3 February 2004 EPIC pn-CCD detector aboard XMM-Newton: status of the background calibration
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We report on the current status of the background calibration of the EPIC pn-CCD camera on board XMM-Newton. The intrinsic background is comprised of internal electronic noise, and continuous and fluorescent X-ray emission induced by high-energy particles. Soft protons passing through the X-ray telescope (and finally also true cosmic X-rays) contribute to the registered events. The camera background has been monitored by using data in closed filter positions for three years; we review the spectral, spatial, and temporal distribution, for all commissioned instrument modes. This paper also discusses briefly the effects on scientific data analysis and conclusions for further observations and detectors.
© (2004) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Michael J. Freyberg, Michael J. Freyberg, Ulrich G. Briel, Ulrich G. Briel, Konrad Dennerl, Konrad Dennerl, Frank Haberl, Frank Haberl, Gisela D. Hartner, Gisela D. Hartner, Elmar Pfeffermann, Elmar Pfeffermann, Eckhard Kendziorra, Eckhard Kendziorra, Marcus G. F. Kirsch, Marcus G. F. Kirsch, David H. Lumb, David H. Lumb, } "EPIC pn-CCD detector aboard XMM-Newton: status of the background calibration", Proc. SPIE 5165, X-Ray and Gamma-Ray Instrumentation for Astronomy XIII, (3 February 2004); doi: 10.1117/12.506277; https://doi.org/10.1117/12.506277


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