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<ri:Resource created="2004-11-22T12:22:54Z" status="active" updated="2018-12-05T19:59:33Z" version="1.2" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:sn="http://www.ivoa.net/xml/SkyNode/v0.2" xmlns:vr="http://www.ivoa.net/xml/VOResource/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/VOResource/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VOResource.xsd" xsi:type="vs0:CatalogService">
          <validationLevel validatedBy="ivo://archive.stsci.edu/nvoregistry">2</validationLevel>
          <title>Sloan Digital Sky Survey</title>
          <shortName>SDSS</shortName>
          <identifier>ivo://sdss.jhu/openskynode/sdss</identifier>
          <curation>
            <publisher>         JHU      </publisher>
            <creator>
              <name>William O'Mullane</name>
            </creator>
            <contact>
              <name>vo-helpdesk</name>
              <email>vo-help@skysrv.pha.jhu.edu</email>
            </contact>
          </curation>
          <content>
            <subject>OpenSkyNode</subject>
            <subject>Galaxy</subject>
            <subject>Star</subject>
            <description>         This SkyNode points to the latest public SDSS catalog data release         available at http://cas.sdss.org/   The Sloan Digital Sky Survey is         the most ambitious astronomical survey ever undertaken. The survey         will map one-quarter of the entire sky in detail, determining the         positions and absolute brightnesses of hundreds of millions of         celestial objects. It will also measure the distances to more than a         million galaxies and quasars. The SDSS addresses fascinating,         fundamental questions about the universe. With the survey, astronomers         will be able to see the large-scale patterns of galaxies: sheets and         voids through the whole universe. Scientists have many ideas about how         the universe evolved, and different patterns of large-scale structure         point to different theories. The Sloan Digital Sky Survey will tell us         which theories are right - or whether we will have to come up with         entirely new ideas.      </description>
            <referenceURL>http://cas.sdss.org/</referenceURL>
          </content>
          <capability xsi:type="sn:OpenSkyNode" standardID="ivo://ivoa.net/std/OpenSkyNode">
            <validationLevel validatedBy="ivo://archive.stsci.edu/nvoregistry">2</validationLevel>
            <interface xsi:type="vr:WebService" role="std">
              <accessURL use="full">http://openskyquery.net/nodes//SDSS/nodeb.asmx</accessURL>
            </interface>
            <compliance>Full</compliance>
            <longitude>-76</longitude>
            <latitude>39</latitude>
            <maxRecords>5000</maxRecords>
            <primaryTable>photoprimary</primaryTable>
            <primaryKey>objid</primaryKey>
          </capability>
          <coverage>
            <waveband>Optical</waveband>
          </coverage>
        </ri:Resource>