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<ri:Resource created="2005-08-20T21:09:02Z" 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>XMM/CFDS catalogue</title><shortName>J/MNRAS/350/785</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/350/785</identifier><altIdentifier>doi:10.26093/cds/vizier.73500785</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Waskett T.J.</name></creator><creator><name>Eales S.A.</name></creator><creator><name>Gear W.K.</name></creator><creator><name>McCracken H.J.</name></creator><creator><name>Brodwin M.</name></creator><creator><name>Nandra K.,Laird E.S.</name></creator><creator><name>Lilly S.</name></creator><date role="Updated">2024-06-29T20:15:00Z</date><date role="Created">2005-08-20T21:09:02Z</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>galaxies</subject><subject>photometry</subject><subject>redshifted</subject><description>We present the X-ray source catalogues for the XMM surveys of the 3-h and 14-h (also known as the Groth Strip) Canada-France Redshift Survey fields (0.5-10keV flux range ~2x10^-15^-10^-13^erg/cm^2^/s). We use a subset of the XMM sources, which have Chandra positions, to determine the best method of obtaining optical identifications of sources with only XMM positions. We find optical identifications for 79 per cent of the XMM sources for which there are deep optical images. The sources without optical identifications are likely to be optically fainter and have higher redshifts than the sources with identifications. We have estimated 'photometric redshifts' for the identified sources, calibrating our method using ~200 galaxies in the fields with spectroscopic redshifts. We find that the redshift distribution has a strong peak at z~0.7.</description><source format="bibcode">2004MNRAS.350..785W</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/350/785</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/B/xmm">B/xmm : XMM-Newton Observation Log (XMM-Newton SOC, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/225">VII/225 : The Canada-France Redshift Survey (CFRS) (Lilly+, 1995)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/464/79">J/ApJ/464/79 : CFRS XI: High-z field galaxies morphology (Schade+ 1996)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/481/49">J/ApJ/481/49 : CFRS XIV. Field galaxies up to z=1 (Hammer+ 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/142/1">J/ApJS/142/1 : DEEP Groth Strip Survey. II. (Simard+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/599/1006">J/ApJ/599/1006 : DEEP Groth Strip Survey. VII. (Kobulnicky+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/571/136">J/ApJ/571/136 : DEEP Groth Strip survey. X. 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PN camera HR ratio (1)</description><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_HRPN</name><description>? rms uncertainty on HRPN</description><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>HRM1</name><description>? MOS1 camera HR ratio (1)</description><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_HRM1</name><description>? rms uncertainty on HRM1</description><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>HRM2</name><description>? MOS2 camera HR ratio (1)</description><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_HRM2</name><description>? rms uncertainty on HRM2</description><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Notes</name><description>Notes (G1)</description><dataType xsi:type="vs:VOTableType" arraysize="6*">char</dataType></column></table><table><name>J/MNRAS/350/785/tablea34</name><description>ID properties of the 86 3h and 126 14h fields XMM sources</description><column><name>DEJ2000</name><description>CDFS declination in decimal degrees (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Offset</name><description>? Offset between XMM source and CFDF object</description><unit>arcsec</unit><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>P'</name><description>? 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Photometric redshift from UBVRIZ photometry</description><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>n_zUBVRIZ</name><description>[*] *: less reliable redshift</description><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Notes</name><description>Notes (G1)</description><dataType xsi:type="vs:VOTableType" arraysize="9*">char</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>[WEG2004]</name><description>Source designation, 3h NNN or 14h NNN</description><dataType xsi:type="vs:VOTableType" arraysize="7*">char</dataType></column><column><name>CFDF</name><description>? 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