most citedThe major upgrade of the MAGIC telescopes, Part I: The hardware improvements and the commissioning of the system

265 citations · 659 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.IM201530 cited

FACT - Monitoring Blazars at Very High Energies

D. Dorner, M. L. Ahnen, M. Bergmann +26

The First G-APD Cherenkov Telescope (FACT) was built on the Canary Island of La Palma in October 2011 as a proof of principle for silicon based photosensors in Cherenkov Astronomy.…

astro-ph.HE2014184 cited

Black hole lightning due to particle acceleration at subhorizon scales

MAGIC Collaboration, J. Aleksić, S. Ansoldi +151

Supermassive black holes with masses of millions to billions of solar masses are commonly found in the centers of galaxies. Astronomers seek to image jet formation using radio inte…

astro-ph.HE201420 cited

Discovery of very high energy gamma-ray emission from the blazar 1ES 0033+595 by the MAGIC telescopes

J. Aleksić, S. Ansoldi, L. A. Antonelli +157

The number of known very high energy (VHE) blazars is , which is very small in comparison to the number of blazars detected in other frequencies. This situation is a hand…

astro-ph.HE201475 cited

Multiwavelength observations of Mrk 501 in 2008

MAGIC Collaboration, J. Aleksić, S. Ansoldi +256

Mrk 501 is one of the brightest blazars at TeV energies and has been extensively studied since its first VHE detection in 1996. Our goal is to characterize in detail the source gam…

astro-ph.IM2014265 cited

The major upgrade of the MAGIC telescopes, Part I: The hardware improvements and the commissioning of the system

MAGIC Collaboration, J. Aleksic, S. Ansoldi +162

The MAGIC telescopes are two Imaging Atmospheric Cherenkov Telescopes (IACTs) located on the Canary island of La Palma. The telescopes are designed to measure Cherenkov light from…

astro-ph.HE201440 cited

Discovery of TeV gamma-ray emission from the pulsar wind nebula 3C 58 by MAGIC

MAGIC Collaboration, J. Aleksić, S. Ansoldi +145

The pulsar wind nebula (PWN) 3C 58 is one of the historical very-high-energy (VHE; E>100 GeV) gamma-ray source candidates. It is energized by one of the highest spin-down power pul…