Prospects for detecting Gamma-Ray Bursts with the Cherenkov Telescope Array

被引：0

作者：

Di Girolamo, T. ^{[1
,2
]}

Bissaldi, E. ^{[3
,4
]}

Di Pierro, F. ^{[5
]}

Gasparetto, T. ^{[6
]}

Longo, F. ^{[6
,7
]}

Vallania, P. ^{[5
,8
]}

Vigorito, C. F. ^{[8
,9
]}

机构：

[1] Univ Napoli Federico II, Naples, Italy

[2] Ist Nazl Fis Nucl, Sez Napoli, Naples, Italy

[3] Ist Nazl Fis Nucl, Sez Bari, Bari, Italy

[4] Politecn Bari, Bari, Italy

[5] Osserv Astrofis Torino, Ist Nazl Astrofis, Turin, Italy

[6] Univ Trieste, Trieste, Italy

[7] Ist Nazl Fis Nucl, Sez Trieste Udine, Trieste, Italy

[8] Ist Nazl Fis Nucl, Sez Torino, Turin, Italy

[9] Univ Torino, Turin, Italy

来源：

NUCLEAR AND PARTICLE PHYSICS PROCEEDINGS | 2017年 / 291卷

关键词：

Cherenkov telescopes; High-energy gamma rays; Gamma-ray bursts; EXTRAGALACTIC BACKGROUND LIGHT; FERMI OBSERVATIONS;

D O I：

10.1016/j.nuclphysbps.2017.06.010

中图分类号：

O412 [相对论、场论]; O572.2 [粒子物理学];

学科分类号：

摘要：

The Large Area Telescope (LAT) on the Fermi gamma-ray satellite telescope observes Gamma-Ray Bursts (GRBs) at energies above 100 MeV. Thanks to a new detection algorithm and a new event reconstruction, it is expected to publish a catalogue with more than 100 GRBs. This work aims at revising the prospects for GRB alerts with the Cherenkov Telescope Array (CTA) based on the new LAT results. We start by considering the simulation of the observations with the full CTA of two extremely bright events, the long GRB 130427A and the short GRB 090510; then we investigate how these GRBs would be observed by different subsamples of the array pointing to different directions, adopting the "coupled divergent" mode.

引用

页码：44 / 47

页数：4

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