2024ApJ...960...21P

Query : 2024ApJ...960...21P

2024ApJ...960...21P - Astrophys. J., 960, 21 (2024/January-1)

Gamma-Ray Burst Observations by the High-Energy Particle Detector on board the China Seismo-Electromagnetic Satellite between 2019 and 2021.

PALMA F., MARTUCCI M., NEUBUSER C., SOTGIU A., FOLLEGA F.M., UBERTINI P., BAZZANO A., RODI J.C., AMMENDOLA R., BADONI D., BARTOCCI S., BATTISTON R., BEOLE S., BERTELLO I., BURGER W.J., CAMPANA D., CICONE A., CIPOLLONE P., COLI S., CONTI L., CONTIN A., CRISTOFORETTI M., D'ANGELO G., DE ANGELIS F., DE DONATO C., DE SANTIS C., DIEGO P., DI LUCA A., FIORENZA E., GEBBIA G., IUPPA R., LEGA A., LOLLI M., MARTINO B., MASCIANTONIO G., MERGE M., MESE M., MORBIDINI A., NOZZOLI F., NUCCILLI F., OLIVA A., OSTERIA G., PALMONARI F., PANICO B., PAPINI E., PARMENTIER A., PERCIBALLI S., PERFETTO F., PERINELLI A., PICOZZA P., PIERSANTI M., POZZATO M., REBUSTINI G., RECCHIUTI D., RICCI E., RICCI M., RICCIARINI S.B., RUSSI A., SAHNOUN Z., SAVINO U., SCOTTI V., SHEN X., SPARVOLI R., TOFANI S., VERTOLLI N., VILONA V., VITALE V., ZANNONI U., ZEREN Z., ZOFFOLI S. and ZUCCON P.

Abstract (from CDS):

In this paper we report the detection of five strong gamma-ray bursts (GRBs) by the High-Energy Particle Detector (HEPD-01) mounted on board the China Seismo-Electromagnetic Satellite, operational since 2018 on a Sun-synchronous polar orbit at a ∼507 km altitude and 97° inclination. HEPD-01 was designed to detect high-energy electrons in the energy range 3-100 MeV, protons in the range 30-300 MeV, and light nuclei in the range 30-300 MeV n–1. Nonetheless, Monte Carlo simulations have shown HEPD-01 is sensitive to gamma-ray photons in the energy range 300 keV-50 MeV, even if with a moderate effective area above ∼5 MeV. A dedicated time correlation analysis between GRBs reported in literature and signals from a set of HEPD-01 trigger configuration masks has confirmed the anticipated detector sensitivity to high-energy photons. A comparison between the simultaneous time profiles of HEPD-01 electron fluxes and photons from GRB190114C, GRB190305A, GRB190928A, GRB200826B, and GRB211211A has shown a remarkable similarity, in spite of the different energy ranges. The high-energy response, with peak sensitivity at about 2 MeV, and moderate effective area of the detector in the actual flight configuration explain why these five GRBs, characterized by a fluence above ∼3 × 10–5 erg cm–2 in the energy interval 300 keV-50 MeV, have been detected.

Abstract Copyright: © 2023. The Author(s). Published by the American Astronomical Society.

Journal keyword(s): Cosmic ray detectors - Gamma-ray bursts - Particle astrophysics

Simbad objects: 8

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Number of rows : 8
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026 		#notes
1 GRB 190305A gB 00 46 30.36 -50 20 55.7           ~ 13 0
2 GRB 190114C gB 03 38 01.18 -26 56 47.8           ~ 343 0
3 SN 2019jrj SN* 03 38 01.190 -26 56 46.77           ~ 10 0
4 GrW 170817 GWE 13 09 48.0850 -23 22 53.343           ~ 2683 0
5 SDSS J140910.47+275320.8 G 14 09 10.47535 +27 53 20.8393           ~ 279 0
6 GRB 221009A gB 19 13 03.85 +19 46 22.7           ~ 433 0
7 GRB 200826B gB ~ ~           ~ 7 0
8 GRB 190928A gB ~ ~           ~ 16 0

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