X-Ray Sources Overdensity Around 3C 295

Details X-Ray Sources Overdensity Around 3C 295 X-Ray Sources Overdensity Around 3C 295

2003-10-17

arxiv.org/abs/astro-ph/0310506v1

Astronomy and Astrophysics

Astrophysics

2 pages, 4 postscript figures; to appear in the proceedings of the "Multiwavelength Cosmology" workshop, Mykonos, Greece, 2003

Scientific paper

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.

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