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GRB 130427A: a nearby ordinary monster.

Maselli, A; Melandri, A; Nava, L; Mundell, CG; Kawai, N; Campana, S; Covino, S; ... Tagliaferri, G; + view all (2014) GRB 130427A: a nearby ordinary monster. Science , 343 (6166) pp. 48-51. 10.1126/science.1242279. Green open access

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Abstract

Long-duration gamma-ray bursts (GRBs) are an extremely rare outcome of the collapse of massive stars and are typically found in the distant universe. Because of its intrinsic luminosity (L ~ 3 × 10(53) ergs per second) and its relative proximity (z = 0.34), GRB 130427A reached the highest fluence observed in the γ-ray band. Here, we present a comprehensive multiwavelength view of GRB 130427A with Swift, the 2-meter Liverpool and Faulkes telescopes, and by other ground-based facilities, highlighting the evolution of the burst emission from the prompt to the afterglow phase. The properties of GRB 130427A are similar to those of the most luminous, high-redshift GRBs, suggesting that a common central engine is responsible for producing GRBs in both the contemporary and the early universe and over the full range of GRB isotropic energies.

Type: Article
Title: GRB 130427A: a nearby ordinary monster.
Location: United States
Open access status: An open access version is available from UCL Discovery
DOI: 10.1126/science.1242279
Publisher version: http://dx.doi.org/10.1126/science.1242279
Language: English
Additional information: © 2014 American Association for the Advancement of Science. All Rights Reserved.
UCL classification: UCL
UCL > Provost and Vice Provost Offices > UCL BEAMS
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Space and Climate Physics
URI: https://discovery.ucl.ac.uk/id/eprint/1420678
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