Showing 1–20 of 33 results
/ Date/ Name
Aug 26, 2025Prospects for dark matter observations in dwarf spheroidal galaxies with the Cherenkov Telescope Array ObservatoryJul 2, 2025H.E.S.S. programme searching for VHE gamma rays associated with FRBsJun 2, 2025Science Prospects for the Southern Wide-field Gamma-ray Observatory: SWGOJan 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 J1813-178Mar 7, 2024Dark Matter Line Searches with the Cherenkov Telescope ArrayJan 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 TeraelectronvoltsSep 7, 2023Prospects for $γ$-ray observations of the Perseus galaxy cluster with the Cherenkov Telescope ArrayJun 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?Oct 7, 2021Epoch of Reionization Power Spectrum Limits from Murchison Widefield Array Data Targeted at EoR1 FieldJul 30, 2021Constraining the 21cm brightness temperature of the IGM at $z$=6.6 around LAEs with the Murchison Widefield ArrayJun 1, 2021Search for dark matter annihilation signals from unidentified Fermi-LAT objects with H.E.S.SMay 27, 2021A new MWA limit on the 21 cm Power Spectrum at Redshifts $\sim$ 13 $-$ 17Feb 7, 2020Deep multi-redshift limits on Epoch of Reionisation 21cm Power Spectra from Four Seasons of Murchison Widefield Array ObservationsNov 22, 2019First Season MWA Phase II EoR Power Spectrum Results at Redshift 7May 17, 2019Gridded and direct Epoch of Reionisation bispectrum estimates using the Murchison Widefield ArraySep 18, 2018Assessment of ionospheric activity tolerances for Epoch of Reionisation science with the Murchison Widefield ArrayJul 14, 2018Comparing Redundant and Sky Model Based Interferometric Calibration: A First Look with Phase II of the MWA