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About

Amar Aryan is an astrophysicist specializing in the multi-wavelength study of gamma-ray bursts (GRBs) and their connection to core-collapse supernovae. His research focuses on unraveling the complex emission mechanisms of GRBs, from prompt gamma-ray emission to early optical afterglows, with particular attention to reverse shock signatures and very-high-energy (VHE) detections. Aryan’s most cited work includes a detailed analysis of GRB 201015A and GRB 201216C, two VHE-detected bursts, where he performed time-resolved spectroscopy using Bayesian methods to characterize the onset of the external forward shock. He has also investigated dark GRBs, such as GRB 150309A, probing whether their faint optical emission stems from dust extinction or high redshift. His contributions to observational astronomy extend to advocating for the 3.6m Devasthal Optical Telescope (DOT) in India, highlighting its longitudinal advantage for time-domain follow-up of transients. With over 48 citations across his key papers, Aryan is establishing himself as a rising figure in GRB astrophysics, bridging prompt emission physics with early afterglow observations to deepen our understanding of these extreme cosmic explosions.