INTEGRAL view of GRB 221009A

被引:0
|
作者
Savchenko, Volodymyr [1 ,2 ]
Ubertini, Pietro [3 ]
Bazzano, Angela [3 ]
Rodi, James Craig [3 ]
Jourdain, Elisabeth [4 ]
Roques, Jean-Pierre [4 ]
Martin-Carrillo, Antonio [8 ]
Hanlon, Lorraine [8 ]
Mereghetti, Sandro [5 ]
Tiengo, Andrea [5 ,6 ]
Laurent, Philippe [7 ]
Gotz, Diego [7 ]
Ferrigno, Carlo [1 ]
Kuulkers, Erik [9 ]
机构
[1] Univ Geneva, Dept Astron, Chemin Ecogia 16, CH-1290 Versoix, Switzerland
[2] Ecole Polytech Fed Lausanne, Lausanne, Switzerland
[3] Natl Inst Astrophys, IAPS, I-00133 Rome, Italy
[4] IRAP, Toulouse, France
[5] Ist Nazl Astrofis, Ist Astrofis Spaziale & Fis Cosm Milano, Via A Corti 12, I-20133 Milan, Italy
[6] Scuola Univ Super IUSS Pavia, Piazza Vittoria 15, I-27100 Pavia, Italy
[7] Univ Paris Saclay, Univ Paris Cite, CEA, CNRS,AIM, F-91191 Gif Sur Yvette, France
[8] Univ Coll Dublin, Sch Phys, Dublin, Ireland
[9] European Space Res & Technol Ctr ESTEC, European Space Agcy ESA, Keplerlaan 1, NL-2201 AZ Noordwijk, Netherlands
关键词
gamma rays: general; X-rays: bursts; GAMMA-RAY BURST; JEM-X; GRAVITATIONAL-WAVES; PROMPT EMISSION; AFTERGLOW; COMPONENT; IBIS; SPI; SPECTROMETER; GRB-990123;
D O I
10.1051/0004-6361/202346336
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The gamma-ray burst GRB 221009A is among the most luminous of its kind and its proximity to Earth has made it an exceptionally rare observational event. The International Gamma-ray Astrophysics Laboratory (INTEGRAL) was in an optimal aspect position to use its all-sky instruments for recording the prompt emission and early gamma-ray afterglow in unprecedented detail. Following the initial detection, a swiftly scheduled follow-up observation allowed for the hard X-ray afterglow time and spectral evolution to be observed for up to almost a week. The INTEGRAL hard X-ray and soft gamma-ray observations have started to bridge the energy gap between the traditionally well-studied soft X-ray afterglow and the high-energy afterglow observed by Fermi/LAT. We discuss the possible implications of these observations for follow-ups of multi-messenger transients with hard X-ray and gamma-ray telescopes.
引用
收藏
页数:8
相关论文
共 50 条
  • [31] Model Constraints Based on the IceCube Neutrino Nondetection of GRB 221009A
    Ai, Shunke
    Gao, He
    ASTROPHYSICAL JOURNAL, 2023, 944 (02):
  • [32] GRB 221009A, Its Precursor, and Two Afterglows in the Fermi Data
    Stern, B.
    Tkachev, I.
    JETP LETTERS, 2023, 118 (08) : 553 - 559
  • [33] Naked Forward Shock Seen in the TeV Afterglow Data of GRB 221009A
    Khangulyan, Dmitry
    Aharonian, Felix
    Taylor, Andrew M.
    ASTROPHYSICAL JOURNAL, 2024, 966 (01):
  • [34] Constraints on Lorentz invariance violation from the LHAASO observation of GRB 221009A
    Yang, Yu -Ming
    Bi, Xiao-Jun
    Yin, Peng-Fei
    JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS, 2024, (04):
  • [35] Constraining the Jet Composition of GRB 221009A with the Prompt TeV Emission Limit
    Dai, Cui-Yuan
    Wang, Xiang-Yu
    Liu, Ruo-Yu
    Zhang, Bing
    ASTROPHYSICAL JOURNAL LETTERS, 2023, 957 (02)
  • [36] Implication from GRB 221009A: Can TeV emission come from the GRB prompt phase?
    Kai Wang
    Zhi-Peng Ma
    Ruo-Yu Liu
    Yuan-Chuan Zou
    Zhuo Li
    Zi-Gao Dai
    Science China Physics, Mechanics & Astronomy, 2023, 66
  • [37] Observability of the Very-High-Energy Emission from GRB 221009A
    Galanti, Giorgio
    Nava, Lara
    Roncadelli, Marco
    Tavecchio, Fabrizio
    Bonnoli, Giacomo
    PHYSICAL REVIEW LETTERS, 2023, 131 (25)
  • [38] GRB 221009A Gamma Rays from the Radiative Decay of Heavy Neutrinos?
    Smirnov, Alexei Y.
    Trautner, Andreas
    PHYSICAL REVIEW LETTERS, 2023, 131 (02)
  • [39] Implication of Jet Physics from MeV Line Emission of GRB 221009A
    Zhang, Zhen
    Lin, Haoxiang
    Li, Zhuo
    Xiong, Shao-Lin
    Zhang, Yan-Qiu
    Zhang, Qinyuan
    Yi, Shu-Xu
    Wang, Xilu
    ASTROPHYSICAL JOURNAL LETTERS, 2024, 973 (01)
  • [40] Expansion and Spectral Softening of the Dust-scattering Rings of GRB 221009A
    Zhao, Guoying
    Shen, Rong-Feng
    ASTROPHYSICAL JOURNAL, 2024, 970 (02):