The Astrophysical Journal (Jan 2025)

The Nature of Optical Afterglows without Gamma-Ray Bursts: Identification of AT2023lcr and Multiwavelength Modeling

  • Maggie L. Li,
  • Anna Y. Q. Ho,
  • Geoffrey Ryan,
  • Daniel A. Perley,
  • Gavin P. Lamb,
  • Nayana A.J.,
  • Igor Andreoni,
  • G. C. Anupama,
  • Eric C. Bellm,
  • Edo Berger,
  • Joshua S. Bloom,
  • Eric Burns,
  • Ilaria Caiazzo,
  • Poonam Chandra,
  • Michael W. Coughlin,
  • Kareem El-Badry,
  • Matthew J. Graham,
  • Mansi Kasliwal,
  • Garrett K. Keating,
  • S. R. Kulkarni,
  • Harsh Kumar,
  • Frank J. Masci,
  • Richard A. Perley,
  • Josiah Purdum,
  • Ramprasad Rao,
  • Antonio C. Rodriguez,
  • Ben Rusholme,
  • Nikhil Sarin,
  • Jesper Sollerman,
  • Gokul P. Srinivasaragavan,
  • Vishwajeet Swain,
  • Zachary Vanderbosch

DOI
https://doi.org/10.3847/1538-4357/adc800
Journal volume & issue
Vol. 985, no. 1
p. 124

Abstract

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In the past few years, the improved sensitivity and cadence of wide-field optical surveys have enabled the discovery of several afterglows without associated detected gamma-ray bursts (GRBs). We present the identification, observations, and multiwavelength modeling of a recent such afterglow (AT 2023lcr), and model three literature events (AT 2020blt, AT 2021any, and AT 2021lfa) in a consistent fashion. For each event, we consider the following possibilities as to why a GRB was not observed: (1) the jet was off-axis; (2) the jet had a low initial Lorentz factor; and (3) the afterglow was the result of an on-axis classical GRB (on-axis jet with physical parameters typical of the GRB population), but the emission was undetected by gamma-ray satellites. We estimate all physical parameters using afterglowpy and Markov Chain Monte Carlo methods from emcee . We find that AT 2023lcr, AT 2020blt, and AT 2021any are consistent with on-axis classical GRBs, and AT 2021lfa is consistent with both on-axis low Lorentz factor (Γ _0 ≈ 5–13) and off-axis ( θ _obs = 2 θ _jet ) high Lorentz factor (Γ _0 ≈ 100) jets.

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