AGN<sc>FITTER-RX:</sc> Modeling the radio-to-X-ray spectral energy distributions of AGNs

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dc.contributor.authorMartinez-Ramirez, L. N.
dc.contributor.authorRivera, G. Calistro
dc.contributor.authorLusso, E.
dc.contributor.authorBauer, F. E.
dc.contributor.authorNardini, E.
dc.contributor.authorBuchner, J.
dc.contributor.authorBrown, M. J. I.
dc.contributor.authorPineda, J. C. B.
dc.contributor.authorTemple, M. J.
dc.contributor.authorBanerji, M.
dc.contributor.authorStalevski, M.
dc.contributor.authorHennawi, J. F.
dc.date.accessioned2025-01-20T16:11:41Z
dc.date.available2025-01-20T16:11:41Z
dc.date.issued2024
dc.description.abstractWe present new advancements in the modeling of the spectral energy distributions (SEDs) of active galaxies by introducing the radio-to-X-ray fitting capabilities of the publicly available Bayesian code AGNFITTER. The new code release, called AGNFITTER-RX, models the broad-band photometry covering the radio, infrared (IR), optical, ultraviolet (UV), and X-ray bands consistently using a combination of theoretical and semi-empirical models of the active galactic nucleus (AGN) and host-galaxy emission. This framework enables the detailed characterization of four physical components of the active nuclei, namely the accretion disk, the hot dusty torus, the relativistic jets and core radio emission, and the hot corona, and can be used to model three components within the host galaxy: stellar populations, cold dust, and the radio emission from the star-forming regions. Applying AGNFITTER-RX to a diverse sample of 36 AGN SEDs at z less than or similar to 0.7 from the AGN SED ATLAS, we investigated and compared the performance of state-of-the-art torus and accretion disk emission models in terms of fit quality and inferred physical parameters. We find that clumpy torus models that include polar winds and semi-empirical accretion disk templates including emission-line features significantly increase the fit quality in 67% of the sources by reducing by 2 sigma fit residuals in the 1.5-5 mu m and 0.7 mu m regimes. We demonstrate that, by applying AGNFITTER-RX to photometric data, we are able to estimate the inclination and opening angles of the torus, consistent with spectroscopic classifications within the AGN unified model, as well as black hole masses congruent with virial estimates based on H alpha. We investigate wavelength-dependent AGN fractions across the spectrum for Type 1 and Type 2 AGNs, finding dominant AGN fractions in radio, mid-infrared, and X-ray bands, which are in agreement with the findings from empirical methods for AGN selection. The wavelength coverage and the flexibility for the inclusion of state-of-the-art theoretical models make AGNFITTER-RX a unique tool for the further development of SED modeling for AGNs in present and future radio-to-X-ray galaxy surveys.
dc.fuente.origenWOS
dc.identifier.doi10.1051/0004-6361/202449329
dc.identifier.eissn1432-0746
dc.identifier.issn0004-6361
dc.identifier.urihttps://doi.org/10.1051/0004-6361/202449329
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/90287
dc.identifier.wosidWOS:001283163300002
dc.language.isoen
dc.revistaAstronomy & astrophysics
dc.rightsacceso restringido
dc.subjectmethods: statistical
dc.subjectgalaxies: active
dc.subjectgalaxies: nuclei
dc.subjectquasars: general
dc.titleAGN<sc>FITTER-RX:</sc> Modeling the radio-to-X-ray spectral energy distributions of AGNs
dc.typeartículo
dc.volumen688
sipa.indexWOS
sipa.trazabilidadWOS;2025-01-12
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