activity
20192022
most citedInvestigating the blazar TXS 0506+056 through sharp multi-wavelength eyes during 2017-2019

29 citations · 82 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.HE202212 cited

Gamma-ray observations of MAXI J1820+070 during the 2018 outburst

H. Abe, S. Abe, V. A. Acciari +439

MAXI J1820+070 is a low-mass X-ray binary with a black hole as a compact object. This binary underwent an exceptionally bright X-ray outburst from March to October 2018, showing ev…

astro-ph.HE202229 cited

Investigating the blazar TXS 0506+056 through sharp multi-wavelength eyes during 2017-2019

MAGIC Collaboration, V. A. Acciari, T. Aniello +213

The blazar TXS 0506+056 got into the spotlight of the astrophysical community in September 2017, when a high-energy neutrino detected by IceCube (IceCube-170922A) was associated at…

astro-ph.HE202110 cited

Statistical properties of flux variations in blazar light curves at GeV and TeV energies

Sarah M. Wagner, Paul R. Burd, Daniela Dorner +23

Despite numerous detections of individual flares, the physical origin of the rapid variability observed from blazars remains uncertain. Using Bayesian blocks and the Eisenstein-Hut…

astro-ph.HE20211 cited

Relentless multi-wavelength variability of Mrk 421 and Mrk 501

Vitalii Sliusar, Axel Arbet-Engels, Dominik Baack +18

Mrk 421 and Mrk 501 are two close, bright and well-studied high-synchrotron-peaked blazars, which feature bright and persistent GeV and TeV emission. We use the longest and densest…

astro-ph.HE20211 cited

Multi-wavelength study of Mrk 421 during a TeV flare

A. Gokus, A. Kreikenbohm, K. Leiter +31

The blazar Mrk 421 shows frequent, short flares in the TeV energy regime. Due to the fast nature of such episodes, we often fail to obtain sufficient simultaneous information about…

astro-ph.HE202028 cited

An intermittent extreme BL Lac: MWL study of 1ES 2344+514 in an enhanced state

MAGIC Collaboration, V. A. Acciari, S. Ansoldi +215

Extreme High-frequency BL~Lacs (EHBL) feature their synchrotron peak of the broadband spectral energy distribution (SED) at 10\,Hz. The BL~Lac object 1ES~23…