Aims:We searched for very high energy (VHE) γ-ray emission from the supernova remnant Cassiopeia A Methods: The shell-type supernova remnant Cassiopeia A was observed with the 17 m MAGIC telescope between July 2006 and January 2007 for a total time of 47 h. Results: The source was detected above an energy of 250 GeV with a significance of 5.2σ and a photon flux above 1 TeV of (7.3 ± 0.7_stat ± 2.2_sys) × 10-13 cm-2s-1. The photon spectrum is compatible with a power law dN/dE ∝ E-Γ with a photon index Γ = 2.3 ± 0.2_stat ± 0.2_sys. The source is point-like within the angular resolution of the telescope
Observations with imaging atmospheric Cherenkov telescopes (IACTs) have enhanced our knowledge of ne...
We report the detection of a new source of very high energy (VHE; Eγ>=100 GeV) γ-ray emission locate...
We present evidence that the very high energy (VHE, E \u3e 100 GeV) gamma-ray emission coincident wi...
Aims:We searched for very high energy (VHE) γ-ray emission from the supernova remnant Cassiopeia A M...
Aims.We searched for very high energy (VHE) γ-ray emission from the supernova remnant Cassiopeia A ...
Aims. We searched for very high energy (VHE)gamma-ray emission from the supernova remnant Cassiopeia...
Aims. We searched for very high energy (VHE)gamma-ray emission from the supernova remnant Cassiopeia...
We report on observations of very high energy gamma rays from the shell-type supernova remnant (SNR)...
SNR G24.7+0.6 is a 9.5 kyrs radio and γ-ray supernova remnant evolving in a dense medium. In the GeV...
232 hours of data were accumulated from 1997 to 1999, using the HEGRA Stereoscopic Cherenkov Telesco...
PG 1553+113 is a very high energy (VHE, E > 100 GeV) γ -ray emitter classified as a BL Lac object...
We observed the first known very high energy (VHE) γ-ray-emitting unidentified source, TeV J2032+413...
Observations with imaging atmospheric Cherenkov telescopes (IACTs) have enhanced our knowledge of ne...
We report the detection of a new source of very high energy (VHE; Eγ>=100 GeV) γ-ray emission locate...
We present evidence that the very high energy (VHE, E \u3e 100 GeV) gamma-ray emission coincident wi...
Aims:We searched for very high energy (VHE) γ-ray emission from the supernova remnant Cassiopeia A M...
Aims.We searched for very high energy (VHE) γ-ray emission from the supernova remnant Cassiopeia A ...
Aims. We searched for very high energy (VHE)gamma-ray emission from the supernova remnant Cassiopeia...
Aims. We searched for very high energy (VHE)gamma-ray emission from the supernova remnant Cassiopeia...
We report on observations of very high energy gamma rays from the shell-type supernova remnant (SNR)...
SNR G24.7+0.6 is a 9.5 kyrs radio and γ-ray supernova remnant evolving in a dense medium. In the GeV...
232 hours of data were accumulated from 1997 to 1999, using the HEGRA Stereoscopic Cherenkov Telesco...
PG 1553+113 is a very high energy (VHE, E > 100 GeV) γ -ray emitter classified as a BL Lac object...
We observed the first known very high energy (VHE) γ-ray-emitting unidentified source, TeV J2032+413...
Observations with imaging atmospheric Cherenkov telescopes (IACTs) have enhanced our knowledge of ne...
We report the detection of a new source of very high energy (VHE; Eγ>=100 GeV) γ-ray emission locate...
We present evidence that the very high energy (VHE, E \u3e 100 GeV) gamma-ray emission coincident wi...