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We present an accurate characterization of the particle background behaviouron XMM-Newton based on the entire EPIC archive. This corresponds to the largestEPIC data set ever examined. Our results have been obtained thanks to thecollaboration between the FP7 European program EXTraS and the ESA R&D ATHENAactivity AREMBES. We used as a diagnostic an improved version of the diagnosticwhich compares the data collected in unexposed region of the detector with theregion of the field of view in the EPIC-MOS. We will show that the inField-of-View excess background is made up of two different components, oneassociated to flares produced by soft protons and the other one to alow-intensity background. Its origin needs to be further investigated.

A Systematic Analysis of the XMM-Newton Background: II. Properties of the in-Field-Of-View Excess Component