E-viri
Recenzirano
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Jogler, T.; Bosch-Ramon, V.; Cortina, J.; Paredes, J.M.; Perez-Torres, M.A.; Ribó, M.; Rico, J.; Sidro, N.; Torres, D.F.
Nuclear instruments & methods in physics research. Section A, Accelerators, spectrometers, detectors and associated equipment, 04/2008, Letnik: 588, Številka: 1-2Journal Article
The MAGIC collaboration discovered with their 17m diameter imaging atmospheric Cherenkov telescope, the High Mass X-ray Binary (HMXB) LS I +61 303 at VHE (VHE,E>50GeV)γ-rays. The emission from LS I +61 303 was found to be variable, and the source was visible at energies above 200GeV in different runs during some orbital phases only. These orbital phases do not coincide with the periastron passage. Here we report the results of the analysis of the LS I +61 303 MAGIC observations.
