Model images of the clumpy (top row) and disk + wind (bottom rows) models fit to the nuclear continuum spectrum of J1010 as they would look projected on the sky. The models correspond to the ones described by the parameters of the 50 percentile given in Tables 2 and 3. In the case of the clumpy model, τ_V = 160 and Y = 20 were used instead of the values shown in Table 2 because the latter are outside the parameter range from which images are computed in HyperCat, but this have negligible impact of torus emission and cloud distribution. The last row is a zoom-in of the disk + wind model showing the same physical region as the clumpy model shown in the top row (30 × 30 pc²), since the middle row covers a FOV of 300 × 300 pc². The physical sizes were computed by assuming a bolometric luminosity of 10⁴⁵ erg s⁻¹, and in the case of the disk + wind model, a pixel scale = 0.19 × r_sub, with r_sub = 0.288 pc for the largest graphite grains. From left to right, the panels correspond to torus model emission at 5, 8, 10, 20, and 1000 μm, and to the cloud distribution considering all the mass. All the panels are shown in logarithmic color scale and they are normalized to the peak of emission. The black cross in the top and bottom panels indicates the position of the AGN.