Add to ORKGThe flat-spectrum radio-quasar 3C279 (z=0.536) is the most distant object detected at very high energy (VHE) gamma-rays. It is thus an important beacon for the study of the interaction of the VHE gamma-rays with the Extra-galactic Background Light (EBL). Previous observations by EGRET showed a highly variable flux that can differ up to a factor of 100. In this paper results from an observation campaign with the MAGIC telescope during an optical flare in January 2007 will be presented and previous MAGIC results from 2006 will be summarized
The atmospheric Cherenkov gamma-ray telescope MAGIC, designed for a low-energy threshold, has detect...
The atmospheric Cherenkov gamma-ray telescope MAGIC, designed for a low-energy threshold, has detect...
The atmospheric Cherenkov gamma- ray telescope MAGIC, designed for a low- energy threshold, has dete...
The quasar 3C 279 is one of the best-observed flat spectrum radio quasars. It is located at a compar...
We study the multifrequency emission and spectral properties of the quasar 3C 279. We observed 3C 27...
3C 279, the first quasar discovered to emit VHE gamma-rays by the MAGIC telescope in 2006, was reobs...
We study the multifrequency emission and spectral properties of the quasar3C 279 aimed at identifyin...
Context. 3C 279, the first quasar discovered to emit VHE \u3b3-rays by the MAGIC telescope in 2006, ...
Context. 3C 279, the first quasar discovered to emit VHE gamma-rays by the MAGIC telescope in 2006, ...
Context. 3C 279, the first quasar discovered to emit VHE γ-rays by the MAGIC telescope in 2006, was ...
Abstract: The high luminosity blazar 3C279 has been discovered by the EGRET instrument on board the ...
The MAGIC telescopes discovered Very High Energy (VHE, E>100 GeV) γ-ray emission com- ing from the d...
Among more than fifty blazars detected in very high energy (VHE, E>100GeV) gamma-rays, only three be...
3C 279 is one of the best studied flat spectrum radio quasars located at a comparatively large redsh...
The atmospheric Cherenkov gamma-ray telescope MAGIC, designed for a low-energy threshold, has detect...
The atmospheric Cherenkov gamma-ray telescope MAGIC, designed for a low-energy threshold, has detect...
The atmospheric Cherenkov gamma- ray telescope MAGIC, designed for a low- energy threshold, has dete...
The quasar 3C 279 is one of the best-observed flat spectrum radio quasars. It is located at a compar...
We study the multifrequency emission and spectral properties of the quasar 3C 279. We observed 3C 27...
3C 279, the first quasar discovered to emit VHE gamma-rays by the MAGIC telescope in 2006, was reobs...
We study the multifrequency emission and spectral properties of the quasar3C 279 aimed at identifyin...
Context. 3C 279, the first quasar discovered to emit VHE \u3b3-rays by the MAGIC telescope in 2006, ...
Context. 3C 279, the first quasar discovered to emit VHE gamma-rays by the MAGIC telescope in 2006, ...
Context. 3C 279, the first quasar discovered to emit VHE γ-rays by the MAGIC telescope in 2006, was ...
Abstract: The high luminosity blazar 3C279 has been discovered by the EGRET instrument on board the ...
The MAGIC telescopes discovered Very High Energy (VHE, E>100 GeV) γ-ray emission com- ing from the d...
Among more than fifty blazars detected in very high energy (VHE, E>100GeV) gamma-rays, only three be...
3C 279 is one of the best studied flat spectrum radio quasars located at a comparatively large redsh...
The atmospheric Cherenkov gamma-ray telescope MAGIC, designed for a low-energy threshold, has detect...
The atmospheric Cherenkov gamma-ray telescope MAGIC, designed for a low-energy threshold, has detect...
The atmospheric Cherenkov gamma- ray telescope MAGIC, designed for a low- energy threshold, has dete...