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Search for Gamma-Ray Burst Associations with Gravitational-wave Candidates

  • B. Abidkhanov
  • , B. Ahmedov
  • , O. Burkhonov
  • , A. Abdujabbarov
  • , C. Zhou
  • , C. Yuan*
  • *Corresponding author for this work
  • New Uzbekistan University
  • Academy of Sciences of the Republic of Uzbekistan
  • School of Physics, Harbin Institute of Technology
  • National University of Uzbekistan named after Mirzo Ulugbek

Research output: Contribution to journalArticlepeer-review

Abstract

Motivated by the confirmed multimessenger event GW170817/GRB 170817A, we carry out an archival search for temporal and spatial associations between gamma-ray bursts (GRBs) and both significant and subthreshold gravitational wave (GW) candidates reported in the public search products of GWTC-2.1, GWTC-3, and GWTC-4.0. GRB trigger times and sky positions are taken from the GRBweb compilation of Swift-BAT and Fermi-GBM. GW candidates from the search pipelines are correlated with GRBs using time windows from 1 s to 103 s and spatial consistency tests based on the released sky-localization maps. We find no statistically significant GW–GRB associations on short timescales comparable to that of GW170817/GRB 170817A. The closest temporal connection is found between GRB 231126A and the GW candidate 231126_010928, with a delay of Δt = 164.692 s, and with the GRB localization overlapping a high-probability region of the GW skymap. From the associated three-dimensional BAYESTAR localization, we infer a luminosity distance of (Formula presented) DL=3951−1970+2497  Mpc (90% credible interval). For this candidate, we additionally performed Bayesian parameter estimation using Bilby with Markov Chain Monte Carlo sampling to obtain posterior parameters.

Original languageEnglish
Article number56
JournalAstrophysical Journal
Volume1006
Issue number1
DOIs
StatePublished - 20 Jul 2026
Externally publishedYes

Keywords

  • Astrophysical processes (104)

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