The Faint X-ray Source Population Near the 3C 295 cluster

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dc.creatorD'Elia, V.
dc.creatorFiore, F.
dc.creatorElvis, M.
dc.creatorCappi, M.
dc.creatorMathur, S.
dc.creatorMazzotta, P.
dc.creatorFalco, E.
dc.creatorCocchia, F.
dc.date2004-06-03
dc.date.accessioned2026-07-07T02:13:25Z
dc.date.available2026-07-07T02:13:25Z
dc.descriptionWe 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.
dc.descriptionProceeding of the workshop "Outskirts of Galaxy Clusters: intense life in the suburbs" Turin, March 12-16, 2004; 3 pages, 6 .ps figures
dc.identifierhttps://arxiv.org/abs/astro-ph/0406080
dc.identifierhttp://arxiv.org/abs/astro-ph/0406080
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/7805
dc.subjectAstrophysics
dc.titleThe Faint X-ray Source Population Near the 3C 295 cluster
dc.typetext

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