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<ri:Resource created="2017-06-08T15:55:21Z" status="active" updated="2020-02-12T19:53:23Z" version="1.2" xmlns:cs="http://www.ivoa.net/xml/ConeSearch/v1.0" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:vs0="http://www.ivoa.net/xml/VODataService/v1.0" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.ivoa.net/xml/ConeSearch/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/ConeSearch.xsd" xsi:type="vs0:CatalogService">
          <validationLevel validatedBy="ivo://archive.stsci.edu/nvoregistry">2</validationLevel>
          <title>Kepler K2 Ecliptic Plane Input Catalog </title>
          <shortName>K2 EPIC</shortName>
          <identifier>ivo://archive.stsci.edu/kepler/k2_epic</identifier>
          <altIdentifier>doi:10.17909/T93W28</altIdentifier>
          <curation>
            <publisher ivo-id="ivo://archive.stsci.edu/stsci-arc">
Space Telescope Science Institute Archive
</publisher>
            <creator>
              <name>Kepler K2 Project</name>
              <logo/>
            </creator>
            <creator>
              <name>MAST</name>
              <logo/>
            </creator>
            <contact>
              <name>Randy Thompson</name>
              <email>archive@stsci.edu</email>
            </contact>
          </curation>
          <content>
            <subject>Exoplanet astronomy</subject>
            <subject>Stars</subject>
            <subject>Galaxies</subject>
            <subject>Exoplanets</subject>
            <subject>Variable stars</subject>
            <description>
Launched in 2009, the Kepler Mission is surveying a region of our galaxy to determine what fraction of stars 
in our galaxy have planets and measure the size distribution of those exoplanets. 
Although Kepler completed its primary mission to determine the fraction of stars that have planets in 2013, 
it is continuing the search, using a more limited survey mode, under the new name K2. 

The K2 Ecliptic Plane Input Catalog is the primary source of information about 
objects observed as potential targets for the K2 mission, as the Kepler Input Catalog was used for the original Kepler mission. 
</description>
            <referenceURL>http://archive.stsci.edu/kepler/</referenceURL>
            <type>Archive</type>
            <contentLevel>Research</contentLevel>
          </content>
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            <validationLevel validatedBy="ivo://archive.stsci.edu/nvoregistry">2</validationLevel>
            <description/>
            <interface xsi:type="vs0:ParamHTTP" role="std" version="">
              <accessURL use="base">http://archive.stsci.edu/k2/epic/search.php?</accessURL>
              <queryType>GET</queryType>
            </interface>
            <maxSR>180</maxSR>
            <verbosity>false</verbosity>
          </capability>
          <coverage>
            <waveband>Optical</waveband>
          </coverage>
        </ri:Resource>