  The late-time high-resolution X-ray and radio observations of
GRB980425/SN1998bw, the closest known gamma ray burst (GRB) associated with a
supernova (SN) explosion, may have actually resolved the hyperluminal source
that produced the GRB and its afterglow. Its hyperluminal speed ~350c is
consistent with that expected in the cannonball (CB) model of GRBs. The
observed superluminal expansion of the late-time radio image of
GRB030329/SN2003dh, the GRB with the brightest and longest followed up radio
afterglow to date, is also consistent with that expected in the CB model of
GRBs and extrapolates to an apparent early-time hyperluminal expansion.
