Between the beginning of its full-scale scientific operations in 2007 and 2012, the VERITAS Cherenkov telescope array observed more than 130 blazars; of these, 26 were detected as very-high-energy (VHE; E > 100 GeV) γ-ray sources. In this work, we present the analysis results of a sample of 114 undetected objects. The observations constitute a total live-time of ~570 hr. The sample includes several unidentified Fermi-Large Area Telescope (LAT) sources (located at high Galactic latitude) as well as all the sources from the second Fermi-LAT catalog that are contained within the field of view of the VERITAS observations. We have also performed optical spectroscopy measurements in order to estimate the redshift of some of these blazars that do ...
Very-high-energy (VHE; > 100 GeV) gamma-ray emission from the blazar RGB J2243+203 was discov...
We report on the VERITAS discovery of very high energy (VHE) gamma-ray emission above 200 GeV from t...
International audienceWe report on our study of high-energy properties of two peculiar TeV emitters:...
Between the beginning of its full-scale scientific operations in 2007 and 2012, the VERITAS Cherenko...
Between the beginning of its full-scale scientific operations in 2007 and 2012, the VERITAS Cherenko...
Abstract: The VERITAS array of Cherenkov telescopes was used to observe ≈ 130 blazars from 2007 to 2...
Aims. We study the possible detection of and properties of very high-energy (VHE) γ-ray emission (in...
VERITAS is an array of four 12-m atmospheric Cherenkov telescopes, designed to observe the very-high...
Aims. We study the possible detection of and properties of very high-energy (VHE) γ-ray emission (in...
We report on VERITAS very high energy (VHE; E > 100 GeV) observations of six blazars selected from t...
The number of known very high energy (VHE) blazars is ~50, which is very small in comparison to the ...
Context. Blazars are the most numerous class of high-energy (HE; E ∼ 50 MeV−100 GeV) and very high-e...
HESS J1943+213 is a very high energy (VHE; >100 GeV) γ-ray source in the direction of the Galactic p...
The number of known very high energy (VHE) blazars is \u2dc50, which is very small in comparison to ...
The number of known very high energy (VHE) blazars is ∼50, which is very small in comparison to the ...
Very-high-energy (VHE; > 100 GeV) gamma-ray emission from the blazar RGB J2243+203 was discov...
We report on the VERITAS discovery of very high energy (VHE) gamma-ray emission above 200 GeV from t...
International audienceWe report on our study of high-energy properties of two peculiar TeV emitters:...
Between the beginning of its full-scale scientific operations in 2007 and 2012, the VERITAS Cherenko...
Between the beginning of its full-scale scientific operations in 2007 and 2012, the VERITAS Cherenko...
Abstract: The VERITAS array of Cherenkov telescopes was used to observe ≈ 130 blazars from 2007 to 2...
Aims. We study the possible detection of and properties of very high-energy (VHE) γ-ray emission (in...
VERITAS is an array of four 12-m atmospheric Cherenkov telescopes, designed to observe the very-high...
Aims. We study the possible detection of and properties of very high-energy (VHE) γ-ray emission (in...
We report on VERITAS very high energy (VHE; E > 100 GeV) observations of six blazars selected from t...
The number of known very high energy (VHE) blazars is ~50, which is very small in comparison to the ...
Context. Blazars are the most numerous class of high-energy (HE; E ∼ 50 MeV−100 GeV) and very high-e...
HESS J1943+213 is a very high energy (VHE; >100 GeV) γ-ray source in the direction of the Galactic p...
The number of known very high energy (VHE) blazars is \u2dc50, which is very small in comparison to ...
The number of known very high energy (VHE) blazars is ∼50, which is very small in comparison to the ...
Very-high-energy (VHE; > 100 GeV) gamma-ray emission from the blazar RGB J2243+203 was discov...
We report on the VERITAS discovery of very high energy (VHE) gamma-ray emission above 200 GeV from t...
International audienceWe report on our study of high-energy properties of two peculiar TeV emitters:...