Showing 1–20 of 28 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 observationsOct 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 $-$ 17May 5, 2020Calibration database for the Murchison Widefield Array All-Sky Virtual ObservatoryFeb 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 ArrayMay 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 5, 2018Measuring the global 21-cm signal with the MWA-I: improved measurements of the Galactic synchrotron background using lunar occultationAug 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 MWAFeb 26, 2018A Serendipitous MWA Search for Narrow-band and Broad-band Low Frequency Radio Transmissions from 1I/2017 U1 'OumuamuaJul 7, 2017A high resolution foreground model for the MWA EoR1 field: model and implications for EoR power spectrum analysis