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Table 3:

IR and X-ray luminosities.
Source $\log L_{\rm IR}^{\rm tot}$a $\log L_{\rm IR}^{\rm AGN}$a $\log L_{\rm IR}^{\rm SB}$a $\log L_{\rm IR,RTM}^{\rm tot}$b $\log L_{\rm IR,RTM}^{\rm AGN}$b $\log L_{\rm IR,RTM}^{\rm SB}$b $\log L_{\rm X}^{\rm AGN}$c $N_{\rm H}$d
  (erg s-1) (erg s-1) (erg s-1) (erg s-1) (erg s-1) (erg s-1) (erg s-1) (cm-2)

Class A HLIRG

PG 1206+459 		48.0 48.0 0 47.8 47.8 <46.7 $\rm 45.11^{+0.02}_{-0.04}$ ...
PG 1247+267 48.8 48.8 0 47.9 47.9 <46.8 $\rm 45.93^{+0.02}_{-0.03}$ ...
IRAS F12509+3122 47.6 46.8 47.5 47.0 46.8 46.6 $\rm 42.26^{+0.05}_{-0.05}$ ...
IRAS 14026+4341e 46.5 45.8 46.5 46.5 46.3 46.1 $\rm 42.7^{+0.2}_{-0.5}$ ...
IRAS F14218+3845 47.1 46.5 46.9 46.9 46.1 46.8 $\rm 44.60^{+0.03}_{-0.03}$ ...
IRAS 16347+7037 48.5 48.5 0 47.7 47.7 <46.8 $\rm 46.00^{+0.07}_{-0.09}$ ...
IRAS 18216+6418 47.1 46.9 46.6 46.8 46.6 46.4 $\rm 45.6^{+0.04}_{-0.05}$ ...

Class B HLIRG

IRAS F00235+1024 		46.7 46.4 46.4 46.7 46.4 46.4 <42.2 >1025
IRAS 07380-2342 47.0 46.7 46.7 47.0 46.8 46.5 <41.7 ...
IRAS 00182-7112 46.6 46.3 46.3 46.7 <46.5 46.7 44.82+0.16-0.14 >1025
IRAS 09104+4109 47.3 47.1 46.8 46.8 46.8 <46.2 $\rm 45.30^{+0.36}_{-0.09}$ >1025
IRAS 12514+1027 46.7 46.5 46.2 46.5 46.2 46.2 $\rm 43.3^{+1.4}_{-0.7}$ $(4^{+20}_{-3})\times10^{23}$
IRAS F15307+3252 47.9 47.6 47.6 46.9 46.6 46.7 $\rm 45.49^{+0.09}_{-0.11}$ >1025

Notes. (a) IR luminosities (1-1000  $\mu{\rm m}$) estimated using our SED fitting.
(b) IR luminosities (1-1000  $\mu{\rm m}$) estimated by the analysis of the IR SED using RTM (Rowan-Robinson 2000; Farrah et al. 2002a).
(c) Absorption corrected 2-10 keV luminosities from Ruiz et al. (2007).
(d) Intrinsic absorption estimated using X-ray spectra (Ruiz et al. 2007).
(e) The X-ray luminosity of this source has been calculated from 2XMMi fluxes (Watson et al. 2009), and it is not corrected for absorption.


Source LaTeX | All tables | In the text

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