Showing 1–20 of 42 results
/ Date/ Name
Aug 6, 2025Improved limits on the 21cm signal at z=6.5-7.0 with the MWA using Gaussian informationMay 14, 2025Limits on the 21 cm power spectrum at z=6.5-7.0 from MWA observationsJul 30, 2024Mitigating calibration errors from mutual coupling with time-domain filtering of 21 cm cosmological radio observationsJun 12, 2024Investigating Mutual Coupling in the Hydrogen Epoch of Reionization Array and Mitigating its Effects on the 21-cm Power SpectrumOct 7, 2021Epoch of Reionization Power Spectrum Limits from Murchison Widefield Array Data Targeted at EoR1 FieldJul 30, 2021Constraining the 21cm brightness temperature of the IGM at $z$=6.6 around LAEs with the Murchison Widefield ArrayMay 27, 2021A new MWA limit on the 21 cm Power Spectrum at Redshifts $\sim$ 13 $-$ 17Feb 7, 2020Deep multi-redshift limits on Epoch of Reionisation 21cm Power Spectra from Four Seasons of Murchison Widefield Array ObservationsNov 22, 2019First Season MWA Phase II EoR Power Spectrum Results at Redshift 7Oct 7, 2019Science with the Murchison Widefield Array: Phase I Results and Phase II OpportunitiesOct 6, 2019A VOEvent based automatic trigger system for the Murchison Widefield ArrayJul 21, 2019A high time resolution study of the millisecond pulsar J2241-5236 at frequencies below 300 MHzMay 17, 2019Gridded and direct Epoch of Reionisation bispectrum estimates using the Murchison Widefield ArrayNov 3, 2018Hunting for radio emission from the intermittent pulsar J1107-5907 at low frequenciesOct 10, 2018No low-frequency emission from extremely bright Fast Radio BurstsSep 18, 2018Assessment of ionospheric activity tolerances for Epoch of Reionisation science with the Murchison Widefield ArraySep 17, 2018The Phase II Murchison Widefield Array: Design OverviewAug 14, 2018In situ measurement of MWA primary beam variation using ORBCOMMJul 18, 2018Observations of Low-Frequency Radio Emission from Millisecond Pulsars and Multipath Propagation in the Interstellar MediumJul 14, 2018Comparing Redundant and Sky Model Based Interferometric Calibration: A First Look with Phase II of the MWA