Figure 7 from Comprehensive Broadband X-Ray and Multiwavelength Study of Active Galactic Nuclei in 57 Local Luminous and Ultraluminous Infrared Galaxies Observed with NuSTAR and/or Swift/BAT

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Comprehensive Broadband X-Ray and Multiwavelength Study of Active Galactic Nuclei in 57 Local Luminous and Ultraluminous Infrared Galaxies Observed with NuSTAR and/or Swift/BAT

Authors: Satoshi Yamada, Yoshihiro Ueda, Atsushi Tanimoto, Masatoshi Imanishi, Yoshiki Toba, Claudio Ricci, and George C. Privon

2021 The Astrophysical Journal Supplement Series 257 61.

Provider: AAS Journals

Caption: Figure 7.

Bolometric–to–X-ray correction vs. black hole mass. The black solid line and gray shaded area represent the relation and its 1σ dispersion found by Martocchia et al. (2017) for WISSH quasars, PG quasars, and XMM-COSMOS Seyfert 1s. The black dashed line shows a typical value of κ_bol,X = 20. Symbols and colors are the same as in Figure 3.

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