The time structure of Cherenkov images generated by TeV γ-rays and by cosmic rays
- 31 July 1999
- journal article
- Published by Elsevier in Astroparticle Physics
- Vol. 11 (3) , 363-377
- https://doi.org/10.1016/s0927-6505(99)00003-1
Abstract
No abstract availableKeywords
All Related Versions
This publication has 9 references indexed in Scilit:
- Measurement of the radial distribution of Cherenkov light generated by TeV γ-ray air showersAstroparticle Physics, 1999
- Measurable difference in Cherenkov light between gamma and hadron induced EASAstroparticle Physics, 1998
- Characteristics of the multi-telescope coincidence trigger of the HEGRA IACT systemAstroparticle Physics, 1998
- Pulse shape selection in very high energy gamma-ray astronomyJournal of Physics G: Nuclear and Particle Physics, 1998
- First results on the performance of the HEGRA IACT arrayAstroparticle Physics, 1997
- Trigger conditions and effective areas of imaging air Cherenkov telescopesAstroparticle Physics, 1996
- The atmospheric Cherenkov technique in Very High Energy Gamma-Ray AstronomySpace Science Reviews, 1996
- Instrumentation for very high energy gamma-ray astronomyExperimental Astronomy, 1995
- The relation of Cerenkov time profile widths to the distance to maximum of air showersJournal of Physics G: Nuclear Physics, 1983