A comprehensive search of BATSE Spectroscopy Detector data from 117 GRBs ha
s uncovered 13 statistically significant line candidates. The case of a can
didate in GRB 930916 is discussed. In the data of SD 2 there appears to be
a emission line at 46 keV, however the line is not seen in the data of SD 7
. Simulations indicate that the lack of agreement between the results from
SD 2 and SD 7 is implausible but not impossible.