Pradas & Kerp study the effects of proton flares on XMM EPIC MOS and PN detectors. The find an unreported soft (<0.5 keV) additional background in MOS1.
Hicks & Mushotzky analyze XMM OM data from a sample of 33 galaxies and find a significant UV excess in many central galaxies in cooling flow clusters.
Chluba & Sunyaev point out that induced emission of the softer photon slightly increases the two-photon decay rate of the 2s level of hydrogen. This is important for calculations of cosmological reionization and changes CMB temperature and polarization anisotropies.
Hilton et al. cross-correlate the 2dFGRS and REFLEX.
Gallo et al. find a possible line-like emission feature at 8 keV in an XMM spectrum of a Sy 1.2.
Kirsch et al. give the results of XMM observations of the Crab and discuss its use as an X-ray calibrator.
Kirsch et al. present trend data for the XMM EPIC detectors.
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