Infrared Signatures of Dusty Tori Formed by MHD-Driven Outflows

File Description 1. Integrated AGN + Dust Spectra (calibrated_total_spectra_r-*.zip) Processed spectra (primary source + dust emission) for four model grids ($p=0.5, 1.0, 1.5, 2.0$), including foreground/internal extinction and bolometric energy corrections. 2. Bayesian Fitting Results (Fitting_result.zip) This archive contains the complete output from our analysis for the 25 AGN sample: fitting_data/: Best-fit model spectra vs. observational data. bayesian_result/: Full Bayesian posterior distributions for all parameters. fitting_figures/: Diagnostic plots showing best-fit results and spectral features. Naming Convention for .data files The filenames follow a standardized schema representing the physical parameters of the specific model grid: M: Black hole mass ($\log_{10}(M_{\rm{BH}}/M_\odot)$) m: Normalized accretion rate ($\dot{m}$) DGR: Dust-to-gas ratio ($-10*\log_{10}(DGR)$) OA: Opening angle of the torus ($\theta_{\rm{open}}$) Y: Radial extent ($R_{\rm{out}}/R_{\rm{sub}}$) VA: Viewing angle ($\theta_{\rm{view}}$) Example: Total_M60_m01_DGR20_OA20_Y20_VA0.data corresponds to $\log M_{\rm{BH}}=6.0$, $\dot{m}=0.1$, $DGR=10^{-2.0}$, $\theta_{\rm{open}}=20^{\circ}$, $Y=20$, $\theta_{\rm{view}}=20^{\circ}$.