Denis Bastieri

TL;DR: In this paper, the authors present the simultaneous Swift and Fermi observations of the bright GRB 100728A and its afterglow and discuss the broadband properties of this burst within both the internal and external shock scenarios, with a particular emphasis on the relation between X-ray flares, the GeV emission and a continued long-duration central engine activity as their power source.

TL;DR: The Cherenkov Telescope Array (CTA) as mentioned in this paper is the major next-generation observatory for ground-based very high-energy gamma-ray astronomy, which will improve the sensitivity of current groundbased instruments by a factor of five to twenty, depending on the energy, greatly improving both their angular and energy resolutions over four decades in energy.

TL;DR: The Major Atmospheric Gamma Imaging Cerenkov (MAGIC) telescope participated in three multi-wavelength (MWL) campaigns, observing the blazar Markarian (Mkn) 421 during the nights of April 28 and 29, 2006, and June 14, 2006.

TL;DR: In this paper, the authors reported the discovery by the Large Area Telescope (LAT) onboard the Fermi Gamma-ray Space Telescope of high-energy gamma-ray (GeV) emission from the flat-spectrum radio quasar PKS 1454-354 (z=1.424).

TL;DR: In this article, the authors reported the discovery of γ-ray pulsations from the young radio and X-ray PSR J0205 + 6449 located in the Galactic supernova remnant 3C 58.4 GeV.