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<ri:Resource created="2006-11-05T14:34:44Z" 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 Deep Field North survey. XII</title><shortName>J/AJ/124/2351</shortName><identifier>ivo://CDS.VizieR/J/AJ/124/2351</identifier><altIdentifier>doi:10.26093/cds/vizier.51242351</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Bauer F.E.</name></creator><creator><name>Alexander D.M.</name></creator><creator><name>Brandt W.N.</name></creator><creator><name>Hornschemeier A.E.</name></creator><creator><name>Vignali C.,Garmire G.P.</name></creator><creator><name>Schneider D.P.</name></creator><date role="Updated">2023-04-06T16:50:52Z</date><date role="Created">2006-11-05T14:34:44Z</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>radio-sources</subject><description>We investigate the relationship between faint X-ray and 1.4GHz radio source populations detected within 3' of the Hubble Deep Field (North) using the 1Ms Chandra (Cat. &lt;J/AJ/122/2810&gt;) and 40{mu}Jy VLA (Cat. &lt;J/ApJ/533/611&gt;) surveys. Within this region, we find that ~42% of the 62 X-ray sources have radio counterparts and ~71% of the 28 radio sources have X-ray counterparts; thus, a 40{mu}Jy VLA survey at 1.4GHz appears to be well matched to a 1Ms Chandra observation.</description><source format="bibcode">2002AJ....124.2351B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/124/2351</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship><relationship><relationshipType>IsServedBy</relationshipType><relatedResource>Conesearch service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/533/611">J/ApJ/533/611 : 1.4GHz survey in HDF region (Richards+, 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/554/742">J/ApJ/554/742 : Chandra Deep Survey of the HDF-N (Hornschemeier+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/122/2810">J/AJ/122/2810 : Chandra Deep Field North Survey. 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