BASS - XLIII. Optical, UV, and X-ray emission properties of unobscured Swift/BAT active galactic nuclei

Open Access

Fig. 26.

14–195 keV bolometric correction (κ_{14 − 195}) against the intrinsic luminosity in the 14–195 keV energy bin (L_{14 − 195}). The solid black line shows the best-fit relation we obtained (Sect. 7.4.3, Table 4). The shaded gray region shows the one sigma confidence interval for our best-fit relation.

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