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      The XGIS instrument on-board THESEUS: Monte Carlo simulations for response, background, and sensitivity

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          Abstract

          The response of the X and Gamma Imaging Spectrometer (XGIS) instrument onboard the Transient High Energy Sky and Early Universe Surveyor (THESEUS) mission, selected by ESA for an assessment phase in the framework of the Cosmic Vision M5 launch opportunity, has been extensively modeled with a Monte Carlo Geant-4 based software. In this paper, the expected sources of background in the Low Earth Orbit foreseen for THESEUS are described (e.g. diffuse photon backgrounds, cosmic-ray populations, Earth albedo emission) and the simulated on-board background environment and its effects on the instrumental performance is shown.

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          Author and article information

          Journal
          17 February 2021
          Article
          2102.08699
          da7a5059-3c93-44cf-9b2c-fe6d80f4c867

          http://creativecommons.org/licenses/by-nc-sa/4.0/

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          Custom metadata
          Proceedings of the SPIE 2020, paper 11444-275. arXiv admin note: text overlap with arXiv:2101.03017
          astro-ph.IM

          Instrumentation & Methods for astrophysics
          Instrumentation & Methods for astrophysics

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