Analysis of background cosmic ray rate in the 2010-2012 period from the LAGO-chacaltaya detectors

H. Asorey, Pedro Miranda Loza, A. Núñez-Castiñeyra, L. A. Núñez, J. Salinas, C. Sarmiento-Cano, Rolando Ticona Peralta, A. Velarde

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3 Citas (Scopus)

Resumen

The Latin American Giant Observatory (LAGO) is an extended Cosmic Rays observatory composed by a network of Cherenkov Detectors (WCDs) spread over Latin America. This work will report the analysis of three years of data from three LAGO WCD located in Cerro Chacaltaya, Bolivia, at 5200 m a.s.l. Background cosmic ray rate from these detectors is checked for DAQ issues and inconsistencies, and corrected for atmospheric effects. An analysis for short transients up to the minute timescale is performed, in search for coincidence with transients observed by satellites. Sidereal and solar long term epoch data analysis are also presented.

Idioma originalInglés
Número de artículo414
PublicaciónProceedings of Science
Volumen30-July-2015
EstadoPublicada - 2015
Evento34th International Cosmic Ray Conference, ICRC 2015 - The Hague, Países Bajos
Duración: 30 jul. 20156 ago. 2015

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