Speaker
Mr
Christian Sarmiento-Cano
(Universidad Industrial de Santander)
Description
The Latin American Giant Observatory (LAGO) is an extended Cosmic Rays observatory composed by a network of Water 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.
| Registration number following "ICRC2015-I/" | 881 |
|---|---|
| Collaboration | LAGO |
Primary authors
Mr
Christian Sarmiento-Cano
(Universidad Industrial de Santander)
Hernan Asorey
(Comision Nacional de Energia Atomica)
Luis A. Núñez
(University of Los Andes)
Dr
Luis Nunez
(Universidad Industrial de Santander)
Co-authors
Mr
Carlos Nina
(Instituto de Investigaciones Físicas, Universidad Mayor de San Andrés, La Paz, Bolivia)
Mr
Juan Salinas
(Instituto de Investigaciones Físicas, Universidad Mayor de San Andrés, La Paz, Bolivia)
Mr
Padro Miranda
(Instituto de Investigaciones Físicas, Universidad Mayor de San Andrés, La Paz, Bolivia)
Dr
Rolando Ticona
(Instituto de Investigaciones Físicas, Universidad Mayor de San Andrés, La Paz, Bolivia)
