How Does the Polar Dust Affect the Correlation between Dust Covering Factor and Eddington Ratio in Type 1 Quasars Selected from the Sloan Digital Sky Survey Data Release 16?

We revisit the dependence of covering factor (CF) dust torus on physical properties active galactic nuclei (AGNs) by taking into account an AGN polar emission. The CF is converted from a ratio infrared (IR) luminosity contributed ($L_{\rm IR}^{\rm torus}$) and bolometric bol}$), assuming non-linear relation between intrinsic CF. select 37,181 type 1 quasars at $z < 0.7$ Sloan Digital Sky Survey Data Release 16 quasar catalog. Their $L_{\rm bol}$, black hole mass ($M_{\rm BH}$), Eddington ($\lambda_{\rm Edd}$) are derived spectral fitting with QSFit. conduct energy distribution decomposition using X-CIGALE clumpy model to estimate torus}$ without being affected contribution stellar IR For 5720 whose quantities securely determined, we perform correlation analysis (i) (ii) $M_{\rm BH}$, (iii) $\lambda_{\rm Edd}$. As result, anti-correlations for CF-$L_{\rm CF-$M_{\rm CF-$\lambda_{\rm Edd}$ confirmed. find that incorporating emission makes those stronger which compared considering it. This indicates wind provably driven radiative pressure one key components regulate obscuring material AGNs.