Abstract: We present the first detection of very high energy (VHE;> 100 GeV) gamma-ray emission from MAGIC J2001+435 with the MAGIC stereoscopic system. MAGIC J2001+435 is a BL Lac object with a redshift z> 0.11. This source was identified as a promising candidate for VHE detection using Fermi-LAT photons above 10 GeV, which triggered observations with MAGIC in November 2009 and July – September 2010. The object was detected with MAGIC at a significance of 6.3 standard deviations during a 1.3-hour-long observation on July 16, and exhibited 15.8 % of the flux of the Crab nebula in the energy range above 70 GeV. The source was not detected during the other days, which implies strong variability in the VHE range. Dedicated multi-instrume...
Motivated by the prediction of a high TeV luminosity we investigated whether the blazar 1ES 1727+502...
Blazars, active galactic nuclei whose jet axis is pointed towards the observer, constitute the most ...
The number of known very high energy (VHE) blazars is ~50, which is very small in comparison to the ...
Abstract: Blazars, active galactic nuclei whose jet axis is pointed towards the observer, constitute...
We aim to characterize the broadband emission from 2FGL J2001.1+4352, which has been associated with...
OT 081 is a luminous blazar well known for its variability in many energy bands. The very-high-energ...
MAGIC, a stereoscopic cherenkov telescope array, sensitive to gamma-rays between 50 GeV and several ...
OT 081 is a luminous blazar well known for its variability in many energy bands. The very-high-energ...
Aims: We aim to characterize the broadband emission from 2FGL J2001.1+4352, which has been associate...
Aims. We aim to characterize the broadband emission from 2FGL J2001.1+4352, which has been associate...
Motivated by the prediction of a high TeV luminosity we investigated whether the blazar 1ES 1727+502...
Abstract: We present results of multi-wavelength (MWL) observations of the high-frequency-peaked BL ...
The number of known very high energy (VHE) blazars is ∼50, which is very small in comparison to the ...
Blazars, active galactic nuclei whose jet axis is pointed towards the observer, constitute the most ...
Motivated by the prediction of a high TeV luminosity we investigated whether the blazar 1ES 1727+502...
Blazars, active galactic nuclei whose jet axis is pointed towards the observer, constitute the most ...
The number of known very high energy (VHE) blazars is ~50, which is very small in comparison to the ...
Abstract: Blazars, active galactic nuclei whose jet axis is pointed towards the observer, constitute...
We aim to characterize the broadband emission from 2FGL J2001.1+4352, which has been associated with...
OT 081 is a luminous blazar well known for its variability in many energy bands. The very-high-energ...
MAGIC, a stereoscopic cherenkov telescope array, sensitive to gamma-rays between 50 GeV and several ...
OT 081 is a luminous blazar well known for its variability in many energy bands. The very-high-energ...
Aims: We aim to characterize the broadband emission from 2FGL J2001.1+4352, which has been associate...
Aims. We aim to characterize the broadband emission from 2FGL J2001.1+4352, which has been associate...
Motivated by the prediction of a high TeV luminosity we investigated whether the blazar 1ES 1727+502...
Abstract: We present results of multi-wavelength (MWL) observations of the high-frequency-peaked BL ...
The number of known very high energy (VHE) blazars is ∼50, which is very small in comparison to the ...
Blazars, active galactic nuclei whose jet axis is pointed towards the observer, constitute the most ...
Motivated by the prediction of a high TeV luminosity we investigated whether the blazar 1ES 1727+502...
Blazars, active galactic nuclei whose jet axis is pointed towards the observer, constitute the most ...
The number of known very high energy (VHE) blazars is ~50, which is very small in comparison to the ...