Showing 1–20 of 28 results
/ Date/ Name
Jul 14, 2018Comparing Redundant and Sky Model Based Interferometric Calibration: A First Look with Phase II of the MWAJan 16, 2015The low-frequency environment of the Murchison Widefield Array: radio-frequency interference analysis and mitigationJun 19, 2015Confirmation of Wide-Field Signatures in Redshifted 21 cm Power SpectraJul 19, 2016Low frequency observations of linearly polarized structures in the interstellar medium near the south Galactic poleJul 13, 2016A High Reliability Survey of Discrete Epoch of Reionization Foreground Sources in the MWA EoR0 FieldJan 22, 2016The Importance of Wide-field Foreground Removal for 21 cm Cosmology: A Demonstration With Early MWA Epoch of Reionization ObservationsFeb 29, 2016High-energy sources at low radio frequency: the Murchison Widefield Array view of Fermi blazarsApr 29, 2016First Limits on the 21 cm Power Spectrum during the Epoch of X-ray heatingAug 22, 2016First Season MWA EoR Power Spectrum Results at Redshift 7Jul 8, 2014WSClean: an implementation of a fast, generic wide-field imager for radio astronomyFeb 6, 2016Parametrising Epoch of Reionization foregrounds: A deep survey of low-frequency point-source spectra with the MWAJul 5, 2015Ionospheric modelling using GPS to calibrate the MWA. 1: Comparison of first order ionospheric effects between GPS models and MWA observationsMay 23, 2016The Murchison Widefield Array 21 cm Power Spectrum Analysis MethodologyNov 6, 2014Modelling of the Spectral Energy Distribution of Fornax A: Leptonic and Hadronic Production of High Energy Emission from the Radio LobesAug 13, 2013On the detection and tracking of space debris using the Murchison Widefield Array. I. Simulations and test observations demonstrate feasibilityJul 17, 2015Broadband Spectral Modeling of the Extreme Gigahertz-Peaked Spectrum Radio Source PKS B0008-421Nov 22, 2019First Season MWA Phase II EoR Power Spectrum Results at Redshift 7Sep 10, 2014First Look Murchison Widefield Array observations of Abell 3667Jan 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 Data