J/A+A/583/A120ivo://CDS.VizieR/J/A+A/583/A120doi:10.26093/cds/vizier.35830120CDSSiebenmorgen R.Heymann F.Efstathiou A.2015-11-03T07:29:30Z2015-11-03T08:06:36ZCDS support team

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

cds-question@unistra.frastronomical-modelsactive-galactic-nucleispectral-energy-distributionWe assume that dust near active galactic nuclei (AGNs) is distributed in a torus-like geometry, which can be described as a clumpy medium or a homogeneous disk, or as a combination of the two (i.e. a two-phase medium). The dust particles considered are fluffy and have higher submillimeter emissivities than grains in the diffuse interstellar medium. The dust-photon interaction is treated in a fully self-consistent three-dimensional radiative transfer code. We provide an AGN library of spectral energy distributions (SEDs). Its purpose is to quickly obtain estimates of the basic parameters of the AGNs, such as the intrinsic luminosity of the central source, the viewing angle, the inner radius, the volume filling factor and optical depth of the clouds, and the optical depth of the disk midplane, and to predict the flux at yet unobserved wavelengths. The procedure is simple and consists of finding an element in the library that matches the observations. We discuss the general properties of the models and in particular the 10um silicate band. The AGN library accounts well for the observed scatter of the feature strengths and wavelengths of the peak emission. AGN extinction curves are discussed and we find that there is no direct one-to-one link between the observed extinction and the wavelength dependence of the dust cross sections. We show that objects in the library cover the observed range of mid-infrared colors of known AGNs. The validity of the approach is demonstrated by matching the SEDs of a number of representative objects: Four Seyferts and two quasars for which we present new Herschel photometry, two radio galaxies, and one hyperluminous infrared galaxy. Strikingly, for the five luminous objects we find that pure AGN models fit the SED without needing to postulate starburst activity.2015A&A...583A.120Shttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/583/A120CatalogResearchIsServedByTAP VizieR generic servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/583/A120https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/583/A120http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/583/A120https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/583/A120https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/583/A120http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/583/A120GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapdefaultJ/A+A/583/A120/listList of SED filesplotSEDmeta.ref.urlcharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintRInner radius of the dusty torus1e+15cmphys.size.radiusintVcCloud volume filling factor%meta.bib.volumefloatAcOptical depth (in V) of the individual cloudphys.absorption.opticalDepthfloatAdOptical depth (in V) of the disk midplanephys.absorption.opticalDepthintthCentral value of bin viewing angle measured from the pole (z-axis)degsrc.orbital.inclinationintFileNameName of the SED file in subdirectory sedlibmeta.id;meta.filechar