Mid-infrared and hard X-ray emission in AGN

DOI

We use mid-infrared spectral decomposition to separate the 6{mu}m mid-infrared AGN continuum from the host emission in the ISO low resolution spectra of 71 active galaxies and compare the results to observed and intrinsic 2-10keV hard X-ray fluxes from the literature.

Cone search capability for table J/A+A/418/465/table1 (Data for Seyfert sample)

Identifier
DOI http://doi.org/10.26093/cds/vizier.34180465
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/418/465
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/418/465
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/418/465
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/418/465
Provenance
Creator Lutz D.; Maiolino R.; Spoon H.W.W.; Moorwood A.F.M.
Publisher CDS
Publication Year 2007
Rights https://cds.unistra.fr/vizier-org/licences_vizier.html
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Representation
Resource Type Dataset; AstroObjects
Discipline Astrophysics and Astronomy; Cosmology; Galactic and extragalactic Astronomy; High Energy Astrophysics; Natural Sciences; Observational Astronomy; Physics