Status of the EPIC/MOS calibration onboard XMM-Newton

被引：3

作者：

Ferrando, P ^{[1
]}

Abbey, AF ^{[1
]}

Altieri, B ^{[1
]}

Arnaud, M ^{[1
]}

Bennie, PJ ^{[1
]}

Dadina, M ^{[1
]}

Denby, M ^{[1
]}

Ghizzardi, S ^{[1
]}

Griffiths, RG ^{[1
]}

Kirsch, M ^{[1
]}

La Palombara, N ^{[1
]}

de Luca, A ^{[1
]}

Lumb, D ^{[1
]}

Molendi, S ^{[1
]}

Neumann, D ^{[1
]}

Sauvageot, JL ^{[1
]}

Saxton, RD ^{[1
]}

Sembay, S ^{[1
]}

Tiengo, A ^{[1
]}

Turner, MJL ^{[1
]}

机构：

[1] CEA Saclay, Serv Astrophys, F-91191 Gif Sur Yvette, 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 instrumentation : EPIC/MOS CCDs;

D O I：

10.1117/12.461310

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The XMM-Newton observatory has the largest collecting area flown so far for an X-ray imaging system, resulting in a very high sensitivity over a broad spectral range. In order to exploit fully these performances, an accurate Calibration of the XMM-Newton instruments is required. This calibration is being continuously updated, in order to refine the stable calibration parameters as well as to account, for the detector response changes induced by radiation damage. We report here on the current overall status of the EPIC/MOS cameras calibrations. and in particular on the recent work involving Charge Transfer Inefficiency evolution and recovery.

引用

页码：232 / 242

页数：11

共 22 条

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