activity
20172022
most citedDeep multi-redshift limits on Epoch of Reionisation 21cm Power Spectra from Four Seasons of Murchison Widefield Array Observations

224 citations · 537 across the 22 of their papers we have counts for

collaborators

22 papers

astro-ph.HE2022★ 4 cited

A targeted search for repeating fast radio bursts with the MWA

J. Tian, G. E. Anderson, P. J. Hancock +7

We present a targeted search for low-frequency (144--215\,MHz) FRB emission from five repeating FRBs using 23.3\,hr of archival data taken with the Murchison Widefield Array (MWA)…

astro-ph.HE2022★ 13 cited

Spectral analysis of 22 radio pulsars using SKA-Low precursor stations

C. P. Lee, N. D. R. Bhat, M. Sokolowski +4

We present the first observational study of pulsars performed with the second-generation precursor stations to the low-frequency component of the Square Kilometre Array (SKA-Low):…

astro-ph.IM2022★ 2 cited

System equivalent flux density of Stokes I, Q, U, V of a polarimetric interferometer

A. T. Sutinjo, D. C. X. Ung, M. Sokolowski

We present the system equivalent flux density (SEFD) expressions for all four Stokes parameters: I, Q, U, V. The expressions were derived based on our derivation of SEFD I (for Sto…

astro-ph.HE2022★ 6 cited

High time resolution search for prompt radio emission from the long GRB 210419A with the Murchison Widefield Array

J. Tian, G. E. Anderson, P. J. Hancock +15

We present a low-frequency (170\textendash200\,MHz) search for prompt radio emission associated with the long GRB 210419A using the rapid-response mode of the Murchison Widefield A…

astro-ph.IM2022★ 18 cited

What is the SKA-Low Sensitivity for Your Favourite Radio Source ?

M. Sokolowski, S. J. Tingay, D. B. Davidson +8

The SKA will be the largest radio astronomy observatory ever built, providing unprecedented sensitivity over a very broad frequency (50 MHz to 15.3 GHz). The SKA-Low (50 - 350 MHz)…

astro-ph.IM2022

System design and calibration of SITARA -- a global 21 cm short spacing interferometer prototype

Jishnu N. Thekkeppattu, Benjamin McKinley, Cathryn M. Trott +2

Global 21-cm experiments require exquisitely precise calibration of the measurement systems in order to separate the weak 21-cm signal from Galactic and extragalactic foregrounds a…