The X and Gamma-Ray Imager and Spectrometer Onboard THESEUS—Status and Technological Progresses

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Authors: Giulia Mattioli, C. Labanti, Enrico Virgilli, L. Amati, G. Bertuccio, R. Campana, G. Baldazzi, Smiriti Srivastava, Edoardo Borciani, Paolo Calabretto, Marco Grassi, P. Malcovati
+10 more E. J. Marchesini, Filippo Mele, Ajay Sharma, Evgeny Demenev, F. Ficorella, David Novel, G. Pepponi, G. La Rosa, Paolo Nogara, Giuseppe Sottile
Cited by: 2
References: 20

Abstract

Gamma-Ray Bursts (GRBs) are intense bursts of high-energy photons which, in just a few seconds, outshine all other γ-ray emitters in the sky. Due to their extreme luminosity, GRBs are not only important as high-energy astrophysical phenomena but also serve as valuable probe models of the far, high-redshift Universe. The importance of these events has pushed the High-Energy Astrophysics community to propose new mission concepts over the past decade, prompting dedicated research and development efforts to achieve the required technological readiness levels. The X and Gamma-Ray Imager and Spectrometer (XGIS) is one of the two GRB monitors onboard the proposed, upcoming THESEUS space mission. Building on strong heritage from previous studies, ongoing developments and optimizations are focused on enhancing the instrument’s capabilities and increasing its technological maturity. This work presents the current status of the XGIS instrument and the latest technological advancements achieved in preparation for its deployment on THESEUS.

Fields of Study & Subjects

Gamma-ray bursts and supernovae CCD and CMOS Imaging Sensors Particle Detector Development and Performance

Publication details

Journal / source
Particles
Publisher
MDPI AG
Volume
9
Issue
1
Pages
3–3
Publication date
8 January 2026
Language
EN