Paper
13 December 2000 In-orbit calibration of the XMM-Newton telescopes
Philippe Gondoin, Bernd Aschenbach, Christian Erd, David H. Lumb, S. Majerowicz, Doris Neumann, Jean Luc Sauvageot
Author Affiliations +
Abstract
The High Throughput X-ray Spectroscopy Mission XMM-Newton of the European Space Agency (ESA) was launched on December 10, 1999 by an Ariane V rocket. The satellite observatory uses three grazing incidence telescopes coupled to reflection grating spectrometers and x-ray CCD cameras. Each x-ray telescope consists of 58 Wolter I mirrors which are nested in a coaxial and cofocal configuration. The XMM-Newton Science Operation Center has completed a coherent program for the in- orbit calibration and performance verification of the x-ray observatory. This paper presents first measurement results of the x-ray telescopes image quality and effective area obtained during this campaign.
© (2000) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Philippe Gondoin, Bernd Aschenbach, Christian Erd, David H. Lumb, S. Majerowicz, Doris Neumann, and Jean Luc Sauvageot "In-orbit calibration of the XMM-Newton telescopes", Proc. SPIE 4140, X-Ray and Gamma-Ray Instrumentation for Astronomy XI, (13 December 2000); https://doi.org/10.1117/12.409103
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Cited by 29 scholarly publications.
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KEYWORDS
Telescopes

X-ray telescopes

Calibration

Point spread functions

Mirrors

X-rays

Space telescopes

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