Properties of the background of EPIC-pn onboard XMM-Newton

被引:53
作者
Katayama, H
Takahashi, I
Ikebe, Y
Matsushita, K
Freyberg, MJ
机构
[1] Max Planck Inst Extraterr Phys, D-85741 Garching, Germany
[2] Osaka Univ, Dept Earth & Space Sci, Grad Sch Sci, Toyonaka, Osaka 5600043, Japan
[3] Univ Tokyo, Dept Phys, Bunkyo Ku, Tokyo 1130033, Japan
来源
ASTRONOMY & ASTROPHYSICS | 2004年 / 414卷 / 02期
关键词
X-rays : general; instrumentation : detectors;
D O I
10.1051/0004-6361:20031687
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We have investigated the background properties of EPIC-pn onboard XMM-Newton to establish the background subtraction method. Count rates of the background vary violently by two orders of magnitude at the maximum, while during the most quiet period, these are stable within 8% at a 1sigma level. The overall spectrum is dominated by particle events above 5 keV, and its spatial variation is also found. The long-term variation of the background is also investigated with CAL CLOSED data, where the filter wheel was in closed position with the internal calibration source illuminating the sensitive area. The average background count rate decreased by 20% from March 2000 to January 2001, but it regained in February 2001. For the modeling of the background spectrum, we investigate relations between the 2.0-7.0 keV count rate and some characteristic parameters. The 2.0-7.0 keV background count rate shows a good correlation with the count rate of events outside the field of view. This correlation is usable for the modeling of the background.
引用
收藏
页码:767 / 776
页数:10
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