Measurement of the Flux of Ultrahigh Energy Cosmic Rays from Monocular Observations by the High Resolution Fly's Eye Experiment

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dc.creators Eye Collaboration
dc.date2002-08-12
dc.date2003-10-14
dc.date.accessioned2026-07-07T10:31:22Z
dc.date.available2026-07-07T10:31:22Z
dc.descriptionWe have measured the cosmic ray spectrum above 10^17.2 eV using the two air fluorescence detectors of the High Resolution Fly's Eye observatory operating in monocular mode. We describe the detector, photo-tube and atmospheric calibrations, as well as the analysis techniques for the two detectors. We fit the spectrum to a model consisting of galactic and extra-galactic sources.
dc.description4 pages, 4 figures. Uses 10pt.rtx, amsmath.sty, aps.rtx, revsymb.sty, revtex4.cls
dc.identifierhttps://arxiv.org/abs/astro-ph/0208243
dc.identifierhttp://arxiv.org/abs/astro-ph/0208243
dc.identifierPhys.Rev.Lett.92:151101,2004
dc.identifierdoi:10.1103/PhysRevLett.92.151101
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/178384
dc.subjectAstrophysics
dc.titleMeasurement of the Flux of Ultrahigh Energy Cosmic Rays from Monocular Observations by the High Resolution Fly's Eye Experiment
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