We describe a Bayesian methodology to evaluate the consistency between
the reported Ginga and BATSE detections of absorption features in gam
ma-ray burst spectra. Currently no features have been detected by BATS
E, but this methodology will still be applicable if and when such feat
ures are discovered. The Bayesian methodology permits the comparison o
f hypotheses regarding the two detectors' observations and makes expli
cit the subjective aspects of our analysis (e.g., the quantification o
f our confidence in detector performance). We also present non-Bayesia
n consistency statistics. Based on preliminary calculations of line de
tectability, we find that both the Bayesian and non-Bayesian technique
s show that the BATSE and Ginga observations are consistent given our
understanding of these detectors.