EPJ Web of Conferences
Volume 121, 2016Roma International Conference on Astroparticle Physics 2014 (RICAP-14)
|Number of page(s)||7|
|Published online||06 July 2016|
Institut de Física d'Altes Energies, Spain
a e-mail: email@example.com
Published online: 6 July 2016
The present generation of Imaging Air Cherenkov Telescopes (IACTs) has greatly improved our knowledge on the Very High Energy (VHE) side of our Universe. The MAGIC IACTs operate since 2004 with one telescope and since 2009 as a two telescope stereoscopic system. I will outline a few of our latest and most relevant results: the discovery of pulsed emission from the Crab pulsar at VHE, recently found to extend up to 400 GeV and along the “bridge” of the light curve, the measurement of the Crab nebula spectrum over three decades of energy, the discovery of VHE γ-ray emission from the PWN 3C 58, the very rapid emission of IC 310, in addition to dark matter studies. The results that will be described here and the planned deep observations in the next years will pave the path for the future generation of IACTs.
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