Showing 1–20 of 46 results
/ Date/ Name
Apr 9, 2026Chasing Gamma-Ray Signals from Binary Neutron Star Coalescences with the Cherenkov Telescope Array: Prospects and Observing StrategiesFeb 28, 2026A Particle Detector Array deployed to the Murchison Widefield Array in the Murchison Radio-astronomy ObservatoryAug 26, 2025Prospects for dark matter observations in dwarf spheroidal galaxies with the Cherenkov Telescope Array ObservatoryAug 6, 2025Improved limits on the 21cm signal at z=6.5-7.0 with the MWA using Gaussian informationMay 14, 2025Limits on the 21 cm power spectrum at z=6.5-7.0 from MWA observationsAug 30, 2023Probing the jet size of two Black hole X-ray Binaries in the hard stateAug 9, 2023Demonstration of Orbit Determination for LEO Objects using the Murchison Widefield ArrayFeb 15, 2023Search for neutrino counterparts to the gravitational wave sources from LIGO/Virgo O3 run with the ANTARES detectorDec 22, 2022Hint for a TeV neutrino emission from the Galactic Ridge with ANTARESFeb 28, 2022Search for Magnetic Monopoles with ten years of the ANTARES neutrino telescopeJan 27, 2022Search for solar atmospheric neutrinos with the ANTARES neutrino telescopeJan 18, 2022Search for Spatial Correlations of Neutrinos with Ultra-High-Energy Cosmic RaysOct 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 ArrayMay 27, 2021A new MWA limit on the 21 cm Power Spectrum at Redshifts $\sim$ 13 $-$ 17May 14, 2020The SKA Particle Array Prototype: The First Particle Detector at the Murchison Radio-astronomy ObservatoryMay 5, 2020Calibration database for the Murchison Widefield Array All-Sky Virtual ObservatoryFeb 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 7Oct 7, 2019Science with the Murchison Widefield Array: Phase I Results and Phase II Opportunities