A Stochastic Approach To Reconstruct Gamma Ray Burst Lightcurves

Understand

Gamma-Ray Bursts (GRBs), being observed at high redshift (z = 9.4), vital to cosmological studies and investigating Population III stars.

• To tackle these studies, we need correlations among relevant GRB variables with the requirement of small uncertainties on their variables.
• Thus, we must have good coverage of GRB light curves (LCs).
• However, gaps in the LC hinder the precise determination of GRB properties and are often unavoidable.