Motivated by the Costamante & Ghisellini (2002) predictions we investigated if the blazar 1ES 1727+502 (z=0.055) is emitting very high energy (VHE, E>100 GeV) gamma rays. We observed the BL Lac object 1ES 1727+502 in stereoscopic mode with the two MAGIC telescopes during 14 nights between May 6th and June 10th 2011, for a total effective observing time of 12.6 hours. For the study of the multiwavelength spectral energy distribution (SED) we use simultaneous optical R-band data from the KVA telescope, archival UV/optical and X-ray observations by instruments UVOT and XRT on board of the Swift satellite and high energy (HE, 0.1 GeV - 100 GeV) gamma-ray data from the Fermi-LAT instrument. We detect, for the first time, VHE gamma-ray emi...
The number of known very high energy (VHE) blazars is ∼50, which is very small in comparison to the ...
The Major Atmospheric Gamma-ray Imaging Cherenkov (MAGIC) telescopes observed S2 0109+22 in 2015 Jul...
The Major Atmospheric Gamma-ray Imaging Cherenkov (MAGIC) telescopes observed S2 0109+22 in 2015 Jul...
Motivated by the prediction of a high TeV luminosity we investigated whether the blazar 1ES 1727+502...
Motivated by the Costamante & Ghisellini (2002) predictions we investigated if the blazar 1ES 1727+5...
Motivated by the prediction of a high TeV luminosity we investigated whether the blazar 1ES 1727+502...
The number of known very high energy (VHE) blazars is ∼50, which is very small in comparison to the ...
We study the non-thermal jet emission of the BL Lac object B3 2247+381 during a high optical state. ...
Aims. We present a study of the very high energy (VHE ; E>100 GeV) gamma-ray emission of the blaz...
The number of known very high energy (VHE) blazars is ∼50, which is very small in comparison to the ...
The number of known very high energy (VHE) blazars is ~50, which is very small in comparison to the ...
Extreme high-energy-peaked BL Lac objects (EHBLs) are an emerging class of blazars. Their typical tw...
We aim to characterize the broadband emission from 2FGL J2001.1+4352, which has been associated with...
We present the first detection of the nearby (z=0.084) low-luminosity BL Lac object 1ES 1741+196 in ...
We present a study of the very high energy (VHE; E > 100 GeV) gamma-ray emission of the blazar PKS 1...
The number of known very high energy (VHE) blazars is ∼50, which is very small in comparison to the ...
The Major Atmospheric Gamma-ray Imaging Cherenkov (MAGIC) telescopes observed S2 0109+22 in 2015 Jul...
The Major Atmospheric Gamma-ray Imaging Cherenkov (MAGIC) telescopes observed S2 0109+22 in 2015 Jul...
Motivated by the prediction of a high TeV luminosity we investigated whether the blazar 1ES 1727+502...
Motivated by the Costamante & Ghisellini (2002) predictions we investigated if the blazar 1ES 1727+5...
Motivated by the prediction of a high TeV luminosity we investigated whether the blazar 1ES 1727+502...
The number of known very high energy (VHE) blazars is ∼50, which is very small in comparison to the ...
We study the non-thermal jet emission of the BL Lac object B3 2247+381 during a high optical state. ...
Aims. We present a study of the very high energy (VHE ; E>100 GeV) gamma-ray emission of the blaz...
The number of known very high energy (VHE) blazars is ∼50, which is very small in comparison to the ...
The number of known very high energy (VHE) blazars is ~50, which is very small in comparison to the ...
Extreme high-energy-peaked BL Lac objects (EHBLs) are an emerging class of blazars. Their typical tw...
We aim to characterize the broadband emission from 2FGL J2001.1+4352, which has been associated with...
We present the first detection of the nearby (z=0.084) low-luminosity BL Lac object 1ES 1741+196 in ...
We present a study of the very high energy (VHE; E > 100 GeV) gamma-ray emission of the blazar PKS 1...
The number of known very high energy (VHE) blazars is ∼50, which is very small in comparison to the ...
The Major Atmospheric Gamma-ray Imaging Cherenkov (MAGIC) telescopes observed S2 0109+22 in 2015 Jul...
The Major Atmospheric Gamma-ray Imaging Cherenkov (MAGIC) telescopes observed S2 0109+22 in 2015 Jul...