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Table · dataset · 2026

SED analysis of X-ray selected AGN in Stripe 82

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We perform a systematic, multiwavelength spectral energy distribution (SED) analysis of X-ray detected active galactic nuclei (AGNs) at z=0.2-0.8 with Sloan Digital Sky Survey (SDSS) counterparts in the Stripe 82 region, consisting of 60 type 1 and 137 type 2 AGNs covering a 2-10keV luminosity range of 41.6<logLx<4.7.

Description

The latest CIGALE code, where dusty polar components are included, is employed. To obtain reliable host and AGN parameters in type 1 AGNs, we utilize the image-decomposed optical SEDs of host galaxies by Li et al. based on the Subaru Hyper-Suprime Cam images.

The mean ratio of black hole masses (MBH) and stellar masses (Mstellar) of our X-ray detected type 1 AGN sample, log(M_BH_/M_stellar_)=-2.7\pm0.5, is close to the local relation between BH and stellar masses as reported by Li et al. for SDSS quasars. This ratio is slightly lower than that found for more luminous (logL_bol_>45) type 1 AGNs at z~1.5. This can be explained by the AGN luminosity dependence of log(M_BH_/M_stellar_), which little evolves with redshift.

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We confirm the trend that the UV-to-X-ray slope ({alpha}_OX_) or X-ray-to-bolometric correction factor ({kappa}_2-10_) increases with AGN luminosity or Eddington ratio. We find that type 1 and type 2 AGNs with the same luminosity ranges share similar host stellar mass distributions, whereas type 2s tend to show smaller AGN luminosities than type 1s. This supports the luminosity-dependent (or Eddington-ratio-dependent) unified scheme.

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Stated by source
Optical · X-Ray
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Astronomical sciences 74% · Image 65%
Provenance · 1 source records, 11 field assertions
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IVOA Registry (Virtual Observatory)ivo://cds.vizier/j/apj/961/24615 d agoJSON v1
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