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      <Title>A new wide-separation Einstein Cross at z=2.7</Title>
      
      <Abstract>We propose ACS F555W and F814W imaging observations of a new wide-separation Einstein Cross selected from SDSS spectroscopy through a bright anomalous emission line and confirmed recently with Keck imaging and spectroscopy.  The source galaxy is a moderately luminous (L~0.2L*) Lyman-alpha emitter at z=2.699, which is magnified and extended by more than a factor of twenty, making it one of the most accessible high-redshift bright Ly-a emitters on the sky.  Its apparent flux is only 1.2 magnitudes fainter than MS1612-cB58, making this an ideal system for detailed study of the metallicity and initial mass function of a high-redshift star forming galaxy.  The Einstein Radius is ~1.8arcsec, one of the widest known, making future spectroscopic ground-based followup optimal.  This angle subtends ~5 kpc at the lens galaxy at z=0.331.  The high resolution, high signal to noise imaging we propose to obtain will allow us to build accurate lensing models, including source reconstructions; combined with existing and planned Keck spectroscopy, will make possible a map of the host dark matter halo density profile to greater than one effective light radius; and will reveal lower surface brightness features associated with the bright star-forming knot lensed into the Cross.  Finally, it will be an exquisite Hubble Heritage galaxy, which will be indispensable for many other applications.  We are requesting a very modest proprietary period, in order to provide high-level reductions and ancillary data publically available simultaneously.</Abstract>
      
      <PrincipalInvestigator
         Honorific="Dr."
         FirstName="Leonidas"
         LastName="Moustakas"
         ESAMember="false"
         UniqueID="4210"
         AddressVerifiedCycle="15">
         
         <Address
            Institution="Jet Propulsion Laboratory"
            USState="CA"
            Country="USA" />
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         Honorific="Dr."
         FirstName="Daniel"
         LastName="Stern"
         ESAMember="false"
         UniqueID="4419"
         AdminUSPI="false"
         Contact="false"
         AddressVerifiedCycle="15">
         
         <Address
            Institution="Jet Propulsion Laboratory"
            USState="CA"
            Country="USA" />
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      <CoInvestigator
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         FirstName="Adam"
         MiddleInitial="S."
         LastName="Bolton"
         ESAMember="false"
         UniqueID="7373"
         AdminUSPI="false"
         Contact="false"
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         <Address
            Institution="Smithsonian Institution Astrophysical Observatory"
            USState="MA"
            Country="USA" />
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      <CoInvestigator
         Honorific="Prof."
         FirstName="Scott"
         LastName="Burles"
         ESAMember="false"
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         Contact="false"
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         <Address
            Institution="Massachusetts Institute of Technology"
            USState="MA"
            Country="USA" />
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      <CoInvestigator
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         FirstName="Arjun"
         LastName="Dey"
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         <Address
            Institution="National Optical Astronomy Observatories, AURA"
            USState="AZ"
            Country="USA" />
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         <Address
            Institution="University of California - Berkeley"
            USState="CA"
            Country="USA" />
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         Attachment="/Users/leonidas/work/proposals/hst15/phase15-cross.pdf">
         
         <ScientificCategory>COSMOLOGY</ScientificCategory>
         
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            Keyword="GALAXY HALOS" />
         
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            Keyword="GALAXY MORPHOLOGY AND STRUCTURE" />
         
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            Keyword="GRAVITATIONAL LENSING" />
         
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