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Balmer decrements are large for both narrow-line and broad-line AGN in our sample. Although the extinction of the AGN continuum and broad-line regions only requires extinction on small scales, extinction of the narrow-line region requires extinction on much larger scales. Albeit with only a small sample, our near-IR spectra show that these sources indeed have the fraction of broad- to narrow-line sources that one would expect for such luminous sources, despite being too obscured to appear in optically selected samples. 342409 has the second largest infrared luminosity of sources at low enough redshifts to observe the silicate absorption feature. The second are AGN whose optical light is obscured on much larger scales ("host-obscured" AGN). As we discuss above, the selection of optically faint luminous infrared galaxies will naturally select "host-obscured" sources. The fact that we see hints of extended but very faint optical emission in many of our sources supports this view (Dey et al. If this is the case, then we might expect to see silicate emission in our sample of very luminous type personalized air Force 1 Shadow sports shoes optically faint ULIRGS. However, this population was selected to have faint optical (i.e., rest-frame UV) magnitudes. 0.8 mJy optically faint luminous infrared galaxies harbor AGN