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|Title: ||The European Photon Imaging Camera on XMM-Newton: the MOS cameras|
|Authors: ||Turner, Martin J. L.|
Cole, Richard E.
Di Coco, G.
Holland, Andrew D.
La Palombara, N.
Pounds, Kenneth A.
|Issue Date: ||2001|
|Publisher: ||EDP Sciences|
|Citation: ||Astronomy and Astrophysics, 2001, 365, L27-L35|
|Abstract: ||The EPIC focal plane imaging spectrometers on XMM-Newton use CCDs to record the images and spectra of celestial X-ray sources focused by the three X-ray mirrors. There is one camera at the focus of each mirror; two of the cameras contain seven MOS CCDs, while the third uses twelve PN CCDs, defining a circular field of view of 30' diameter in each case. The CCDs were specially developed for EPIC, and combine high quality imaging with spectral resolution close to the Fano limit. A filter wheel carrying three kinds of X-ray transparent light blocking filter, a fully closed, and a fully open position, is fitted to each EPIC instrument. The CCDs
are cooled passively and are under full closed loop thermal control. A radio-active source is fitted for internal calibration. Data are processed on-board to save telemetry by removing cosmic ray tracks, and generating X-ray event files; a variety of different instrument modes are available to increase the dynamic range of the instrument and to enable fast timing. The instruments were calibrated using laboratory X-ray beams, and synchrotron generated
monochromatic X-ray beams before launch; in-orbit calibration makes use of a variety of celestial X-ray targets. The current calibration is better than 10% over the entire energy range of 0.2 to 10 keV. All three instruments survived launch and are performing nominally in orbit. In particular full field-of-view coverage is available, all
electronic modes work, and the energy resolution is close to pre-launch values. Radiation damage is well within pre-launch predictions and does not yet impact on the energy resolution. The scientific results from EPIC amply fulfil pre-launch expectations.|
|DOI Link: ||10.1051/0004-6361:20000087|
|Version: ||Publisher PDF|
|Rights: ||© The European Southern Observatory (ESO) 2001. Deposited with permission of the publisher.|
|Appears in Collections:||Published Articles, Dept. of Physics and Astronomy|
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