activity
20182021
most citedAn intermittent extreme BL Lac: MWL study of 1ES 2344+514 in an enhanced state

28 citations · 51 across the 3 of their papers we have counts for

collaborators

6 papers

astro-ph.HE202122 cited

The relentless variability of Mrk 421 from the TeV to the radio

Axel Arbet-Engels, Dominik Baack, Matteo Balbo +22

The origin of the gamma-ray emission of the blazar Mrk 421 is still a matter of debate. We used 5.5 years of unbiased observing campaign data, obtained using the FACT telescope and…

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…

astro-ph.HE2020

Study of the variable broadband emission of Markarian 501 during the most extreme Swift X-ray activity

MAGIC Collaboration, V. A. Acciari, S. Ansoldi +185

Mrk501 is a very high-energy (VHE) gamma-ray blazar located at z=0.034. During a period of two weeks in July 2014, the highest X-ray activity of Mrk501 was observed in ~14 years of…

astro-ph.HE20191 cited

5.5 years multi-wavelength variability of Mrk 421: evidences of leptonic emission from the radio to TeV

Vitalii Sliusar, Axel Arbet-Engels, Dominik Baack +25

Mrk 421 is a high-synchrotron-peaked blazar featuring bright and persistent GeV and TeV emission. We use the longest and densest ongoing unbiased observing campaign obtained at TeV…

astro-ph.HE2019

FACT -- Multi-wavelength analysis of more than 30 flares of Mrk 421

Vitalii Sliusar, Axel Arbet-Engels, Dominik Baack +22

Mrk 421 is a high-synchrotron-peaked blazar featuring bright and persistent GeV and TeV emission. We use multi-wavelength light curves of Mrk 421 spanning 5.5 years with FACT (TeV)…

astro-ph.HE2018

The extreme HBL behaviour of Markarian 501 during 2012

M. L. Ahnen, S. Ansoldi, L. A. Antonelli +276

A multiwavelength campaign was organized to take place between March and July of 2012. Excellent temporal coverage was obtained with more than 25 instruments, including the MAGIC,…