The interpretation of the observed gamma-ray burst V/V(max) statistic
in terms of spatial distributions is model-dependent. Detection of gam
ma-ray bursts requires the counting rate in one or more detectors to e
xceed aa threshold C(lim) determined from a time-dependent background
rate B(t). The sampling depth of the burst detector is thus time-depen
dent, and, if burst sources are non-uniform in space, the observed dis
tribution will be affected by B(t). We demonstrate this effect with aa
simple geometric distribution of standard candles and argue that V/V(
max) statistic without information on threshold variations is insuffic
ient for rigorous data analysis. Peak count rates and threshold values
must be given separately for all events in order to facilitate aa mea
ningful comparison of observations with theoretical distribution model
s.