**Table 1:** Summary properties of the X-ray sources in the region of KUG 0214-057.
Source^a	RA	Dec	Count rate^b	HR1^c	HR2	HR3	$\log_{10} f_{\rm X}$ ^d	z^e	$\log_{10} L_X$ ^f
name	J2000.0		[count s^-1]
A	02 17 20.60	-05 28 55.1	0.00499 $\pm$ 0.00043	0.83 $\pm$ 0.07	-0.59 $\pm$ 0.07	-0.59 $\pm$ 0.29	-13.87	0.018	39.98
B	02 17 19.88	-05 28 39.8	0.00377 $\pm$ 0.00039	0.81 $\pm$ 0.08	-0.59 $\pm$ 0.07	-0.41 $\pm$ 0.34	-13.99	0.018	39.86
C	02 17 18.13	-05 28 30.5	0.00370 $\pm$ 0.00044	0.63 $\pm$ 0.09	-0.68 $\pm$ 0.08	-0.25 $\pm$ 0.38	-14.00	0.018	39.85
D	02 17 16.77	-05 28 40.8	0.00245 $\pm$ 0.00036	1.00 $\pm$ 0.04	-0.50 $\pm$ 0.12	-0.44 $\pm$ 0.37	-14.17	0.018	39.67
E	02 17 18.62	-05 29 21.3	0.12428 $\pm$ 0.00131	0.57 $\pm$ 0.01	-0.73 $\pm$ 0.01	-0.42 $\pm$ 0.02	-12.47	0.634	44.76

^a IAU designations of sources are as follows: A XMMU J021729.6-052855; B XMMU J021719.9-052840; C XMMU J021718.1-052831; D XMMU J021716.8-052841; E XMMU J021718.6-052921.
^b X-ray count rate in 0.3-10 keV band expressed in EPIC pn count s^-1.
^c Hardness ratios HR1, HR2 and HR3 are defined in the caption to Fig. 3.
^d X-ray flux in 0.3-10 keV band [ $\rm erg\ cm^{-2}\ s^{-1}$ ] assuming a nominal power-law spectrum with $\Gamma =1.7$ and absorption column density $N_{\rm H}=2.5\times 10^{20}~\rm cm^{-2}$ .
^e Assumed redshift (see text).
^f X-ray luminosity in 0.3-10 keV band [ $\rm erg\ s^{-1}$ ].

Source LaTeX | All tables | In the text

	1 Introduction
	2 Observations and data analysis
	3 Results and discussion
	4 Conclusions
	References