M. Meyer

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: The detection of variable gamma-ray emission above 100 gigaelectron volts from the microquasar LS I 61 + 303 is reported, which suggests that the emission is periodic.

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, the MAGIC observations were analyzed for a possible correlation with energy, as suggested by some models of quantum gravity (QG), which predict a vacuum refractive index similar or equal to 1 + (E/M-QGn)(n), n = 1, 2.71 +/- 2.57) x 10(-6) s/GeV2, respectively.