  The LAGO (Latin American Giant Observatory) observatory is an experiment that
spans over Latin America in a wide range of latitudes that gives different
rigidity cut offs for the enter of cosmic rays in the atmosphere. The
motivation of the Observatory is to study atmospheric radiation and space
weather through the measurement of the secondary emission of low energy cosmic
rays at ground level using Water Cherenkov Detectors (WCD). This work presents
the contributions of the LAGO collaboration to the 2019 36th ICRC.
