Reconstruction accuracy of the surface detector array of the Pierre Auger Observatory

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dc.creatorAuger Collaboration
dc.creatorAve, M.
dc.date2007-09-13
dc.date.accessioned2026-07-07T08:29:22Z
dc.date.available2026-07-07T08:29:22Z
dc.descriptionThe reconstruction of extensive air showers (arrival direction, core position and energy estimation) by the surface detector of the Pierre Auger Observatory is discussed together with the corresponding accuracy. We determine the angular reconstruction accuracy as a function of the station multiplicity by using two different aproaches. We discuss statistical and systematic uncertainties in the determination of the signal at 1000 m from the core, S(1000), which is used to estimate the primary energy.
dc.descriptionContribution to the 30th International Cosmic Ray Conference, Merida, Mexico, July 2007, 4 pages, 6 figures
dc.identifierhttps://arxiv.org/abs/0709.2125
dc.identifierhttp://arxiv.org/abs/0709.2125
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/137943
dc.subjectAstrophysics
dc.titleReconstruction accuracy of the surface detector array of the Pierre Auger Observatory
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