Table 1: Sources detected by the EPIC camera at a signal-to-noise level >3 in the innermost 1 $\hbox {$^\prime $ }$ around the ESO509-IG066 galaxy pair centroid. "E'' and "W'' refer to the components of the AGN pair. Count Rates (CR) refer to the combined MOS cameras in the 0.2-15 keV band. The Error Box (EB) is purely statistics.
Source RA (J2000) Dec (J2000) EB CR

( $\hbox{$^{\prime\prime}$ }$ ) (s^-1)

W 13 $^{\rm h}$ 34 $^{\rm m}$ 39 $.\!\!^{\rm s}$ 7 -23 $^{\circ}$ 26 $\hbox {$^\prime $ }$ 48 $\hbox{$^{\prime\prime}$ }$ 7 $0.658 \pm 0.018$

E 13 $^{\rm h}$ 34 $^{\rm m}$ 40 $.\!\!^{\rm s}$ 8 -23 $^{\circ}$ 26 $\hbox {$^\prime $ }$ 45 $\hbox{$^{\prime\prime}$ }$ 10 $0.512 \pm 0.016$

**Table 1:** Sources detected by the EPIC camera at a signal-to-noise level >3 in the innermost 1 $\hbox {$^\prime $ }$ around the ESO509-IG066 galaxy pair centroid. "E'' and "W'' refer to the components of the AGN pair. Count Rates (CR) refer to the combined MOS cameras in the 0.2-15 keV band. The Error Box (EB) is purely statistics.
Source	RA (J2000)	Dec (J2000)	EB	CR
			( $\hbox{$^{\prime\prime}$ }$ )	(s^-1)
W	13 $^{\rm h}$ 34 $^{\rm m}$ 39 $.\!\!^{\rm s}$ 7	-23 $^{\circ}$ 26 $\hbox {$^\prime $ }$ 48 $\hbox{$^{\prime\prime}$ }$	7	$0.658 \pm 0.018$
E	13 $^{\rm h}$ 34 $^{\rm m}$ 40 $.\!\!^{\rm s}$ 8	-23 $^{\circ}$ 26 $\hbox {$^\prime $ }$ 45 $\hbox{$^{\prime\prime}$ }$	10	$0.512 \pm 0.016$

Source LaTeX | All tables | In the text

	1 Introduction
	2 The data
	3 Discussion
	References