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Table 1.

Models considered when studying properties of cLRDs.

Property
Column density max: integrates the column outmax80: when radiation
density from the position of pressure on dusty gas
the MBH to the host galaxy dominates excludes from the
virial radius integration the inner 80 pc
around the MBH

MBHs distr: MBH masses are extracted distr overm: MBH masses distr sEdd: Eddington ratios
from the MBH-Mstar are extracted from the MBH- are extracted in log space
relation from G20 while Eddington Mstar relation from P24 while from a normal distribution
ratios are extracted in log Eddington ratios are extracted centered in log(0.5) with
space from a normal distribution in log space from a normal standard deviation 0.5 dex
centered in log(0.25) with standard distribution centered in with
deviation 0.5 dex log(0.25) standard deviation 0.5 dex

dust MW-like: a mass fraction SMC-like: 100% silicates
of 54% in silicates and 46% with MRN size distribution
in carbonaceous grains with
MRN size distribution cut
out at 0.25 μm)

Notes. “max” integrates the column density from the position of the MBH to the host galaxy virial radius; “outmax80” integrates the column density from outside an 80-pc sphere around the MBH to the host galaxy virial radius to mimic the effect of radiation pressure on dust.

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