The Agile Alert System For Gamma-Ray Transients
astro-ph.IM
/ Authors
A. Bulgarelli, M. Trifoglio, F. Gianotti, M. Tavani, N. Parmiggiani, V. Fioretti, A. W. Chen, S. Vercellone, C. Pittori, F. Verrecchia
and 19 more authors
F. Lucarelli, P. Santolamazza, G. Fanari, P. Giommi, D. Beneventano, A. Argan, A. Trois, E. Scalise, F. Longo, A. Pellizzoni, G. Pucella, S. Colafrancesco, V. Conforti, P. Tempesta, M. Cerone, P. Sabatini, G. Annoni, G. Valentini, L. Salotti
/ Abstract
In recent years, a new generation of space missions offered great opportunities of discovery in high-energy astrophysics. In this article we focus on the scientific operations of the Gamma-Ray Imaging Detector (GRID) onboard the AGILE space mission. The AGILE-GRID, sensitive in the energy range of 30 MeV-30 GeV, has detected many gamma-ray transients of galactic and extragalactic origins. This work presents the AGILE innovative approach to fast gamma-ray transient detection, which is a challenging task and a crucial part of the AGILE scientific program. The goals are to describe: (1) the AGILE Gamma-Ray Alert System, (2) a new algorithm for blind search identification of transients within a short processing time, (3) the AGILE procedure for gamma-ray transient alert management, and (4) the likelihood of ratio tests that are necessary to evaluate the post-trial statistical significance of the results. Special algorithms and an optimized sequence of tasks are necessary to reach our goal. Data are automatically analyzed at every orbital downlink by an alert pipeline operating on different timescales. As proper flux thresholds are exceeded, alerts are automatically generated and sent as SMS messages to cellular telephones, e-mails, and push notifications of an application for smartphones and tablets. These alerts are crosschecked with the results of two pipelines, and a manual analysis is performed. Being a small scientific-class mission, AGILE is characterized by optimization of both scientific analysis and ground-segment resources. The system is capable of generating alerts within two to three hours of a data downlink, an unprecedented reaction time in gamma-ray astrophysics.