X-ray spectral study of hot gas in three clusters of galaxies

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Table 1:

Previously known parameters for the studied sources.
Object	WFC flux^a	ROSAT flux^b	Redshift^c
J1539	0.82	1.68 ^d,e	0.0728 ^d
		2.49 ^f
J1601	1.28	2.41 ^f	0.1530 ^g
J0812	1.14	3.93 ^f	0.0620 ^g

Notes. ^(a) 2-10 keV, 10^-14 W m^-2 for Crab-like spectrum (i.e. a power law with a photon index of 2). ^(b) 0.1-2.4 keV, 10^-14 W m^-2. ^(c) Determined using optical spectroscopy. ^(d) From REFLEX (Böhringer et al. 2004). ^(e) Using a Raymond-Smith model (Raymond & Smith 1977). ^(g) From CIZA (Ebeling et al. 2002).

Source LaTeX | All tables | In the text

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