Reconstruction of the EAS core position with the ARGO-YBJ detector

Details Reconstruction of the EAS core position with the ARGO-YBJ detector Reconstruction of the EAS core position with the ARGO-YBJ detector

Aug 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001icrc....7.2927m&link_type=abstract

Proceedings of the 27th International Cosmic Ray Conference. 07-15 August, 2001. Hamburg, Germany. Under the auspices of the Int

Physics

Scientific paper

The ARGO-YBJ detector is a full coverage array presently under construction at the Yangbajing Laboratory (Tibet, P.R. China, 4300 m a.s.l.). ARGO-YBJ will provide a detailed space-time picture of the front of small size air showers. In the analysis of the ARGO-YBJ data, a precise reconstruction of the shower parameters is of crucial importance to point to gamma ray sources. We present some different techniques exploited to determine the shower core position. The influence of the core reconstruction accuracy on the detector acceptance is discussed.

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