Author/Authors :
Baixeras، نويسنده , , C. and Bastieri، نويسنده , , D. and Bigongiari، نويسنده , , C. and Blanch، نويسنده , , O. and Blanchot، نويسنده , , Jochen G. and Bock، نويسنده , , R. and Bretz، نويسنده , , T. and Chilingarian، نويسنده , , A. and Coarasa، نويسنده , , J.A. and Colombo، نويسنده , , E. and Contreras، نويسنده , , J.C. and Corti، نويسنده , , D. and Cortina، نويسنده , , J. and Domingo، نويسنده , , C. and Domingo، نويسنده , , E. and Ferenc، نويسنده ,
Abstract :
Major Atmospheric Gamma Imaging Cherenkov telescope is starting its operations with a set of engineering runs to tune the telescope subsystem elements to be ready for the first physics campaign. Many technical improvements have been developed and implemented in several elements of the telescope to reach the lowest energy threshold ever obtained by an Imaging Atmospheric Cherenkov Telescope. A general description of the telescope is presented. The commissioning of the telescopeʹs elements is described and the expected performances are reviewed with the final detector set-up.
