The high-frequency peaked BL Lac type object (HBL) 1ES 1959+650 is one of the brightest blazars in the very-high-energy (VHE, E & 100 GeV) gamma-ray sky. HBLs have been proposed as possible neutrino emitters implying the presence of hadrons in the emission mechanisms. In 2002, AMANDA reported neutrino candidates from this source simultaneously observed with a gamma-ray flaring activity without an X-ray emission enhancement, interpreted as an orphan flare. Standard one-zone synchrotron self-Compton (SSC) emission models cannot explain this behavior. The MAGIC telescopes have been observing 1ES 1959+650 since 2004. An extreme outburst triggered by multiwavelength observations reaching 300% of the Crab nebula flux level above 300 GeV was detec...
Extreme High-frequency BL~Lacs (EHBL) feature their synchrotron peak of the broadband spectral energ...
Motivated by the prediction of a high TeV luminosity we investigated whether the blazar 1ES 1727+502...
Motivated by the prediction of a high TeV luminosity we investigated whether the blazar 1ES 1727+502...
The high-frequency peaked BL Lac type object (HBL) 1ES 1959+650 is one of the brightest blazars in t...
1ES 1959+650 is a bright TeV high-frequency-peaked BL Lac object exhibiting interesting features lik...
Context. The BL Lac object 1ES 0647+250 is one of the few distant γ-ray emitting blazars detected at...
Context. The BL Lac object 1ES 0647+250 is one of the few distant γ-ray emitting blazars detected at...
The high-frequency-peaked BL Lac (HBL) 1ES 0806+524 (z = 0.138) was discovered in very high energy (...
The high-peaked BL Lac object 1ES 0647+250 is one of the few distant blazars detected at very-high-e...
International audienceWe present here the results of the analysis of the $\gamma$-ray blazar, 1ES 12...
The high-frequency-peaked BL Lac (HBL) 1ES 0806+524 (z = 0.138) was discovered in very high energy (...
Extreme High-frequency BL~Lacs (EHBL) feature their synchrotron peak of the broadband spectral energ...
Motivated by the prediction of a high TeV luminosity we investigated whether the blazar 1ES 1727+502...
Motivated by the prediction of a high TeV luminosity we investigated whether the blazar 1ES 1727+502...
The high-frequency peaked BL Lac type object (HBL) 1ES 1959+650 is one of the brightest blazars in t...
1ES 1959+650 is a bright TeV high-frequency-peaked BL Lac object exhibiting interesting features lik...
Context. The BL Lac object 1ES 0647+250 is one of the few distant γ-ray emitting blazars detected at...
Context. The BL Lac object 1ES 0647+250 is one of the few distant γ-ray emitting blazars detected at...
The high-frequency-peaked BL Lac (HBL) 1ES 0806+524 (z = 0.138) was discovered in very high energy (...
The high-peaked BL Lac object 1ES 0647+250 is one of the few distant blazars detected at very-high-e...
International audienceWe present here the results of the analysis of the $\gamma$-ray blazar, 1ES 12...
The high-frequency-peaked BL Lac (HBL) 1ES 0806+524 (z = 0.138) was discovered in very high energy (...
Extreme High-frequency BL~Lacs (EHBL) feature their synchrotron peak of the broadband spectral energ...
Motivated by the prediction of a high TeV luminosity we investigated whether the blazar 1ES 1727+502...
Motivated by the prediction of a high TeV luminosity we investigated whether the blazar 1ES 1727+502...