Context. Gamma-ray bursts are cosmological sources emitting radiation from the gamma-rays to the radio band. Substantial observational efforts have been devoted...
MAGIC observations and multifrequency properties of the flat spectrum radio quasar 3C 279 in 2011
Aims: We study the multifrequency emission and spectral properties of the quasar3C 279 aimed at identifying the radiation processes taking place in the source...
MAGIC Observations and multiwavelength properties of the quasar 3C 279 in 2007 and 2009
Context. 3C 279, the first quasar discovered to emit VHE γ-rays by the MAGIC telescope in 2006, was reobserved by MAGIC in January 2007 during a major optical...
MAGIC observations of MWC 656, the only known Be/BH system
Context. MWC 656 has recently been established as the first observationally detected high-mass X-ray binary system containing a Be star and a black hole (BH)...
MAGIC observations of PG 1553+113 during a multiwavelength campaign in July 2006
The active galactic nucleus PG 1553+113 was observed by the MAGIC telescope in July 2006 during a multiwavelength campaign, in which telescopes in the optical...
MAGIC observations of the diffuse γ-ray emission in the vicinity of the Galactic center
Aims: In the presence of a sufficient amount of target material, γ-rays can be used as a tracer in the search for sources of Galactic cosmic rays (CRs). Here we...
MAGIC observations of the February 2014 flare of 1ES 1011+496 and ensuing constraint of the EBL density
Context. During February-March 2014, the MAGIC telescopes observed the high-frequency peaked BL Lac 1ES 1011+496 (z = 0.212) in flaring state at very-high...
MAGIC observations of the giant radio galaxy M 87 in a low-emission state between 2005 and 2007
Context. We present the results of a long M 87 monitoring campaign in very high energy γ-rays with the MAGIC-I Cherenkov telescope. Aims: We aim to model the...
MAGIC observations provide compelling evidence of hadronic multi-TeV emission from the putative PeVatron SNR G106.3+2.7
Context. Certain types of supernova remnants (SNRs) in our Galaxy are assumed to be PeVatrons, capable of accelerating cosmic rays (CRs) to ~ PeV energies...