  We apply XCLUMPY, an X-ray spectral model from a clumpy torus in an active
galactic nucleus (AGN), to the broadband X-ray spectra of 10 obscured AGNs
observed with both Suzaku and NuSTAR. The infrared spectra of these AGNs were
analyzed with the CLUMPY code. Since XCLUMPY adopts the same clump distribution
as that in the CLUMPY, we can directly compare the torus parameters obtained
from the X-ray spectra and those from the infrared ones. The torus angular
widths determined from the infrared spectra ($\sigma_{\mathrm{IR}}$) are
systematically larger than those from the X-ray data ($\sigma_{\mathrm{X}}$);
the difference ($\sigma_{\mathrm{IR}}-\sigma_{\mathrm{X}}$) correlates with the
inclination angle determined from the X-ray spectrum. These results can be
explained by the contribution from dusty polar outflows to the observed
infrared flux, which becomes more significant at higher inclinations (more
edge-on views). The ratio of the hydrogen column density and V-band extinction
in the line of sight absorber shows large scatter ($\simeq$1 dex) around the
Galactic value, suggesting that a significant fraction of AGNs have dust-rich
circumnuclear environments.
