Angular clustering of X-ray point-like sources in the XMM Large Scale Structure Survey

被引：0
作者：
Garcet, O [1 ]
Gandhi, P
Gosset, E
Gueguen, A
Pacaud, F
Pierre, M
Surdej, J
机构：
[1] Univ Liege, Inst Astrophys & Geophys, Liege, Belgium
[2] European So Observ, Santiago 19001, Chile
[3] CEA, DSM, DAPNIA Serv Astronphys, F-91191 Gif Sur Yvette, France
来源：
PROCEEDINGS OF THE X-RAY UNIVERSE 2005, VOLS 1 AND 2 | 2006年 / 604卷
关键词：
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We present the log(N)-log(S) diagram and an angular clustering analysis of point-like X-ray sources for the XMM-Newton Large Scale Structure (XMM-LSS) Survey. Though designed to study the properties and evolution of distant X-ray clusters up to z similar to 1, the large contiguous area planned for the full XMM-LSS survey is ideal for studying X-ray-selected AGN and their clustering properties. Our goal is to test the AGN unified scheme paradigm by studying the clustering of X-ray point-like sources. A clustering analysis of a 4.2 deg(2) contiguous region in the soft ([0.5-2] keV) and hard ([210] keV) energy bands is presented here. The angular correlation function and the nearest neighbour test have been performed in each band. Both tests only reveal a weak clustering in the soft X-ray band.
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页码：617 / +
页数：2
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