  We present BeppoSAX GRBM and WFC light curves of GRB980425 and NFI follow-up
data taken in 1998 April, May, and November. The first NFI observation has
detected within the 8' radius error box of the GRB an X-ray source positionally
consistent with the supernova SN 1998bw, exploded within a day of GRB980425,
and a fainter X-ray source, not consistent with the position of the supernova.
The former source is detected in the following NFI pointings and exhibits a
decline of a factor of two in six months. If it is associated with SN 1998bw,
this is the first detection of hard X-ray emission from a Type I supernova. The
latter source exhibits only marginally significant variability. Based on these
data, it is not possible to select either source as a firm candidate for the
GRB counterpart.
