Due to technical problems on the CERN SSO system, logging in is currently failing for many users. Details on the SSB
July 29, 2015 to August 6, 2015
World Forum
Europe/Amsterdam timezone

Performance of the MAGIC telescopes after the major upgrade

Aug 3, 2015, 12:15 PM
Yangtze 1 (World Forum)

Yangtze 1

World Forum

Churchillplein 10 2517 JW Den Haag The Netherlands
Oral contribution GA-IN Parallel GA11 Instruments / Prospects


Julian Sitarek (University of Łódź)


MAGIC is a system of two Imaging Atmospheric Cherenkov Telescopes located in the Canary island of La Palma, Spain. During summer 2011 and 2012 it underwent a major upgrade. The main subsystems upgraded were the MAGIC-I camera and its trigger system and the readout system of both telescopes. We use observations of the Crab Nebula taken at low and medium zenith angles to assess the key performance parameters of the MAGIC stereo system. For low zenith angle observations, the standard trigger threshold of the MAGIC telescopes is about 50 GeV. The integral sensitivity for point-like sources with Crab Nebula-like spectrum above 220 GeV is (0.66+/-0.03)% of Crab Nebula flux in 50 h of observations. The angular resolution, defined as the sigma of a 2-dimensional Gaussian distribution, at energies of a few hundred GeV is below 0.07 degree, while the energy resolution is around 16%. We investigate the effect of the systematic uncertainty on the data taken with the MAGIC telescopes after the upgrade. We estimate that the systematic uncertainties can be divided in the following components: < 15% in energy scale, 11-18% in flux normalization and +/-0.15 for the slope of the energy spectrum.
Collaboration MAGIC
Registration number following "ICRC2015-I/" 500

Primary author

Julian Sitarek (University of Łódź)


Presentation materials

There are no materials yet.