Resumen
``Pi of the Sky'' is a system of wide field-of-view robotic telescopes, which search for short timescale astrophysical phenomena, especially for prompt optical GRB emission. In July 2013 the final ``Pi of the Sky'' detector system, with 16 CCD cameras on 4 mounts, was comissioned and integrated into the citizen-science network GLORIA (GLobal Robotic-telescope Intelligent Array). It is available to GLORIA users for scheduled observations. Selected archive data from the ``Pi of the Sky'' prototype telescope in Chile was also used to implement off-line demonstrator experiment for GLORIA. Thanks to the wide field of view of the telescope the selected sample of about 500 images allows for variability analysis of bright objects of different kind. Image processing is based on the LUIZA framework, which was implemented for GLORIA for efficient and flexible data analysis, based on the experience from high energy physics experiments.
