The BL Lac Object 1ES 1426+428, at a red-shift of z=0.129, has been monitored by the CAT telescope from February 1998 to June 2000. The accumulation of 26 hours of observations shows a gamma-ray signal of 321 events above 250 GeV at 5.2 standard deviations, determined using data analysis cuts adapted to a weak, steep-spectrum source. The source emission has an average flux of Phi_diff(400 GeV) = 6.73 +/- 1.27stat +/- 1.45syst x 10^-11 /cm^-2/s/TeV, and a very steep spectrum, with a differential spectral index of gamma = -3.60 +/- 0.57 which can be refined to gamma = -3.66 +/- 0.41 using a higher flux data subset. If, as expected from its broad-band properties, the Very High Energy emission is hard at the source, these observations support a...
The BL Lacertae (BL Lac) object 1ES 2344+514 (1ES 2344), at a redshift of 0.044, was discovered as a...
The VERITAS collaboration reports the detection of very-high-energy gamma-ray emission from the high...
The VERITAS collaboration reports the detection of very-high-energy gamma-ray emission from the high...
The BL Lac Object 1ES 1426+428, at a red-shift of z=0.129, has been monitored by the CAT telescope f...
The BL Lac Object 1ES 1426+428, at a red-shift of $z=0.129$, has been monitored by the Ca
A very high energy gamma-ray signal has been detected at the 5.5sigma level from H1426+ 428, an X-ra...
The BL Lac object H1426+428 was recently detected as a high-energy gamma-ray source by the VERITAS c...
The low-frequency peaked BL Lac (LBL) object BL Lacertae was observed with the MAGIC telescope from ...
A very high energy γ-ray signal has been detected at the 5.5 σ level from H1426+428, an X-ray-select...
In 2005 and 2006, the MAGIC telescope observed very high energy gamma-ray emission from the distant ...
In 2005 and 2006, the MAGIC telescope observed very high energy gamma-ray emission from the distant ...
The high-frequency-peaked BL-Lacertae object \objectname{1ES 0806+524}, at redshift z=0.138, was obs...
The MAGIC telescope has observed very high energy gamma-ray emission from the AGN 1ES 2344+514. A ga...
The high-frequency-peaked BL Lacertae object 1ES 0806+524, at redshift z = 0.138, was observed in th...
The BL Lacertae (BL Lac) object 1ES 2344+514 (1ES 2344), at a redshift of 0.044, was discovered as a...
The BL Lacertae (BL Lac) object 1ES 2344+514 (1ES 2344), at a redshift of 0.044, was discovered as a...
The VERITAS collaboration reports the detection of very-high-energy gamma-ray emission from the high...
The VERITAS collaboration reports the detection of very-high-energy gamma-ray emission from the high...
The BL Lac Object 1ES 1426+428, at a red-shift of z=0.129, has been monitored by the CAT telescope f...
The BL Lac Object 1ES 1426+428, at a red-shift of $z=0.129$, has been monitored by the Ca
A very high energy gamma-ray signal has been detected at the 5.5sigma level from H1426+ 428, an X-ra...
The BL Lac object H1426+428 was recently detected as a high-energy gamma-ray source by the VERITAS c...
The low-frequency peaked BL Lac (LBL) object BL Lacertae was observed with the MAGIC telescope from ...
A very high energy γ-ray signal has been detected at the 5.5 σ level from H1426+428, an X-ray-select...
In 2005 and 2006, the MAGIC telescope observed very high energy gamma-ray emission from the distant ...
In 2005 and 2006, the MAGIC telescope observed very high energy gamma-ray emission from the distant ...
The high-frequency-peaked BL-Lacertae object \objectname{1ES 0806+524}, at redshift z=0.138, was obs...
The MAGIC telescope has observed very high energy gamma-ray emission from the AGN 1ES 2344+514. A ga...
The high-frequency-peaked BL Lacertae object 1ES 0806+524, at redshift z = 0.138, was observed in th...
The BL Lacertae (BL Lac) object 1ES 2344+514 (1ES 2344), at a redshift of 0.044, was discovered as a...
The BL Lacertae (BL Lac) object 1ES 2344+514 (1ES 2344), at a redshift of 0.044, was discovered as a...
The VERITAS collaboration reports the detection of very-high-energy gamma-ray emission from the high...
The VERITAS collaboration reports the detection of very-high-energy gamma-ray emission from the high...