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<HSTProposal
   Phase1ID="1555"
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   <!--Date: Wed Jun 30 17:21:15 GMT 2021-->
   
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            <SubmissionLog>Assigned ID: 1555

----- Attempting Submission 1 (Wed Apr 07 17:13:45 GMT 2021) -----
HST Phase I Proposal 1555  successfully submitted.
Receipt: # 1555-1

----- Attempting Submission 2 (Fri Apr 09 18:53:38 GMT 2021) -----</SubmissionLog>
            
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   <ProposalInformation
      Category="AR"
      SnapPriority="Normal Priority"
      PureParallelProposal="false"
      Cycle="29"
      STScIEditNumber="0">
      
      <Title>Sculpting Hubble's Exoplanet Legacy: A Comprehensive Uniform Dataset of Exoplanet Transmission Spectra</Title>
      
      <Abstract>HST launched the field of exoplanet atmospheres, thanks in large part to it's unprecedented ability to gather high precision time series spectroscopy from the UV to near-IR. Scores of exoplanet atmospheres have been been detected, with atmospheric features found in planets ranging from Jupiter down to mini-Neptune masses. While the archive is rich with exoplanet data on more than 70 exoplanets, the full potential of this data has not even begun to be realized, as no comprehensive effort has been made to reduce and compile this eclectic set of spectra together. Unfortunately, one cannot simply download a calibrated exoplanet spectrum from the MAST archive, as time series data has not been supported by STScI in this manner. The majority of this data has been published, but typically not with the latest reduction methods and calibration issues between instruments is common which complicates using literature HST spectra for JWST analysis.  This archive program fills this need, generating a complete and homogeneous set of calibrated exoplanet spectra, and their ancillary data products, to a central STScI MAST location and makes publicly available all the software tools. With a modern analysis, nearly a large program of previously discarded orbits can be used. With a homogenous database of exoplanet spectra, our program enables comparative planetology studies on a wide scale, where we can gain the maximum leverage on what the physical effects environmental factors may have on the clouds seen in the optical and molecular features observed in the infrared. This database will provide a legacy set of HST near-UV and optical exoplanet spectra, ready to be utilized for JWST.</Abstract>
      
      <PrincipalInvestigator
         Honorific="Prof."
         FirstName="David"
         MiddleInitial="K."
         LastName="Sing"
         ESAMember="false"
         CSAMember="false"
         Retired="false"
         UniqueID="7102"
         Institution="The Johns Hopkins University"
         Country="USA"
         State="MD"
         Contact="true" />
      
      <CoInvestigator
         Honorific="Dr."
         FirstName="Mercedes"
         LastName="Lopez-Morales"
         ESAMember="false"
         CSAMember="false"
         Retired="false"
         UniqueID="13898"
         Institution="Smithsonian Institution Astrophysical Observatory"
         Country="USA"
         State="MA"
         Contact="false"
         AdminUSPI="false" />
      
      <CoInvestigator
         Honorific="Dr."
         FirstName="Munazza"
         LastName="Alam"
         ESAMember="false"
         CSAMember="false"
         Retired="false"
         UniqueID="21461"
         Institution="Harvard University"
         Country="USA"
         State="MA"
         Contact="false"
         AdminUSPI="false" />
      
      <CoInvestigator
         Honorific="Dr."
         FirstName="Kevin"
         LastName="Stevenson"
         ESAMember="false"
         CSAMember="false"
         Retired="false"
         UniqueID="12419"
         Institution="The Johns Hopkins University Applied Physics Laboratory"
         Country="USA"
         State="MD"
         Contact="false"
         AdminUSPI="false" />
      
      <CoInvestigator
         Honorific="Dr."
         FirstName="Hannah"
         LastName="Wakeford"
         ESAMember="true"
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         Retired="false"
         UniqueID="13756"
         Institution="University of Bristol"
         Country="GBR"
         State="England"
         Contact="false"
         AdminUSPI="false" />
      
      <CoInvestigator
         Honorific="Dr."
         FirstName="Nikolay"
         LastName="Nikolov"
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         Retired="false"
         UniqueID="39110"
         Institution="Space Telescope Science Institute"
         Country="USA"
         State="MD"
         Contact="false"
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      <CoInvestigator
         FirstName="Nestor"
         LastName="Espinoza"
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         UniqueID="27592"
         Institution="Space Telescope Science Institute"
         Country="USA"
         State="MD"
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      <CoInvestigator
         Honorific="Dr."
         FirstName="Thomas"
         LastName="Mikal-Evans"
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         CSAMember="false"
         Retired="false"
         UniqueID="16389"
         Institution="Massachusetts Institute of Technology"
         Country="USA"
         State="MA"
         Contact="false"
         AdminUSPI="false" />
      
      <CoInvestigator
         FirstName="Zafar"
         LastName="Rustamkulov"
         ESAMember="false"
         CSAMember="false"
         Retired="false"
         UniqueID="27413"
         Institution="The Johns Hopkins University"
         Country="USA"
         State="MD"
         Contact="false"
         AdminUSPI="false" />
      
      <CoInvestigator
         Honorific="Ms."
         FirstName="Natalie"
         LastName="Allen"
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         CSAMember="false"
         Retired="false"
         UniqueID="39857"
         Institution="The Johns Hopkins University"
         Country="USA"
         State="MD"
         Contact="false"
         AdminUSPI="false" />
      
      <CoInvestigator
         Honorific="Mr."
         FirstName="Jayshil"
         MiddleInitial="A"
         LastName="Patel"
         ESAMember="false"
         CSAMember="false"
         Retired="false"
         UniqueID="26486"
         Institution="Sardar Vallabhbhai National Institute of Technology, Surat-7"
         Country="IND"
         State="Gujarat"
         Contact="false"
         AdminUSPI="false" />
      
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      <TeamExpertise>Prof. David Sing has significant experience and expertise in the setup and reduction of HST STIS and WFC3 observations. Prof. Sing is also an expert in exoplanet transit observations, leading many HST observing programs targeting transiting planets over the last 10 cycles. He has published 43 refereed papers over the last 12 years on HST-collected transiting exoplanet data. 
Z. Rustamkulov and N. Allen are PhD students at JHU advised by Prof. Sing and is focusing his PhD on the observations of transiting exoplanets.
Dr. Hannah Wakeford, T. Mikal-Evans, and K Stevenson are experts in WFC3 data reduction in transiting exoplanets.
Dr. N. Nikolov and M. Alam are experts in STIS data reduction in transiting exoplanets.
Dr. M. Lopez-Morales and N. Espinoza are experts in stellar astrophysics and transiting exoplanets.</TeamExpertise>
      
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         Attachment="/Users/sing/OneDrive - Johns Hopkins/PROPOSALS/HST/cycle29/Sing_Comprhensive_Archive/Hubble_Legacy_AR.pdf">
         
         <ScientificCategory>Exoplanets and Exoplanet Formation</ScientificCategory>
         
         <ScientificKeyword1
            Keyword="Exoplanet Atmospheres" />
         
         <ScientificKeyword2
            Keyword="Exoplanet Atmospheric Composition" />
         
         <ScientificKeyword3
            Keyword="Transits" />
         
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         <Budget>Legacy</Budget>
         
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         <FundamentalPhysics>false</FundamentalPhysics>
         
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