Ever since the discovery of the Cosmic Gamma-Ray Bursts we have search
ed for the quiescent counterparts of these mysterious flashes. Without
definite counterparts our pictures of the sources must remain vague.
The review discusses a number of techniques which have been applied to
the gamma burst localization problem and their limitations. The most
accurate technique to-date is the Interplanetary Network (IPN) timing
technique. Considering the lack of success in the searches for counter
parts in even the smallest gamma burst error boxes, it seems, that the
next generation of satellite gamma burst detectors must be designed t
o allow immediate follow-up with sensitive telescopes. Concepts to ach
ieve this goal are discussed.