Fig. 4.

Left: example of the SIXTE simulated image of an 80 ks ATHENA/WFI observation. Cosmic X-ray background, Galactic foreground, and particle background are included as well as telescope vignetting and PSF degradation with an off-axis angle. The blue circles on the left correspond to the size of r500 of the input groups, which are located at z = 2.0 with M500 = 5 × 1013 M⊙. Right: wavelet image of this SIXTE simulated image. The blue circles represent the detected sources after SEXTRACTOR and the maximum likelihood fitting detection algorithm are run; three sources are undetected by our algorithm.
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