The GRB/SN Connection: An Improved Spectral Flux Distribution for the SN-like Component to the Afterglow of GRB 970228, the Non-Detection of a SN-like Component to the Afterglow of GRB 990510, and GRBs as Beacons to Locate SNe at Redshifts Z≈4–5

AIP Conference Proceedings - United States

doi 10.1063/1.1361573