Figure 5 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 5.

Left panel: X-ray-based Eddington ratio vs. galaxy separation, where κ_bol,X (=﹩{L}_{\mathrm{bol},\mathrm{AGN}}^{(\mathrm{IR})}﹩/L₂₋₁₀) = 20 is assumed. Right panel: IR-based Eddington ratio vs. galaxy, where the bolometric AGN luminosities based on the IR results are adopted. The black dashed line shows the Eddington limit (λ_Edd = 1). Symbols and colors are the same as in Figure 3.

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