During the first observation cycle of the MAGIC telescope, 9 successful GRB follow-up observations were performed. For 2 bursts, the obser- vation started even while the prompt emission was still ongoing. In none of these observations a significant excess over background could be detected. We present a direct determination of the MAGIC sensitivity in GRB observation mode from the Crab Nebula and the obtained upper limits for the 9 observations. At energies around 100 GeV, MAGIC is currently the fastest and most sensitive GRB detector in the world
On 14th January 2019, the MAGIC collaboration achieved the first significant detection at TeV energi...
"The MAGIC Cherenkov telescope in La Palma has observed GRB050713A 40s after T0. This observation, ...
During its first data cycle, between 2005 and the beginning of 2006, the fast repositioning system o...
During the first observation cycle of the MAGIC telescope, 9 successful GRB follow-up observations w...
Since the beginning of its operation in April 2005, the MAGIC telescope was able to observe ten diff...
Indications of a GeV component in the emission from gamma-ray bursts (GRBs) are known since the Ener...
MAGIC is currently the most suitable instrument to perform observations of the prompt an early after...
During its first data cycle, between 2005 and the beginning of 2006, the fast repositioning system o...
The long-duration gamma-ray burst GRB 050713a was observed by the MAGIC Telescope 40 s after the bur...
The long-duration gamma-ray burst GRB 050713a was observed by the MAGIC Telescope 40 s after the bur...
The long-duration GRB050713a was observed by the MAGIC Telescope, 40 seconds after the burst onset, ...
On 14th January 2019, the MAGIC collaboration achieved the first significant detection at TeV energi...
"The MAGIC Cherenkov telescope in La Palma has observed GRB050713A 40s after T0. This observation, ...
During its first data cycle, between 2005 and the beginning of 2006, the fast repositioning system o...
During the first observation cycle of the MAGIC telescope, 9 successful GRB follow-up observations w...
Since the beginning of its operation in April 2005, the MAGIC telescope was able to observe ten diff...
Indications of a GeV component in the emission from gamma-ray bursts (GRBs) are known since the Ener...
MAGIC is currently the most suitable instrument to perform observations of the prompt an early after...
During its first data cycle, between 2005 and the beginning of 2006, the fast repositioning system o...
The long-duration gamma-ray burst GRB 050713a was observed by the MAGIC Telescope 40 s after the bur...
The long-duration gamma-ray burst GRB 050713a was observed by the MAGIC Telescope 40 s after the bur...
The long-duration GRB050713a was observed by the MAGIC Telescope, 40 seconds after the burst onset, ...
On 14th January 2019, the MAGIC collaboration achieved the first significant detection at TeV energi...
"The MAGIC Cherenkov telescope in La Palma has observed GRB050713A 40s after T0. This observation, ...
During its first data cycle, between 2005 and the beginning of 2006, the fast repositioning system o...
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