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We apply XCLUMPY, an X-ray spectral model from a clumpy torus in an activegalactic nucleus (AGN), to the broadband X-ray spectra of 10 obscured AGNsobserved with both Suzaku and NuSTAR. The infrared spectra of these AGNs wereanalyzed with the CLUMPY code. Since XCLUMPY adopts the same clump distributionas that in the CLUMPY, we can directly compare the torus parameters obtainedfrom the X-ray spectra and those from the infrared ones. The torus angularwidths determined from the infrared spectra ($\sigma_{\mathrm{IR}}$) aresystematically larger than those from the X-ray data ($\sigma_{\mathrm{X}}$);the difference ($\sigma_{\mathrm{IR}}-\sigma_{\mathrm{X}}$) correlates with theinclination angle determined from the X-ray spectrum. These results can beexplained by the contribution from dusty polar outflows to the observedinfrared flux, which becomes more significant at higher inclinations (moreedge-on views). The ratio of the hydrogen column density and V-band extinctionin the line of sight absorber shows large scatter ($\simeq$1 dex) around theGalactic value, suggesting that a significant fraction of AGNs have dust-richcircumnuclear environments.

Application of X-Ray Clumpy Torus Model (XCLUMPY) to 10 Obscured Active Galactic Nuclei Observed with Suzaku and NuSTAR