Evidence for a supernova in reanalyzed optical and near-infrared images ofGRB 970228

We present B-, V-, R-C-, I-C-, J-, H-, K-, and K'-band observations of the optical transient (OT) associated with GRB 970228, based on a reanalysis of previously used images and unpublished data. In order to minimize calibrat ion differences, we have collected and analyzed most of the photometry and consistently determined the magnitude of the OT relative to a set of second ary held stars. We confirm our earlier finding that the early decay of the light curves (before 1997 March 6) was faster than that at intermediate tim es (between 1997 March 6 and April 7). At late times the light curves resum e a fast decay (after 1997 April 7). The early-time observations of GRB 970 228 are consistent with relativistic blast-wave models, but the intermediat e- and late-time observations are hard to understand in this framework. The observations are well explained by an initial power-law decay with alpha = -1.51 +/- 0.06 modified at later times by a Type Ic supernova light curve. Together with the evidence for GRB 980326 and GRB 980425, this gives furth er support for the idea that at least some gamma-ray bursts are associated with a possibly rare type of supernova.