Astronomy & Astrophysics

Table 6: Best fit parameters of an absorbed power-law model for X-ray bright unidentified X-ray sources in the Cha I XMM-Newton field.
Designation $\chi^2_{\rm red}$ $N_{\rm H}$ $\Gamma$ $f_{\rm x}$

(d.o.f.) [ ${\rm 10^{22}}~{\rm cm^{-2}}$ ] [ ${\rm erg/cm^2/s}$ ]

XMM-Cha I-18 0.91 (3) 3.4 2.76 $1.6 \times 10^{-13}$

XMM-Cha I-35 0.89 (25) 0.91 1.47 $3.4 \times 10^{-13}$

XMM-Cha I-44 0.80 (6) 0.73 1.73 $4.0 \times 10^{-14}$

**Table 6:** Best fit parameters of an absorbed power-law model for X-ray bright unidentified X-ray sources in the Cha I *XMM-Newton* field.
Designation	$\chi^2_{\rm red}$	$N_{\rm H}$	$\Gamma$	$f_{\rm x}$
	(d.o.f.)	[ ${\rm 10^{22}}~{\rm cm^{-2}}$ ]		[ ${\rm erg/cm^2/s}$ ]
XMM-Cha I-18	0.91 (3)	3.4	2.76	$1.6 \times 10^{-13}$
XMM-Cha I-35	0.89 (25)	0.91	1.47	$3.4 \times 10^{-13}$
XMM-Cha I-44	0.80 (6)	0.73	1.73	$4.0 \times 10^{-14}$

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