BeppoSAX has been added to the 3rd Interplanetary Network of gamma-ray
burst detectors. Of the 8 events observed to date by Ulysses and the
BeppoSAX Gamma Ray Burst Monitor (GRBM), four have been localized by t
riangulation, resulting in annuli whose 3 sigma widths are as small as
63''. These data give error boxes whose sizes are sometimes smaller t
han those obtained with the SAX Wide Field Camera (WFC). They can be u
sed to confirm the association between fading X-ray and optical source
s and gamma-ray bursts.