Showing 1–20 of 58 results
/ Date/ Name
Aug 6, 2020A perfect power-law spectrum even at highest frequencies: The Toothbrush relicNov 15, 2023Probing diffuse radio emission in bridges between galaxy clusters with uGMRTFeb 23, 2022The LOFAR Two-metre Sky Survey -- V. Second data releaseMay 24, 2022Particle re-acceleration and diffuse radio sources in the galaxy cluster Abell 1550Oct 7, 2019Science with the Murchison Widefield Array: Phase I Results and Phase II OpportunitiesFeb 6, 2017LOFAR MSSS: Discovery of a 2.56 Mpc giant radio galaxy associated with a disturbed galaxy groupSep 5, 2024Ageing and dynamics of the tailed radio galaxies in Abell 2142Mar 11, 2025Relighting the fire in Hickson Compact Group (HCG) 15: magnetised fossil plasma revealed by the SKA Pathfinders & PrecursorsMay 13, 2025The Evolutionary Map of the Universe: A new radio atlas for the southern hemisphere skyDec 13, 2021A MeerKAT-meets-LOFAR Study of MS 1455.0+2232: A 590 kiloparsec 'Mini'-Halo in a Sloshing Cool-Core ClusterFeb 9, 2024Evolutionary Map of the Universe (EMU): a pilot search for diffuse, non-thermal radio emission in galaxy clusters with the Australian SKA PathfinderJun 1, 2017LOFAR MSSS: The Scaling Relation between AGN Cavity Power and Radio Luminosity at Low Radio FrequenciesJul 14, 2016Deep observations of the Super-CLASS super-cluster at 325 MHz with the GMRT: the low-frequency source catalogueMar 14, 2024First evidence of a connection between cluster-scale diffuse radio emission in cool-core galaxy clusters and sloshing featuresJan 12, 2022The galaxy group NGC 507: newly detected AGN remnant plasma transported by sloshingOct 21, 2025GLEAM-300: The GaLactic and Extragalactic All-sky Murchison Widefield Array (GLEAM) survey at 300 MHzFeb 17, 2026The LOFAR Two-metre Sky Survey: VII. Third Data ReleaseJan 27, 2026RM-Tools: Software for Analyzing Polarized Radio SpectraMay 26, 2023RMTable2023 and PolSpectra2023: standards for reporting polarization and Faraday rotation measurements of radio sourcesNov 5, 2018Cold gas outflows from the Small Magellanic Cloud traced with ASKAP