Study of the angular resolution of the ARGO-YBJ detector

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The 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.
10 pages, Presented at the "Incontro Nazionale di Astrofisica delle Alte Energie", Rome 15-16 May 2003

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