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<ri:Resource created="2011-12-13T07:49:45Z" 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>Seyfert galaxies in the mid-IR</title><shortName>J/ApJ/705/14</shortName><identifier>ivo://CDS.VizieR/J/ApJ/705/14</identifier><altIdentifier>doi:10.26093/cds/vizier.17050014</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Deo R.P.</name></creator><creator><name>Richards G.T.</name></creator><creator><name>Crenshaw D.M.</name></creator><creator><name>Kraemer S.B.</name></creator><date role="Updated">2017-07-04T07:08:49Z</date><date role="Created">2011-12-13T07:49:45Z</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>seyfert-galaxies</subject><subject>infrared-astronomy</subject><subject>spectroscopy</subject><description>An analysis of archival mid-infrared (mid-IR) spectra of Seyfert galaxies from the Spitzer Space Telescope observations is presented. We characterize the nature of the mid-IR active nuclear continuum by subtracting a template starburst spectrum from the Seyfert spectra. The long wavelength part of the spectrum contains a strong contribution from the starburst-heated cool dust; this is used to effectively separate starburst-dominated Seyferts from those dominated by the active nuclear continuum. Within the latter category, the strength of the active nuclear continuum drops rapidly beyond ~20um. On average, type 2 Seyferts have weaker short-wavelength active nuclear continua as compared to type 1 Seyferts. Type 2 Seyferts can be divided into two types, those with strong polycyclic aromatic hydrocarbon (PAH) bands and those without.</description><source format="bibcode">2009ApJ...705...14D</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/705/14</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/248">VII/248 : Quasars and Active Galactic Nuclei (12th Ed.) (Veron+ 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/173">VII/173 : Catalogue of Seyfert Galaxies (Lipovetsky+, 1988)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/473/369">J/A+A/473/369 : VISIR/VLT mid-infrared imaging of Seyfert nuclei (Haas+,</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/418/465">J/A+A/418/465 : Mid-infrared and hard X-ray emission in AGN (Lutz+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/125/349">J/ApJS/125/349 : Morphology of 12micron Seyfert Galaxies (Hunt+, 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/other/PBeiO/18.7">J/other/PBeiO/18.7 : Far infrared Seyfert galaxies (Liu 1991)</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/ApJ/705/14</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/705/14</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/705/14</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/705/14</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/705/14</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/705/14</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/ApJ/705/14/catalog (Seyfert galaxies studied: optical and mid-IR properties)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/705/14/catalog?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/705/14/catalog?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/705/14/catalog?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>146.0685833</ra><dec>9.771</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/909 941 2251 2564 4352 4439 4488 4992 5284 5795 5975 6458 6977 7132 7214 7424 7522 7642 7713 7869 7921 8492 8675 8845 8922 9231 9632 9882 10364 10404 10501 10817 10912 10927 11029 11416 11490 12306 17061 17183 17525 17529 17748 18246 18783 18794 18919 19283 19296 19619 19883 20230 21016 22638 22654 23171 23233 24896 25054 25083 25135 25518 25610 25790 25907 26148 26932 27191 27767 27914 27945 28517 28574 28593 28609 31259 32931 33034 34294 34531 34534 35447 35623 36618 36668 36716 36733 36861 40221 40410 43677 43748 43806 43877 43925 44507 45779 45816 45883 46399 46442 46481 46615 46811 46987 47047 47415</spatial><spectral>6.6214843819315255e-21 3.6117180714086103e-20</spectral><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/705/14?format=ascii</footprint><waveband>Infrared</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/705/14/table3</name><description>Starburst-to-AGN flux density ratios</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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