International audienceWe present here the results of the analysis of the $\gamma$-ray blazar, 1ES 1215+303, over a 10-year period, from 2008 to 2017, measured at high energies (HE; 200 MeV $$ 100 GeV) by Fermi-LAT and VERITAS. This is the longest temporal study of this high-frequency-peaked BL Lac object (HBL) at $\gamma$-ray energies to date. The spectrum follows a log parabola over this time period, and its HE and VHE spectra are well-connected. Its flux is sufficiently strong at HE to allow us to bin the Fermi-LAT data in 3-day intervals, enabling us to investigate the temporal evolution of the flux in unprecedented detail. Several flaring episodes were detected and evidence for an overall trend of increasing flux over the span of the 10...
We report on the VERITAS discovery of very high energy (VHE) gamma-ray emission above 200 GeV from t...
We report on VERITAS observations of the BL Lac object B2 1215+30 between 2008 and 2012. During this...
The number of known very high energy (VHE) blazars is ∼50, which is very small in comparison to the ...
International audienceWe present here the results of the analysis of the $\gamma$-ray blazar, 1ES 12...
International audienceBlazars are known for their variability on a wide range of timescales at all w...
Blazars are known for their variability on a wide range of timescales at all wavelengths. Most studi...
We present results from an intensive VERITAS monitoring campaign of the high-frequency peaked BL Lac...
The high-frequency peaked BL Lac type object (HBL) 1ES 1959+650 is one of the brightest blazars in t...
We present results from an intensive VERITAS monitoring campaign of the high-frequency peaked BL Lac...
International audienceWe report on the recent flaring activities from the BL Lac source 1ES 1215+303...
The high-frequency peaked BL Lac type object (HBL) 1ES 1959+650 is one of the brightest blazars in t...
Context. The BL Lac object 1ES 0647+250 is one of the few distant γ-ray emitting blazars detected at...
Context. The BL Lac object 1ES 0647+250 is one of the few distant γ-ray emitting blazars detected at...
Blazars are known for their variability on a wide range of timescales at all wavelengths. Most studi...
We report on VERITAS observations of the BL Lac object B2 1215+30 between 2008 and 2012. During this...
We report on the VERITAS discovery of very high energy (VHE) gamma-ray emission above 200 GeV from t...
We report on VERITAS observations of the BL Lac object B2 1215+30 between 2008 and 2012. During this...
The number of known very high energy (VHE) blazars is ∼50, which is very small in comparison to the ...
International audienceWe present here the results of the analysis of the $\gamma$-ray blazar, 1ES 12...
International audienceBlazars are known for their variability on a wide range of timescales at all w...
Blazars are known for their variability on a wide range of timescales at all wavelengths. Most studi...
We present results from an intensive VERITAS monitoring campaign of the high-frequency peaked BL Lac...
The high-frequency peaked BL Lac type object (HBL) 1ES 1959+650 is one of the brightest blazars in t...
We present results from an intensive VERITAS monitoring campaign of the high-frequency peaked BL Lac...
International audienceWe report on the recent flaring activities from the BL Lac source 1ES 1215+303...
The high-frequency peaked BL Lac type object (HBL) 1ES 1959+650 is one of the brightest blazars in t...
Context. The BL Lac object 1ES 0647+250 is one of the few distant γ-ray emitting blazars detected at...
Context. The BL Lac object 1ES 0647+250 is one of the few distant γ-ray emitting blazars detected at...
Blazars are known for their variability on a wide range of timescales at all wavelengths. Most studi...
We report on VERITAS observations of the BL Lac object B2 1215+30 between 2008 and 2012. During this...
We report on the VERITAS discovery of very high energy (VHE) gamma-ray emission above 200 GeV from t...
We report on VERITAS observations of the BL Lac object B2 1215+30 between 2008 and 2012. During this...
The number of known very high energy (VHE) blazars is ∼50, which is very small in comparison to the ...