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<HSTProposal
   Phase1ID="518"
   Phase2ID="13708"
   Phase="Phase II"
   AptVersion="Version 22.2 ">
   <!--**********************************************************************************************************************-->
   <!--This file is automatically generated and should not be edited by hand. Editing this file directly is at your own risk.-->
   <!--**********************************************************************************************************************-->
   <!--APT Output Product-->
   <!---->
   <!--APT Version: Version 22.2 -->
   <!--Date: Fri Jul 18 16:19:40 GMT 2014-->
   
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            AptVersion="Version 22.0.2 "
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            HasErrors="false"
            Cycle="22"
            IncludeSysInfo="true"
            NotificationAddress="nicole.reindl@uni-tuebingen.de"
            AssignedID="518">
            
            <SystemInformation
               os.arch="amd64"
               os.name="Windows 7"
               os.version="6.1"
               java.version="1.7.0_10"
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            <SubmissionCommentsCheckSum>0</SubmissionCommentsCheckSum>
            
            <SubmissionLog>Assigned ID: 518

----- Attempting Submission 1 (Fri Apr 11 15:04:48 GMT 2014) -----
  HST Phase I Proposal 518 (sao.apt) successfully submitted.</SubmissionLog>
            
            <DiagnosticJustification />
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         Key="Phase2SubmissionData">
         
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            AptVersion="Version 22.2 "
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            IncludeSysInfo="true"
            NotificationAddress="nicole.reindl@uni-tuebingen.de">
            
            <SystemInformation
               os.arch="amd64"
               os.name="Windows 7"
               os.version="6.1"
               java.version="1.7.0_60"
               Runtime.maxMemory="1212"
               linux.distribution="not available"
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               screens="1366x768" />
            
            <ErrorText>For the best data quality, it is strongly recommended that all four FP-POS positions be used when observing at a given COS CENWAVE setting.</ErrorText>
            
            <SubmissionComments />
            
            <SubmissionCommentsCheckSum>0</SubmissionCommentsCheckSum>
            
            <SubmissionLog>----- Attempting Submission 1 (Thu Jul 17 15:21:09 GMT 2014) -----</SubmissionLog>
            
            <Phase2DiagnosticJustification>There is no constraints on using all FP-POS for the NUV. If we would do so, we would lose too much exposure time, so we prefer to use only one FP-POS for the NUV observations.</Phase2DiagnosticJustification>
         </Phase2SubmissionData>
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   <ProposalInformation
      Category="GO"
      PureParallelProposal="false"
      Cycle="22"
      STScIEditNumber="1">
      
      <Title>Following the rapid evolution of the central star of the Stingray Nebula in real time</Title>
      
      <Abstract>SAO 244567 is an unusually fast evolving star. Within twenty years only, it has turned from a B-type supergiant into the central star of the Stingray nebula. Space and ground-based observations obtained over the last decades have revealed  that its spectrum changes noticeably over just a few years, showing stellar evolution in real time. Previous analysis indicates it must be a low mass star and thus the observed fast evolution is in strong contradiction with canonical post-asymptotic giant branch (AGB) evolution. A late He-shell flash is able to account for the rapid evolution. This scenario would predict an evolution back to the  AGB, e.g. a decrease of the effective temperature (which is already indicated by the FUSE observations in 2006) and an increase of luminosity. With COS spectroscopy we want to follow the  evolution of the surface properties of SAO 244567 to verify this thesis. The very compact nebula of SAO 244567 makes it impossible to derive these parameters from optical spectra, because most of the photospheric lines are blended by nebular emission lines thus they are not suitable for a spectral analysis. The derived surface parameters will establish constraints for late thermal pulse evolutionary calculations. With these calculations we aim not only to explain the nature of SAO 244567, but they also will provide a deeper insight in the formation process of hydrogen deficient stars, which make up 25% of the post AGB-stars and white dwarfs.</Abstract>
      
      <PrincipalInvestigator
         Honorific="Ms."
         FirstName="Nicole"
         LastName="Reindl"
         ESAMember="true"
         UniqueID="13417"
         Institution="Eberhard Karls Universitat, Tubingen"
         Country="DEU"
         Contact="true" />
      
      <CoInvestigator
         Honorific="Prof."
         FirstName="Klaus"
         LastName="Werner"
         ESAMember="true"
         UniqueID="12842"
         Institution="Eberhard Karls Universitat, Tubingen"
         Country="DEU"
         Contact="false"
         AdminUSPI="false"
         CoPI="true" />
      
      <CoInvestigator
         Honorific="Dr."
         FirstName="Thomas"
         LastName="Rauch"
         ESAMember="true"
         UniqueID="12841"
         Institution="Eberhard Karls Universitat, Tubingen"
         Country="DEU"
         Contact="false"
         AdminUSPI="false"
         CoPI="true" />
      
      <CoInvestigator
         Honorific="Dr."
         FirstName="Marcelo Miguel"
         LastName="Miller Bertolami"
         ESAMember="true"
         UniqueID="16902"
         Institution="Max-Planck-Institut fur Astrophysik"
         Country="DEU"
         Contact="false"
         AdminUSPI="false"
         CoPI="true" />
      
      <CoInvestigator
         Honorific="Dr."
         FirstName="Mudumba"
         LastName="Parthasarathy"
         ESAMember="false"
         UniqueID="2016"
         Institution="Indian Institute of Astrophysics"
         Country="IND"
         State="Bangalore"
         Contact="false"
         AdminUSPI="false"
         CoPI="true" />
      
      <Questions>
         
         <Phase2Questions>
            
            <ObservingDescription>FUV (medium and low resolution) and NUV (low resolution) spectra of SAO244567 (star) shall be observed within 1 visit.
Orbit 1 to 4: COS/PSA G130M with central wavelength 1222 A. One different FP-POS per orbit.
Orbit 5:  COS/PSA G140L with central wavelength 1280 A. COS/PSA G230L with central wavelengths 3360 A and 2635 A.</ObservingDescription>
         </Phase2Questions>
      </Questions>
      
      <Orbits
         ThisCycle2GyroPrimary="5" />
      
      <Phase1ProposalInformation
         TotalTargets="1"
         Attachment="/solaris/user1/mlink/work/C:\Users\Nicole\Desktop\phase1-GO.pdf"
         ProposalSize="SMALL">
         
         <ScientificCategory>HOT STARS</ScientificCategory>
         
         <ScientificKeyword1
            Keyword="Atmospheres And Chromospheres" />
         
         <ScientificKeyword2
            Keyword="Central Stars Of Planetary Nebulae" />
         
         <ScientificKeyword3
            Keyword="Chemical Abundances" />
         
         <ScientificKeyword4
            Keyword="Stellar Evolution And Models" />
         
         <ScientificKeyword5
            Keyword="White Dwarfs" />
         
         <ProprietaryPeriod>Default</ProprietaryPeriod>
         
         <CalibProp>false</CalibProp>
         
         <UvInit>true</UvInit>
         
         <Treasury>false</Treasury>
         
         <MultiCycleTreasury>false</MultiCycleTreasury>
         
         <Theory>false</Theory>
      </Phase1ProposalInformation>
      
      <Phase2ProposalInformation
         PCFlag="true"
         ProposalSize="SMALL_CYCLE21">
         
         <Availability>SUPPORTED</Availability>
      </Phase2ProposalInformation>
   </ProposalInformation>
   
   <Targets>
      
      <FixedTarget
         Name="NAME-STINGRAY-NEBULA"
         Number="1"
         ReferenceFrame="ICRS"
         RAPMUnits="MAS_PER_YEAR"
         DecPMUnits="MAS_PER_YEAR"
         Epoch="2000"
         ProvisionalCoordinates="17 16 21.0800 -59 29 23.30">
         
         <PrimaryCategory>STAR</PrimaryCategory>
         
         <PrimaryDescription>
            
            <Description>PLANETARY NEBULA CENTRAL STAR</Description>
         </PrimaryDescription>
         
         <Comments>This object was generated by the targetselector and retrieved from the SIMBAD database.</Comments>
         
         <AlternateNames />
         
         <EquatorialPosition
            Value="17 16 21.0800 -59 29 23.30">
            
            <RAUnc
               Arcsec="1" />
            
            <DECUnc
               Arcsec="1" />
            
            <Equinox>J2000</Equinox>
         </EquatorialPosition>
         
         <Equinox>J2000</Equinox>
         
         <Fluxes>
            
            <BroadBandMagnitude
               Band="V"
               Magnitude="15.0"
               MagnitudeUnc="0.8" />
            
            <OtherFluxes>f_max(at 1200A) = 3.2*10^-13 erg cm^2 s^-1 A^-1, f_min (at 1200A) = 0.8 *10^-13 erg cm^2 s^-1 A^-1</OtherFluxes>
         </Fluxes>
      </FixedTarget>
   </Targets>
   
   <Observations>
      
      <Observation
         TargetName="NAME-STINGRAY-NEBULA"
         Instrument="COS"
         Number="1"
         NumberOfOrbits="5"
         NumberOfIterations="1"
         TotalOrbits="5"
         PureParallel="false"
         CoordinatedParallel="false"
         TargetOfOpportunity="No"
         CVZ="false"
         Duplication="false">
         
         <Configurations>
            
            <Configuration>
               
               <Config>COS/FUV</Config>
               
               <ScienceMode>Spectroscopic</ScienceMode>
               
               <Coronography>No</Coronography>
               
               <Polarimetry>No</Polarimetry>
               
               <SpectralElement>G130M</SpectralElement>
               
               <Wavelength>1222</Wavelength>
            </Configuration>
            
            <Configuration>
               
               <Config>COS/FUV</Config>
               
               <ScienceMode>Spectroscopic</ScienceMode>
               
               <Coronography>No</Coronography>
               
               <Polarimetry>No</Polarimetry>
               
               <SpectralElement>G140L</SpectralElement>
               
               <Wavelength>1280</Wavelength>
            </Configuration>
            
            <Configuration>
               
               <Config>COS/NUV</Config>
               
               <ScienceMode>Spectroscopic</ScienceMode>
               
               <Coronography>No</Coronography>
               
               <Polarimetry>No</Polarimetry>
               
               <SpectralElement>G230L</SpectralElement>
               
               <Wavelength>3360</Wavelength>
            </Configuration>
            
            <Configuration>
               
               <Config>COS/NUV</Config>
               
               <ScienceMode>Spectroscopic</ScienceMode>
               
               <Coronography>No</Coronography>
               
               <Polarimetry>No</Polarimetry>
               
               <SpectralElement>G230L</SpectralElement>
               
               <Wavelength>2635</Wavelength>
            </Configuration>
         </Configurations>
         
         <ObservationRequirements
            NoConstraints="true" />
         
         <AladinPhase1Requirements
            Detector="COS/FUV"
            Aperture="PSA/BOA"
            MosaicHeight=""
            MosaicWidth=""
            MosaicTileOverlap="10.0"
            AladinOrientationAngle="">
            
            <CoordinatedParallels />
            
            <AladinPhase1SubExposure0
               PrimaryPatternPosition="0"
               CopyNumber="0"
               IsDeleteAcceptable="false"
               PosTargX="0.0"
               PosTargY="0.0" />
         </AladinPhase1Requirements>
         
         <SuitabilityResults
            DaysHigh="0"
            DaysHighMed="0"
            DaysLowMed="0"
            DaysLow="0"
            OrbitsPerDay="0.0"
            ObservationRequirements="NOCONSTRAINTS" />
      </Observation>
   </Observations>
   
   <Datasets />
   
   <Patterns />
   
   <Visits>
      
      <Visit
         Number="01"
         Status="implementation"
         After=""
         Before="">
         
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               <OpToolDataDate>
                  
                  <Time>1405610059522</Time>
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               <OpToolDataString>
                  
                  <Value>C:\Users\Nicole\Documents\OP-cache\sao-v01.xml</Value>
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            <ToolDataItem
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               <VpVisitData>
                  
                  <StVisitSchedulingWindows
                     Binary="true"
                     UpToDate="false"
                     StSchedulingPCF="1406851200000 0.0 1409443200000 1.0 1410998399000 0.0 1411430400000 1.0 1411862399000 0.0 1415059200000 1.0 1415404799000 0.0 1424476800000 1.0 1425686398999 0.0 1429228800000 1.0 1430351998999 0.0 1433376000000 1.0 1434844798999 0.0 1437696000000 1.0 1439251198999 0.0 1442448000000 1.0 1444003198999 0.0 1444176000000 1.0 1444867198999 0.0 1453377600000 1.0 1453420798999 0.0 1457481600000 1.0 1458604798999 0.0 1459296000000">
                     
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                        Name="Target Visibility"
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                     <AncillaryData
                        Title="Comments"
                        Label="Comments">
                        
                        <String>The scheduling data was generated by CASM 22.2.</String>
                        
                        <String>CASM was run in Phase II mode.</String>
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                  </StVisitSchedulingWindows>
                  
                  <AncillaryData
                     Title="Roll Ranges Report"
                     Label="Roll Ranges Report"
                     Header="  Target: NAME-STINGRAY-NEBULA&#xA;  RA: 17 16 21.0800&#xA;  DEC: -59 29 23.30&#xA;  Dates: 8/1/2014 -- 3/30/2016&#xA;&#xA;Day&#x9;Available Roll Ranges (U3 Angles)">
                     
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