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05 February 2025

» arxiv » astro-ph/0406080

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The Faint X-ray Source Population Near the 3C 295 cluster
V. D’Elia ; F. Fiore ; M. Elvis ; M. Cappi ; S. Mathur ; P. Mazzotta ; E. Falco & F. Cocchia ;
Date:	3 Jun 2004
Subject:	astro-ph
Abstract:	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.
Source:	arXiv, astro-ph/0406080
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