Characteristics of the Multi-Telescope Coincidence Trigger of the HEGRA IACT System

The HEGRA–collaboration is operating a system of imaging atmospheric Cherenkov telescopes to search for sources of TeV–γ–rays. Air showers are observed in stereoscopic mode with several telescopes simultaneously. To trigger the telescope system a versatile two–level trigger scheme has been implemented, which allows a significant reduction of the energy threshold with respect to single telescopes. The technical implementation of this trigger scheme and the performance of the trigger system are described. Results include the dependence of singleand multi-telescope trigger rates on the trigger thresholds, on the orientation of the telescopes, and on the type of the primary particle.