The synchrotron shock model (SSM) for gamma-ray burst emission makes a test
able prediction: that the observed low-energy power-law photon number spect
ral index cannot exceed -2/3 (where the photon model is defined with a posi
tive index: dN/dE proportional to E-alpha). We have collected time-resolved
spectral fit parameters for over 100 bright bursts observed by the Burst A
nd Transient Source Experiment on board the Compton Gamma Ray Observatory.
Using this database, we find 23 bursts in which the spectral index limit of
the SSM is violated. We discuss elements of the analysis methodology that
affect the robustness of this result, as well as some of the escape hatches
left for the SSM by theory.