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<ri:Resource created="2014-08-13T14:16:46Z" 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>SEDs of type I AGN in COSMOS. I. XMM-COSMOS</title><shortName>J/ApJ/759/6</shortName><identifier>ivo://CDS.VizieR/J/ApJ/759/6</identifier><altIdentifier>doi:10.26093/cds/vizier.17590006</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Elvis M.</name></creator><creator><name>Hao H.</name></creator><creator><name>Civano F.</name></creator><creator><name>Brusa M.</name></creator><creator><name>Salvato M.</name></creator><creator><name>Bongiorno A.</name></creator><creator><name>Capak P.,Zamorani G.</name></creator><creator><name>Comastri A.</name></creator><creator><name>Jahnke K.</name></creator><creator><name>Lusso E.</name></creator><creator><name>Mainieri V.</name></creator><creator><name>Trump J.R.,Ho L.C.</name></creator><creator><name>Aussel H.</name></creator><creator><name>Cappelluti N.</name></creator><creator><name>Cisternas M.</name></creator><creator><name>Frayer D.</name></creator><creator><name>Gilli R.,Hasinger G.</name></creator><creator><name>Huchra J.P.</name></creator><creator><name>Impey C.D.</name></creator><creator><name>Koekemoer A.M.</name></creator><creator><name>Lanzuisi G.,Le Floc'h E.</name></creator><creator><name>Lilly S.J.</name></creator><creator><name>Liu Y.</name></creator><creator><name>McCarthy P.</name></creator><creator><name>McCracken H.J.</name></creator><creator><name>Merloni A.,Roeser H.-J.</name></creator><creator><name>Sanders D.B.</name></creator><creator><name>Sargent M.</name></creator><creator><name>Scoville N.</name></creator><creator><name>Schinnerer E.,Schiminovich D.</name></creator><creator><name>Silverman J.</name></creator><creator><name>Taniguchi Y.</name></creator><creator><name>Vignali C.</name></creator><creator><name>Urry C.M.,Zamojski M.A.</name></creator><creator><name>Zatloukal M.</name></creator><date role="Updated">2017-09-19T14:21:12Z</date><date role="Created">2014-08-13T14:16:46Z</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>active-galactic-nuclei</subject><subject>spectral-energy-distribution</subject><subject>x-ray-sources</subject><subject>ultraviolet-photometry</subject><subject>infrared-photometry</subject><subject>visible-astronomy</subject><subject>broad-band-photometry</subject><subject>radio-sources</subject><subject>surveys</subject><description>The "Cosmic Evolution Survey" (COSMOS) enables the study of the spectral energy distributions (SEDs) of active galactic nuclei (AGNs) because of the deep coverage and rich sampling of frequencies from X-ray to radio. Here we present an SED catalog of 413 X-ray (XMM-Newton)-selected type 1 (emission line FWHM&gt;2000km/s) AGNs with Magellan, SDSS, or VLT spectrum. The SEDs are corrected for Galactic extinction, broad emission line contributions, constrained variability, and host galaxy contribution. We present the mean SED and the dispersion SEDs after the above corrections in the rest-frame 1.4GHz to 40keV, and show examples of the variety of SEDs encountered. In the near-infrared to optical (rest frame ~8{mu}m-4000{AA}), the photometry is complete for the whole sample and the mean SED is derived from detections only. Reddening and host galaxy contamination could account for a large fraction of the observed SED variety.</description><source format="bibcode">2012ApJ...759....6E</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/759/6</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/VII/260">VII/260 : The SDSS-DR7 quasar catalog (Schneider+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/284">II/284 : COSMOS Multi-Wavelength Photometry Catalog (Capak+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/206/4">J/ApJS/206/4 : SEDs for luminous QSOs (Krawczyk+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/201/30">J/ApJS/201/30 : The Chandra COSMOS survey. 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