… Our model predictions for torus emission and the implications for IR observations are
presented in xx 3Y5, while in x 6 we discuss aspects of clumpiness that are unrelated to the IR …

… of AGN clumpy tori in Nenkova et al. (2002), Elitzur et al. (2004), and Elitzur (2006, 2007). …
In a companion paper (Nenkova et al. 2008, hereafter Paper II) we present the assembly of …

… :O or C:M curves, respectively. The curves are reliable only up to distances of ∼6 kpc, beyond
… All modelling was performed with our public code Dusty (Ivezić, Nenkova & Elitzur 1999). …

We discovered a bug in the code that performed the calculation of torus emission in the
published version of this article. The spectral shape of the torus flux is not affected; the error …

… we present here and those of Ivezic & Elitzur (1997)… 6 m region plus a connection point at
7.8 m, and the intermediate- and longwavelength intervals become 13.2Y14.5 and 26.0Y31.5 m…

… extent, which the dust's optical properties determine (Sirocky et al. 2008). We plot several
characteristic examples in Figure 6. Spherical distributions of clumps occupy a distinct region …

… In this paper we perform a thorough comparison between two of the most popular models
in the literature, namely the smooth models by Fritz et al. and the clumpy models by Nenkova …

… -density models (Nenkova et al. 2008b). Realistic unification explains away the remainder. …
of these earlier figures are afflicted by the computer bug reported in Nenkova et al. (2010). …

… A formalism for handling clumpy media was developed by Nenkova et al. (2002, 2008a, …
We employed Clumpy to produce a large database 6 of model SEDs f λ = λF λ /F AGN , with …

… 6 we present the total SED and its thermal and scattered components, along with the
primary source emission, for face-on and edge-on view. As it can be seen from the figure, the …