The experiment for detection of optical flashes related to gamma-ray b
ursts is briefly described and discussed. The aim of the proposal is t
o develop a reliable monitoring service at optical wavelengths and to
solve the question whether or not the gamma-ray bursts are accompanied
by optical emissions. The detection of these phenomena at optical wav
elengths could significantly help to answer the question of the physic
al nature of gamma-ray bursters (still unknown). The Optical Transient
Monitor (OTM) represents a low-cost automatic operation experiment wi
th good time resolution, medium sensitivity, low (0.1-degrees) angular
resolution, and excellent background elimination. A double CCD camera
with wide-field lenses will monitor approximately 13% of the full sky
hemisphere for optical transient phenomena. Two such systems are plan
ned, separated by 100 km to be able to eliminate all effects in the Ea
rth's atmosphere and nearby space.