Showing 1–20 of 20 results
/ Date/ Name
Sep 10, 2025Time-Dependent Modeling of the Sub-Hour Spectral Evolution During the 2013 Outburst of Mrk 421Jul 7, 2025Testing the ubiquitous presence of very high energy emission in gamma-ray bursts with the MAGIC telescopesOct 30, 2024Insights from the first flaring activity of a high-synchrotron-peaked blazar with X-ray polarization and VHE gamma raysDec 17, 2023First characterization of the emission behavior of Mrk421 from radio to VHE gamma rays with simultaneous X-ray polarization measurementsOct 5, 2022Multi-messenger characterization of Mrk 501 during historically low X-ray and $γ$-ray activityFeb 15, 2022Proton acceleration in thermonuclear nova explosions revealed by gamma raysDec 8, 2021Dual-high-frequency VLBI study of blazar-jet brightness-temperature gradients and collimation profilesJul 1, 2021Sensitivity to light sterile neutrino mixing parameters with KM3NeT/ORCAJun 10, 2021Investigation of the correlation patterns and the Compton dominance variability of Mrk 421 in 2017Mar 17, 2021Determining the Neutrino Mass Ordering and Oscillation Parameters with KM3NeT/ORCAFeb 11, 2021The KM3NeT potential for the next core-collapse supernova observation with neutrinosJun 6, 2019Dependence of atmospheric muon flux on seawater depth measured with the first KM3NeT detection unitsJan 13, 2019MAGIC and Fermi-LAT gamma-ray results on unassociated HAWC sourcesNov 14, 2016A search for spectral hysteresis and energy-dependent time lags from X-ray and TeV gamma-ray observations of Mrk 421Oct 6, 2016Very High-Energy Gamma-Ray Follow-Up Program Using Neutrino Triggers from IceCubeDec 14, 2015Very-high-energy gamma-rays from the Universe's middle age: detection of the z=0.940 blazar PKS 1441+25 with MAGICSep 16, 2015First NuSTAR Observations of Mrk 501 within a Radio to TeV Multi-Instrument CampaignMay 5, 2014Deep sea tests of a prototype of the KM3NeT digital optical moduleJul 8, 2013CTA contributions to the 33rd International Cosmic Ray Conference (ICRC2013)Nov 22, 2011The 2010 very high energy gamma-ray flare & 10 years of multi-wavelength observations of M 87