Study of Gamma-Ray Bursts observed by MAGIC experiment.
III - Astrofisica
Aula 32B-1 - Giovedì 20 h 11:00 - 13:00
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This work is focused on the observational strategy for transient sources with the MAGIC experiment, a stereoscopic system of two Imaging Atmospheric Cherenkov Telescopes (IACTs) used to detect $\gamma$-rays. The fast response time of the instrument and its ability to work at a low energy threshold allow to get constraining upper limits on the value of the flux emitted by these sources. These limits are then compared with a theoretical model in order to evaluate the Syncrotron-Self Compton (SSC) emission for high and very high energies.