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<ri:Resource created="2007-12-01T07:29:55Z" 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>Chandra obs. of Serpens star-forming region</title><shortName>J/A+A/463/275</shortName><identifier>ivo://CDS.VizieR/J/A+A/463/275</identifier><altIdentifier>doi:10.26093/cds/vizier.34630275</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Giardino G.</name></creator><creator><name>Favata F.</name></creator><creator><name>Micela G.</name></creator><creator><name>Sciortino S.</name></creator><creator><name>Winston E.</name></creator><date role="Updated">2007-12-01T06:33:58Z</date><date role="Created">2007-12-01T07:29:55Z</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>stellar-associations</subject><subject>young-stellar-objects</subject><subject>pre-main-sequence-stars</subject><subject>x-ray-sources</subject><description>To study the properties of X-ray emission from young stellar objects (YSOs) through their evolution from Class I to Class III and determine whether Class 0 protostars emit X-rays. A deep Chandra X-ray observation of the Serpens star-forming region was obtained. 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