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arxiv: 1705.04171 · v1 · pith:4WVJYIL7new · submitted 2017-05-11 · 🌌 astro-ph.HE · astro-ph.IM

A Systematic Analysis of the XMM-Newton Background: I. Dataset and Extraction Procedures

classification 🌌 astro-ph.HE astro-ph.IM
keywords backgroundxmm-newtonanalysisathenacomponentsdifferentmissionparticle-induced
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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.

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