Author/Authors :
Jogler، نويسنده , , T. and Bosch-Ramon، نويسنده , , V. and Cortina، نويسنده , , J. and Paredes، نويسنده , , J.M. and Perez-Torres، نويسنده , , M.A. and Ribَ، نويسنده , , M. and Rico، نويسنده , , J. and Sidro، نويسنده , , N. and Torres، نويسنده , , D.F.، نويسنده ,
Abstract :
The MAGIC collaboration discovered with their 17 m diameter imaging atmospheric Cherenkov telescope, the High Mass X-ray Binary (HMXB) LS I + 61 303 at VHE ( VHE , E > 50 GeV ) γ -rays. The emission from LS I + 61 303 was found to be variable, and the source was visible at energies above 200 GeV 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.
Keywords :
binary , ? -Rays , LSI , TEV
