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----- Attempting Submission 1 (Fri Dec 04 20:31:32 GMT 2015) -----</SubmissionLog>
            
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            <SubmissionLog>----- Attempting Submission 1 (Sat Dec 12 00:06:55 GMT 2015) -----
HST Phase II Proposal 14450 (HSTSLSNDDT2phaseII.apt) successfully submitted.
Receipt: # 14450-1

----- Attempting Submission 2 (Mon Dec 14 22:57:31 GMT 2015) -----</SubmissionLog>
            
            <Phase2DiagnosticJustification>It warns about doing a courser acquisition with COS if the position is not known to better than 0.4", which is the accuracy of our position.  If an additional acquisition is needed we can add it.</Phase2DiagnosticJustification>
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      <Title>Ultraviolet Spectroscopy of the Unprecedented Rebrightening of the Most Luminous Supernova</Title>
      
      <Abstract>ASASSN-15lh/SN2015L has been classified as a hydrogen-poor superluminous supernova (SLSN-I) which is more luminous than any supernova previously observed.  It has already emitted more than 3 x 10^51 ergs of luminosity, most of which was emitted at UV wavelengths.  After fading for two months it began rebrightening in the UV, a behavior never before seen.  We propose to obtain HST/STIS UV spectroscopy in order to determine the nature of the UV emission (thermal or line emission) and the composition of the ejecta and intervening material.  While this phase is not yet understood--and the motivation for this proposal--we do not expect it to last long.  For this reason we request Director's Discretionary Time for a non-distruptive Target of Opportunity observation.</Abstract>
      
      <PrincipalInvestigator
         Honorific="Dr."
         FirstName="Peter"
         MiddleInitial="J."
         LastName="Brown"
         ESAMember="false"
         Retired="false"
         UniqueID="13695"
         Institution="Texas A &amp; M University"
         Country="USA"
         State="TX"
         Contact="true" />
      
      <CoInvestigator
         Honorific="Dr."
         FirstName="Jeff"
         LastName="Cooke"
         ESAMember="false"
         Retired="false"
         UniqueID="8306"
         Institution="Swinburne University of Technology"
         Country="AUS"
         State="VIC"
         Contact="false"
         AdminUSPI="false" />
      
      <CoInvestigator
         Honorific="Dr."
         FirstName="Jeremy"
         MiddleInitial="R."
         LastName="Mould"
         ESAMember="false"
         Retired="false"
         UniqueID="1895"
         Institution="Swinburne University of Technology"
         Country="AUS"
         State="VIC"
         Contact="false"
         AdminUSPI="false" />
      
      <CoInvestigator
         Honorific="Dr."
         FirstName="Lifan"
         LastName="Wang"
         ESAMember="false"
         Retired="false"
         UniqueID="5558"
         Institution="Texas A &amp; M University"
         Country="USA"
         State="TX"
         Contact="false"
         AdminUSPI="false" />
      
      <CoInvestigator
         Honorific="Mr."
         FirstName="Yi"
         LastName="Yang"
         ESAMember="false"
         Retired="false"
         UniqueID="17974"
         Institution="Texas A &amp; M University"
         Country="USA"
         State="TX"
         Contact="false"
         AdminUSPI="false" />
      
      <Questions>
         
         <Phase2Questions>
            
            <ObservingDescription>We will use STIS/MAMA with G230L to obtain NUV spectroscopy of the SN covering the bulk of the flux seen with Swift/UVOT photometry.  We will use STIS/CCD with G430L to obtain NUV/optical spectroscopy bridging the UV with optical.  We will use COS/FUV with G140L to cover the spectral region around Lyman alpha.


The target becomes unobservable from January 2-Feb 20, so we desire to observe the last week of December as the source may fade before it becomes observable again.</ObservingDescription>
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      <Phase1ProposalInformation
         Attachment="/Users/pbrown/Desktop/Dropbox/SN/proposals/HSTSLSNDDT/HSTSLSNDDT2.pdf">
         
         <ScientificCategory>HOT STARS</ScientificCategory>
         
         <ScientificKeyword1
            Keyword="Host Galaxies" />
         
         <ScientificKeyword2
            Keyword="Massive Stars" />
         
         <ScientificKeyword3
            Keyword="Supernovae" />
         
         <ScientificKeyword4
            Keyword="UV-Bright Stars" />
         
         <ProprietaryPeriod
            Default="false">0</ProprietaryPeriod>
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         PCFlag="false"
         ProposalSize="SMALL_CYCLE21">
         
         <Availability>SUPPORTED</Availability>
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         ReferenceFrame="ICRS"
         ProvisionalCoordinates="22 02 15.4500 -61 39 34.64">
         
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            <Description>SUPERNOVA</Description>
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         <Extended>NO</Extended>
         
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            <AlternateName>SN2015L</AlternateName>
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            <OtherFluxes>uvm2=17 (vega)</OtherFluxes>
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               <Wavelength>1425</Wavelength>
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