The hard X-ray view of bright infrared galaxies | Astronomy & Astrophysics (A&A)

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Table 2:

Average signals (or $5\sigma$ upper limits) detected for the various subsamples at hard X-rays (18-80 keV) and at 60 $\mu$ m.
Sample	Srcs	Exp.	Ct rate	$F_{18{-}80~{\rm keV}}$	$F_{\rm 60~\mu m}$
		Ms	ct/s	10^-10 cgs	Jy
Seyfert 1	14	1.7	2.25 $\pm$ 0.02	1.28	18.3
S1 - 4151¹	13	1.4	0.51 $\pm$ 0.02	0.29	19.3
Seyfert 2	64	12.1	0.87 $\pm$ 0.01	0.49	31.1
Seyfert	93	16.1	1.04 $\pm$ 0.01	0.59	28.9
ULIRGs	12	4.1	<0.06	<0.034	10.2
Liners	41	7.5	<0.045	<0.026	29.6
LIRGs	144	26.7	<0.02	<0.011	12.9
non Seyfert	520	96.0	<0.013	<0.0074	19.1

¹ Includes all Seyfert 1 galaxies excepting NGC 4151.
Effective hard X-ray exposure, count rates and integrated flux are provided together with the average 60 $\mu$ m flux. The hard X-ray detection significances for the first four samples are 119, 23, 122 and 147 respectively.

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