Data analysis methods for XMM-Newton observations of extended sources.: Application to bright massive clusters of galaxies at z=0.2

被引：21

作者：

Marty, PB ^{[1
]}

Kneib, JP ^{[1
]}

Sadat, R ^{[1
]}

Ebeling, H ^{[1
]}

Smail, I ^{[1
]}

机构：

[1] IAS, F-91405 Orsay, France

来源：

X-RAY AND GAMMA-RAY TELESCOPES AND INSTRUMENTS FOR ASTRONOMY, PTS 1 AND 2 | 2003年 / 4851卷

关键词：

missions : XMM-Newton; X-rays : general; techniques : spectro-imaging; galaxies : clusters : individual : Abell 209; cosmology : observations;

D O I：

10.1117/12.461330

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

In this paper, a review is given of methods useful for XMM-Newton EPIC data analysis of extended sources, along with some applications to a bright massive cluster of galaxies at z = 0.2. Abell 209. This may constitute an introduction to that kind of advanced analysis, complementing cookbooks that can be found over the internet, the XMM-Newton, EPIC calibration status document,(13) and the data analysis workshops organised in VILSPA, which were only dedicated so far to point sources analysis. In addition, new spectro-imaging techniques are proposed, in order to measure for instance the intracluster medium mass and temperature profiles, or even maps.

引用

页码：208 / 222

页数：15

共 31 条

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