M. Laatiaoui

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: The MAGIC telescope took data of very high energy gamma-ray emission from the blazar Markarian 421 (Mrk 421) between 2004 November and 2005 April as mentioned in this paper, and a combined analysis of data samples recorded under different observational conditions, down to gamma- ray energies of 100 GeV.

TL;DR: The highfrequency-peaked BL Lacertae object Markarian 180 (Mrk 180) was observed to have an optical outburst in 2006 March, triggering a Target of Opportunity observation with the MAGIC telescope as discussed by the authors.

TL;DR: In this article, the MAGIC observations of the source HESS J1834 - 087 were used to detect a differential gamma-ray flux consistent with a power law, described as dN(gamma)/(dA dt dE) = (3.7 +/- 0.6) x 10(-12) (E/TeV)-1.3 -0.3 (W41).

TL;DR: MAGIC as discussed by the authors is the largest ground-based gamma ray telescope with an energy threshold as low as 30 GeV, and it is scheduled to reach full operation by the end of 2003.