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<ri:Resource created="2025-04-28T13:14:34Z" status="active" updated="2026-07-02T11:58:48Z" 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>X-ray to FIR observations for an AGN sample</title><shortName>J/ApJ/941/46</shortName><identifier>ivo://CDS.VizieR/J/ApJ/941/46</identifier><altIdentifier>doi:10.26093/cds/vizier/ba-xd-1e</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Spinoglio L.</name></creator><creator><name>Fernandez-Ontiveros J.A.</name></creator><creator><name>Malkan M.A.</name></creator><date role="Updated">2026-07-02T11:58:48Z</date><date role="Created">2025-04-28T13:14:34Z</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>redshifted</subject><subject>visible-astronomy</subject><subject>x-ray-sources</subject><subject>infrared-astronomy</subject><subject>spectroscopy</subject><subject>black-holes</subject><description>The high-ionization mid-IR lines, excited in the narrow-line regions of active galactic nuclei (AGN), barely affected by stellar excitation and dust extinction, trace the AGN bolometric power. We used the complete 12um sample of Seyfert galaxies, for which 100/116 objects have reliable 2-10keV observations. The [NeV] and [OIV] mid-IR lines linearly correlate with several AGN bolometric indicators (intrinsic 2-10keV and observed 14-195keV X-ray emission, compact nuclear 12um emission, [OIII]{lambda}5007{AA} line emission) in terms of both flux and luminosity. No evidence of systematic differences in these correlations is found among the Seyfert populations, including types 1 and 2 and Compton-thick and Compton-thin AGN. Nevertheless, we find that a sequence of high-to-low Eddington ratios together with strong- to-weak line excitation (traced by the [OIV]/[NeII] line ratio) encompasses from type 1 through type 2 AGN to low-ionization nuclear emission-line region galaxies, showing intrinsic differences in these three AGN populations. A positive correlation between the black hole accretion rate (BHAR) and the star formation rate (SFR) is found, but no correlation between the specific SFR and the ratio BHAR/M_BH_, simply reflecting the fact that the more massive a galaxy is, the more it is forming stars and feeding its central black hole. The JWST, just beginning operations, will allow large samples of AGN to be observed in these lines in the nearby universe (z&lt;0.9).</description><source format="bibcode">2022ApJ...941...46S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/941/46</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/157">VII/157 : The Extended 12um galaxy sample (Rush+ 1993)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/453/616">J/ApJ/453/616 : JHKL photometry of 12 micron galaxy sample (Spinoglio+ 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/121/473">J/ApJS/121/473 : A diagnostic diagram for Seyfert 2 Galaxies (Bassani+, 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/161/185">J/ApJS/161/185 : GIS catalog project : source catalog II (Ueda+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/648/111">J/ApJ/648/111 : Chandra sources near AGNs (Levenson+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/679/140">J/ApJ/679/140 : IR measurement of quasar obscuration (Treister+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/524/A64">J/A+A/524/A64 : The 54-month Palermo BAT-survey catalogue (Cusumano+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/709/1257">J/ApJ/709/1257 : Spitzer-IRS sp. of Seyfert galaxies. 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Nuclear Flux at 12um (5)</description><unit>mJy</unit><ucd>phot.flux;em.IR.8-15um</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>F(K)GAL</name><description>Galaxy K band flux density</description><unit>Jy</unit><ucd>phot.mag;em.IR.K</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>F(K)TOT</name><description>Total K band flux density</description><unit>Jy</unit><ucd>phot.mag;em.IR.K</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>F(K)NUC</name><description>Nuclear K band flux density</description><unit>Jy</unit><ucd>phot.mag;em.IR.K</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>logMgal</name><description>[8.5/11.3]? Log of galaxy mass in solar units</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>r_logMgal</name><description>Reference for logMgal (1)</description><ucd>meta.ref;phys.mass</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>logLBol(IR)</name><description>[41.28/46]? Log of bolometric luminosity (2)</description><unit>log(1e-07W)</unit><ucd>phys.luminosity;phot.flux.bol;em.IR</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>logMBH</name><description>[5.8/9]? 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Log of intrinsic 2-10keV X-ray luminosity</description><unit>log(1e-07W)</unit><ucd>phys.luminosity;em.X-ray.medium</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>logL14-195keV</name><description>[38.6/46.4]? Log of observed 14-195keV X-ray luminosity in erg/s</description><unit>log(1e-07W)</unit><ucd>phys.luminosity;em.X-ray.hard</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>logLBol(X)</name><description>[41.17/46.21]? Log of bolometric luminosity (from 2-10keV)</description><unit>log(1e-07W)</unit><ucd>phys.luminosity;phot.flux.bol;em.X-ray.medium</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Ref</name><description>References and notes (2)</description><ucd>meta.ref</ucd><dataType xsi:type="vs:VOTableType" arraysize="9*">char</dataType></column><column><name>l_F[NeII]</name><description>Limit flag for F[NeII]</description><ucd>meta.code.error;phot.flux;em.IR.8-15um</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>F[NeII]</name><description>[0.2/520]? Flux of [NeII]12.8um (1)</description><unit>1e-17W.m**-2</unit><ucd>phot.flux;em.line;em.IR.8-15um</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>l_F[NeV]1</name><description>Limit flag for F[NeV]1</description><ucd>meta.code.error;phot.flux;em.IR.8-15um</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>F[NeV]1</name><description>[0.38/1110]? Flux of [NeV]14.3um (1)</description><unit>1e-17W.m**-2</unit><ucd>phot.flux;em.line;em.IR.8-15um</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>F[NeIII]</name><description>[0.6/2100]? Flux of [NeIII]15.5um (1)</description><unit>1e-17W.m**-2</unit><ucd>phot.flux;em.line;em.IR.15-30um</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>l_F[NeV]2</name><description>Limit flag for F[NeV]2</description><ucd>meta.code.error;phot.flux;em.IR.15-30um</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>F[NeV]2</name><description>[0/800]? Flux of [NeV] 24.3um (1)</description><unit>1e-17W.m**-2</unit><ucd>phot.flux;em.line;em.IR.15-30um</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>l_F[OIV]</name><description>Limit flag for F[OIV]</description><ucd>meta.code.error;phot.flux;em.IR.15-30um</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>F[OIV]</name><description>[0.6/2200]? Flux of [OIV]25.9um (1)</description><unit>1e-17W.m**-2</unit><ucd>phot.flux;em.line;em.IR.15-30um</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>l_F(PAH11.3)</name><description>Limit flag for F(PAH11.3)</description><ucd>meta.code.error;phot.flux;em.IR.8-15um</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>F(PAH11.3)</name><description>[4.5/1200]? Flux of PAH11.3um (2)</description><unit>1e-17W.m**-2</unit><ucd>phot.flux;em.line;em.IR.8-15um</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>F[CII]</name><description>[1.6/1361]? Flux of [CII]158um (3)</description><unit>1e-17W.m**-2</unit><ucd>phot.flux;em.line;em.mm.1500-3000GHz</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table><table><name>J/ApJ/941/46/table3</name><description>Observed and absorption corrected 2-10keV fluxes and luminosities for Compton thick objects</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>Seq</name><description>[9/116] Sequential catalog number</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Name</name><description>Galaxy name used in other tables</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="15*">char</dataType></column><column><name>OType</name><description>AGN classification</description><ucd>meta.code.class;src.class</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column><column><name>l_logNH</name><description>Limit flag on logNH</description><ucd>meta.code.error;phys.columnDensity</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>logNH</name><description>[23.55/25.1] Log of the Hydrogen intrinsic absorption column density</description><unit>log(cm**-2)</unit><ucd>phys.columnDensity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>FX(OBS)</name><description>[0.08/4.9] Observed 2-10keV flux in 10^-12^erg/s/cm^2^</description><unit>1e-15W.m**-2</unit><ucd>phot.flux;em.X-ray.medium</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>FX(COR)</name><description>[4.6/120] Absorption corrected 2-10keV flux, 10^-12^erg/s/cm^2^</description><unit>1e-15W.m**-2</unit><ucd>phot.flux;em.X-ray.medium;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logLX(OBS)</name><description>[39.28/42.07] Log of the observed 2-10keV luminosity, erg/s</description><unit>log(1e-07W)</unit><ucd>phys.luminosity;em.X-ray.medium</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logLX(COR)</name><description>[40.2/43.69] Log of the absorption corrected 2-10keV luminosity, erg/s</description><unit>log(1e-07W)</unit><ucd>phys.luminosity;em.X-ray.medium;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Ref</name><description>References (1)</description><ucd>meta.ref</ucd><dataType xsi:type="vs:VOTableType" arraysize="4*">char</dataType></column></table></schema></tableset></ri:Resource>