We report on the results from the observations in very high energy band (VHE, Eγ ≥ 100 GeV) of the γ -ray binary LS I +61 303 and the black hole X-ray binary (BHXB) Cygnus X-1. LS I +61 303 was recently discovered at VHE by MAGIC [1] and here we present the preliminary results from an extensive observation campaign, comprising 112 observation hours covering 4 orbital cycles, aiming at determining the time-dependent features of the VHE emission. Cygnus X-1 was observed for a total of 40 hours during 26 nights, spanning the period between June and November 2006. We report on the results of the searches for steady and variable γ -ray signals from Cyngus X-1, including the first experimental evidence for an intense fl...
The binary system LS I +61 303 is one of four γ-ray binaries known. The system was studied inte...
Galactic transients, X-ray and gamma-ray binaries provide a proper environment for particle ac-celer...
The MAGIC collaboration has recently reported the discovery of gamma-ray emission from the binary sy...
We report on the results from the observations in the very high energy band (VHE; E\u3b3 65 100 GeV...
The microquasar Cygnus X-1 displays the two typical soft and hard X-ray states of a black hole trans...
The microquasar Cygnus X-1 displays the two typical soft and hard X-ray states of a black hole trans...
We report on the results from the observations in the very high energy band ( VHE; GeV) of the black...
We report on the results from the observations in the very high energy band ( VHE; GeV) of the black...
We report on the results from the observations in the very high energy band ( VHE; GeV) of the black...
Here we report the discovery of very high energy gamma-ray emission from the radio emitting X-ray bi...
The microquasar Cygnus X-1 displays the two typical soft and hard X-ray states of a black-hole trans...
The binary star system LS I +61 303, recently discovered by the MAGIC Telescope, was investigated in...
We report on the results from the observations in very high energy band (VHE, E_gamma > 100 GeV) of ...
The improvement on the Imaging Air Cherenkov Technique (IACT) led to the discovery of a new type of ...
The MAGIC collaboration discovered with their 17 m diameter imaging atmospheric Cherenkov telescope,...
The binary system LS I +61 303 is one of four γ-ray binaries known. The system was studied inte...
Galactic transients, X-ray and gamma-ray binaries provide a proper environment for particle ac-celer...
The MAGIC collaboration has recently reported the discovery of gamma-ray emission from the binary sy...
We report on the results from the observations in the very high energy band (VHE; E\u3b3 65 100 GeV...
The microquasar Cygnus X-1 displays the two typical soft and hard X-ray states of a black hole trans...
The microquasar Cygnus X-1 displays the two typical soft and hard X-ray states of a black hole trans...
We report on the results from the observations in the very high energy band ( VHE; GeV) of the black...
We report on the results from the observations in the very high energy band ( VHE; GeV) of the black...
We report on the results from the observations in the very high energy band ( VHE; GeV) of the black...
Here we report the discovery of very high energy gamma-ray emission from the radio emitting X-ray bi...
The microquasar Cygnus X-1 displays the two typical soft and hard X-ray states of a black-hole trans...
The binary star system LS I +61 303, recently discovered by the MAGIC Telescope, was investigated in...
We report on the results from the observations in very high energy band (VHE, E_gamma > 100 GeV) of ...
The improvement on the Imaging Air Cherenkov Technique (IACT) led to the discovery of a new type of ...
The MAGIC collaboration discovered with their 17 m diameter imaging atmospheric Cherenkov telescope,...
The binary system LS I +61 303 is one of four γ-ray binaries known. The system was studied inte...
Galactic transients, X-ray and gamma-ray binaries provide a proper environment for particle ac-celer...
The MAGIC collaboration has recently reported the discovery of gamma-ray emission from the binary sy...