Image Details
Caption: Figure 3.
Left panel: variation of X-ray bolometric correction (κ2−10) as a function of αOX. The blue circles, green diamonds, purple down-triangles, red up-triangles, and orange squares represent the data points from NGC 1566, NGC 2617, Mrk 590, Mrk 1018, and IRAS 23226–3843, respectively. The yellow stars represent the binned data point. The black line represents the best fits (Equation (4)) of the data. The green dashed line represents the κ2−10−αOX relation for unobscured BASS AGNs (K. K. Gupta et al. 2024). Right panel: same as right panel but with binned data. The shaded regions represent the 1-σ scatter.
© 2026. The Author(s). Published by the American Astronomical Society.