalInformation>
      
      <Phase2ProposalInformation
         PCFlag="false">
         
         <Availability>SUPPORTED</Availability>
      </Phase2ProposalInformation>
   </ProposalInformation>
   
   <Targets>
      
      <FixedTarget
         Name="M31-RV"
         Number="1"
         ReferenceFrame="WFPC2">
         
         <PrimaryCategory>EXT-STAR</PrimaryCategory>
         
         <PrimaryDescription>
            
            <Description>CLASSICAL NOVA</Description>
         </PrimaryDescription>
         
         <Comments />
         
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            <BroadBandMagnitude
               Band="V"
               Magnitude="23.2" />
         </Fluxes>
         
         <AlternateNames />
         
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               Hrs="00"
               Mins="43"
               Secs="2.4330" />
            
            <RAUnc
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            <DEC
               Degrees="+41"
               Arcmin="12"
               Arcsec="56.17" />
            
            <DECUnc
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            <Equinox>J2000</Equinox>
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         <ProvisionalRA>00 43 2.4330</ProvisionalRA>
         
         <ProvisionalDEC>+41 12 56.17</ProvisionalDEC>
         
         <Equinox>J2000</Equinox>
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         TargetName="M31-RV"
         Instrument="ACS"
         Number="1"
         NumberOfOrbits="1"
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         TotalOrbits="1"
         PureParallel="false"
         CoordinatedParallel="false"
         TargetOfOpportunity="false"
         CVZ="false"
         Duplication="false">
         
         <Configurations>
            
            <Configuration>
               
               <Config>ACS/SBC</Config>
               
               <ScienceMode>Imaging</ScienceMode>
               
               <Coronography>No</Coronography>
               
               <Polarimetry>No</Polarimetry>
               
               <SpectralElement>F140LP</SpectralElement>
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         <ObservationRequirements
            NoConstraints="true" />
         
         <AladinPhase1Requirements
            Detector="ACS/SBC"
            Aperture="SBC"
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            MosaicTileOverlap="10.0"
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            <Configuration>
               
               <Config>WFPC2</Config>
               
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               <Polarimetry>No</Polarimetry>
               
               <SpectralElement>F300W</SpectralElement>
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               <Config>WFPC2</Config>
               
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               <Config>WFPC2</Config>
               
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               <Config>WFPC2</Config>
               
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