The AGILE Pipeline for Gravitational Waves Events Follow-up

被引：0

作者：

Zoli, A. ^{[1
]}

Bulgarelli, A. ^{[1
]}

Tavani, M. ^{[2
]}

Fioretti, V ^{[1
]}

Marisaldi, M. ^{[1
]}

Parmiggiani, N. ^{[3
]}

Fuschino, F. ^{[1
]}

Gianotti, F. ^{[1
]}

Trifoglio, M. ^{[1
]}

机构：

[1] INAF IASF Bologna, Via Gobetti 101, I-40129 Bologna, Italy

[2] INAF IAPS Roma, Via Fosso Cavaliere 100, I-00133 Rome, Italy

[3] Univ Modena & Reggio Emilia, Dipartimento Sci & Metodi Ingn, Modena, Italy

来源：

ASTRONOMICAL DATA ANALYSIS SOFTWARE AND SYSTEMS XXVI | 2019年 / 521卷

关键词：

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The first direct detection of gravitational waves (GW) by Advanced LIGO detectors in September 2015 has drawn the attention of the astrophysical community that is now searching for the electromagnetic counterparts of the detected GW events. The AGILE (Astro-Rivelatore Gamma a Immagini Leggero) mission is primarily devoted to the high-energy astrophysical study of gamma-ray sources in the 30 MeV to 30 GeV energy range. The capability of the AGILE satellite for the discovery of transients is unique: the actual spinning configuration of the satellite, together with a large field of view and a good sensitivity of F = (1 2) x 10(-8) erg cm(-2) s(-)1 for 100s integrations, provides a coverage of 80% of the sky, with each position exposed for 100 seconds, 200 times a day. The AGILE team signed a memorandum of understanding (MoU) with the LIGO/Virgo collaboration to follow the GW notices provided through the GCN network.

引用

页码：139 / 142

页数：4

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