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   <!--Date: Fri Mar 15 11:29:42 GMT 2013-->
   
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      <Title>The extreme X-ray weakness of PG 0043+039</Title>
      
      <Abstract>The majority of broad absorption line quasars are X-ray weak which is usually explained by the absorption of the out-flowing wind in combination with the winds velocity shear. PG 0043+039 is the most extreme X-ray weak quasar known to date, but shows surprisingly only a very weak broad absorption line system. A conclusive interpretation is hampered by the absence of simultaneous measurements which is mandatory as both, the X-ray flux and the broad absorption system are known to be variable. We propose simultaneous XMM-Newton, HST (1 orbit) and 10m Hobby-Eberly or SALT Telescope observations in order to characterize simultaneously PG 0043-036|*|s X-ray emission and (broad) absorption (line system) properties.</Abstract>
      
      <PrincipalInvestigator
         Honorific="Dr."
         FirstName="Norbert"
         LastName="Schartel"
         ESAMember="true"
         UniqueID="13278"
         Institution="European Space Agency - ESTEC"
         Country="NLD"
         Contact="true" />
      
      <CoInvestigator
         Honorific="Dr."
         FirstName="Maria"
         LastName="Santos-Lleo"
         ESAMember="true"
         UniqueID="3308"
         Institution="European Space Agency - ESTEC"
         Country="NLD"
         Contact="false"
         AdminUSPI="false" />
      
      <CoInvestigator
         Honorific="Prof."
         FirstName="Wolfram"
         LastName="Kollatschny"
         ESAMember="true"
         UniqueID="1143"
         Institution="Universitats-Sternwarte Gottingen"
         Country="DEU"
         Contact="true"
         AdminUSPI="false" />
      
      <CoInvestigator
         Honorific="Dr."
         FirstName="Lucia"
         LastName="Ballo"
         ESAMember="true"
         UniqueID="13282"
         Institution="Instituto de Fisica de Cantabria"
         Country="ESP"
         Contact="false"
         AdminUSPI="false" />
      
      <CoInvestigator
         Honorific="Dr."
         FirstName="Pedro"
         LastName="Rodriguez"
         ESAMember="true"
         UniqueID="13281"
         Institution="European Space Agency - ESTEC"
         Country="NLD"
         Contact="false"
         AdminUSPI="false" />
      
      <Questions>
         
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            <ObservingDescription>The UV spectrum of this quasar should be taken simultaneously with XMM observations. A UV spectrum of this variable quasar has been taken before with HST-FOS-G190H in 1991 (Turnshek et al., ApJ 476,40 (1997)).

The target coordinates are taken from "The large quasar reference frame (LQRF). An optical representation of the ICRS" Andrei, A. H., Souchay, J., Zacharias, N., et al., A&amp;A 505,385 (2009).</ObservingDescription>
            
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            <AdditionalComments />
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         Attachment="/user/bethp/work/C:\Users\blacker\SPD Support\XMM-Joint-Program\69083-Merged.pdf">
         
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         <Theory>false</Theory>
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         <Availability>SUPPORTED</Availability>
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         Name="PG0043+039"
         Number="1"
         ReferenceFrame="ICRS"
         Redshift="0.385120"
         ProvisionalCoordinates="00 45 47.2000 +04 10 23.00">
         
         <PrimaryCategory>GALAXY</PrimaryCategory>
         
         <PrimaryDescription>
            
            <Description>QSO</Description>
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         <Comments />
         
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               Magnitude="15.9"
               MagnitudeUnc="0.5" />
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         NumberOfIterations="1"
         TotalOrbits="1"
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               <Polarimetry>No</Polarimetry>
               
               <SpectralElement>G140L</SpectralElement>
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         <Comments>HST observations should be done simultaneously with XMM observations.</Comments>
         
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            <TicNumOverruns>0</TicNumOverruns>
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         <GuidingTolerance>
            
            <Angle />
         </GuidingTolerance>
         
         <SeqWithin>
            
            <VisitList />
         </SeqWithin>
         
         <OnHoldComments />
         
         <Exposure
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            TimePerExposure="78.8"
            RealtimeAnalysis="false"
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            Shadow="false"
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            NewObsetFullAcq="false"
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            <MaxDur />
            
            <MinDur />
            
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            <InstrumentParameters />
            
            <SubExposures>
               
               <SubExposure
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         <Exposure
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            <MaxDur />
            
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            <InstrumentParameters
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         </Exposure>
      </Visit>
   </Visits>
</HSTProposal>

