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<ri:Resource created="2011-01-21T09:38:01Z" 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>Nuclear activity in ULIRGs</title><shortName>J/MNRAS/405/2505</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/405/2505</identifier><altIdentifier>doi:10.26093/cds/vizier.74052505</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Nardini E.</name></creator><creator><name>Risaliti G.</name></creator><creator><name>Watabe Y.</name></creator><creator><name>Salvati M.</name></creator><creator><name>Sani E.</name></creator><date role="Updated">2024-07-11T20:16:52Z</date><date role="Created">2011-01-21T09:38:01Z</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>galaxies</subject><subject>infrared-sources</subject><description>We present the results of a 5-8um spectral analysis performed on the largest sample of local ultraluminous infrared galaxies (ULIRGs) selected so far, consisting of 164 objects up to a redshift of ~0.35. The unprecedented sensitivity of the Infrared Spectrograph onboard Spitzer allowed us to develop an effective diagnostic method to quantify the active galactic nucleus (AGN) and starburst (SB) contribution to this class of objects. The large AGN over SB brightness ratio at 5-8um and the sharp difference between the spectral properties of AGN and SB galaxies in this wavelength range make it possible to detect even faint or obscured nuclear activity, and disentangle its emission from that of star formation. By defining a simple model we are also able to estimate the intrinsic bolometric corrections for both the AGN and SB components, and obtain the relative AGN/SB contribution to the total luminosity of each source.</description><source format="bibcode">2010MNRAS.405.2505N</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/405/2505</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/AJ/121/97">J/AJ/121/97 : K-band spectroscopy of ULIRGs (Murphy+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/409/115">J/A+A/409/115 : VLA imaging of IRAS 1 Jy ULIRG sample (Nagar+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/131/1942">J/AJ/131/1942 : 2MASS observations of IRAS 1Jy ULIRGs (Chen+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/640/167">J/ApJ/640/167 : AGNs and ULIRGs in the CDF-South (Alonso-Herrero+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/467/565">J/A+A/467/565 : z=1-3 ULIRGs from the Spitzer SWIRE survey (Berta+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/658/778">J/ApJ/658/778 : Spitzer mid-IR spectroscopy of z~2 ULIRGs (Yan+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/375/115">J/MNRAS/375/115 : ULIRGs galaxies in SDSS, 2dF and 6dF (Hwang+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/674/172">J/ApJ/674/172 : Oxygen abundances of LIRGs and ULIRGs (Rupke+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/182/628">J/ApJS/182/628 : Spitzer quasar and ULIRG evolution study (Veilleux+, 2009)</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/MNRAS/405/2505</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/405/2505</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/405/2505</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/405/2505</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/405/2505</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South 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