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<ri:Resource created="2007-10-28T16:21:36Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" xmlns:cs="http://www.ivoa.net/xml/ConeSearch/v1.0" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" xmlns:vs="http://www.ivoa.net/xml/VODataService/v1.1" 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 http://www.ivoa.net/xml/VOResource/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VOResource.xsd http://www.ivoa.net/xml/VODataService/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/VODataService.xsd" xsi:type="vs:CatalogService"><title>Catalog of X-ray sources in the CYDER fields</title><shortName>J/ApJ/621/104</shortName><identifier>ivo://CDS.VizieR/J/ApJ/621/104</identifier><altIdentifier>doi:10.26093/cds/vizier.16210104</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Treister E.</name></creator><creator><name>Castander F.J.</name></creator><creator><name>Maccarone T.J.</name></creator><creator><name>Gawiser E.</name></creator><creator><name>Coppi P.S.,Urry C.M.</name></creator><creator><name>Maza J.</name></creator><creator><name>Herrera D.</name></creator><creator><name>Gonzalez V.</name></creator><creator><name>Montoya C.</name></creator><creator><name>Pineda P.</name></creator><date role="Updated">2007-10-28T15:25:20Z</date><date role="Created">2007-10-28T16:21:36Z</date><contact><name>CDS support team</name><address>CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France</address><email>cds-question@unistra.fr</email></contact></curation><content><subject>x-ray-sources</subject><subject>surveys</subject><subject>photometry</subject><description>We present the first results from the Calan-Yale Deep Extragalactic Research (CYDER) survey. The main goal of this survey is to study serendipitous X-ray sources detected by Chandra in an intermediate flux range (10^-15^ to 10^-12^ergs/s) that comprises most of the X-ray background. 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