Matches in SemOpenAlex for { <https://semopenalex.org/work/W2884620105> ?p ?o ?g. }
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- W2884620105 abstract "We present a uniform broadband X-ray (0.5–100.0 keV) spectral analysis of 12 Swift/Burst Alert Telescope selected Compton-thick () active galactic nuclei (CTAGNs) observed with Suzaku. The Suzaku data of three objects are published here for the first time. We fit the Suzaku and Swift spectra with models utilizing an analytic reflection code and those utilizing the Monte-Carlo-based model from an AGN torus by Ikeda et al. The main results are as follows: (1) The estimated intrinsic luminosity of a CTAGN strongly depends on the model; applying Compton scattering to the transmitted component in an analytic model may largely overestimate the intrinsic luminosity at large column densities. (2) Unabsorbed reflection components are commonly observed, suggesting that the tori are clumpy. (3) Most of CTAGNs show small scattering fractions (<0.5%), implying a buried AGN nature. (4) Comparison with the results obtained for Compton-thin AGNs suggests that the properties of these CTAGNs can be understood as a smooth extension from Compton-thin AGNs with heavier obscuration; we find no evidence that the bulk of the population of hard-X-ray-selected CTAGNs are different from less obscured objects." @default.
- W2884620105 created "2018-08-03" @default.
- W2884620105 creator A5016120295 @default.
- W2884620105 creator A5018689413 @default.
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- W2884620105 creator A5059137989 @default.
- W2884620105 creator A5088633109 @default.
- W2884620105 creator A5089452386 @default.
- W2884620105 date "2018-02-01" @default.
- W2884620105 modified "2023-09-26" @default.
- W2884620105 title "<i>Suzaku</i>Observations of Heavily Obscured (Compton-thick) Active Galactic Nuclei Selected by the<i>Swift</i>/BAT Hard X-Ray Survey" @default.
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