Abstract

GRB 030329 displayed one of the brightest optical afterglows ever. We have followed the radio afterglow of GRB 030329 for over 5 years using the GMRT and WSRT at low radio frequencies. This is the longest as well as the lowest frequency follow up of any GRB afterglow ever.

Radio observations of a GRB afterglow provide a unique probe of the physics of the blast wave at late times, when the expansion of the fireball slows down to non‐relativistic speeds. Our GMRT‐WSRT observations suggest that the afterglow of GRB030329 entered the non‐relativistic phase around 60 days after the burst. The estimate of the fireball energy content, in this near‐isotropic phase is much less susceptible to the collimation‐related uncertainties arising in the relativistic phase. We have also been closely monitoring the evolution of the afterglow to look for possible signatures of emission from a counter jet, but no conclusive evidence has so far been found.