SNR G24.7+0.6 is a 9.5 kyrs radio and gamma-ray supernova remnant evolving in a dense medium. In the GeV regime, SNR G24.7+0.6 (3FHL J1834.1-0706e/FGFS J1834.1-0706) shows a hard spectral index (Gamma similar to 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 gamma-ray emission from an extended source located 0.34 degrees 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 identif...
Context. Diffusive shock acceleration (DSA) is the most promising mechanism that accelerates Galacti...
While supernova remnants (SNRs) are widely thought to be powerful cosmicray accelerators, indirect e...
Composite supernova remnants (SNRs) constitute a small subclass of the remnants of massive stellar e...
SNR G24.7+0.6 is a 9.5 kyrs radio and gamma-ray supernova remnant evolving in a dense medium. In the...
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...
It is widely believed that the bulk of the Galactic cosmic rays are accelerated in supernova remnant...
We have analysed the Fermi Large Area Telescope (LAT) data on the SNR G73.9+0.9. We have confirmed a...
The supernova remnant (SNR) W49B originated from a core-collapse supernova that occurred between one...
Context. Certain types of supernova remnants (SNRs) in our Galaxy are assumed to be PeVatrons, capab...
We present a detailed analysis of the GeV gamma-ray emission toward the supernova remnant (SNR) G8.7...
Aims:We searched for very high energy (VHE) γ-ray emission from the supernova remnant Cassiopeia A M...
The SNR G106.3+2.7, detected at 1--100 TeV energies by different $\gamma$-ray facilities, is one of ...
Observations with imaging atmospheric Cherenkov telescopes (IACTs) have enhanced our knowledge of ne...
Context. Diffusive shock acceleration (DSA) is the most promising mechanism that accelerates Galacti...
While supernova remnants (SNRs) are widely thought to be powerful cosmicray accelerators, indirect e...
Composite supernova remnants (SNRs) constitute a small subclass of the remnants of massive stellar e...
SNR G24.7+0.6 is a 9.5 kyrs radio and gamma-ray supernova remnant evolving in a dense medium. In the...
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...
It is widely believed that the bulk of the Galactic cosmic rays are accelerated in supernova remnant...
We have analysed the Fermi Large Area Telescope (LAT) data on the SNR G73.9+0.9. We have confirmed a...
The supernova remnant (SNR) W49B originated from a core-collapse supernova that occurred between one...
Context. Certain types of supernova remnants (SNRs) in our Galaxy are assumed to be PeVatrons, capab...
We present a detailed analysis of the GeV gamma-ray emission toward the supernova remnant (SNR) G8.7...
Aims:We searched for very high energy (VHE) γ-ray emission from the supernova remnant Cassiopeia A M...
The SNR G106.3+2.7, detected at 1--100 TeV energies by different $\gamma$-ray facilities, is one of ...
Observations with imaging atmospheric Cherenkov telescopes (IACTs) have enhanced our knowledge of ne...
Context. Diffusive shock acceleration (DSA) is the most promising mechanism that accelerates Galacti...
While supernova remnants (SNRs) are widely thought to be powerful cosmicray accelerators, indirect e...
Composite supernova remnants (SNRs) constitute a small subclass of the remnants of massive stellar e...