Fig. 2
XMM-Newton/EPIC pn 0.5–2 keV and 2–7 keV images (first and second panels), XMM-Newton/OM UVW2 (2120 Å) images for the galaxies observed with this filter (third panel). The third panel of Arp299 and MCG+04-48-002 corresponds to the XMM-Newton/OM UVM2 (2310 Å) filter. Spitzer/IRAC 3.6 μm images (forth panel). For reference we represent in the third and forth panels the smoothed 0.5–7 keV contours. The white line in the right panels represents 5 kpc at the distance of the galaxy. All images are shown in a square root scale. North is up and east is to the left.
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