Discovery of very high energy γ-ray emission from the blazar 1ES 0033+595 by the MAGIC telescopes
The number of known very high energy (VHE) blazars is ∼50, which is very small in comparison to the number of blazars detected in other frequencies. This situation is a handicap for population studies of blazars, which emit about half of their luminosity in the γ-ray domain. Moreover, VHE blazars, i...
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Veröffentlicht in: | Monthly Notices of the Royal Astronomical Society 2015-01, Vol.446 (1), p.217-225 |
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