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 ...
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 BL Lac object 1ES 1011+496 was discovered at very high energy (VHE, E > 100GeV) \u3b3-rays by Ma...
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 ...
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 ...
PG 1553+113 is a very high energy (VHE, E > 100 GeV) γ -ray emitter classified as a BL Lac object...
Extreme high-frequency-peaked BL Lac objects (EHBLs) are blazars that exhibit extremely energetic sy...
Extreme high-energy-peaked BL Lac objects (EHBLs) are an emerging class of blazars. Their typical tw...
We present the first detection of the nearby (z = 0.084) low-luminosity BL Lac object 1ES 1741+196 i...
PG 1553+113 is a very high energy (VHE, E>100 GeV) γ-ray emitter classified as a BL Lac object. Its ...
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 BL Lac object 1ES 1011+496 was discovered at very high energy (VHE, E > 100GeV) \u3b3-rays by Ma...
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 ...
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 ...
PG 1553+113 is a very high energy (VHE, E > 100 GeV) γ -ray emitter classified as a BL Lac object...
Extreme high-frequency-peaked BL Lac objects (EHBLs) are blazars that exhibit extremely energetic sy...
Extreme high-energy-peaked BL Lac objects (EHBLs) are an emerging class of blazars. Their typical tw...
We present the first detection of the nearby (z = 0.084) low-luminosity BL Lac object 1ES 1741+196 i...
PG 1553+113 is a very high energy (VHE, E>100 GeV) γ-ray emitter classified as a BL Lac object. Its ...
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 BL Lac object 1ES 1011+496 was discovered at very high energy (VHE, E > 100GeV) \u3b3-rays by Ma...