Abstract:
The short gamma-ray burst (GRB) 170817A was the first GRB associated with a gravitational-wave event. Due
to the exceptionally low luminosity of the prompt γ-ray and the afterglow emission, the origin of both radiation
components is highly debated. The most discussed models for the burst and the afterglow include a regular
GRB jet seen off-axis and the emission from the cocoon encompassing a “choked” jet. Here, we report low
radio frequency observations at 610 and 1390 MHz obtained with the Giant Metrewave Radio Telescope. Our
observations span a range of ∼7 to ∼152 days after the burst. The afterglow started to emerge at these low
frequencies about 60 days after the burst. The 1390 MHz light curve barely evolved between 60 and 150 days,
but its evolution is also marginally consistent with an Fν ∝ t
0.8 rise seen in higher frequencies. We model
the radio data and archival X-ray, optical, and high-frequency radio data with models of top-hat and Gaussian
structured GRB jets. We performed a Markov Chain Monte Carlo analysis of the structured-jet parameter
space. Though highly degenerate, useful bounds on the posterior probability distributions can be obtained.
Our bounds of the viewing angle are consistent with that inferred from the gravitational-wave signal. We
estimate the energy budget in prompt emission to be an order of magnitude lower than that in the afterglow
blast wave.
