Showing 1–20 of 32 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. telescopesJul 2, 2025H.E.S.S. programme searching for VHE gamma rays associated with FRBsJan 21, 2025Detection of very-high-energy gamma-ray emission from Eta Carinae during its 2020 periastron passageMar 25, 2024Unveiling extended gamma-ray emission around HESS J1813-178Jan 30, 2024The SRG/eROSITA all-sky survey: First X-ray catalogues and data release of the western Galactic hemisphereJan 29, 2024Acceleration and transport of relativistic electrons in the jets of the microquasar SS 433Oct 9, 2023Discovery of a Radiation Component from the Vela Pulsar Reaching 20 TeraelectronvoltsJun 30, 2023Multiwavelength Observations of the Blazar PKS 0735+178 in Spatial and Temporal Coincidence with an Astrophysical Neutrino Candidate IceCube-211208AFeb 27, 2023HESS J1809$-$193: a halo of escaped electrons around a pulsar wind nebula?Feb 6, 2022Probing Cosmic Inflation with the LiteBIRD Cosmic Microwave Background Polarization SurveyJun 28, 2021The eROSITA Final Equatorial-Depth Survey (eFEDS): Presenting The Demographics of X-ray Emission From Normal GalaxiesJun 1, 2021Search for dark matter annihilation signals from unidentified Fermi-LAT objects with H.E.S.SFeb 1, 2021Overview of the Medium and High Frequency Telescopes of the LiteBIRD satellite missionJan 29, 2021LiteBIRD: JAXA's new strategic L-class mission for all-sky surveys of cosmic microwave background polarizationJan 16, 2021Concept Design of Low Frequency Telescope for CMB B-mode Polarization satellite LiteBIRDDec 10, 2020Detection of large-scale X-ray bubbles in the Milky Way haloOct 7, 2020The eROSITA X-ray telescope on SRGOct 7, 2019Discovery of a very young high-mass X-ray binary associated with the supernova remnant MCSNRJ0513-6724 in the LMCMar 11, 2019Electromagnetic probes of primordial black holes as dark matterMay 15, 2018Search for $γ$-ray line signals from dark matter annihilations in the inner Galactic halo from ten years of observations with H.E.S.S