  We present a statistical analysis of the Chandra observation of the source
field around the 3C 295 galaxy cluster ($z=0.46$). Three different methods of
analysis, namely a chip by chip logN-logS, a two dimentional Kolmogorov-Smirnov
(KS) test, and the angular correlation function (ACF) show a strong overdensity
of sources in the North-East of the field, that may indicate a filament of the
large scale structure of the Universe toward 3C 295.
