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          <title>HST  Archival Pure Parallels Project</title>
          <shortName>HST.APPP</shortName>
          <identifier>ivo://mast.stsci/siap/hst.appp</identifier>
          <altIdentifier>doi:10.17909/T9MG69</altIdentifier>
          <curation>
            <publisher ivo-id="ivo://archive.stsci.edu/stsci-arc">Space Telescope Science Institute Archive</publisher>
            <creator>
              <name>Casertano, et al</name>
            </creator>
            <version>1.0</version>
            <contact>
              <name>Archive Branch, STScI</name>
              <email>archive@stsci.edu</email>
            </contact>
          </curation>
          <content>
            <subject>Observational astronomy</subject>
            <subject>Optical  Astronomy</subject>
            <description>         The Archival Pure Parallel Project processed and combined about 2,000 WFPC2 images, primarily in the wide UBVI filters, obtained in parallel with other HST instruments. Combined, drizzled, cosmic-ray cleaned images were produced for each pointing. These data can be used to address a wide range of science topics: measuring the cosmic shear on scales from 20" to 2'; discovering ~ 50 starforming galaxies at z ~ 4; finding optical counterparts to AGNs in wide-area radio and X-ray catalogs; improving the determination of the scale length of the Galactic disk; and studying stellar populations down to 1 solar mass for about 25 separate lines of sight in the Magellanic Clouds.      </description>
            <referenceURL>http://archive.stsci.edu/prepds/appp/</referenceURL>
            <type>Archive</type>
            <contentLevel>Research</contentLevel>
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          <facility>HST</facility>
          <instrument>WFPC2</instrument>
          <coverage>
            <waveband>Optical</waveband>
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