Blue circles and gray squares represent the variation of the X-ray bolometric correction (κ₂₋₁₀) as a function of the Eddington ratio (λ_Edd) for the variable AGN studied here and for unobscured AGNs in BASS from K. K. Gupta et al. (2025), respectively. The blue dashed–dotted and orange solid lines represent the best fit for our sample (Equation (3)) and unobscured BAT AGNs (Equation (2) of K. K. Gupta et al. 2025), respectively. The red dotted line shows the best-fit relation of κ₂₋₁₀−λ_Edd for unobscured BAT AGNs with high-redshift quasars, taken from K. K. Gupta et al. (2025). The green dashed line shows the κ₂₋₁₀−λ_Edd relation from F. Duras et al. (2020). The blue shaded region represents the 1σ scatter from the present study.