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Kaizer, J. Rothe, J. Schieck, J. Zeman, K. Sch\\\"affner, L. Canonica, L. Pattavina, L. Stodolsky, M. Je\\v{s}kovsk\\'y, M. Mancuso, M. Olmi, M. Stahlberg, M. Willers, N. Ferreiro Iachellini, P. Bauer, P. Gorla, P. Povinec, R. Breier, R. Strauss, S. Di Lorenzo, S. Fichtinger, S. Sch\\\"onert, T. Ortmann, V. Mokina, V. Palu\\v{s}ov\\'a, V. Schipperges, V. Zema, W. Potzel","submitted_at":"2019-08-19T15:26:38Z","abstract_excerpt":"The CRESST (Cryogenic Rare Event Search with Superconducting Thermometers) dark matter search experiment aims for the detection of dark matter particles via elastic scattering off nuclei in $\\mathrm{CaWO_4}$ crystals. To understand the CRESST electromagnetic background due to the bulk contamination in the employed materials, a model based on Monte Carlo simulations was developed using the Geant4 simulation toolkit. The results of the simulation are applied to the TUM40 detector module of CRESST-II phase 2. 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