activity
20112023
most citedAn improved map of the Galactic Faraday sky

252 citations · 998 across the 34 of their papers we have counts for

collaborators

35 papers

astro-ph.IM2023★ 5 cited

Correcting Bandwidth Depolarization by Extreme Faraday Rotation

Maxwell A. Fine, Cameron L. Van Eck, Luke Pratley

Measurements of the polarization of radio emission are subject to a number of depolarization effects such as bandwidth depolarization, which is caused by the averaging effect of a…

astro-ph.GA2021★ 10 cited

The Global Magneto-Ionic Medium Survey (GMIMS): The brightest polarized region in the Southern sky at 75cm and its implications for Radio Loop II

Alec J. M. Thomson, T. L. Landecker, N. M. McClure-Griffiths +16

Using the Global Magneto-Ionic Medium Survey (GMIMS) Low-Band South (LBS) southern sky polarization survey, covering 300 to 480 MHz at 81 arcmin resolution, we reveal the brightest…

cs.IT2021★ 5 cited

Sparse image reconstruction on the sphere: a general approach with uncertainty quantification

Matthew A. Price, Luke Pratley, Jason D. McEwen

Inverse problems defined naturally on the sphere are becoming increasingly of interest. In this article we provide a general framework for evaluation of inverse problems on the sph…

astro-ph.IM2020★ 7 cited

Removing non-physical structure in fitted Faraday rotated signals: non-parametric QU-fitting

Luke Pratley, Melanie Johnston-Hollitt, Bryan M. Gaensler

Next-generation spectro-polarimetric broadband surveys will probe cosmic magnetic fields in unprecedented detail, using the magneto-optical effect known as Faraday rotation. Howeve…

astro-ph.IM2020

Novel perspectives gained from new reconstruction algorithms

Luke Pratley, Melanie Johnston-Hollitt, Jason D. McEwen

Since the 1970s, much of traditional interferometric imaging has been built around variations of the CLEAN algorithm, in both terminology, methodology, and algorithm development. R…

astro-ph.GA2020

Magnetism Science with the Square Kilometre Array

George Heald, Sui Ann Mao, Valentina Vacca +41

The Square Kilometre Array (SKA) will answer fundamental questions about the origin, evolution, properties, and influence of magnetic fields throughout the Universe. Magnetic field…

astro-ph.IM2020

Offline and online reconstruction for radio interferometric imaging

Xiaohao Cai, Luke Pratley, Jason D. McEwen

Radio astronomy is transitioning to a big-data era due to the emerging generation of radio interferometric (RI) telescopes, such as the Square Kilometre Array (SKA), which will acq…

astro-ph.CO2020★ 28 cited

Spherical Bayesian mass-mapping with uncertainties: full sky observations on the celestial sphere

Matthew A. Price, Jason D. McEwen, L. Pratley +1

To date weak gravitational lensing surveys have typically been restricted to small fields of view, such that the has been sufficiently satisfied.…

astro-ph.IM2019★ 9 cited

Wide-band Rotation Measure Synthesis

Luke Pratley, Melanie Johnston-Hollitt

Rotation measure synthesis allows the estimation of Faraday dispersion via a Fourier transform and is the primary tool to probe cosmic magnetic fields. We show this can be consider…

astro-ph.IM2019★ 1 cited

Load balancing for distributed interferometric image reconstruction

Luke Pratley, Jason D. McEwen

We present a new algorithm to perform wide-field radio interferometric image reconstruction, with exact non-coplanar correction, that scales to big-data. This algorithm allows us t…

astro-ph.IM2019★ 5 cited

-stacking -projection hybrid algorithm for wide-field interferometric imaging: implementation details and improvements

L. Pratley, M. Johnston-Hollitt, J. D. McEwen

We present a detailed discussion of the implementation strategies for a recently developed -stacking -projection hybrid algorithm used to reconstruct wide-field interferometr…

astro-ph.IM2019★ 3 cited

Sparse Image Reconstruction for the SPIDER Optical Interferometric Telescope

Luke Pratley, Jason D. McEwen

The concept of a recently proposed small-scale interferometric optical imaging device, an instrument known as the Segmented Planar Imaging Detector for Electro-optical Reconnaissan…

astro-ph.IM2019★ 2 cited

Distributed and parallel sparse convex optimization for radio interferometry with PURIFY

Luke Pratley, Jason D. McEwen, Mayeul d'Avezac +4

Next generation radio interferometric telescopes are entering an era of big data with extremely large data sets. While these telescopes can observe the sky in higher sensitivity an…

physics.optics2018★ 18 cited

Approximate T-matrix and optical properties of spheroidal particles to third order in size parameter

Matt R. A. Majic, Luke Pratley, Dmitri Schebarchov +3

We here calculate the series expansion of the T-matrix for a spheroidal particle in the small-size/long-wavelength limit, up to third lowest order with respect to the size paramete…

astro-ph.IM2018★ 17 cited

A fast and exact -stacking and -projection hybrid algorithm for wide-field interferometric imaging

Luke Pratley, Melanie Johnston-Hollitt, Jason D. McEwen

The standard wide-field imaging technique, the -projection, allows correction for wide-fields of view for non-coplanar radio interferometric arrays. However, calculating exact c…

astro-ph.IM2017★ 1 cited

Online radio interferometric imaging: assimilating and discarding visibilities on arrival

Xiaohao Cai, Luke Pratley, Jason D. McEwen

The emerging generation of radio interferometric (RI) telescopes, such as the Square Kilometre Array (SKA), will acquire massive volumes of data and transition radio astronomy to a…

astro-ph.CO2017★ 5 cited

Upper limits on a radio halo in Abell 3667 at 1.4 GHz

M. Johnston-Hollitt, L. Pratley

The presence of a radio halo in the massive, merging cluster Abell 3667 has recently become a focus of debate in the literature following a putative halo detection at 2.4 GHz despi…

astro-ph.GA2017★ 19 cited

LOFAR MSSS: The Scaling Relation between AGN Cavity Power and Radio Luminosity at Low Radio Frequencies

G. Kokotanekov, M. Wise, G. H. Heald +35

We present a new analysis of the widely used relation between cavity power and radio luminosity in clusters of galaxies with evidence for strong AGN feedback. We study the correlat…

astro-ph.IM2017

PURIFYing real radio interferometric observations

Luke Pratley, Jason D. McEwen, Mayeul d'Avezac +3

Next-generation radio interferometers, such as the Square Kilometre Array (SKA), will revolutionise our understanding of the universe through their unprecedented sensitivity and re…

astro-ph.GA2017★ 19 cited

LOFAR MSSS: Discovery of a 2.56 Mpc giant radio galaxy associated with a disturbed galaxy group

A. O. Clarke, G. Heald, T. Jarrett +40

We report on the discovery in the LOFAR Multifrequency Snapshot Sky Survey (MSSS) of a giant radio galaxy (GRG) with a projected size of Mpc projected on the sky. I…

astro-ph.IM2017★ 15 cited

The w-effect in interferometric imaging: from a fast sparse measurement operator to super-resolution

Arwa Dabbech, Laura Wolz, Luke Pratley +2

Modern radio telescopes, such as the Square Kilometre Array (SKA), will probe the radio sky over large fields-of-view, which results in large w-modulations of the sky image. This e…

astro-ph.IM2016★ 61 cited

Robust sparse image reconstruction of radio interferometric observations with purify

Luke Pratley, Jason D. McEwen, Mayeul d'Avezac +3

Next-generation radio interferometers, such as the Square Kilometre Array (SKA), will revolutionise our understanding of the universe through their unprecedented sensitivity and re…

astro-ph.CO2016★ 27 cited

ATCA observations of the MACS-Planck Radio Halo Cluster Project - I. New detection of a radio halo in PLCK G285.0-23.7

Gerardo Martinez Aviles, Chiara Ferrari, Melanie Johnston-Hollitt +12

We investigate the possible presence of diffuse radio emission in the intermediate redshift, massive cluster PLCK G285.0-23.7 (z=0.39, M_500 = 8.39 x 10^(14) M_Sun). Our 16cm-band…

astro-ph.IM2016★ 26 cited

An improved method for polarimetric image restoration in interferometry

Luke Pratley, Melanie Johnston-Hollitt

Interferometric radio astronomy data require the effects of limited coverage in the Fourier plane to be accounted for via a deconvolution process. For the last 40 years this proces…