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   <!--Date: Fri Apr 07 23:48:12 GMT 2017-->
   
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            NotificationAddress="vickykhaire@gmail.com"
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            <SubmissionLog>Assigned ID: 1024

----- Attempting Submission 1 (Fri Apr 07 22:44:51 GMT 2017) -----
HST Phase I Proposal 1024 (igmz1.apt) successfully submitted.
Receipt: # 1024-1

----- Attempting Submission 2 (Fri Apr 07 22:51:26 GMT 2017) -----
HST Phase I Proposal 1024 (igmz1.apt) successfully submitted.
Receipt: # 1024-2

----- Attempting Submission 3 (Fri Apr 07 23:48:12 GMT 2017) -----</SubmissionLog>
            
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   <ProposalInformation
      Category="AR"
      PureParallelProposal="false"
      Cycle="25"
      STScIEditNumber="0">
      
      <Title>Filling the Void: A Comprehensive Survey of the Intergalactic Medium at z~1 Using STIS/COS Archival Spectra</Title>
      
      <Abstract>There exists a large void in our understanding of the intergalactic medium (IGM) at z=0.5-1.5, spanning a significant cosmic time of 4 Gyr. This hole resulted from a paucity of near-UV QSO spectra, which were historically very expensive to obtain.  However, with the advent of COS and the HST UV initiative, sufficient STIS/COS NUV spectra have finally become available, enabling the first statistical analyses.  We propose a comprehensive study of the z~1 IGM using the Ly-alpha forest of 26 archival QSO spectra. This analysis will: (1) measure the distribution of HI absorbers to several percent precision down to log NHI &lt; 13 to test our model of the IGM, and determine  the extragalactic UV background (UVB) at that epoch; (2) measure the Ly-alpha forest power spectrum to ~12%, providing another precision test of LCDM and our theory of the IGM; (3) measure the thermal state of the IGM, which reflects the balance of heating (photoheating, HI/HeII reionization) and cooling (Hubble expansion) of cosmic baryons, and directly verify the predicted cooldown of IGM gas after reionization for the first time; (4) generate high-quality reductions, coadds, and continuum fits that will be released to the public to enable other science cases. These results, along with our state-of-the-art hydrodynamical simulations, and theoretical models of the UVB, will fill the 4 Gyr hole in our understanding of the IGM. When combined with existing HST and ground-based data from lower and higher z, they will lead to a complete, empirical description of the IGM from HI reionization to the present, spanning more than 10 Gyr of cosmic history, adding substantially to Hubble's legacy of discovery on the IGM.</Abstract>
      
      <PrincipalInvestigator
         FirstName="Vikram"
         LastName="Khaire"
         ESAMember="false"
         CSAMember="false"
         Retired="false"
         UniqueID="19887"
         Institution="IUCAA"
         Country="IND"
         State="MAHARASHTRA"
         Contact="true"
         AdminCoI="CoI: Prof. Joseph Hennawi " />
      
      <CoInvestigator
         FirstName="Michael"
         LastName="Walther"
         ESAMember="false"
         CSAMember="false"
         Retired="false"
         UniqueID="17793"
         Institution="University of California - Santa Barbara"
         Country="USA"
         State="CA"
         Contact="true"
         AdminUSPI="false"
         CoPI="true" />
      
      <CoInvestigator
         Honorific="Prof."
         FirstName="Joseph"
         LastName="Hennawi"
         ESAMember="false"
         CSAMember="false"
         Retired="false"
         UniqueID="7082"
         Institution="University of California - Santa Barbara"
         Country="USA"
         State="CA"
         Contact="false"
         AdminUSPI="true" />
      
      <CoInvestigator
         Honorific="Dr."
         FirstName="Jason"
         MiddleInitial="X."
         LastName="Prochaska"
         ESAMember="false"
         CSAMember="false"
         Retired="false"
         UniqueID="4705"
         Institution="University of California - Santa Cruz"
         Country="USA"
         State="CA"
         Contact="false"
         AdminUSPI="false" />
      
      <CoInvestigator
         Honorific="Dr."
         FirstName="Gabor"
         LastName="Worseck"
         ESAMember="true"
         CSAMember="false"
         Retired="false"
         UniqueID="8575"
         Institution="Max-Planck-Institut fur Astronomie, Heidelberg"
         Country="DEU"
         Contact="false"
         AdminUSPI="false" />
      
      <CoInvestigator
         Honorific="Dr."
         FirstName="Jose"
         LastName="Onorbe"
         ESAMember="true"
         CSAMember="false"
         Retired="false"
         UniqueID="12976"
         Institution="Max-Planck-Institut fur Astronomie, Heidelberg"
         Country="DEU"
         Contact="false"
         AdminUSPI="false" />
      
      <CoInvestigator
         Honorific="Dr."
         FirstName="Zarija"
         LastName="Lukic"
         ESAMember="false"
         CSAMember="false"
         Retired="false"
         UniqueID="21351"
         Institution="Lawrence Berkeley National Laboratory"
         Country="USA"
         State="CA"
         Contact="false"
         AdminUSPI="false" />
      
      <Questions>
         
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            <ObservingDescription />
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      <Phase1ProposalInformation
         Attachment="/home/walther/Dropbox/igm_z1_archival/z1IGM-AR_v10.pdf">
         
         <ScientificCategory>Galaxies and the IGM</ScientificCategory>
         
         <SecondaryScientificCategory>Cosmology</SecondaryScientificCategory>
         
         <ScientificKeyword1
            Keyword="Lyman-Alpha Forest" />
         
         <ScientificKeyword2
            Keyword="Metal Absorption Systems" />
         
         <ScientificKeyword3
            Keyword="Simulations and Models" />
         
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            Default="true">0</ProprietaryPeriod>
         
         <Budget>Regular</Budget>
         
         <CalibProp>false</CalibProp>
         
         <UvInit>true</UvInit>
         
         <Theory>false</Theory>
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         <Availability>SUPPORTED</Availability>
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         NumberOfDatasets="14"
         RetrievalMethod="FTP"
         RetrievalPlan="Data transfer will take place over the course of one day" />
      
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         Number="2"
         NumberOfDatasets="20"
         RetrievalMethod="FTP"
         RetrievalPlan="Data transfer will take place over the course of one day" />
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