activity
20032018
most citedVariable VHE gamma-ray emission from Markarian 501

547 citations · 8.3k across the 89 of their papers we have counts for

collaborators

90 papers

astro-ph.HE2018★ 132 cited

Long-term optical monitoring of TeV emitting Blazars

K. Nilsson, E. Lindfors, L. O. Takalo +17

We present 10 years of R-band monitoring data of 31 northern blazars which were either detected at very high energy (VHE) gamma rays or listed as potential VHE gamma-ray emitters.…

astro-ph.HE2016★ 15 cited

Multi-Wavelength Observations of the Blazar 1ES 1011+496 in Spring 2008

The MAGIC Collaboration, M. L. Ahnen, S. Ansoldi +158

The BL Lac object 1ES 1011+496 was discovered at Very High Energy gamma-rays by MAGIC in spring 2007. Before that the source was little studied in different wavelengths. Therefore…

astro-ph.HE2013★ 135 cited

The awakening of BL Lacertae: observations by Fermi, Swift, and the GASP-WEBT

C. M. Raiteri, M. Villata, F. D'Ammando +4

Since the launch of the Fermi satellite, BL Lacertae has been moderately active at gamma-rays and optical frequencies until May 2011, when the source started a series of strong fla…

astro-ph.HE2012★ 39 cited

The Simultaneous Low State Spectral Energy Distribution of 1ES 2344+514 from Radio to Very High Energies

MAGIC Collaboration, J. Aleksić, L. A. Antonelli +191

[Abridged] Context. To construct and interpret the spectral energy distribution (SED) of BL Lacertae objects, simultaneous broad-band observations are mandatory. Aims. We present t…

astro-ph.HE2012★ 64 cited

Variability of the blazar 4C 38.41 (B3 1633+382) from GHz frequencies to GeV energies

C. M. Raiteri, M. Villata, P. S. Smith +74

The quasar-type blazar 4C 38.41 (B3 1633+382) experienced a large outburst in 2011, which was detected throughout the entire electromagnetic spectrum. We present the results of low…

astro-ph.HE2012★ 42 cited

MAGIC observations of the giant radio galaxy M87 in a low-emission state between 2005 and 2007

MAGIC Collaboration, J. Aleksić, E. A. Alvarez +155

We present the results of a long M87 monitoring campaign in very high energy -rays with the MAGIC-I Cherenkov telescope. We aim to model the persistent non-thermal jet emission…