F. Zandanel

TL;DR: The MAGIC telescope was used to observe the blazar Markarian 501 (Mrk 501) at energies above 100 GeV from May through July 2005 as mentioned in this paper, and the high sensitivity of the instrument enabled the determination of the flux and spectrum of the source on a night-by-night basis.

TL;DR: In this article, very high energy (VHE) gamma-ray observations of the Crab Nebula with the MAGIC telescope were reported, where the gamma spectrum can be described by a curved power law dF/dE = f(0)(E/300 GeV).

TL;DR: The MAGIC observations were performed for a total of 40 hours during 26 nights, spanning the period between 2006 June and November, and the results from the observations in the very high energy band (VHE; GeV) of the black E = 100 g hole X-ray binary (BHXB) Cygnus X-1 were reported in this article.

TL;DR: In this paper, an application of the tree classification method Random Forest (RF), as used in the analysis of data from the ground-based gamma telescope MAGIC, is described, and critical issues of the method and its implementation are discussed.

TL;DR: In this article, the MAGIC J0616 + 225 was used to detect a very high energy (VHE; E-gamma >= 100 GeV) gamma-ray emission located close to the Galactic plane, which is spatially coincident with supernova remnant IC 443.