J/ApJ/964/117ivo://CDS.VizieR/J/ApJ/964/117CDSSpinoglio L.Fernandez-Ontiveros J.A.Malkan M.A.2026-08-07T07:52:08Z2026-08-07T08:12:18ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.frspectral-energy-distributionactive-galactic-nucleiseyfert-galaxiesinfrared-photometryultraviolet-astronomyx-ray-sourcesredshiftedradio-sourcesWe measure the bolometric luminosity of a complete and unbiased 12{mu}m-selected sample of active galactic nuclei (AGN) in the local Universe. For each galaxy, we used a 10-band radio-to-X-ray spectral energy distribution (SED) to isolate the genuine AGN continuum in each band, including subarcsecond measurements where available, and correcting those contaminated by the host galaxy. We derive the median SED of Seyfert type 1 AGN, Seyferts with hidden broad lines (HBLs), Seyferts of type 2, and LINER nuclei in our sample. The median Seyfert 1 SED shows the characteristic blue bump feature in the UV, but nevertheless, the largest contribution to the bolometric luminosity comes from the IR and X-ray continua. The median SEDs of both HBL and type 2 AGN are affected by starlight contamination in the optical/UV. The median SED of HBL AGN is consistent with that of Seyfert 1s, when an extinction of AV~1.2mag is applied. The comprehensive SEDs allowed us to measure accurate bolometric luminosities and derive robust bolometric corrections for the different tracers. The 12{mu}m and K-band nuclear luminosities have good linear correlations with the bolometric luminosity, similar to those in the X-rays. We derive bolometric corrections for either continuum bands (K band, 12{mu}m, 2-10keV, and 14-195keV) or narrow emission lines (mid-IR high-ionization lines of [OIV] and [NeV] and optical [OIII]5007{AA}) as well as for combinations of IR continuum and line emission. A combination of continuum plus line emission accurately predicts the bolometric luminosity up to quasar luminosities (~10^46^erg/s).2024ApJ...964..117Shttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/964/117CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toII/156 : IRAS Faint Source Catalog, |b| > 10, Version 2.0 (Moshir+ 1989)VII/178 : Optical Extragalactic Emission-line Objects (Hewitt+ 1991)VII/157 : The Extended 12um galaxy sample (Rush+ 1993)II/335 : Revised cat. of GALEX UV sources (GUVcat_AIS GR6+7) (Bianchi+ 2017)J/ApJ/269/352 : Quasar evolution (Schmidt+, 1983)J/ApJS/95/1 : Atlas of Quasar Energy Distributions (Elvis+ 1994)J/ApJ/453/616 : JHKL photometry of 12 micron galaxy sample (Spinoglio+ 1995)J/ApJS/121/473 : A diagnostic diagram for Seyfert 2 Galaxies (Bassani+, 1999)J/A+A/418/465 : Mid-infrared and hard X-ray emission in AGN (Lutz+, 2004)J/ApJS/166/470 : SDSS-Spitzer type I QSOs IR photometry (Richards+, 2006)J/A+A/487/119 : AGN in XMM-Newton Hard Bright Survey (Della Ceca+, 2008)J/A+A/524/A64 : The 54-month Palermo BAT-survey catalogue (Cusumano+, 2010)J/ApJ/709/1257 : Spitzer-IRS sp. of Seyfert galaxies. II. (Tommasin+, 2010)J/ApJ/713/L11 : X-ray properties of Seyfert 1 galaxies (Zhou+, 2010)J/MNRAS/413/1206 : XMM survey of 12um selected galaxies (Brightman+, 2011)J/ApJS/206/4 : SED and bol. corrections for luminous QSOs (Krawczyk+, 2013)J/MNRAS/439/1648 : Subarcsecond mid-infrared atlas of local AGN (Asmus+, 2014)J/A+A/588/A70 : Hard X-ray view of the soft excess in AGN (Boissay+, 2016)J/MNRAS/459/1602 : AGN sample in the northern XMM-XXL field (Liu+, 2016)J/ApJS/233/17 : Swift/BAT AGN sp. survey. V. X-ray data (Ricci+, 2017)J/ApJS/235/4 : 105-month Swift-BAT all-sky hard X-ray survey (Oh+, 2018)J/MNRAS/489/5046 : GALEX absolute calibration based on WDs (Wall+, 2019)J/ApJ/884/136 : PAH features of star-forming gal. using Spitzer (Xie+, 2019)J/ApJ/900/124 : Galaxies within 150Mpc observed with Chandra (Bi+, 2020)J/MNRAS/504/5726 : IR lines of AGNs accretion disk (Fernandez-Ontiveros+, 2021)J/ApJ/941/46 : X-ray to FIR obs. for an AGN sample (Spinoglio+, 2022)J/A+A/671/A34 : The WISSH quasars project. XI. (Saccheo+, 2023)J/ApJS/265/37 : Multiwavelength SED analysis of GOALS ULIRGs (Yamada+, 2023)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/964/117https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/964/117http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/964/117https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/964/117https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/964/117http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/964/117GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/ApJ/964/117/sample (AGN (Table 1), radio to NIR (Table 2) and UV to X-rays nuclear photometry and derived bolometric fluxes and luminosities (Table 3))https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/964/117/sample?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/964/117/sample?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/964/117/sample?GETtext/xml+votable180.050000true1.5812520.2027780.0055555555555555566/909 941 2251 2309 2564 4439 4488 5116 5284 5975 6977 7214 7424 7552 7606 7642 7713 7777 7921 8492 8673 8845 8922 9882 10265 10364 10404 10475 10817 10912 10927 11027 11029 11101 11206 11490 12306 16740 17061 17183 17529 17748 17754 18683 18783 18794 19070 19283 19619 19730 19883 20489 21016 22632 22638 22654 23171 23233 23323 24896 25054 25083 25135 25518 25610 25790 25907 26148 26292 26932 27191 27767 27914 27945 28517 28609 31259 32930-32931 33034 33325 33958 34099 34294 34531 34534 35447 35623 35993 36299 36457 36618 36668 36716 36861 40410 43748 43806 43877 43925 44448 44507 45587 45779 45816 45883 46399 46442 46481 46615 46811 46987 47047 47169 47415 490425.5658981862942334e-24 1.4134638842407062e-18https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/964/117?format=asciiX-rayUVInfraredRadiodefaultJ/ApJ/964/117/sampleAGN (Table 1), radio to NIR (Table 2) and UV to X-rays nuclear photometry and derived bolometric fluxes and luminosities (Table 3)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintONameOther name(s)meta.idcharRLRadio-loud nucleus indicated with "RL" (10 occurrences) (1)meta.notecharl_F8.4Limit flag on F8.4meta.code.errorcharF8.4[0.2/41725]? VLA 8.4GHz nuclear flux density (Thean+ 2000MNRAS.314..573T)mJyphot.flux.density;em.radio.6-12GHzfloatnullablel_F12VLTLimit flag on F12VLTmeta.code.errorcharF12VLT[3.7/10206]? VLT-VISIR 12um subarcsecond nuclear flux density (2)mJyphot.flux.density;em.IR.8-15umfloatnullablef_F12VLTFlag on F12VLT (2)meta.codecharA14Display data from Asmus+ 2014, J/MNRAS/439/1648 within 15"meta.ref.urlintnullableF12IRS[24.6/2042]? Spitzer-IRS 12 micron continuum flux density (3)mJyphot.flux.density;em.IR.8-15umfloatnullablel_R12Limit flag on R12meta.code.errorcharR12[0.8/26.8]? Ratio between F12IRS and F12VLTphot.flux;arith.ratio;em.IR.8-15umfloatnullableF7[8.7/929]? Spitzer-IRS 7 micron continuum flux density (4)mJyphot.flux.density;em.IR.4-8um;spect.continuumfloatnullableF5.8[6/494]? Spitzer-IRAC 5.8 micron flux density corrected for R12mJyphot.flux.density;em.IR.4-8umfloatnullableF4.5[5/384]? Spitzer-IRAC 4.5 micron flux density corrected for R12mJyphot.flux.density;em.IR.4-8umfloatnullableFK[0.27/196]? 2.2 micron nuclear flux density derived from Keck/2MASS observations (Spinoglio+ 2022, J/ApJ/941/46)mJyphot.flux.density;em.IR.K;obsfloatnullablel_FNUVLimit flag on FNUVmeta.code.errorcharFNUV[0.003/17.4]? Near-ultraviolet flux (NUV) density (5)mJyphot.flux.density;em.UV.200-300nmfloatnullablel_FFUVLimit flag on FFUVmeta.code.errorcharFFUV[0.01/11.3]? Far-ultraviolet flux (FUV) density (5)mJyphot.flux.density;em.UV.100-200nmfloatnullableF2-10[0.01/210]? 2-10keV absorption corrected x-ray flux; 10^-12^erg/s/cm^2^1e-15W.m**-2phot.flux;em.X-ray.mediumfloatnullabler_F2-10[1/31]? Reference for F2-10 (7)meta.ref;phot.flux;em.X-ray.mediumintnullableF14-195[4/619]? 14-195keV observed x-ray flux; 10^-12^erg/s/cm^2^1e-15W.m**-2phot.flux;em.X-ray.hardfloatnullabler_F14-195[32/34]? Reference for F14-195 (7)meta.ref;phot.flux;em.X-ray.hardintnullablel_FbolLimit flag on Fbolmeta.code.errorcharFbol[0.16/8995]? Computed bolometric flux (see text); 10^-12^erg/s/cm^2^1e-15W.m**-2phot.flux.bolfloatnullablef_FbolFlag on Fbol (8)meta.codecharl_logLbolLimit flag on logLbolmeta.code.errorcharlogLbol[40/47.7]? Log of bolometric luminosity; erg/slog(1e-07W)phys.luminosity;phot.flux.bolfloatnullableGamma1[1/5.7]? Photon index of 2-10keV observations (6)spect.index;em.X-ray.mediumfloatnullableB11Display data from Brightman+ 2011, J/MNRAS/413/1206 within 30"meta.ref.urlintnullableGamma2[1.6/2.5]? Photon index of 14-195keV observations from Oh+ 2018, J/ApJS/235/4spect.index;em.X-ray.hardfloatnullableR17Display data from Ricci+ 2017, J/ApJS/233/17 within 5"meta.ref.urlintnullableSimbadNameSimbad column added by the CDSmeta.idcharnullableNEDNED column added by the CDSmeta.ref.urlcharNameGalaxy name as in Spinoglio+ (2022, J/ApJ/941/46)meta.id;meta.maincharRAJ2000Right ascension in hours (J2000)pos.eq.ra;meta.mainDEJ2000Declination in degrees (J2000)pos.eq.dec;meta.mainz[-0.00013/0.2] Spectroscopic redshiftsrc.redshiftdoubleTypeAGN type (G1)src.classcharCTCompton thick nucleus indicated with "CT" (15 occurrences)meta.codechar