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

Open Access

Fig. 22.

4400 Å bolometric correction as a function of (a) the 4400 Å monochromatic luminosity and (b) the bolometric luminosity. We find a very weak correlation in both cases (Sect. 7.4.2, Table 4) shown as the black line. Hence, we show the best fit with a constant value as well (dashed red line). For both cases, we get a value of $κ_{4400 Å} = 7.9 \pm 0.3$ $\kappa_{\mathrm{4400\,\AA}} = 7.9 \pm 0.3$ .

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