20 pages, 12 figures, Accepted for publication in Astroparticle PhysicsH.E.S.S. -- The High Energy Stereoscopic System-- is a new system of large atmospheric Cherenkov telescopes for GeV/TeV Gamma-ray astronomy. This paper describes the trigger system of H.E.S.S. with emphasis on the multi-telescope array level trigger. The system trigger requires the simultaneous detection of air-showers by several telescopes at the hardware level. This requirement allows a suppression of background events which in turn leads to a lower system energy threshold for the detection of Gamma-rays. The implementation of the H.E.S.S. trigger system is presented along with data taken to characterise its performance
Abstract: Arrays of Cherenkov telescopes typically use multi-level trigger schemes to keep the rate ...
The H.E.S.S. Imaging Atmospheric Cherenkov Telescope Array is currently the most sensitive instrumen...
The surface detector array of the Pierre Auger Observatory consists of 1600 water-Cherenkov detector...
20 pages, 12 figures, Accepted for publication in Astroparticle PhysicsH.E.S.S. -- The High Energy S...
H.E.S.S.—The High Energy Stereoscopic System—is a new system of large atmospheric Cherenkov telescop...
The High Energy Stereoscopic System (H.E.S.S.) is a new system of large atmospheric Cherenkov telesc...
The High Energy Stereoscopic System (H.E.S.S.) is an array of five Imaging Atmospheric Cherenkov Tel...
The High Energy Stereoscopic System (H.E.S.S.) consists of an array of four ground-based imaging atm...
The H.E.S.S., experiment (High Energy Stereoscopic System) is an array of four imaging Cherenkov tel...
H.E.S.S. is an array of imaging atmospheric Cherenkov telescopes for ground based gamma-ray astronom...
The High Energy Stereoscopic System (H.E.S.S.) is one of the currently operating Imaging Atmospheric...
The High Energy Stereoscopic System (H.E.S.S.) is an array of five imaging atmospheric Cherenkov tel...
The High Energy Stereoscopic System (H.E.S.S.) is an array of four imaging atmospheric Cherenkov tel...
The High Energy Stereoscopic System (H.E.S.S.) is an array of five Imaging Atmospheric Cherenkov Tel...
Abstract: Arrays of Cherenkov telescopes typically use multi-level trigger schemes to keep the rate ...
The H.E.S.S. Imaging Atmospheric Cherenkov Telescope Array is currently the most sensitive instrumen...
The surface detector array of the Pierre Auger Observatory consists of 1600 water-Cherenkov detector...
20 pages, 12 figures, Accepted for publication in Astroparticle PhysicsH.E.S.S. -- The High Energy S...
H.E.S.S.—The High Energy Stereoscopic System—is a new system of large atmospheric Cherenkov telescop...
The High Energy Stereoscopic System (H.E.S.S.) is a new system of large atmospheric Cherenkov telesc...
The High Energy Stereoscopic System (H.E.S.S.) is an array of five Imaging Atmospheric Cherenkov Tel...
The High Energy Stereoscopic System (H.E.S.S.) consists of an array of four ground-based imaging atm...
The H.E.S.S., experiment (High Energy Stereoscopic System) is an array of four imaging Cherenkov tel...
H.E.S.S. is an array of imaging atmospheric Cherenkov telescopes for ground based gamma-ray astronom...
The High Energy Stereoscopic System (H.E.S.S.) is one of the currently operating Imaging Atmospheric...
The High Energy Stereoscopic System (H.E.S.S.) is an array of five imaging atmospheric Cherenkov tel...
The High Energy Stereoscopic System (H.E.S.S.) is an array of four imaging atmospheric Cherenkov tel...
The High Energy Stereoscopic System (H.E.S.S.) is an array of five Imaging Atmospheric Cherenkov Tel...
Abstract: Arrays of Cherenkov telescopes typically use multi-level trigger schemes to keep the rate ...
The H.E.S.S. Imaging Atmospheric Cherenkov Telescope Array is currently the most sensitive instrumen...
The surface detector array of the Pierre Auger Observatory consists of 1600 water-Cherenkov detector...