Measurement of the flux of ultra high energy cosmic rays by the stereo technique
- 31 August 2009
- journal article
- Published by Elsevier in Astroparticle Physics
- Vol. 32 (1) , 53-60
- https://doi.org/10.1016/j.astropartphys.2009.06.001
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This publication has 18 references indexed in Scilit:
- First Observation of the Greisen-Zatsepin-Kuzmin SuppressionPhysical Review Letters, 2008
- Studies of systematic uncertainties in the estimation of the monocular aperture of the HiRes experimentAstroparticle Physics, 2007
- Measurement of pressure dependent fluorescence yield of air: Calibration factor for UHECR detectorsAstroparticle Physics, 2006
- A measurement of time-averaged aerosol optical depth using air-showers observed in stereo by HiResAstroparticle Physics, 2006
- Comparison of air fluorescence and ionization measurements of EM shower depth profiles: Test of a UHECR detector techniqueAstroparticle Physics, 2006
- Photon yields from nitrogen gas and dry air excited by electronsAstroparticle Physics, 2003
- A measurement of the average longitudinal development profile of cosmic ray air showers between 1017 and 1018 eVAstroparticle Physics, 2001
- Measurement of the Cosmic‐Ray Energy Spectrum and Composition from 1017to 1018.3eV Using a Hybrid TechniqueThe Astrophysical Journal, 2001
- Evidence for Changing of Cosmic Ray Composition betweenandeV from Multicomponent MeasurementsPhysical Review Letters, 2000
- Evidence for correlated changes in the spectrum and composition of cosmic rays at extremely high energiesPhysical Review Letters, 1993