Study of the angular resolution of the ARGO-YBJ detector

Simple item page
dc.creatorDi Sciascio, Giuseppe
dc.creatorRossi, Elvira
dc.date2003-09-03
dc.date.accessioned2026-07-07T02:09:24Z
dc.date.available2026-07-07T02:09:24Z
dc.descriptionThe determination of the arrival direction of gamma-induced air showers in the ARGO-YBJ experiment has been investigated using different algorithms in the reconstruction procedure. The calculation has been performed, as a function of pad multiplicity, for different primary energies. The performance of a conical correction to the shower front with a suitable fixed cone slope is discussed.
dc.description10 pages, Presented at the "Incontro Nazionale di Astrofisica delle Alte Energie", Rome 15-16 May 2003
dc.identifierhttps://arxiv.org/abs/astro-ph/0309108
dc.identifierhttp://arxiv.org/abs/astro-ph/0309108
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/6418
dc.subjectAstrophysics
dc.titleStudy of the angular resolution of the ARGO-YBJ detector
dc.typetext

Files

Collections

arXiv