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<ri:Resource created="2007-11-25T14:51:22Z" 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>VISIR/VLT mid-infrared imaging of Seyfert nuclei</title><shortName>J/A+A/473/369</shortName><identifier>ivo://CDS.VizieR/J/A+A/473/369</identifier><altIdentifier>doi:10.26093/cds/vizier.34730369</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Haas M.</name></creator><creator><name>Siebenmorgen R.</name></creator><creator><name>Pantin E.</name></creator><creator><name>Horst H.</name></creator><creator><name>Smette A.</name></creator><creator><name>Kaufl H.-U.,Lagage P.-O.</name></creator><creator><name>Chini R.</name></creator><date role="Updated">2017-10-02T19:28:25Z</date><date role="Created">2007-11-25T14:51:22Z</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>seyfert-galaxies</subject><subject>galaxies</subject><subject>infrared-sources</subject><description>Half of the Seyfert-2 galaxies escaped detection of broad lines in their polarised spectra observed so far. Some authors have suspected that these non-HBLRs contain real Sy2 nuclei without intrinsic broad line region hidden behind a dust torus. If this were true, then their nuclear structure would fundamentally differ from that of Sy2s with polarised broad lines: in particular, they would not be explained by orientation-based AGN unification. Further arguments for two physically different Sy2 populations have been derived from the warm and cool IRAS F25/F60 ratios. These ratios, however, refer to the entire host galaxies and are unsuitable to conclusively establish the absence of a nuclear dust torus. Instead, a study of the Seyfert-2 dichotomy should be performed on the basis of nuclear properties only. Here we present the first comparison between [OIII] {lambda} 5007{AA} and mid-infrared imaging at matching spatial resolution. The aim is to check whether the nuclear dust emission scales with AGN luminosity as traced by [OIII].</description><source format="bibcode">2007A&amp;A...473..369H</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/473/369</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/VIII/65">VIII/65 : 1.4GHz NRAO VLA Sky Survey (NVSS) (Condon+ 1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VIII/71">VIII/71 : The FIRST Survey Catalog, Version 03Apr11 (Becker+ 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/156">II/156 : IRAS Faint Source Catalog |b|&gt;10, Version 2.0 (Moshir+ 1989)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/126/1607">J/AJ/126/1607 : IRAS Revised Bright Galaxy Sample (Sanders+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/98/477">J/ApJS/98/477 : Optical spectral atlas of Seyfert nuclei (Ho+ 1995)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/112/315">J/ApJS/112/315 : Spectroscopic parameters of Seyfert nuclei (Ho+ 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/141/23">J/ApJS/141/23 : JHK' imaging photometry of Seyfert 1. I. (Enya+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/141/31">J/ApJS/141/31 : JHK' imaging photometry of Seyfert 1. II. (Enya+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/366/480">J/MNRAS/366/480 : Emission-line properties of Seyfert 2 nuclei (Gu+, 2006)</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/473/369</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/473/369</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/473/369</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/473/369</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/473/369</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/473/369</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/473/369/table3 (Source parameters)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/473/369/table3?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/473/369/table3?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/473/369/table3?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>201.3650633</ra><dec>-43.0191125</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/941 2248 2251 2564 4369 4439 4447 4488 5564 5975 6977 7132 7214 7606 7642 7713 7869 8261 8299 8492 8845 8922 9449 9882 10364 10454 10475 10560 10912 10927 11027 11029 11490 11886 11898 12306 12380 17529 17727 17754 17850 18246 18794 18897 19070 19283 19296 19619 19883 20014 20230 21016 21450 22632 22654 23171 23233 23323 24896 25518 25610 25890 25907 26071 26148 26393 26561 27191 27464 27721 27767 27945 28517 28593 29795 33325 34531 34534 35447 36299 36668 36716 36786 38268 38704 40221 40410 41586 43262 43339 43677 43806 43925 44507 45883 46399 46615 46811 46987 47047 47169 49042</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/473/369?format=ascii</footprint><waveband>Infrared</waveband></coverage><tableset><schema><name>default</name><table><name>J/A+A/473/369/table3</name><description>Source parameters</description><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>Name</name><description>Source name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="14*">char</dataType></column><column><name>Dist</name><description>Distance (1)</description><unit>Mpc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>SType</name><description>Seyfert type</description><ucd>src.class</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>HBLR</name><description>Hidden broad line region flag (2)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="4*">char</dataType></column><column><name>l_F12umn</name><description>Limit flag for 3-sigma upper limit in case of non-detection</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>F12umn</name><description>Nuclear flux ay 12um</description><unit>mJy</unit><ucd>phot.flux.density;em.IR.8-15um</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>r_F12umn</name><description>[1/13] References for nuclear 12um flux</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>l_F12um</name><description>Limit flag on F12um</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>F12um</name><description>Total flux density at 12um (3)</description><unit>Jy</unit><ucd>phot.flux.density;em.IR.8-15um</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>l_F25um</name><description>Limit flag on F25um</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>F25um</name><description>Total flux density at 25um (3)</description><unit>Jy</unit><ucd>phot.flux.density;em.IR.15-30um</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F60um</name><description>Total flux density at 60um (3)</description><unit>Jy</unit><ucd>phot.flux.density;em.IR.30-60um</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>l_F100um</name><description>Limit flag on F100um</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>F100um</name><description>Total flux density at 100um (3)</description><unit>Jy</unit><ucd>phot.flux.density;em.IR.60-100um</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>[OIII]</name><description>Line flux at [OIII]</description><unit>1e-19W.m**-2</unit><ucd>phot.flux;em.line.Hbeta</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Hbeta</name><description>? 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