MAGIC observation of the prompt and afterglow emission from GRBs

被引：0

作者：

Galante, Nicola ^{[1
]}

Bastieri, Denis ^{[2
]}

Gaug, Markus ^{[3
]}

Garczarczyk, Markus ^{[1
]}

Longo, Francesco ^{[4
]}

Scapin, Valeria ^{[5
]}

机构：

[1] Max Planck Inst Phys & Astrophys, Fohringer Ring 6, D-80805 Munich, Germany

[2] Univ Padua, I-35131 Padua, Italy

[3] Inst Astrofisica Canarias, E-38205 Tenerife, Spain

[4] INFN Trieste, I-34127 Trieste, Italy

[5] Univ Udine, I-33100 Udine, Italy

来源：

GAMMA-RAY BURSTS 2007 | 2008年 / 1000卷

关键词：

MAGIC GRB; gamma-ray; bursts; Cherenkov IACT; gamma astroparticle;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

During two years since the beginning of operation, the MAGIC telescope could observe several GRB events in the prompt and early afterglow phase. Thanks to its innovative design, the telescope could promptly react to incoming GCN alerts, rapidly slew to the burst coordinates within on average 45 seconds, performing observations with an energy threshold spanning from 80 to 200 GeV. The observations did not reveal any gamma-ray emission. The computed upper limits are compatible with a power law extrapolation, where intrinsic fluxes are evaluated taking into account the attenuation due to the scattering in the Metagalactic Radiation Field.

引用

页码：125 / +

页数：2

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