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18 August 2005 EPIC-pn CCD camera onboard XMM-Newton: an update of the calibration
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Abstract
The X-ray observatory XMM-Newton is now in orbit for more than 5 years. The performance of the EPIC-pn CCD camera has been monitored since and its calibration has been improved steadily. We report in this presentation on our recent investigations in different calibration issues: Data of the on-board Fe-55 calibration source were used for monitoring the charge transfer efficiency (CTE) degradation. A special calibration observation of the line-rich supernova remnant Cas-A in the extended Full Frame Mode was used to refine the energy calibration in this mode. Together with ground measurements, a non-routine observation of the calibration target N132D will lead to an improvement of the CTE correction of the Large Window Mode.
© (2005) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
U. G. Briel, V. Burwitz, K. Dennerl, M. J. Freyberg, U. Geppert, F. Haberl, M. P. Esquej, and M. G. F. Kirsch "EPIC-pn CCD camera onboard XMM-Newton: an update of the calibration", Proc. SPIE 5898, UV, X-Ray, and Gamma-Ray Space Instrumentation for Astronomy XIV, 58980P (18 August 2005); https://doi.org/10.1117/12.616824
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