Sabrina Einecke

TL;DR: The Cherenkov Telescope Array (CTA) as discussed by the authors is a very high-energy (VHE) gamma ray observatory with an international collaboration with more than 1000 members from 27 countries in Europe, Asia, Africa and North and South America.

TL;DR: In this paper, the MAGIC-I camera and its trigger system were replaced with a new one for low and medium zenith angles to assess the key performance parameters of MAGIC stereo system for point-like sources with Crab Nebula-like spectrum.

TL;DR: The Cherenkov Telescope Array (CTA) as mentioned in this paper is the major global observatory for very high energy gamma-ray astronomy over the next decade and beyond, covering a huge range in photon energy from 20 GeV to 300 TeV.

TL;DR: In this article, the authors presented the first joint analysis of gamma-ray data from the MAGIC Cherenkov telescopes and the Fermi Large Area Telescope (LAT) to search for gamma signals from dark matter annihilation in dwarf satellite galaxies, and obtained limits on the annihilation cross-section for dark matter particle masses between 10 GeV and 100 TeV.

TL;DR: The first G-APT Cherenkov Telescope (FACT) as mentioned in this paper was designed to detect cosmic gamma-rays with energies from several hundred GeV up to about 10 TeV using the Imaging AtmosphericCherenkov Technique.