All Tables

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.
Table 2: Best-fit parameters and results for the EPIC spectra of the ESO509-IG066 Galaxy Pair members. $f_{\rm s}$ is the scattering fraction ( $1-f_{\rm s}$ is the absorber covering fraction in the "leaky absorber'' scenario). F is the observed flux in the 0.5-2/2-10 keV energy bands. L is the absorption-corrected luminosity in the 0.5-10 keV energy band.