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SRG/eROSITA background analysis and simulation
Date
2024-01-01
Author
Perinati, Emanuele
Freyberg, Michael J.
Pommranz, Christian M.
Serim, Muhammed Miraç
Yeung, Michael C. H.
Dennerl, Konrad
Friedrich, Susanne
Tenzer, Chris
Santangelo, Andrea
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Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License
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For about five years SRG/eROSITA is the first X-ray telescope in orbit around the second Lagrangian point L2. We present an updated study of its instrumental background based on cleaned data and improved simulations, carried out in the framework of the eROSITA Background Working Group. We also report some analysis of soft proton contamination, from which we make an estimate of the encountered orbital flux. Finally, we outline some ongoing work about pattern analysis in the case of minimum ionising particle rejection switched off.
URI
https://hdl.handle.net/11511/117647
DOI
https://doi.org/10.1117/12.3018702
Conference Name
Conference on Space Telescopes and Instrumentation - Ultraviolet to Gamma Ray
Collections
Department of Physics, Conference / Seminar
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BibTeX
E. Perinati et al., “SRG/eROSITA background analysis and simulation,” Yokohama, Japonya, 2024, vol. 13093, Accessed: 00, 2025. [Online]. Available: https://hdl.handle.net/11511/117647.
