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		| Paper: | 
		MAGIC Observations of AGNs: Scientific Highlights | 
	 
	
		| Volume: | 
		427, Accretion and Ejection in AGN: a Global View | 
	 
	
		| Page: | 
		235 | 
	 
	
		| Authors: | 
		Mazin, D. for the MAGIC collaboration | 
	 
	
	
		| Abstract: | 
		The MAGIC telescope, located on the Canary Island of La Palma, explores the
 universe in γ-rays with energies from 50-60 GeV up to tens of TeV.  Roughly
 40% of the MAGIC duty cycle is devoted to observation of active galactic
 nuclei (AGNs), in which supermassive black holes are believed to be responsible
 for particle acceleration.  By measuring of γ-rays from these sources one
 can study non-thermal processes in plasma jets and fundamental properties of the
 black holes as well as questions of the general physics and cosmology. In this
 paper, we present highlights of MAGIC observations of AGNs in the last two
 years. We also discuss physics consequences of the new discoveries
 concerning the production site of VHE γ-rays in M87, the emission mechanism
 of γ-rays in Mrk 421, limits on the quantum gravity scale from a flare in
 Mrk 501, and limits on the VHE γ-ray horizon derived from the energy
 spectrum of 3C 279. | 
	 
	
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