Context - The pulsar wind nebula (PWN) 3C 58 is one of the historical very high-energy (VHE; E >100 GeV) y-ray source candidates. It is energized by one of the highest spin-down power pulsars known (5% of Crab pulsar) and it has been compared with the Crab nebula because of their morphological similarities. This object was previously observed by imaging atmospheric Cherenkov telescopes (Whipple, VERITAS and MAGIC), although it was not detected, with an upper limit of 2.3 % Crab unit (C.U.) at VHE. It was detected by the Fermi Large Area Telescope (LAT) with a spectrum extending beyond 100 GeV. Aims - We aim to extend the spectrum of 3C 58 beyond the energies reported by the Fermi Collaboration and probe acceleration of particles in the PWN ...
Abstract: We report about very high energy (VHE) γ-ray observations of the Crab Nebula with the MAGI...
Aims: We investigate the extension of the very high-energy spectral tail of the Crab Pulsar at energ...
Aims: We investigate the extension of the very high-energy spectral tail of the Crab Pulsar at energ...
Context. The pulsar wind nebula (PWN) 3C 58 is one of the historical very high-energy (VHE; E > 1...
Context. The pulsar wind nebula (PWN) 3C 58 is one of the historical very high-energy (VHE; E > 1...
Context. The pulsar wind nebula (PWN) 3C 58 is one of the historical very high-energy (VHE; E> 100 G...
The pulsar wind nebula (PWN) 3C 58 is one of the historical very-high-energy (VHE; E>100 GeV) gamma-...
The pulsar wind nebula (PWN) 3C 58 is one of the historical very high-energy (VHE; E> 100 GeV) γ-ray...
The pulsar wind nebula (PWN) 3C 58 is one of the historical very high-energy (VHE; E> 100 GeV) γ-ray...
The pulsar wind nebula (PWN) 3C 58 is one of the historical very high-energy (VHE; E> 100 GeV) γ-ray...
Context. The pulsar wind nebula (PWN) 3C 58 is one of the historical very high-energy (VHE; E> 100 G...
The pulsar wind nebula (PWN) 3C 58 is one of the historical very-high-energy (VHE; E>100 GeV) gamma-...
Context. The pulsar wind nebula (PWN) 3C 58 is one of the historical very high-energy (VHE; E >100 G...
The pulsar wind nebula (PWN) 3C 58 is one of the historical very-high-energy (VHE; E>100 GeV) gamma-...
Aims: We investigate the extension of the very high-energy spectral tail of the Crab Pulsar at energ...
Abstract: We report about very high energy (VHE) γ-ray observations of the Crab Nebula with the MAGI...
Aims: We investigate the extension of the very high-energy spectral tail of the Crab Pulsar at energ...
Aims: We investigate the extension of the very high-energy spectral tail of the Crab Pulsar at energ...
Context. The pulsar wind nebula (PWN) 3C 58 is one of the historical very high-energy (VHE; E > 1...
Context. The pulsar wind nebula (PWN) 3C 58 is one of the historical very high-energy (VHE; E > 1...
Context. The pulsar wind nebula (PWN) 3C 58 is one of the historical very high-energy (VHE; E> 100 G...
The pulsar wind nebula (PWN) 3C 58 is one of the historical very-high-energy (VHE; E>100 GeV) gamma-...
The pulsar wind nebula (PWN) 3C 58 is one of the historical very high-energy (VHE; E> 100 GeV) γ-ray...
The pulsar wind nebula (PWN) 3C 58 is one of the historical very high-energy (VHE; E> 100 GeV) γ-ray...
The pulsar wind nebula (PWN) 3C 58 is one of the historical very high-energy (VHE; E> 100 GeV) γ-ray...
Context. The pulsar wind nebula (PWN) 3C 58 is one of the historical very high-energy (VHE; E> 100 G...
The pulsar wind nebula (PWN) 3C 58 is one of the historical very-high-energy (VHE; E>100 GeV) gamma-...
Context. The pulsar wind nebula (PWN) 3C 58 is one of the historical very high-energy (VHE; E >100 G...
The pulsar wind nebula (PWN) 3C 58 is one of the historical very-high-energy (VHE; E>100 GeV) gamma-...
Aims: We investigate the extension of the very high-energy spectral tail of the Crab Pulsar at energ...
Abstract: We report about very high energy (VHE) γ-ray observations of the Crab Nebula with the MAGI...
Aims: We investigate the extension of the very high-energy spectral tail of the Crab Pulsar at energ...
Aims: We investigate the extension of the very high-energy spectral tail of the Crab Pulsar at energ...