Showing 21–40 of 104 results
/ Date/ Name
Jan 16, 2015The low-frequency environment of the Murchison Widefield Array: radio-frequency interference analysis and mitigationOct 8, 2010Interferometric imaging with the 32 element Murchison Wide-field ArrayJan 31, 2024Formation mechanisms of single-crystalline InN quantum dots fabricated via droplet epitaxyJan 27, 2013The Murchison Widefield Array: solar science with the low frequency SKA PrecursorAug 14, 2018In situ measurement of MWA primary beam variation using ORBCOMMJan 10, 2019The FHD/$\boldsymbol{\varepsilon}$ppsilon Epoch of Reionization Power Spectrum PipelineMay 27, 2021A new MWA limit on the 21 cm Power Spectrum at Redshifts $\sim$ 13 $-$ 17Oct 7, 2021Epoch of Reionization Power Spectrum Limits from Murchison Widefield Array Data Targeted at EoR1 FieldApr 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 7Jun 1, 2015An analysis of the halo and relic radio emission from Abell 3376 from Murchison Widefield Array observationsJul 8, 2014WSClean: an implementation of a fast, generic wide-field imager for radio astronomyFeb 26, 2018A Serendipitous MWA Search for Narrow-band and Broad-band Low Frequency Radio Transmissions from 1I/2017 U1 'OumuamuaFeb 17, 2016Beamforming Errors in Murchison Widefield Array Phased Array Antennas and their effects on Epoch of Reionization ScienceFeb 6, 2016Parametrising Epoch of Reionization foregrounds: A deep survey of low-frequency point-source spectra with the MWADec 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 observationsJan 7, 2000Evidence for TeV Emission from GRB 970417aJul 30, 2024Mitigating calibration errors from mutual coupling with time-domain filtering of 21 cm cosmological radio observationsMay 23, 2016The Murchison Widefield Array 21 cm Power Spectrum Analysis Methodology