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MAGIC is a system of two Imaging Atmospheric Cherenkov Telescopes located atthe Canary Island of La Palma, designed to observe gamma rays with energiesabove 50 GeV. Recently it has undergone an upgrade of the camera, digitaltrigger and readout systems. The upgrade has led to an improvement in theperformance of the telescopes, especially in the lower energy range. Weevaluate the performance of the upgraded MAGIC telescopes using Monte Carlosimulations and a large sample of Crab Nebula data. We study differential andintegral sensitivity of the system, its angular resolution as well as itsenergy resolution.

Physics performance of the upgraded MAGIC telescopes obtained with Crab Nebula data