http://arxiv.org/abs/1705.04171
XMM-Newton is the direct precursor of the future ESA ATHENA mission. A study of its particle-induced background provides therefore significant insight for the ATHENA mission design. We make use of about 12 years of data, products from the third XMM-Newton catalog as well as FP7 EXTraS project to avoid celestial sources contamination and to disentangle the different components of the XMM-Newton particle-induced background. Within the ESA R&D AREMBES collaboration, we built new analysis pipelines to study the different components of this background: this covers time behavior as well as spectral and spatial characteristics.
M. Marelli, D. Salvetti, F. Gastaldello, et. al.
Fri, 12 May 17
17/55
Comments: To appear in Experimental Astronomy, presented at AHEAD Background Workshop, 28-30 November 2016, Rome, Italy. 12 pages, 6 figures
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