Gravitational potential and X-ray luminosities of early-type galaxies observed with XMM-Newton and Chandra

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Volume 501 / No 1 (July I 2009)

A&A, 501 1 (2009) 157-169

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Table 5:

X-ray luminosities within $4~r_{\rm e}$ of each sample galaxy.
Galaxy	$\log L_{\rm ISM}$ ^a	$\log L_{\rm hard}$ ^b	$\log L_{\rm ISM}$ ^a
	projection	projection	deprojection
	(erg/s)	(erg/s)	(erg/s)
IC 1459	40.08	40.28	40.00
NGC 720	40.46	39.91	40.38
NGC 1316	40.63	40.20	40.55
NGC 1332	40.12	39.74	40.04
NGC 1395	40.43	40.16	40.34
NGC 1399	41.13	40.32	40.98
NGC 1549	39.39	39.09	--
NGC 3585	39.36	39.39	--
NGC 3607	40.37	39.86	--
NGC 3665	40.36	39.96	--
NGC 3923	40.74	40.27	40.68
NGC 4365	39.58	39.86	--
NGC 4382	40.25	39.83	--
NGC 4472	41.40	40.51	41.36
NGC 4477	39.96	39.54	--
NGC 4526	39.53	39.64	--
NGC 4552	40.62	40.27	40.60
NGC 4636	41.46	40.27	41.44
NGC 4649	41.00	40.41	40.99
NGC 5044	42.49	41.01	42.41
NGC 5322	40.14	39.82	--
NGC 5846	41.72	40.56	41.70

^a The X-ray luminosity of the thermal emission in the range of 0.3-2.0 keV derived from the projected and deprojected spectra.
^b The X-ray luminosity of the non thermal emission in the range of 0.3-2.0 keV derived from the projected spectra.

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