Detection of very-high energy γ-ray emission from NGC 1275 by the MAGIC telescopes
We report on the detection of very-high energy (VHE, E > 100 GeV) γ-ray emission from NGC 1275, the central radio galaxy of the Perseus cluster of galaxies. The source has been detected by the MAGIC telescopes with a statistical significance of 6.6σ above 100 GeV in 46 h of stereo observations carried out between August 2010 and February 2011. The
Aleksić, J. et al.
Fecha de publicación:
3
2012