Add to ORKGMAGIC is currently the most suitable instrument to perform observations of the prompt an early afterglow emission from Gamma Ray Bursts (GRBs) at energies above 25 GeV. The instrument is designed to have the lowest possible energy threshold and fastest reaction time to GRB Coordinates Network (GCN) alerts. The MAGIC-I telescope started to follow-up GCN alerts in the beginning of 2005. Since then, more than 50 GRB candidates were observed. Just now MAGIC-II, the second telescope has started to operate. Both telescopes together will have a factor of three better sensitivity
The MAGIC Collaboration is building an imaging \u10cerenkov telescope at La Palma site (2200 m a.s.l...
The Major Atmospheric Gamma-ray Imaging Cherenkov (MAGIC) Telescope collaboration is constructing a ...
Gamma-ray bursts are cosmological sources emitting radiation from the gamma-rays to the radio band. ...
The MAGIC Telescope, now taking data with an energy threshold well below 100 GeV, will soon be able ...
Since the beginning of its operation in April 2005, the MAGIC telescope was able to observe ten diff...
The MAGIC Telescope, now taking data with an energy threshold well below 100 GeV, will soon be able ...
During the first observation cycle of the MAGIC telescope, 9 successful GRB follow-up observations w...
The MAGIC Telescope, with its technological solutions which allow the telescope to have a low energy...
17siGamma ray burst (GRBs) are primary targets for all modern IACT telescopes. The MAGIC collaborati...
Gamma-Ray Bursts (GRBs) are one of the main targets for current and next generation Imaging Atmosph...
The MAGIC Imaging Atmospheric Cherenkov Telescope performed a follow-up observation of the SWIFT-BAT...
Indications of a GeV component in the emission from gamma-ray bursts (GRBs) are known since the Ener...
The Major Atmospheric Gamma-ray Imaging Cherenkov (MAGIC) Telescope collaboration is constructing a ...
The MAGIC Telescope, now taking data with an energy threshold well below 100 GeV, will soon be able ...
Starting from the first announcement of unequivocal detection of very high energy (VHE) emission fro...
The MAGIC Collaboration is building an imaging \u10cerenkov telescope at La Palma site (2200 m a.s.l...
The Major Atmospheric Gamma-ray Imaging Cherenkov (MAGIC) Telescope collaboration is constructing a ...
Gamma-ray bursts are cosmological sources emitting radiation from the gamma-rays to the radio band. ...
The MAGIC Telescope, now taking data with an energy threshold well below 100 GeV, will soon be able ...
Since the beginning of its operation in April 2005, the MAGIC telescope was able to observe ten diff...
The MAGIC Telescope, now taking data with an energy threshold well below 100 GeV, will soon be able ...
During the first observation cycle of the MAGIC telescope, 9 successful GRB follow-up observations w...
The MAGIC Telescope, with its technological solutions which allow the telescope to have a low energy...
17siGamma ray burst (GRBs) are primary targets for all modern IACT telescopes. The MAGIC collaborati...
Gamma-Ray Bursts (GRBs) are one of the main targets for current and next generation Imaging Atmosph...
The MAGIC Imaging Atmospheric Cherenkov Telescope performed a follow-up observation of the SWIFT-BAT...
Indications of a GeV component in the emission from gamma-ray bursts (GRBs) are known since the Ener...
The Major Atmospheric Gamma-ray Imaging Cherenkov (MAGIC) Telescope collaboration is constructing a ...
The MAGIC Telescope, now taking data with an energy threshold well below 100 GeV, will soon be able ...
Starting from the first announcement of unequivocal detection of very high energy (VHE) emission fro...
The MAGIC Collaboration is building an imaging \u10cerenkov telescope at La Palma site (2200 m a.s.l...
The Major Atmospheric Gamma-ray Imaging Cherenkov (MAGIC) Telescope collaboration is constructing a ...
Gamma-ray bursts are cosmological sources emitting radiation from the gamma-rays to the radio band. ...