SNR G24.7+0.6 is a 9.5 kyrs radio and γ-ray supernova remnant evolving in a dense medium. In the GeV regime, SNR G24.7+0.6 (3FHL J1834.1–0706e/FGES J1834.1–0706) shows a hard spectral index (Γ ∼ 2) up to 200 GeV, which makes it a good candidate to be observed with Cherenkov telescopes such as MAGIC. We observed the field of view of SNR G24.7+0.6 with the MAGIC telescopes for a total of 31 h. We detect very high-energy γ-ray emission from an extended source located 0.34° away from the centre of the radio SNR. The new source, named MAGIC J1835–069 is detected up to 5 TeV, and its spectrum is well-represented by a power-law function with spectral index of 2.74 ± 0.08. The complexity of the region makes the identification of the origin of the v...
Context. The pulsar wind nebula (PWN) 3C 58 is one of the historical very high-energy (VHE; E> 100 G...
International audienceThe supernova remnant (SNR) W49B originated from a core-collapse supernova tha...
Aims:We searched for very high energy (VHE) γ-ray emission from the supernova remnant Cassiopeia A M...
SNR G24.7+0.6 is a 9.5 kyrs radio and γ-ray supernova remnant evolving in a dense medium. In the GeV...
SNR G24.7+0.6 is a 9.5 kyrs radio and γ-ray supernova remnant evolving in a dense medium. In the GeV...
SNR G24.7+0.6 is a 9.5 kyrs radio and $\gamma$-ray supernova remnant evolving in a dense medium. In ...
SNR G24.7+0.6 is a 9.5 kyrs radio and gamma-ray supernova remnant evolving in a dense medium. In the...
Context. Certain types of supernova remnants (SNRs) in our Galaxy are assumed to be PeVatrons, capab...
Context. γ Cygni is a young supernova remnant located in the Cygnus region. MAGIC (Major Atmospheric...
We have analysed the Fermi Large Area Telescope (LAT) data on the SNR G73.9+0.9. We have confirmed a...
G349.7+0.2 is a young Galactic supernova remnant (SNR) located at the distance of 11.5 kpc and obser...
We report the detection of a new source of very high energy (VHE; Eγ ≥ 100 GeV) γ-ray emission locat...
Hadronic emission from supernova remnant (SNR)–molecular cloud (MC) association systems has been wid...
Context. The pulsar wind nebula (PWN) 3C 58 is one of the historical very high-energy (VHE; E> 100 G...
International audienceThe supernova remnant (SNR) W49B originated from a core-collapse supernova tha...
Aims:We searched for very high energy (VHE) γ-ray emission from the supernova remnant Cassiopeia A M...
SNR G24.7+0.6 is a 9.5 kyrs radio and γ-ray supernova remnant evolving in a dense medium. In the GeV...
SNR G24.7+0.6 is a 9.5 kyrs radio and γ-ray supernova remnant evolving in a dense medium. In the GeV...
SNR G24.7+0.6 is a 9.5 kyrs radio and $\gamma$-ray supernova remnant evolving in a dense medium. In ...
SNR G24.7+0.6 is a 9.5 kyrs radio and gamma-ray supernova remnant evolving in a dense medium. In the...
Context. Certain types of supernova remnants (SNRs) in our Galaxy are assumed to be PeVatrons, capab...
Context. γ Cygni is a young supernova remnant located in the Cygnus region. MAGIC (Major Atmospheric...
We have analysed the Fermi Large Area Telescope (LAT) data on the SNR G73.9+0.9. We have confirmed a...
G349.7+0.2 is a young Galactic supernova remnant (SNR) located at the distance of 11.5 kpc and obser...
We report the detection of a new source of very high energy (VHE; Eγ ≥ 100 GeV) γ-ray emission locat...
Hadronic emission from supernova remnant (SNR)–molecular cloud (MC) association systems has been wid...
Context. The pulsar wind nebula (PWN) 3C 58 is one of the historical very high-energy (VHE; E> 100 G...
International audienceThe supernova remnant (SNR) W49B originated from a core-collapse supernova tha...
Aims:We searched for very high energy (VHE) γ-ray emission from the supernova remnant Cassiopeia A M...