Methods to determine the angular resolution of the HEGRA extended air shower scintillator array
- 31 October 1996
- journal article
- Published by Elsevier in Astroparticle Physics
- Vol. 5 (3-4) , 379-392
- https://doi.org/10.1016/0927-6505(96)00038-2
Abstract
No abstract availableKeywords
This publication has 10 references indexed in Scilit:
- Design and performance of the angle integrating Čerenkov array AIROBICCAstroparticle Physics, 1995
- Monte Carlo simulation of the HEGRA cosmic ray detector performanceNuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, 1995
- Cosmic-ray deficit from the directions of the Moon and the Sun detected with the Tibet air-shower arrayPhysical Review D, 1993
- The CYGNUS extensive air-shower experimentNuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, 1992
- Observation of shadowing of ultrahigh-energy cosmic rays by the Moon and the SunPhysical Review D, 1991
- Design and performance of the Chicago Air Shower ArrayNuclear Physics B - Proceedings Supplements, 1990
- Observation of γ rays >1015 eV from Cygnus X-3Nature, 1983
- Detection of 2 X 10 to the 15th to 2 X 10 to the 16th eV gamma-rays from Cygnus X-3The Astrophysical Journal, 1983
- The interplanetary magnetic field. Solar origin and terrestrial effectsSpace Science Reviews, 1968
- Arrival Directions of Cosmic-Ray Air Showers from the Northern SkyPhysical Review B, 1957