The Astrophysical Journal Letters (Jan 2023)

GRB 221009A: Discovery of an Exceptionally Rare Nearby and Energetic Gamma-Ray Burst

  • Maia A. Williams,
  • Jamie A. Kennea,
  • S. Dichiara,
  • Kohei Kobayashi,
  • Wataru B. Iwakiri,
  • Andrew P. Beardmore,
  • P. A. Evans,
  • Sebastian Heinz,
  • Amy Lien,
  • S. R. Oates,
  • Hitoshi Negoro,
  • S. Bradley Cenko,
  • Douglas J. K. Buisson,
  • Dieter H. Hartmann,
  • Gaurava K. Jaisawal,
  • N. P. M. Kuin,
  • Stephen Lesage,
  • Kim L. Page,
  • Tyler Parsotan,
  • Dheeraj R. Pasham,
  • B. Sbarufatti,
  • Michael H. Siegel,
  • Satoshi Sugita,
  • George Younes,
  • Elena Ambrosi,
  • Zaven Arzoumanian,
  • M. G. Bernardini,
  • S. Campana,
  • Milvia Capalbi,
  • Regina Caputo,
  • Antonino D’Aì,
  • P. D’Avanzo,
  • V. D’Elia,
  • Massimiliano De Pasquale,
  • R. A. J. Eyles-Ferris,
  • Elizabeth Ferrara,
  • Keith C. Gendreau,
  • Jeffrey D. Gropp,
  • Nobuyuki Kawai,
  • Noel Klingler,
  • Sibasish Laha,
  • A. Melandri,
  • Tatehiro Mihara,
  • Michael Moss,
  • Paul O’Brien,
  • Julian P. Osborne,
  • David M. Palmer,
  • Matteo Perri,
  • Motoko Serino,
  • E. Sonbas,
  • Michael Stamatikos,
  • Rhaana Starling,
  • G. Tagliaferri,
  • Aaron Tohuvavohu,
  • Silvia Zane,
  • Houri Ziaeepour

DOI
https://doi.org/10.3847/2041-8213/acbcd1
Journal volume & issue
Vol. 946, no. 1
p. L24

Abstract

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We report the discovery of the unusually bright long-duration gamma-ray burst (GRB), GRB 221009A, as observed by the Neil Gehrels Swift Observatory (Swift), Monitor of All-sky X-ray Image, and Neutron Star Interior Composition Explorer Mission. This energetic GRB was located relatively nearby ( z = 0.151), allowing for sustained observations of the afterglow. The large X-ray luminosity and low Galactic latitude ( b = 4.°3) make GRB 221009A a powerful probe of dust in the Milky Way. Using echo tomography, we map the line-of-sight dust distribution and find evidence for significant column densities at large distances (≳10 kpc). We present analysis of the light curves and spectra at X-ray and UV–optical wavelengths, and find that the X-ray afterglow of GRB 221009A is more than an order of magnitude brighter at T _0 + 4.5 ks than that from any previous GRB observed by Swift. In its rest frame, GRB 221009A is at the high end of the afterglow luminosity distribution, but not uniquely so. In a simulation of randomly generated bursts, only 1 in 10 ^4 long GRBs were as energetic as GRB 221009A; such a large E _γ _,iso implies a narrow jet structure, but the afterglow light curve is inconsistent with simple top-hat jet models. Using the sample of Swift GRBs with redshifts, we estimate that GRBs as energetic and nearby as GRB 221009A occur at a rate of ≲1 per 1000 yr—making this a truly remarkable opportunity unlikely to be repeated in our lifetime.

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