Showing 1–20 of 101 results
/ Date/ Name
May 19, 2020The POlarised GLEAM Survey (POGS) II: Results from an All-Sky Rotation Measure Synthesis Survey at Long WavelengthsSep 25, 2018The POlarised GLEAM Survey (POGS) I: First Results from a Low-Frequency Radio Linear Polarisation Survey of the Southern SkySep 2, 2021The Rapid ASKAP Continuum Survey Paper II: First Stokes I Source Catalogue Data ReleaseDec 9, 2015A pilot ASKAP survey of radio transient events in the region around the intermittent pulsar PSR J1107-5907Feb 10, 2017154 MHz detection of faint, polarized flares from UV CetiJan 22, 2016Wide-field broadband radio imaging with phased array feeds: a pilot multi-epoch continuum survey with ASKAP-BETAJun 3, 2020The Panchromatic Afterglow of GW170817: The full uniform dataset, modeling, comparison with previous results and implicationsSep 16, 2024The CRAFT Coherent (CRACO) upgrade I: System Description and Results of the 110-ms Radio Transient Pilot SurveyOct 20, 2017Calibration and Stokes Imaging with Full Embedded Element Primary Beam Model for the Murchison Widefield ArrayJan 16, 2015The low-frequency environment of the Murchison Widefield Array: radio-frequency interference analysis and mitigationMar 4, 2015Discovery of HI gas in a young radio galaxy at $z = 0.44$ using the Australian Square Kilometre Array PathfinderJan 15, 2025The emission of interpulses by a 6.45-hour period coherent radio transientAug 29, 2024Rocking the BOAT: the ups and downs of the long-term radio light curve for GRB 221009AFeb 3, 2021Australian Square Kilometre Array Pathfinder: I. System DescriptionSep 10, 2014First Look Murchison Widefield Array observations of Abell 3667Nov 5, 2014On the radio properties of the intermediate-mass black hole candidate ESO 243-49 HLX-1Jan 9, 2016CHIPS: The Cosmological HI Power Spectrum EstimatorJun 2, 2015Empirical Covariance Modeling for 21 cm Power Spectrum Estimation: A Method Demonstration and New Limits from Early Murchison Widefield Array 128-Tile DataJul 5, 2017Connecting X-ray absorption and 21cm neutral hydrogen absorption in obscured radio AGNFeb 15, 2009Lofar, E-Lofar and Low-Frequency Vlbi