- Table 1:
Sources detected by the EPIC camera at a signal-to-noise
level >3 in the innermost 1
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
- Table 2:
Best-fit parameters and results for the EPIC
spectra of the ESO509-IG066 Galaxy Pair members.
scattering fraction (
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.