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

来源：

ASTRONOMY & ASTROPHYSICS | 2024年 / 684卷

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

页数：8

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