We present the first detection of the nearby (z = 0.084) low-luminosity BL Lac object 1ES 1741+196 in the very high energy (E > 100 GeV) band. This object lies in a triplet of interacting galaxies. Early predictions had suggested 1ES 1741+196 to be, along with several other high-frequency BL Lac sources, within the reach of MAGIC detectability. Its detection by MAGIC, later confirmed by VERITAS, helps to expand the small population of known TeV BL Lacs. The source was observed with the MAGIC telescopes between 2010 April and 2011 May, collecting 46 h of good quality data. These observations led to the detection of the source at 6.0 σ confidence level, with a steady flux F(>100 GeV) = (6.4 ± 1.7stat ± 2.6syst) × 10-12 ph cm-2s-1 and a differ...
Very High Energy (VHE) gamma-ray emission from the flat spectrum radio quasar PKS 1222+21 (4C 21.35,...
SNR G24.7+0.6 is a 9.5 kyrs radio and γ-ray supernova remnant evolving in a dense medium. In the GeV...
Extreme high-frequency BL Lacs (EHBL) feature their synchrotron peak of the broad-band spectral ener...
We present the first detection of the nearby (z = 0.084) low-luminosity BL Lac object 1ES 1741+196 i...
We present the first detection of the nearby (z = 0.084) low-luminosity BL Lac object 1ES 1741+196 i...
We present the first detection of the nearby (z=0.084) low-luminosity BL Lac object 1ES 1741+196 in ...
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 ...
PG 1553+113 is a very high energy (VHE, E > 100 GeV) γ -ray emitter classified as a BL Lac object...
Extreme high-energy-peaked BL Lac objects (EHBLs) are an emerging class of blazars. Their typical tw...
The number of known very high energy (VHE) blazars is ∼50, which is very small in comparison to the ...
The flat-spectrum radio quasar PKS 1441+25 at a redshift of z = 0.940 is detected between 40 and 250...
PG 1553+113 is a very high energy (VHE, E>100 GeV) γ-ray emitter classified as a BL Lac object. Its ...
Extreme high-frequency-peaked BL Lac objects (EHBLs) are blazars that exhibit extremely energetic sy...
Motivated by the Costamante & Ghisellini (2002) predictions we investigated if the blazar 1ES 1727+5...
Very High Energy (VHE) gamma-ray emission from the flat spectrum radio quasar PKS 1222+21 (4C 21.35,...
SNR G24.7+0.6 is a 9.5 kyrs radio and γ-ray supernova remnant evolving in a dense medium. In the GeV...
Extreme high-frequency BL Lacs (EHBL) feature their synchrotron peak of the broad-band spectral ener...
We present the first detection of the nearby (z = 0.084) low-luminosity BL Lac object 1ES 1741+196 i...
We present the first detection of the nearby (z = 0.084) low-luminosity BL Lac object 1ES 1741+196 i...
We present the first detection of the nearby (z=0.084) low-luminosity BL Lac object 1ES 1741+196 in ...
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 ...
PG 1553+113 is a very high energy (VHE, E > 100 GeV) γ -ray emitter classified as a BL Lac object...
Extreme high-energy-peaked BL Lac objects (EHBLs) are an emerging class of blazars. Their typical tw...
The number of known very high energy (VHE) blazars is ∼50, which is very small in comparison to the ...
The flat-spectrum radio quasar PKS 1441+25 at a redshift of z = 0.940 is detected between 40 and 250...
PG 1553+113 is a very high energy (VHE, E>100 GeV) γ-ray emitter classified as a BL Lac object. Its ...
Extreme high-frequency-peaked BL Lac objects (EHBLs) are blazars that exhibit extremely energetic sy...
Motivated by the Costamante & Ghisellini (2002) predictions we investigated if the blazar 1ES 1727+5...
Very High Energy (VHE) gamma-ray emission from the flat spectrum radio quasar PKS 1222+21 (4C 21.35,...
SNR G24.7+0.6 is a 9.5 kyrs radio and γ-ray supernova remnant evolving in a dense medium. In the GeV...
Extreme high-frequency BL Lacs (EHBL) feature their synchrotron peak of the broad-band spectral ener...