TY - JOUR
T1 - Analysis of background cosmic ray rate in the 2010-2012 period from the LAGO-chacaltaya detectors
AU - Asorey, H.
AU - Miranda Loza, Pedro
AU - Núñez-Castiñeyra, A.
AU - Núñez, L. A.
AU - Salinas, J.
AU - Sarmiento-Cano, C.
AU - Ticona Peralta, Rolando
AU - Velarde, A.
PY - 2015
Y1 - 2015
N2 - 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.
AB - 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.
UR - http://www.scopus.com/inward/record.url?scp=84988723105&partnerID=8YFLogxK
M3 - Artículo de la conferencia
AN - SCOPUS:84988723105
VL - 30-July-2015
JO - Proceedings of Science
JF - Proceedings of Science
SN - 1824-8039
M1 - 414
Y2 - 30 July 2015 through 6 August 2015
ER -