In recent years, a new generation of space missions has offered great opportunities for discovery in high-energy astrophysics. In this article we focus on the scientific operations of the Gamma-Ray Imaging Detector (GRID) on board the AGILE space mission. AGILE-GRID, sensitive in the energy range of 30 MeV–30 GeV, has detected many γ -ray transients of both galactic and extragalactic origin. This work presents the AGILE innovative approach to fast γ -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 γ -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, via e-mail, and via push notifications from 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 γ -ray astrophysics.
THE AGILE ALERT SYSTEM FOR GAMMA-RAY TRANSIENTS / A., Bulgarelli; M., Trifoglio; F., Gianotti; M., Tavani; Parmiggiani, Nicolò; V., Fioretti; A. W., Chen; S., Vercellone; C., Pittori; F., Verrecchia; F., Lucarelli; P., Santolamazza; G., Fanari; P., Giommi; Beneventano, Domenico; 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. - In: THE ASTROPHYSICAL JOURNAL. - ISSN 0004-637X. - STAMPA. - 781:1:(2014), pp. 1-13. [10.1088/0004-637X/781/1/19]
THE AGILE ALERT SYSTEM FOR GAMMA-RAY TRANSIENTS
PARMIGGIANI, Nicolò;BENEVENTANO, Domenico;
2014
Abstract
In recent years, a new generation of space missions has offered great opportunities for discovery in high-energy astrophysics. In this article we focus on the scientific operations of the Gamma-Ray Imaging Detector (GRID) on board the AGILE space mission. AGILE-GRID, sensitive in the energy range of 30 MeV–30 GeV, has detected many γ -ray transients of both galactic and extragalactic origin. This work presents the AGILE innovative approach to fast γ -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 γ -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, via e-mail, and via push notifications from 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 γ -ray astrophysics.
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