We present interplanetary network localization information for 218 gamma-ra
y bursts in the third BATSE catalog obtained by analyzing the arrival times
of these bursts with the Ulysses and Compton Gamma Ray Observatory spacecr
aft. For any given burst observed by these two spacecraft, arrival time ana
lysis (or "triangulation") results in an annulus of possible arrival direct
ions whose half-width varies between 7 " and 32', depending on the intensit
y and time history of the burst and the distance of the Ulysses spacecraft
from Earth. This annulus generally intersects the BATSE error circle, which
results in an average reduction of a factor of 30 of the error box area.