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Table 1

Source properties.

Source D z Type LIR Lxray
[Mpc]

I Zw 1 222 0.0589 Sy 1 44.9 43.7
NGC 424 44.7 0.0110 Sy 2 43.6 43.8
NGC 1068 14.4 0.0038 Sy 2 44.0 43.6
NGC 1365 18.1 0.0055 Sy 1 42.5 42.1
IRAS 05189-2524 167 0.0426 Sy 2 44.6 43.7
H 0557-385 135 0.0339 Sy 1 44.4 43.8
IRAS 09149-6206 222 0.0579 Sy 1 44.9 44.0
MCG-05-23-16 38.8 0.0085 Sy 2 43.5 43.3
Mrk 1239 84.5 0.0200 Sy 1 44.0 43.3
NGC 3281 47.6 0.0107 Sy 2 43.4 43.2
NGC 3783 43.8 0.0097 Sy 1 43.7 43.2
NGC 4151 16.9 0.0033 Sy 1 43.0 42.5
NGC 4507 51.7 0.0118 Sy 2 43.7 43.2
NGC 4593 41.2 0.0090 Sy 1 43.1 42.9
ESO 323-77 64.2 0.0150 Sy 1 43.7 42.8
IRAS 13349+2438 393 0.1076 Sy 1 45.5 43.9
IC 4329 A 68.3 0.0161 Sy 1 44.2 43.9
Circinus 4.2 0.0014 Sy 2 42.7 42.3
NGC 5506 28.7 0.0062 Sy 2 43.4 43.1
NGC 5995 102 0.0252 Sy 2 44.1 43.5
NGC 7469 60.9 0.0163 Sy 1 43.9 43.2

Notes. D: angular-size distance derived from redshift, except for Circinus and NGC 1068; z: redshift (from NED); Type: AGN classification from SIMBAD; LIR: the 12 μm infrared luminosity is given as log (LMIR/ erg s) and the values were obtained from Burtscher et al. (2013), uncertainties are typically lower than 5%; Lxray: the absorption-corrected 2–10 keV X-ray AGN luminosity given as log (Lx/ erg s). The values were collected from Asmus et al. (2015).

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