UV and Gamma-Ray Space Telescope Systems 2004
DOI: 10.1117/12.553180
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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. XMMNewton 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),… Show more

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Cited by 11 publications
(7 citation statements)
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“…An anomaly in the MOS2 spectral data below ∼ 0.8 keV, which probably is related to the MOS redistribution problem in which events from higher energies incorrectly are redistributed downwards (cf. Sembay et al 2004), required exclusion of those MOS2 spectral bins from the analysis.…”
Section: Psr B1929+10mentioning
confidence: 99%
“…An anomaly in the MOS2 spectral data below ∼ 0.8 keV, which probably is related to the MOS redistribution problem in which events from higher energies incorrectly are redistributed downwards (cf. Sembay et al 2004), required exclusion of those MOS2 spectral bins from the analysis.…”
Section: Psr B1929+10mentioning
confidence: 99%
“…The temperature dependence of the CTI of the damaged CCDs varies device to device [15,16]. Therefore, the understating of the temperature dependence allows us a flexible operation in space where the power available is quite limited.…”
Section: Discussionmentioning
confidence: 99%
“…Lowering operating temperature of CCDs also reduced the CTI in the case of the Chandra and XMM-Newton CCDs [15,16].…”
Section: Introductionmentioning
confidence: 96%
“…Therefore, the charge transfer inefficiency (CTI), the fraction of charge loss per transfer, is an important measure in evaluating CCDs. In addition to trap populations and densities, the CTI generally depends on several operation parameters: transfer time [3], operating temperature [4,5,6], amount of transfer charge [7,8,9], and the existence of "sacrificial charge" [10,11,12,13,14,15]. In the case of a photoncounting X-ray CCD, which serves as a spectrometer as well as an imager, the charge loss during transfer results in misidentification of an incident photon energy.…”
Section: Introductionmentioning
confidence: 99%