The AGILE real-time analysis software system to detect short-transient events in the multi-messenger era

被引:3
作者
Parmiggiani, N. [1 ]
Bulgarelli, A. [1 ]
Ursi, A. [2 ,3 ]
Addis, A. [1 ]
Baroncelli, L. [1 ]
Fioretti, V. [1 ]
Di Piano, A. [1 ,4 ]
Panebianco, G. [1 ,5 ]
Tavani, M. [2 ,6 ]
Pittori, C. [7 ,8 ]
Verrecchia, F. [7 ,8 ]
Beneventano, D. [4 ]
机构
[1] INAF OAS Bologna, Via P Gobetti 93-3, I-40129 Bologna, Italy
[2] INAF IAPS Roma, Via Fosso del Cavaliere 100, I-00133 Rome, Italy
[3] ASI, Via Politecn Snc, I-00133 Rome, Italy
[4] Univ Modena & Reggio Emilia, DIEF, Via Pietro Vivarelli 10, I-41125 Modena, Italy
[5] Univ Bologna, Dept Phys & Astron, Via Gobetti 93-2, I-40129 Bologna, Italy
[6] Univ Roma Tor Vergata, Dip Fis, Via Ric Sci 1, I-00078 Monte Porzio Catone, Italy
[7] INAF OAR Roma, Via Frascati 33, I-00078 Monte Porzio Catone, Italy
[8] ASI Space Sci Data Ctr SSDC, Via Politecn Snc, I-00133 Rome, Italy
关键词
Real -time analysis pipeline; Gamma-ray astronomy; Multi-messenger astronomy; Gamma-ray burst; Gravitational waves;
D O I
10.1016/j.ascom.2023.100726
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
AGILE is a space mission launched in 2007 to study X-ray and gamma-ray phenomena through data acquired by different instruments on board the satellite. In the multi-messenger era, the fast detection of transient sources is one of the main goals of space and ground-based gamma-ray observatories. When an observatory detects a transient event, it usually sends science alerts to other facilities through networks such as the General Coordinates Network (GCN), enabling follow-up observations. To achieve this task, real-time analysis (RTA) pipelines are required. This manuscript presents the RTA system developed for the AGILE space mission to detect transient sources on timescales from seconds to one hour. Two types of pipelines are presented. One pipeline executes automated analyses as soon as data are available, sharing the detection of sources with the community; more than 90 automated notices have been sent to the GCN since May 2019. The other pipeline reacts to external science alerts from neutrinos, gravitational waves (GW), etc., to search for electromagnetic counterparts in the AGILE data. The AGILE Team can visualize the results of these analyses using a web platform. The pipelines hereby presented can be a starting point for the development of RTA systems of the next generation of space-based gamma-ray observatories.
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页数:15
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