A First Search for Prompt Radio Emission from a Gravitational-Wave Event

Mar 15, 2019
8 pages
Published in:
  • Astrophys.J.Lett. 877 (2019) 2, L39
  • Published: Jun 4, 2019
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Abstract: (IOP)
Multimessenger observations of the binary neutron star merger GW170817 have enabled the discovery of a diverse array of electromagnetic counterparts to compact binary mergers, including an unambiguous kilonova, a short gamma-ray burst, and a late-time radio jet. Beyond these counterparts, compact binary mergers are additionally predicted to be accompanied by prompt low-frequency radio emission. The successful observation of a prompt radio counterpart would be immensely valuable, but is made difficult by the short delay between the gravitational-wave and prompt electromagnetic signals, as well as by the poor localization of gravitational-wave sources. Here, we present the first search for prompt radio emission accompanying a gravitational-wave event, targeting the binary black hole merger GW170104 detected by the Advanced Laser Interferometer Gravitational-Wave Observatory (LIGO) and Virgo during their second (O2) observing run. Using the Owens Valley Radio Observatory Long Wavelength Array, we search a ∼900 deg2 region for transient radio emission within approximately one hour of GW170104, obtaining an upper limit of 2.5 × 1041 erg s−1 on its equivalent isotropic luminosity between 27 and 84 MHz. We additionally discuss plans to target binary neutron star mergers in Advanced LIGO and Virgo’s upcoming O3 observing run.
Note:
  • 13 pages + appendices, 7 figures, submitted to ApJ
  • gravitational waves
  • radiation mechanisms: non-thermal
  • stars: black holes
  • neutron star: binary
  • binary: compact
  • black hole: binary
  • gamma ray: burst
  • gravitational radiation
  • radio wave
  • electromagnetic