Detailed Study of the Variable Afterglow of GRB 060526
2009
Using one of the largest photometric datasets ever obtained for a GRB, we investigate the highly variable afterglow light curve of Gamma‐Ray Burst 060526. The light curve shows clear deviations from a power‐law behaviour which we attribute to energy injections. We fit the data to a numerical model including 6 energy injections which explains the full temporal behaviour of the light curve in many wavebands, ranging from NIR to X‐rays.
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