Showing 1–17 of 17 results
/ Date/ Name
Mar 23, 2026The second H.E.S.S. gamma-ray burst catalogue: 15 years of observations with the H.E.S.S. telescopesNov 23, 2025Optimizing the potential of KM3NeT in detecting core-collapse supernovaeFeb 12, 2025The ultra-high-energy event KM3-230213A within the global neutrino landscapeAug 13, 2024Measurement of neutrino oscillation parameters with the first six detection units of KM3NeT/ORCAFeb 13, 2024Astronomy potential of KM3NeT/ARCANov 7, 2023Searches for neutrino counterparts of gravitational waves from the LIGO/Virgo third observing run with KM3NeTSep 6, 2023Prospects for combined analyses of hadronic emission from $γ$-ray sources in the Milky Way with CTA and KM3NeTJul 27, 2022Redshift Evolution of the Feedback / Cooling Equilibrium in the Core of 48 SPT Galaxy Clusters: A Joint $\boldsymbol{Chandra}$-SPT-ATCA analysisMar 2, 2022Spitzer and Herschel studies of dust in supernova remnants in the Small Magellanic CloudJul 1, 2021Sensitivity to light sterile neutrino mixing parameters with KM3NeT/ORCAMar 17, 2021Determining the Neutrino Mass Ordering and Oscillation Parameters with KM3NeT/ORCAFeb 11, 2021The KM3NeT potential for the next core-collapse supernova observation with neutrinosOct 7, 2019Science with the Murchison Widefield Array: Phase I Results and Phase II OpportunitiesOct 7, 2019Discovery of a very young high-mass X-ray binary associated with the supernova remnant MCSNRJ0513-6724 in the LMCJun 6, 2019Non-thermal emission from the reverse shock of the youngest galactic Supernova remnant G1.9+0.3Jun 6, 2019Dependence of atmospheric muon flux on seawater depth measured with the first KM3NeT detection unitsSep 17, 2018The Phase II Murchison Widefield Array: Design Overview