Abstract
The performance of the three X-ray telescopes on-board of XMM-Newton is evaluated addressing imaging characteristics and effective collecting area. The agreement with ground calibration data is excellent. The analysis of images and spectra of cosmic X-ray sources, emphazising supernova and supernova remnants, prooves that the telescopes are even better than originally required.
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CITATION STYLE
Aschenbach, B. (2002). In-orbit performance of the XMM-Newton x-ray telescopes: images and spectra. In X-Ray Optics for Astronomy: Telescopes, Multilayers, Spectrometers, and Missions (Vol. 4496, p. 8). SPIE. https://doi.org/10.1117/12.454367
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