<?xml-stylesheet href='/static/xsl/oai.xsl' type='text/xsl'?>
<ri:Resource created="2006-01-13T15:27:16Z" 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 observations of Lockman Hole brightest AGNs</title><shortName>J/A+A/444/79</shortName><identifier>ivo://CDS.VizieR/J/A+A/444/79</identifier><altIdentifier>doi:10.26093/cds/vizier.34440079</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Mateos S.</name></creator><creator><name>Barcons X.</name></creator><creator><name>Carrera F.J.</name></creator><creator><name>Ceballos M.T.</name></creator><creator><name>Hasinger G.,Lehmann I.</name></creator><creator><name>Fabian A.C.</name></creator><creator><name>Streblyanska A.</name></creator><date role="Updated">2006-01-13T14:27:25Z</date><date role="Created">2006-01-13T15:27:16Z</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>active-galactic-nuclei</subject><description>This paper presents the results of a detailed X-ray spectral analysis of a sample of 123 X-ray sources detected with XMM-Newton in the Lockman Hole field. This is the deepest observation carried out with XMM-Newton with more that 600ks of good EPIC-pn data. We have spectra with good signal to noise (&gt;500 source counts) for all objects down to 0.2-12keV fluxes of 5x10^-15^erg/cm^2^/s (flux limit of 6x10^-16^erg/cm^2^/s in the 0.5-2 and 2-10keV bands). At the time of the analysis, we had optical spectroscopic identifications for 60% of the sources, 46 being optical type-1 AGN and 28 optical type-2 AGN. Using a single power law model our sources' average spectral slope hardens at faint 0.5-2keV fluxes but not at faint 2-10keV fluxes.</description><source format="bibcode">2005A&amp;A...444...79M</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/444/79</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/A+A/393/425">J/A+A/393/425 : Spectral analysis of Lockman Hole (Mainieri+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/329/482">J/A+A/329/482 : ROSAT Deep Survey in the Lockman Hole (Hasinger+, 1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/398/901">J/A+A/398/901 : VLA survey at 6cm in the Lockman Hole (Ciliegi+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/413/843">J/A+A/413/843 : Far IR survey in the Lockman Hole (Kawara+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/427/23">J/A+A/427/23 : 14.3um survey in the Lockman Hole (Fadda+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/427/773">J/A+A/427/773 : ISOCAM 14.3um Deep Survey in Lockman Hole (Rodighiero+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/125/2521">J/AJ/125/2521 : 2MASS6x survey of the Lockman Hole (Beichman+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/PASJ/53/445">J/PASJ/53/445 : ASCA Deep survey in Lockman Hole Field (Ishisaki+, 2001)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/444/79</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/444/79</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/444/79</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/444/79</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/444/79</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/444/79</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><capability xsi:type="cs:ConeSearch" standardID="ivo://ivoa.net/std/ConeSearch"><description>Cone search capability for table J/A+A/444/79/table8 (X-ray catalogue)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/444/79/table8?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/444/79/table8?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/444/79/table8?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>163.25775</ra><dec>57.2501917</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/6069 6090 6112</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/444/79?format=ascii</footprint><waveband>X-ray</waveband></coverage><tableset><schema><name>default</name><table><name>J/A+A/444/79/table8</name><description>X-ray catalogue</description><column><name>n_Class</name><description>[* ] **: BAL QSO</description><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>z</name><description>? Redshift</description><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></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>[MBC2005]</name><description>Source sequential number</description><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>RDS</name><description>? X-ray source ROSAT number (RDS NNN)</description><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>RDSO</name><description>Optical Source ROSAT number (RDS NNNA)</description><dataType xsi:type="vs:VOTableType" arraysize="4*">char</dataType></column><column><name>RAJ2000</name><description>Right ascension (J2000.0) (1)</description><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Declination (J2000.0) (1)</description><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Class</name><description>Source classification from optical spectroscopy</description><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>Model</name><description>Best fit spectral model (2)</description><dataType xsi:type="vs:VOTableType" arraysize="6*">char</dataType></column><column><name>Gamma</name><description>Power law spectral slope</description><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Gamma</name><description>Power law spectral slope low error bar</description><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E_Gamma</name><description>Power law spectral slope high error bar</description><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>log(Abs)</name><description>? Logarithm of the column density of excess absorption (3)</description><unit>log(cm**-2)</unit><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_log(Abs)</name><description>? Low error bar of column density of excess absorption</description><unit>log(cm**-2)</unit><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>E_log(Abs)</name><description>? High error bar of column density of excess absorption</description><unit>log(cm**-2)</unit><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>F(0.5-2)keV</name><description>Flux in the [0.5-2]keV band</description><unit>1e-17W.m**-2</unit><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F(2-10)keV</name><description>Flux in the [2-10]keV band</description><unit>1e-17W.m**-2</unit><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>L(0.5-2)keV</name><description>? Logarithm of luminosity in the [0.5-2]keV rest-frame band (4)</description><unit>log(1e-07W)</unit><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>L(2-10)keV</name><description>? Logarithm of the luminosity in the [2-10]keV rest-frame band</description><unit>log(1e-07W)</unit><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table></schema></tableset></ri:Resource>