3-11 July 2007
Merida, Mexico
Mexico/General timezone
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Contribution Poster

Merida, Mexico - Regency (Hyatt)

Electromagnetic and muon primary discrimination from underground scintillator signatures

Speakers

  • Mr. Federico SANCHEZ

Primary authors

  • Mr. Federico SANCHEZ (Departamento de Altas Energias, Instituto de Ciencias Nucleares , Universidad Nacional Autonoma de Mexico, Mexico, D.F., C.P. 04510)

Co-authors

  • Mr. Gustavo MEDINA TANCO (Departamento de Altas Energias, Instituto de Ciencias Nucleares, Universidad Nacional Autonoma de Mexico, Mexico, D.F., C.P. 04510)
  • Mr. Juan Carlos D'OLIVO (Departamento de Altas Energias, Instituto de Ciencias Nucleares, Universidad Nacional Autonoma de Mexico, Mexico, D.F., C.P. 04510)
  • Mr. Eduardo NAHMAD-ACHAR (Departamento de Estructura de la Materia, Instituto de Ciencias Nucleares ,Universidad Nacional Autonoma de Mexico, Mexico, D.F., C.P. 04510)
  • Mr. Jose Francisco VALDES GALICIA (Instituto de Geofisica, Universidad Nacional Autonoma de Mexico,Mexico, D.F., C.P. 04510)

Abstract content

We discuss discrimination techniques and their quantitative efficiency that allow the separation of high energy electron/photon and muon primaries originated in cosmic ray extensive air showers impinging the ground. The experimental setup used in this study is detailed elsewhere in this volume (Sanchez et al.). Several approaches are analyzed, including track timing, footprint characterization and neural networks.

Reference

Proceedings of the 30th International Cosmic Ray Conference; Rogelio Caballero, Juan Carlos D'Olivo, Gustavo Medina-Tanco, Lukas Nellen, Federico A. Sánchez, José F. Valdés-Galicia (eds.); Universidad Nacional Autónoma de México, Mexico City, Mexico, 2008; Vol. 5 (HE part 2), pages 1175-1178