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We report on the torus constraints of the Compton-thick AGN withdouble-peaked optical narrow line region (NLR) emission lines, ANEPD-CXO245, atz=0.449 in the AKARI NEP Deep Field. The unique infrared data on this field,including those from the nine-band photometry over 2-24 $\mu$m with the AKARIInfrared Camera (IRC), and the X-ray spectrum from Chandra allow us toconstrain torus parameters such as the torus optical depth, X-ray absorbingcolumn, torus angular width ($\sigma$) and viewing angle ($i$). We analyze theX-ray spectrum as well as the UV-optical-infrared spectral energy distribution(UOI-SED) with clumpy torus models in X-ray (XCLUMPY; Tanimoto et al. 2019) andinfrared (CLUMPY; Nenkova et al. 2008) respectively. From our current data, theconstraints on $\sigma$--$i$ from both X-rays and UOI show that the line ofsight crosses the torus as expected for a type 2 AGN. We obtain a small X-rayscattering fraction (<0.1%), which suggests narrow torus openings, givingpreference to the bi-polar outflow picture of the double-peaked profile.Comparing the optical depth of the torus from the UOI-SED and the absorbingcolumn density $N_{\rm H}$ from the X-ray spectrum, we find that thegas-to-dust ratio is $\gtrsim 4$ times larger than the Galactic value.

Torus Constraints in ANEPD-CXO245: A Compton-thick AGN with Double-Peaked Narrow Lines