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

被引:4
|
作者
Palma, F. [1 ]
Martucci, M. [1 ]
Neubuser, C. [2 ]
Sotgiu, A. [1 ]
Follega, F. M. [2 ,3 ]
Ubertini, P. [4 ]
Bazzano, A. [4 ]
Rodi, J. C. [4 ]
Ammendola, R. [1 ]
Badoni, D. [1 ]
Bartocci, S. [1 ]
Battiston, R. [2 ,3 ]
Beole, S. [5 ,6 ]
Bertello, I. [4 ]
Burger, W. J. [2 ]
Campana, D. [7 ]
Cicone, A. [8 ]
Cipollone, P. [1 ]
Coli, S. [6 ]
Conti, L. [1 ,9 ]
Contin, A. [10 ,11 ]
Cristoforetti, M. [2 ,12 ]
D'Angelo, G. [4 ]
De Angelis, F. [4 ]
De Donato, C. [1 ]
De Santis, C. [1 ]
Diego, P. [4 ]
Di Luca, A. [2 ,12 ]
Fiorenza, E. [4 ]
Gebbia, G. [2 ,3 ]
Iuppa, R. [2 ,3 ]
Lega, A. [2 ,3 ]
Lolli, M. [11 ]
Martino, B. [13 ]
Masciantonio, G. [1 ]
Merge, M. [1 ,14 ]
Mese, M. [7 ,15 ]
Morbidini, A. [4 ]
Nozzoli, F. [2 ]
Nuccilli, F. [4 ]
Oliva, A. [11 ]
Osteria, G. [7 ]
Palmonari, F. [10 ,11 ]
Panico, B. [7 ,15 ]
Papini, E. [4 ]
Parmentier, A. [4 ]
Perciballi, S. [5 ,6 ]
Perfetto, F. [7 ]
Perinelli, A. [2 ,3 ]
Picozza, P. [1 ,16 ]
机构
[1] Ist Nazl Fis Nucl, Sez Roma Tor Vergata, Via Ric Sci 1, I-00133 Rome, Italy
[2] Ist Nazl Fis Nucl, TIFPA, Via Sommar 14, I-38123 Povo, Trento, Italy
[3] Univ Trento, Via Sommar 14, I-38123 Povo, Trento, Italy
[4] INAF IAPS, Via Fosso Cavaliere 100, I-00133 Rome, Italy
[5] Univ Torino, Via P Giuria 1, I-10125 Turin, Italy
[6] Ist Nazl Fis Nucl, Sez Torino, Via P Giuria 1, I-10125 Turin, Italy
[7] Ist Nazl Fis Nucl, Sez Napoli, Via Cintia, I-80126 Naples, Italy
[8] Univ Aquila, Via Vetoio, I-67100 Laquila, Italy
[9] Uninettuno Univ, Corso V Emanuele II 39, I-00186 Rome, Italy
[10] Univ Bologna, Viale Berti Pichat 6-2, Bologna, Italy
[11] Ist Nazl Fis Nucl, Sez Bologna, Viale Berti Pichat 6-2, Bologna, Italy
[12] Fdn Bruno Kessler, Via Sommar 18, I-38123 Povo, Trento, Italy
[13] CNR, Via Fosso Cavaliere 100, I-00133 Rome, Italy
[14] Italian Space Agcy, Via Politecn, I-00133 Rome, Italy
[15] Univ Napoli Federico II, Via Cintia, I-80126 Naples, Italy
[16] Univ Roma Tor Vergata, Via Ric Sci 1, I-00133 Rome, Italy
[17] Ist Nazl Fis Nucl, LNF, VE Fermi 54, I-00044 Rome, Italy
[18] CNR, IFAC, Via Madonna del Piano 10, I-50019 Florence, Italy
[19] Chinese Acad Sci, Natl Space Sci Ctr, Beijing 100190, Peoples R China
[20] Minist Emergency Management China, Natl Inst Nat Hazards, Beijing 100085, Peoples R China
来源
ASTROPHYSICAL JOURNAL | 2024年 / 960卷 / 01期
关键词
CSES-01; SATELLITE; GRB; 190114C; GIANT FLARE; ERROR BOX; EMISSION; PROMPT; IDENTIFICATION; SUPERNOVA; SPECTRA; PROTONS;
D O I
10.3847/1538-4357/ad06ae
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
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 similar to 507 km altitude and 97 degrees 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 similar to 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 similar to 3 x 10(-5) erg cm(-2) in the energy interval 300 keV-50 MeV, have been detected.
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页数:8
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