The X-ray emission of local luminous infrared galaxies

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Volume 535 (November 2011)

A&A, 535 (2011) A93

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Table 8

AGN luminosity.

Galaxy name	Type		L_{14−195 keV}^a
		(10⁴² erg s^-1)

NGC 3690	Sy2	3.9^b	<10	55	19
MCG−03-34-064	Sy2	15	20	290	1.7
NGC 5135	Sy2	10^b	<16	180	3.9
IC 4518W	Sy2	2.2	18	26	21
MCG+04-48-002	···	6.9	38	120	3.0
NGC 7130	Sy2	10^b	<23	180	5.1
NGC 7469	Sy1	17	39	340	5.0
NGC 7679	Sy1	0.4	15^c	4.1	120

Notes. Intrinsic AGN 2–10 keV, 14–195 keV and bolometric luminosities. We used the bolometric corrections of Marconi et al. (2004).

^(a)

Observed Swift/BAT 14–195 keV luminosity from Tueller et al. (2010). For non-detections we assumed a flux < 3.9 × 10^-11 erg cm^-2 s^-1, which is the 4.8 σ sensitivity achieved for 95% of the sky in this survey.

^(b)

Estimated from the 6.4 keV Fe Kα emission line luminosity using the relation L_FeKα/L_{2−10 keV} = 2 × 10^-3 from Levenson et al. (2006).

^(c)

The L_{14−195 keV} of NGC 7679 is likely to be contaminated by the nearby Seyfert 2 NGC 7682.

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