[en] Understanding the origin of Very High Energy (VHE) gamma-ray emission in explosive astrophysical sources is an open problem. VHE emission can arise via different possible mechanisms such as the leptonic Synchrotron Self-Compton, as well as hadronic processes. Radio emission is generally dominated by non-thermal is generally synchrotron in nature, and is connected with the VHE emission in case of leptonic origin. Hence studying these Astrophysical sources he way from radio bands to VHE emission, provide an undisputed way to pin down the nature of VHE emission. With high sensitivity of recently upgraded Giant Metre wave Radio Telescope (GMRT) in Naranyangaon, Pune and upcoming MACE in Ladakh, scientist's in India are uniquely placed to carry out the multi waveband studies of explosive events and understand their intriguing nature. (author)