Add to ORKG"The MAGIC Cherenkov telescope in La Palma has observed GRB050713A 40s after T0. This observation, started 20 seconds after the alert given by Swift (Trigger #145675; Falcone et al., GCN Circ 3581), thanks to the capability of fast pointing by MAGIC and to the prompt reaction by the operators; it overlapped for around 30 seconds with Swift during the main burst, and lasted 2400 s. The first look at the MAGIC data did not reveal strong gamma ray emission above 175GeV. The flux limit derived at very high energies by MAGIC is 2-3 orders of magnitude lower than the extrapolation from the X band [1]. A detailed analysis is in progress. To our knowledge, this is the first simultaneous observation of a GRB in the X band and in the HE gamma re...
Indications of a GeV component in the emission from gamma-ray bursts (GRBs) are known since the Ener...
On 14th January 2019, the MAGIC collaboration achieved the first significant detection at TeV energi...
During the first observation cycle of the MAGIC telescope, 9 successful GRB follow-up observations w...
"The MAGIC Cherenkov telescope in La Palma has observed GRB050713A 40s after T0. This observation, ...
The long-duration GRB050713a was observed by the MAGIC Telescope, 40 seconds after the burst onset, ...
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...
Starting from the first announcement of unequivocal detection of very high energy (VHE) emission fro...
Gamma-ray bursts (GRBs) are the most energetic phenomena in the Universe. Many aspects of GRB physic...
The MAGIC Imaging Atmospheric Cherenkov Telescope performed a follow-up observation of the SWIFT-BAT...
Since the beginning of its operation in April 2005, the MAGIC telescope was able to observe ten diff...
Gamma-Ray Bursts (GRBs) are one of the main targets for current and next generation Imaging Atmosph...
Gamma-ray bursts are cosmological sources emitting radiation from the gamma-rays to the radio band. ...
Indications of a GeV component in the emission from gamma-ray bursts (GRBs) are known since the Ener...
On 14th January 2019, the MAGIC collaboration achieved the first significant detection at TeV energi...
During the first observation cycle of the MAGIC telescope, 9 successful GRB follow-up observations w...
"The MAGIC Cherenkov telescope in La Palma has observed GRB050713A 40s after T0. This observation, ...
The long-duration GRB050713a was observed by the MAGIC Telescope, 40 seconds after the burst onset, ...
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...
Starting from the first announcement of unequivocal detection of very high energy (VHE) emission fro...
Gamma-ray bursts (GRBs) are the most energetic phenomena in the Universe. Many aspects of GRB physic...
The MAGIC Imaging Atmospheric Cherenkov Telescope performed a follow-up observation of the SWIFT-BAT...
Since the beginning of its operation in April 2005, the MAGIC telescope was able to observe ten diff...
Gamma-Ray Bursts (GRBs) are one of the main targets for current and next generation Imaging Atmosph...
Gamma-ray bursts are cosmological sources emitting radiation from the gamma-rays to the radio band. ...
Indications of a GeV component in the emission from gamma-ray bursts (GRBs) are known since the Ener...
On 14th January 2019, the MAGIC collaboration achieved the first significant detection at TeV energi...
During the first observation cycle of the MAGIC telescope, 9 successful GRB follow-up observations w...