  Simultaneous observations by the large number of gamma-ray burst detectors
operating in the GLAST era will provide the spectra, lightcurves and locations
necessary for studying burst physics and testing the putative relations between
intrinsic burst properties. The detectors' energy band and the accumulation
timescale of their trigger system affect their sensitivity to hard vs. soft and
long vs. short bursts. Coordination of the Swift and GLAST observing plans
consistent with Swift's other science objectives could increase the detection
rate of GLAST bursts with redshifts.
