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Design and preliminary performance study of the broad-band spectrometer detector for POLAR-2

  • Jian Chao Sun
  • , Jiang He
  • , Shuang Nan Zhang
  • , Shao Lin Xiong
  • , Jiang Tao Liu
  • , Yan Bing Xu
  • , Jia Ma
  • , Shuo Wang
  • , Lei Shuai
  • , Xiu Zuo Liang
  • , Hong Bang Liu
  • , Fei Xie
  • , Ming Zeng
  • , Philipp Azzarello
  • , Jörg Bayer
  • , Franck Cadoux
  • , Nicolas De Angelis
  • , Huan Bo Feng
  • , Zu Ke Feng
  • , Min Gao
  • Ramandeep Gill, Jonathan Granot, Jochen Greiner, Alejandro Guzman, Jin Xiu Hu, Yue Huang, Johannes Hulsman, Zheng Huo Jiang, Merlin Kole, Dao Wu Li, Han Cheng Li, Tong Lei Liao, Long Peng, Agnieszka Pollo, Nicolas Produit, Dominik Rybka, Andrea Santangelo, Li Ming Song, Chris Tenzer, Xiao Ming Wang, Yuan Hao Wang, Bo Bing Wu, Pei Lian Wu, Xin Wu, Shuo Xiao, Sheng Yang, Lai Yu Zhang, Lei Zhang, Yong Jie Zhang

Research output: Contribution to journalArticlepeer-review

Abstract

POLAR-2, the successor of the POLAR experiment aboard China’s Tiangong-2 space lab, is set to be deployed on the China Space Station. The POLAR-2 mission aims to conducting high-precision polarization measurements of high-energy transients with a primary focus on Gamma-Ray Bursts (GRBs), following POLAR’s pioneering accurate polarization measurements of GRB prompt emission. One of the key advancements in POLAR-2 is the inclusion of a dedicated Broad-band Spectrometer Detector (BSD) instrument, designed to provide precise measurements of GRB location and spectral parameters, which are critical inputs for accurate polarization analysis of POLAR-2’s dedicated High-energy Polarimetry Detector (HPD), which is made of plastic scintillator bars array. BSD employs a coded-aperture mask imaging technique and pixelated GAGG scintillation crystals, offering a wide half-coded field of view of and an operational energy range of 10–1000 keV. Simulation results indicate that the instrument can achieve a localization accuracy of approximately for faint GRBs similar to GRB 170817A, satisfying the core requirements of GRB polarimetry with HPD. BSD also has moderate capability for GRB polarimetry, particularly at several hundred keV energy. This paper outlines the preliminary design of BSD and presents an overall evaluation of its expected scientific performance, based on extensive Monte Carlo simulations and preliminary ground-based calibration tests.

Original languageEnglish
Article number9
JournalExperimental Astronomy
Volume61
Issue number2
DOIs
StatePublished - 24 Mar 2026

Bibliographical note

Publisher Copyright:
© The Author(s), under exclusive licence to Springer Nature B.V. 2026.

Keywords

  • Coded-aperture mask imaging
  • Gamma-ray bursts
  • POLAR-2
  • Polarimetry
  • Spectrometer

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