The high-frequency-peaked BL Lac (HBL) 1ES 0806+524 (z =0.138) was discovered in very high energy (VHE) γ-rays in 2008. Until now, the broad-band spectrum of 1ES 0806+524 has been only poorly characterized, in particular at high energies. We analysed multiwavelength observations from γ-rays to radio performed from 2011 January to March, which were triggered by the high activity detected at optical frequencies. These observations constitute the most precise determination of the broad-band emission of 1ES 0806+524 to date. The stereoscopic Major Atmospheric Gamma-Ray Imaging Cherenkov (MAGIC) observations yielded a γ-ray signal above 250 GeV of (3.7 ± 0.7) per cent of the Crab Nebula flux with a statistical significance of 9.9σ. The multiwave...
The BL Lac object 1ES 1011+496 was discovered at very high energy (VHE, E > 100GeV) γ-rays by Major ...
PG 1553+113 is a very high energy (VHE, E > 100 GeV) γ -ray emitter classified as a BL Lac object...
Extreme high-frequency BL Lacs (EHBL) feature their synchrotron peak of the broad-band spectral ener...
The high-frequency-peaked BL Lac (HBL) 1ES 0806+524 (z = 0.138) was discovered in very high energy (...
The high-frequency-peaked BL Lac (HBL) 1ES 0806+524 (z=0.138) was discovered in very high energy (VH...
The high-frequency-peaked BL Lac (HBL) 1ES 0806+524 (z = 0.138) was discovered in VHE $\gamma$ rays ...
The BL Lac object 1ES 1011+496 was discovered at very high energy (VHE, E > 100GeV) γ-rays by Major ...
PG 1553+113 is a very high energy (VHE, E > 100 GeV) γ -ray emitter classified as a BL Lac object...
Extreme high-frequency BL Lacs (EHBL) feature their synchrotron peak of the broad-band spectral ener...
The high-frequency-peaked BL Lac (HBL) 1ES 0806+524 (z = 0.138) was discovered in very high energy (...
The high-frequency-peaked BL Lac (HBL) 1ES 0806+524 (z=0.138) was discovered in very high energy (VH...
The high-frequency-peaked BL Lac (HBL) 1ES 0806+524 (z = 0.138) was discovered in VHE $\gamma$ rays ...
The BL Lac object 1ES 1011+496 was discovered at very high energy (VHE, E > 100GeV) γ-rays by Major ...
PG 1553+113 is a very high energy (VHE, E > 100 GeV) γ -ray emitter classified as a BL Lac object...
Extreme high-frequency BL Lacs (EHBL) feature their synchrotron peak of the broad-band spectral ener...