Showing 1–20 of 22 results
/ Date/ Name
Jan 14, 2019Deep observations of the globular cluster M15 with the MAGIC telescopesSep 3, 2018Constraining very-high-energy and optical emission from FRB 121102 with the MAGIC telescopesJun 5, 2017Observation of the Black Widow B1957+20 millisecond pulsar binary system with the MAGIC telescopesDec 12, 2018Discovery of TeV $γ$-ray emission from the neighbourhood of the supernova remnant G24.7+0.6 by MAGICJul 1, 2018Multi-wavelength characterization of the blazar S5~0716+714 during an unprecedented outburst phaseDec 7, 2017Indirect dark matter searches in the dwarf satellite galaxy Ursa Major II with the MAGIC TelescopesAug 11, 2017Search for very-high-energy gamma-ray emission from the microquasar Cygnus X-1 with the MAGIC telescopesJan 7, 2019A Fast Very High Energy $γ$-ray Flare from BL Lacertae during a Period of Multiwavelength activity in June 2015Oct 11, 2018Periastron Observations of TeV Gamma-Ray Emission from a Binary System with a 50-year PeriodJun 14, 2018Detection of persistent VHE gamma-ray emission from PKS 1510-089 by the MAGIC telescopes during low states between 2012 and 2017Aug 13, 2018The extreme HBL behaviour of Markarian 501 during 2012Jun 28, 2018Constraining Dark Matter lifetime with a deep gamma-ray survey of the Perseus Galaxy Cluster with MAGICMay 7, 2018Limits on the flux of tau neutrinos from 1 PeV to 3 EeV with the MAGIC telescopesApr 4, 2017Performance of the MAGIC telescopes under moonlightOct 28, 2016Multiwavelength observations of a VHE gamma-ray flare from PKS 1510-089 in 2015Jul 4, 2017MAGIC observations of the microquasar V404 Cygni during the 2015 outburstNov 2, 2019Statistics of VHE gamma-Rays in Temporal Association with Radio Giant Pulses from the Crab PulsarJan 13, 2019MAGIC and Fermi-LAT gamma-ray results on unassociated HAWC sourcesSep 1, 2017Constraining Lorentz invariance violation using the Crab Pulsar emission observed up to TeV energies by MAGICAug 17, 2017MAGIC Contributions to the 35th International Cosmic Ray Conference (ICRC2017)