The Catalogue of Gamma-Ray Burst Observations by HEPD-01 in the 0.3–50 MeV Energy Range

Abstract The High-Energy Particle Detector (HEPD-01) on board the China Seismo-Electromagnetic Satellite, located on a Sun-synchronous orbit at 500 km of altitude with an inclination of 97°, features a dedicated logic counting low-energy event rates, which proved sensitive to intense Gamma-Ray Burst (GRB). The present work reports a comprehensive analysis of signals induced by GRBs in the event-rate data collected between 2018 August and 2022 June. After accurately modeling the background rate as observed in different passages of the satellite over the same geographical area, we detected significant deviations to be compared with observations of GRB candidates from other observatories. The analysis revealed 12 statistically significant excesses, that have been associated with GRB 181222B, GRB 190114C, GRB 190129B, GRB 190305A, GRB 190928A, GRB 200412B, GRB 200422A, GRB 200826B, GRB 201009A, GRB 210702A, GRB 211211A, and GRB 220624A. We report light curves for 0.3–50 MeV photons, comparing them with findings from other space telescopes. The catalog of observations is published, complete of GRB observation time, duration, integrated counts, and fluence.

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Publication Details

Journal
The Astrophysical Journal
Published
2024-11-26
DOI
https://doi.org/10.3847/1538-4357/ad822c
Citations
3
Primary Topic
Gamma-ray bursts and supernovae
Type
article
Field-Weighted Citation Impact
0.99

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The Catalogue of Gamma-Ray Burst Observations by HEPD-01 in the 0.3–50 MeV Energy Range

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The Catalogue of Gamma-Ray Burst Observations by HEPD-01 in the 0.3–50 MeV Energy Range

Simona Zoffoli, G. Osteria, S. Ricciarini, V. Scotti, D. Campana, R. Battiston, A. Oliva, M. Sorbara, Z. Sahnoun, C. Neubüser, F. Perfetto, Alessandro Sotgiu, M. Martucci, A. Contin, Umberto Savino, F. Nozzoli, Alessio Perinelli, Veronica Vilona, Giuseppe Gebbia, Marco Mese, М. Мерге, M. Lolli, M. Ricci, Leonardo Ricci, Riccardo Nicolaidis, P. Cipollone, B. Panico, A. Lega, C. De Santis, C. De Donato, S. Bartocci, R. Sparvoli, P. Zuccon, P. Picozza, P. Ubertini, Francesco Palma, R. Iuppa, S. Beolè, M. Cristoforetti, F. M. Follega, E. Ricci, G. Masciantonio, W. J. Burger, Andrea di Luca
article en
3 citations

Abstract

Abstract The High-Energy Particle Detector (HEPD-01) on board the China Seismo-Electromagnetic Satellite, located on a Sun-synchronous orbit at 500 km of altitude with an inclination of 97°, features a dedicated logic counting low-energy event rates, which proved sensitive to intense Gamma-Ray Burst (GRB). The present work reports a comprehensive analysis of signals induced by GRBs in the event-rate data collected between 2018 August and 2022 June. After accurately modeling the background rate as observed in different passages of the satellite over the same geographical area, we detected significant deviations to be compared with observations of GRB candidates from other observatories. The analysis revealed 12 statistically significant excesses, that have been associated with GRB 181222B, GRB 190114C, GRB 190129B, GRB 190305A, GRB 190928A, GRB 200412B, GRB 200422A, GRB 200826B, GRB 201009A, GRB 210702A, GRB 211211A, and GRB 220624A. We report light curves for 0.3–50 MeV photons, comparing them with findings from other space telescopes. The catalog of observations is published, complete of GRB observation time, duration, integrated counts, and fluence.

The Astrophysical JournalVol. 976(2)
China National Space Administration, Agenzia Spaziale Italiana, China Earthquake Administration, Nuclear Physics
Affordable and clean energy
Openalex Percentile: Top 22%
Gamma-ray bursts and supernovae
0.99
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