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20012026
most citedDesign Concepts for the Cherenkov Telescope Array

902 citations · 14.3k across the 242 of their papers we have counts for

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12 papers · 1 filter

astro-ph.HE2017★ 43 cited

Indirect dark matter searches in the dwarf satellite galaxy Ursa Major II with the MAGIC Telescopes

MAGIC Collaboration, M. L. Ahnen, S. Ansoldi +142

The dwarf spheroidal galaxy Ursa Major II (UMaII) is believed to be one of the most dark-matter dominated systems among the Milky Way satellites and represents a suitable target fo…

astro-ph.HE2017★ 2 cited

Gamma rays from microquasars Cygnus X-1 and Cygnus X-3

A. Fernández-Barral, O. Blanch, E. de Oña Wilhelmi +8

Gamma-ray observations of microquasars at high and very-high energies can provide valuable information of the acceleration processes inside the jets, the jet-environment interactio…

astro-ph.HE2017

MAGIC VHE Gamma-Ray Observations Of Binary Systems

Daniela Hadasch, Wlodek Bednarek, Oscar Blanch +13

There are several types of Galactic sources that can potentially accelerate charged particles up to GeV and TeV energies. We present here the results of our observations of the sou…

astro-ph.HE2017★ 45 cited

Constraining Lorentz invariance violation using the Crab Pulsar emission observed up to TeV energies by MAGIC

MAGIC Collaboration, M. L. Ahnen, S. Ansoldi +142

Spontaneous breaking of Lorentz symmetry at energies on the order of the Planck energy or lower is predicted by many quantum gravity theories, implying non-trivial dispersion relat…

astro-ph.IM2017★ 1 cited

Performance of the MAGIC telescopes under moonlight

D. Guberman, P. Colin

MAGIC, a system of two imaging atmospheric Cherenkov telescopes, achieves its best performance under dark conditions, i.e. in absence of moonlight or twilight. Since operating the…

astro-ph.HE2017★ 11 cited

MAGIC observations of the microquasar V404 Cygni during the 2015 outburst

M. L. Ahnen, S. Ansoldi, L. A. Antonelli +142

The microquasar V404 Cygni underwent a series of outbursts in 2015, June 15-31, during which its flux in hard X-rays (20-40 keV) reached about 40 times the Crab Nebula flux. Becaus…