  A comprehensive search of BATSE Spectroscopy Detector data from 117 GRBs has
uncovered 13 statistically significant line candidates. The case of a candidate
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.
