Speaker
Description
The intermediate synchrotron-peaked BL Lac B2 1811+31 (z=0.117) underwent a period of high activity from the optical band to very-high-energy (VHE; 100 GeV < E < 100 TeV) gamma rays in 2020. Following a high-state detection by the Large Area Telescope (LAT) on board the Fermi Gamma-ray Space Telescope in the high-energy gamma-ray band (HE; 100 MeV < E < 100 GeV), a dedicated multi-wavelength (MWL) campaign from radio to VHE gamma rays was organized. In this campaign, the MAGIC Telescopes detected for the first-time VHE gamma-ray emission from the source and the broad-band emission was precisely characterized. To put this high state into the context of the source long-term emission, we employed an extensive MWL dataset spanning over 18 years from the radio and optical/UV bands to X rays and HE gamma rays.
In this contribution, we present the long-term MWL behaviour of B2 1811+31, with particular emphasis on the high state. We resolve long-term correlated evolution on timescales ranging from years to weeks in the optical and HE gamma-ray band, as well as variability on timescales of few hours at HE gamma rays during the highest activity period. We observed a significant shift of the synchrotron peak frequency during the flaring activity, which led the source to a borderline state between intermediate and high synchrotron-peaked BL Lac. We discuss the evolution of the source MWL emission in terms of particle acceleration and cooling within multiple regions active in the jet and propose a self-consistent leptonic model to interpret the broad-band emission during the high state.
| Collaboration(s) | MAGIC Collaboration, Fermi-LAT Collaboration, multi-wavelength collaborators |
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