We review the observational status of the Supernova/Gamma‐Ray Burst connection. Most observations collected in the last 15 years show that long duration Gamma‐ray Bursts are associated with broad lines SNe‐Ibc, although a few remarkable exceptions do exist. Current estimates of SN and GRB rates yield a ratio GRB/SNe‐Ibc  less (or much less) than 3%.