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<HSTProposal
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   Phase="Phase II"
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   <!--Date: Thu Nov 20 19:52:58 GMT 2008-->
   
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            NotificationAddress="aprestwich@cfa.harvard.edu"
            AssignedID="11836">
            
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            <SubmissionComments />
            
            <SubmissionLog>----- Attempting Submission 2 (Thu Nov 20 19:52:58 GMT 2008) -----</SubmissionLog>
            
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   <ProposalInformation
      Category="GO"
      PureParallelProposal="false"
      Cycle="17"
      STScIEditNumber="0">
      
      <Title>Chandra Imaging of NGC 922 -- the closest collisional ring galaxy</Title>
      
      <Abstract>Ultra Luminous X-ray sources (ULX) have luminosities many times the Eddington
limit for a stellar black hole and are associated with massive star formation.
This is illustrated by the Chandra image of the Cartwheel, a collisional ring
galaxy. The bulk of the X-ray luminosity is produced by 16 ULX co-incident
with the outer ring of star formation. We request Chandra and HST time to image
another collisional ring galaxy NGC 922. NGC 922 is similar to the Cartwheel,
except that it is nearly three times closer and has higher metallicity. We will
(1) detect fainter sources than was possible for the Cartwheel, (2) use archival
HST data and our new Halpha images to associate X-ray sources with tracers of
star formation and (3) study the effect of metallicity on the formation of ULX.</Abstract>
      
      <PrincipalInvestigator
         Honorific="Dr."
         FirstName="Andrea"
         MiddleInitial="H."
         LastName="Prestwich"
         ESAMember="false"
         UniqueID="4704"
         AddressVerifiedCycle="17">
         
         <Address
            Institution="Smithsonian Institution Astrophysical Observatory"
            USState="MA"
            Country="USA" />
      </PrincipalInvestigator>
      
      <CoInvestigator
         Honorific="Dr."
         FirstName="Andreas"
         LastName="Zezas"
         ESAMember="false"
         UniqueID="6372"
         AdminUSPI="false"
         Contact="false"
         AddressVerifiedCycle="17">
         
         <Address
            Institution="Smithsonian Institution Astrophysical Observatory"
            USState="MA"
            Country="USA" />
      </CoInvestigator>
      
      <CoInvestigator
         Honorific="Dr."
         FirstName="Timothy"
         MiddleInitial="Paul"
         LastName="Roberts"
         ESAMember="true"
         UniqueID="6116"
         AdminUSPI="false"
         Contact="false"
         AddressVerifiedCycle="17">
         
         <Address
            Institution="University of Durham"
            Country="UK" />
      </CoInvestigator>
      
      <CoInvestigator
         Honorific="Prof."
         FirstName="Martin"
         MiddleInitial="J."
         LastName="Ward"
         ESAMember="true"
         UniqueID="2712"
         AdminUSPI="false"
         Contact="false"
         AddressVerifiedCycle="17">
         
         <Address
            Institution="University of Durham"
            Country="UK" />
      </CoInvestigator>
      
      <CoInvestigator
         Honorific="Mr."
         FirstName="Roy"
         MiddleInitial="Erik"
         LastName="Kilgard"
         ESAMember="false"
         UniqueID="7866"
         AdminUSPI="false"
         Contact="false"
         AddressVerifiedCycle="17">
         
         <Address
            Institution="Wesleyan University"
            USState="CT"
            Country="USA" />
      </CoInvestigator>
      
      <CoInvestigator
         Honorific="Dr."
         FirstName="Ginevra"
         LastName="Trinchieri"
         ESAMember="true"
         UniqueID="2603"
         AdminUSPI="false"
         Contact="false"
         AddressVerifiedCycle="17">
         
         <Address
            Institution="Osservatorio Astronomico di Brera, Milano"
            Country="Italy" />
      </CoInvestigator>
      
      <CoInvestigator
         Honorific="Dr."
         FirstName="Anna"
         LastName="Wolter"
         ESAMember="false"
         UniqueID="8458"
         AdminUSPI="false"
         Contact="false"
         AddressVerifiedCycle="17">
         
         <Address
            Institution="Osservatorio Astronomico di Brera, Milano"
            Country="Italy" />
      </CoInvestigator>
      
      <CoInvestigator
         Honorific="Mr."
         FirstName="Ryan"
         LastName="Foltz"
         ESAMember="false"
         AdminUSPI="false"
         Contact="false"
         AddressVerifiedCycle="17">
         
         <Address
            Institution="Smithsonian Institution Astrophysical Observatory"
            USState="MA"
            Country="USA" />
      </CoInvestigator>
      
      <Questions>
         
         <Phase2Questions>
            
            <ObservingDescription>This proposal involves H-alpha line and continuum imaging of the nearby collisional ring galaxy NGC 922.    The F665N filter is used to image the redshifted H-alpha line and the F621 filter used to image the continuum.  We requre at least 5000s in the line filter and 1500s in the continuum.     One of our science goals is to determine the positions of bright X-ray sources relative to the H-alpha ring.  We therefore opt to use the UVIS-CENTER aperture and a LINE dither to fill in the chip gaps (as well as eliminate hot pixels and cosmic ray hits).</ObservingDescription>
            
            <RealtimeJustification />
            
            <CalibrationJustification />
            
            <AdditionalComments />
         </Phase2Questions>
      </Questions>
      
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         ThisCycle2GyroPrimary="1"
         ThisCycle2GyroParallel="0"
         NextCycle2GyroPrimary="0"
         NextCycle2GyroParallel="0"
         AfterNext2GyroPrimary="0"
         AfterNext2GyroParallel="0" />
      
      <Phase1ProposalInformation
         TotalTargets="1">
         
         <ScientificCategory />
         
         <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="NGC-0922"
         Number="1"
         ReferenceFrame="ICRS">
         
         <PrimaryCategory>GALAXY</PrimaryCategory>
         
         <PrimaryDescription>
            
            <Description>INTERACTING GALAXY</Description>
            
            <Description>RING</Description>
            
            <Description>SPIRAL</Description>
            
            <Description>STARBURST</Description>
         </PrimaryDescription>
         
         <Comments>This object was generated by the targetselector and retrieved from the NED database.</Comments>
         
         <Fluxes>
            
            <BroadBandMagnitude
               Band="V"
               Magnitude="12.12" />
         </Fluxes>
         
         <AlternateNames />
         
         <EquatorialPosition>
            
            <RA
               Hrs="02"
               Mins="25"
               Secs="4.4000" />
            
            <RAUnc
               Arcsec="0.1" />
            
            <DEC
               Degrees="-24"
               Arcmin="47"
               Arcsec="17.00" />
            
            <DECUnc
               Arcsec="0.1" />
            
            <Equinox>J2000</Equinox>
         </EquatorialPosition>
         
         <ProvisionalRA>00 00 0.0000</ProvisionalRA>
         
         <ProvisionalDEC>+00 00 0.00</ProvisionalDEC>
         
         <Equinox>J2000</Equinox>
      </FixedTarget>
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   <Observations />
   
   <Datasets />
   
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         <CoordinateFrame>POS-TARG</CoordinateFrame>
         
         <Purpose>DITHER</Purpose>
         
         <SubpatternPurpose>DITHER</SubpatternPurpose>
         
         <SubpatternNumberOfPoints>2</SubpatternNumberOfPoints>
         
         <PointSpacing>2.0</PointSpacing>
         
         <Comments />
         
         <SubpatternPatternType>WFC3-UVIS-DITHER-LINE</SubpatternPatternType>
         
         <LineSpacing />
         
         <SubpatternCenterPattern>false</SubpatternCenterPattern>
         
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         <CenterPattern>false</CenterPattern>
         
         <SubpatternLineSpacing />
         
         <AngleBetweenSides />
         
         <SubpatternPointSpacing>0.145</SubpatternPointSpacing>
         
         <NumberOfPoints>2</NumberOfPoints>
         
         <Orientation>46.84</Orientation>
         
         <SubpatternCoordinateFrame>POS-TARG</SubpatternCoordinateFrame>
         
         <PatternType>LINE</PatternType>
         
         <SubpatternOrientation>46.84</SubpatternOrientation>
         
         <Number>1</Number>
         
         <Sub-Pattern>true</Sub-Pattern>
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   <Visits>
      
      <Visit
         Number="01">
         
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                     <AncillaryData
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                        <String>The scheduling data was generated by CASM 17.2.</String>
                        
                        <String>CASM was run in Phase II mode.</String>
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