Showing 1–20 of 93 results
/ Date/ Name
Feb 20, 2026Single- and double-headed odd radio circles in the LOFAR surveysJan 20, 2018The SAMI Galaxy Survey: gas content and interaction as the drivers of kinematic asymmetryJan 28, 2022Peculiar radio$-$X-ray relationship in active starsJan 3, 2023Polarised radio pulsations from a new T dwarf binaryNov 19, 2018LoTSS/HETDEX: Disentangling star formation and AGN activity in gravitationally-lensed radio-quiet quasarsNov 19, 2018Systematic effects in LOFAR data: A unified calibration strategyAug 30, 2018LOFAR MSSS: Flattening low-frequency radio continuum spectra of nearby galaxiesAug 16, 2021Sub-arcsecond imaging with the International LOFAR Telescope: II. Completion of the LOFAR Long-Baseline Calibrator SurveyAug 16, 2021Sub-arcsecond imaging with the International LOFAR Telescope I. Foundational calibration strategy and pipelineMay 9, 2016Ionospheric Modelling using GPS to Calibrate the MWA. II: Regional ionospheric modelling using GPS and GLONASS to estimate ionospheric gradientsOct 5, 2017The Spectral Energy Distribution of Powerful Starburst Galaxies I: Modelling the Radio ContinuumJun 1, 2015An analysis of the halo and relic radio emission from Abell 3376 from Murchison Widefield Array observationsNov 16, 2016Galactic synchrotron emissivity measurements between 250° < l < 355° from the GLEAM survey with the MWAApr 11, 2018Extended X-ray emission in PKS 1718$-$649Dec 13, 2014The Spectral Variability of the GHz-Peaked Spectrum Radio Source PKS 1718-649 and a Comparison of Absorption ModelsJul 5, 2015Ionospheric modelling using GPS to calibrate the MWA. 1: Comparison of first order ionospheric effects between GPS models and MWA observationsMay 15, 2024Probing particle acceleration in Abell 2256: from to 16 MHz to gamma raysJun 20, 2016Low Radio Frequency Observations and Spectral Modelling of the Remnant of Supernova 1987AJan 24, 2017A study of halo and relic radio emission in merging clusters using the Murchison Widefield ArrayMar 31, 2017Low frequency spectral energy distributions of radio pulsars detected with the Murchison Widefield Array