activity
20072015
most citedVariable VHE gamma-ray emission from Markarian 501

547 citations · 738 across the 5 of their papers we have counts for

collaborators

6 papers

astro-ph.HE2015★ 129 cited

The 2009 multiwavelength campaign on Mrk 421: Variability and correlation studies

MAGIC Collaboration, J. Aleksić, S. Ansoldi +270

We performed a 4.5-month multi-instrument campaign (from radio to VHE gamma rays) on Mrk421 between January 2009 and June 2009, which included VLBA, F-GAMMA, GASP-WEBT, Swift, RXTE…

astro-ph.HE2014★ 40 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…

astro-ph.HE2014★ 3 cited

Search for Very-High-Energy Gamma Rays from the z = 0.896 Quasar 4C +55.17 with the MAGIC telescopes

MAGIC Collaboration, J. Aleksić, S. Ansoldi +157

The bright gamma-ray quasar 4C +55.17 is a distant source () with a hard spectrum at GeV energies as observed by the Large Area Telescope (LAT) on board the {\it Fermi}…

hep-ph2013

Optimized dark matter searches in deep observations of Segue 1 with MAGIC

J. Aleksić, S. Ansoldi, L. A. Antonelli +156

We present the results of stereoscopic observations of the satellite galaxy Segue 1 with the MAGIC Telescopes, carried out between 2011 and 2013. With almost 160 hours of good-qual…

astro-ph2008★ 19 cited

MAGIC upper limits to the VHE gamma-ray flux of 3C454.3 in high emission state

H. Anderhub, S. Vercellone, I. Donnarumma +2

We report upper limits to the very high energy flux (E>100 GeV) of the flat spectrum radio quasar 3C454.3 (z=0.859) derived by the Cherenkov telescope MAGIC during the high states…

astro-ph2007★ 547 cited

Variable VHE gamma-ray emission from Markarian 501

J. Albert et al

The blazar Markarian 501 (Mrk 501) was observed at energies above 0.10 TeV with the MAGIC telescope from May through July 2005. The high sensitivity of the instrument enabled the d…