  In this work the strategy of the Latin American Giant Observatory (LAGO) to
build a Latin American collaboration is presented. Installing Cosmic Rays
detectors settled all around the Continent, from Mexico to the Antarctica, this
collaboration is forming a community that embraces both high energy physicist
and computer scientists. This is so because the data that are measured must be
analytical processed and due to the fact that \textit{a priori} and \textit{a
posteriori} simulations representing the effects of the radiation must be
performed. To perform the calculi, customized codes have been implemented by
the collaboration. With regard to the huge amount of data emerging from this
network of sensors and from the computational simulations performed in a
diversity of computing architectures and e-infrastructures, an effort is being
carried out to catalog and preserve a vast amount of data produced by the
water-Cherenkov Detector network and the complete LAGO simulation workflow that
characterize each site. Metadata, Permanent Identifiers and the facilities from
the LAGO Data Repository are described in this work jointly with the simulation
codes used. These initiatives allow researchers to produce and find data and to
directly use them in a code running by means of a Science Gateway that provides
access to different clusters, Grid and Cloud infrastructures worldwide.
