MARELLI, MARTINOMARTINOMARELLISalvetti, DavidDavidSalvettiGASTALDELLO, FABIOFABIOGASTALDELLOGHIZZARDI, SIMONASIMONAGHIZZARDIMOLENDI, SILVANOSILVANOMOLENDIDE LUCA, AndreaAndreaDE LUCAMORETTI, AlbertoAlbertoMORETTIROSSETTI, MARIACHIARAMARIACHIARAROSSETTITIENGO, ANDREAANDREATIENGO2020-09-032020-09-0320170922-6435http://hdl.handle.net/20.500.12386/27100XMM-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 ∼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.ELETTRONICOenArticle10.1007/s10686-017-9542-52-s2.0-85020539354000419984100005https://link.springer.com/article/10.1007%2Fs10686-017-9542-52017ExA....44..297MFIS/05 - ASTRONOMIA E ASTROFISICAScienze Fisiche Settori ERC (ERC) di riferimento::PE9 Universe sciences: astro-physics/chemistry/biology; solar systems; stellar, galactic and extragalactic astronomy, planetary systems, cosmology, space science, instrumentation