The Astrophysical Journal (Jan 2025)

The Long-lived Broadband Afterglow of Short Gamma-Ray Burst 231117A and the Growing Radio-detected Short Gamma-Ray Burst Population

  • Genevieve Schroeder,
  • Wen-fai Fong,
  • Charles D. Kilpatrick,
  • Alicia Rouco Escorial,
  • Tanmoy Laskar,
  • Anya E. Nugent,
  • Jillian Rastinejad,
  • Kate D. Alexander,
  • Edo Berger,
  • Thomas G. Brink,
  • Ryan Chornock,
  • Clecio R. de Bom,
  • Yuxin Dong,
  • Tarraneh Eftekhari,
  • Alexei V. Filippenko,
  • Celeste Fuentes-Carvajal,
  • Wynn V. Jacobson-Galán,
  • Matthew Malkan,
  • Raffaella Margutti,
  • Jeniveve Pearson,
  • Lauren Rhodes,
  • Ricardo Salinas,
  • David J. Sand,
  • Luidhy Santana-Silva,
  • Andre Santos,
  • Huei Sears,
  • Manisha Shrestha,
  • Nathan Smith,
  • Wayne Webb,
  • Simon de Wet,
  • Yi Yang

DOI
https://doi.org/10.3847/1538-4357/ada9e5
Journal volume & issue
Vol. 982, no. 1
p. 42

Abstract

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We present multiwavelength observations of the Swift short γ -ray burst GRB 231117A, localized to an underlying galaxy at redshift z = 0.257 at a small projected offset (∼2 kpc). We uncover long-lived X-ray Chandra X-ray Observatory and radio/millimeter (VLA, MeerKAT, and ALMA) afterglow emission, detected to ∼37 days and ∼20 days (rest frame), respectively. We measure a wide jet (∼10 $\mathop{.}\limits^{\unicode{x000b0}}$ 4) and relatively high circumburst density (∼0.07 cm ^−3 ) compared to the short GRB population. Our data cannot be easily fit with a standard forward shock model, but they are generally well fit with the incorporation of a refreshed forward shock and a reverse shock at 10 ^−2 cm ^−3 ), consistent with their smaller (10°) jets where observational evidence of collimation may only be detectable at radio wavelengths. Owing to improved observing strategies and the emergence of sensitive radio facilities, the number of radio-detected short GRBs has quadrupled in the past decade.

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