XMM Users' Handbook


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X-ray point-spread function

The first critical parameter determining the quality of an X-ray mirror module is its ability to focus photons. Here lies one of XMM's major strong points: the core of its on-axis point-spread function (PSF) is narrow and varies little over a very wide energy range (0.1-10 keV).



 

European Space Agency - XMM Science Operations Centre