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<ri:Resource created="2008-02-09T15:22:59Z" 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>SEXSI catalog</title><shortName>J/ApJ/596/944</shortName><identifier>ivo://CDS.VizieR/J/ApJ/596/944</identifier><altIdentifier>doi:10.26093/cds/vizier.15960944</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Harrison F.A.</name></creator><creator><name>Eckart M.E.</name></creator><creator><name>Mao P.H.</name></creator><creator><name>Helfand D.J.</name></creator><creator><name>Stern D.</name></creator><date role="Updated">2008-02-09T14:23:52Z</date><date role="Created">2008-02-09T15:22:59Z</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>surveys</subject><subject>x-ray-sources</subject><description>The Serendipitous Extragalactic X-Ray Source Identification (SEXSI) program is designed to extend greatly the sample of identified extragalactic hard X-ray (2-10keV) sources at intermediate fluxes (~10^-13^ to 10^-15^erg/cm^2^/s). SEXSI, which studies sources selected from more than 2deg^2^, provides an essential complement to the Chandra Deep Fields, which reach depths of 5x10^-16^erg/cm^2^/s (2-10keV) but over a total area of less than 0.2deg^2^. In this paper we describe the characteristics of the survey and our X-ray data analysis methodology. We present the cumulative flux distribution for the X-ray sample of 1034 hard sources and discuss the distribution of spectral hardness ratios. Our logN-logS in this intermediate flux range connects to those found in the Deep Fields, and by combining the data sets, we constrain the hard X-ray population over the flux range in which the differential number counts change slope and from which the bulk of the 2-10keV X-ray background arises. We further investigate the logN-logS distribution separately for soft and hard sources in our sample, finding that while a clear change in slope is seen for the softer sample, the hardest sources are well described by a single power law down to the faintest fluxes, consistent with the notion that they lie at lower average redshift.</description><source format="bibcode">2003ApJ...596..944H</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/596/944</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/chandra">B/chandra : The Chandra Archive Log (CXC, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/122/2810">J/AJ/122/2810 : Chandra Deep Field North Survey. 1Ms catalog (Brandt+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/126/539">J/AJ/126/539 : Chandra Deep Fields North &amp; South. 2Ms Cat. (Alexander+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/139/369">J/ApJS/139/369 : Chandra Deep Field South. 1Ms catalog (Giacconi+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/156/35">J/ApJS/156/35 : SEXSI catalog. II (Eckart+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/165/19">J/ApJS/165/19 : SEXSI catalog. 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