In-orbit performance of the EPIC-MOS detectors on XMM-Newton
Abstract
XMM-Newton was launched into space on a highly eccentric 48 hour orbit on December 10th 1999. XMM-Newton is now in its fifth year of operation and has been an outstanding success, observing the Cosmos with imaging, spectroscopy and timing capabilities in the X-ray and optical wavebands. The EPIC-MOS CCD X-ray detectors comprise two out of three of the focal plane instruments on XMM-Newton. In this paper we discuss key aspects of the current status and performance history of the charge transfer ineffiency (CTI), energy resolution and spectral redistribution function (rmf) of EPIC-MOS in its fifth year of operation.
- Publication:
-
UV and Gamma-Ray Space Telescope Systems
- Pub Date:
- October 2004
- DOI:
- 10.1117/12.553180
- arXiv:
- arXiv:astro-ph/0407347
- Bibcode:
- 2004SPIE.5488..264S
- Keywords:
-
- Astrophysics
- E-Print:
- 8 pages, 10 figures, SPIE Glasgow 21-25 June 2004, Session 5488