papers

Publications (28)

astro-ph.SR2014

The low-frequency characteristics of PSR J0437-4715 observed with the Murchison Widefield Array

N. D. Ramesh Bhat, S. M. Ord, S. E. Tremblay +37

We report on the detection of the millisecond pulsar PSR J0437-4715 with the Murchison Widefield Array (MWA) at a frequency of 192 MHz. Our observations show rapid modulations of p…

astro-ph.IM2023

Detection of intended and unintended emissions from Starlink satellites in the SKA-Low frequency range, at the SKA-Low site, with an SKA-Low station analog

Dylan Grigg, Steven Tingay, Marcin Sokolowski +3

Intended and unintended radio emissions from satellites can interfere with sensitive radio telescopes in the frequency ranges of key experiments in astrophysics and cosmology. We d…

astro-ph.IM2022

Optimal Dithering Configuration Mitigating Rayleigh-Backscattering-Induced Distortion in Radioastronomic Optical Fiber Systems

Jacopo Nanni, Andrea Giovannini, Enrico Lenzi +5

In the context of Radioastronomic applications where the Analog Radio-over-Fiber technology is used for the antenna downlink, detrimental nonlinearity effects arise because of the…

astro-ph.IM2017

The Engineering Development Array: A low frequency radio telescope utilising SKA precursor technology

Randall Wayth, Marcin Sokolowski, Tom Booler +21

We describe the design and performance of the Engineering Development Array (EDA), which is a low frequency radio telescope comprising 256 dual-polarisation dipole antennas working…

astro-ph.GA2026

The GLEAM 4-Jy (G4Jy) Sample: III. Further host-galaxy identification, and redshift assessment

Sarah V. White, Precious K. Sejake, Kshitij Thorat +17

In this paper we present 127 new host-galaxy identifications for G4Jy sources (S_151MHz > 4 Jy), based on radio images from MeerKAT, the Very Large Array Sky Survey (VLASS), and th…

astro-ph.GA2023

The Host Galaxy of FRB 20171020A Revisited

Karen Lee-Waddell, Clancy W. James, Stuart D. Ryder +12

The putative host galaxy of FRB 20171020A was first identified as ESO 601-G036 in 2018, but as no repeat bursts have been detected, direct confirmation of the host remains elusive.…

astro-ph.IM2021

The Engineering Development Array 2: design, performance and lessons from an SKA-Low prototype station

Randall Wayth, Marcin Sokolowski, Jess Broderick +21

We present the Engineering Development Array 2, which is one of two instruments built as a second generation prototype station for the future Square Kilometre Array Low Frequency A…

astro-ph.GA2026

The GLEAM 4-Jy (G4Jy) Sample: IV. Multiwavelength data and analysis

Sarah V. White, Precious K. Sejake, Kshitij Thorat +17

We provide an updated 'multiwavelength' version of the G4Jy catalogue (available at https://github.com/svw26/G4Jy, https://zenodo.org/communities/g4jy/records, and through VizieR),…

astro-ph.IM2012

Fast Holographic Deconvolution: a new technique for precision radio interferometry

Ian Sullivan, Miguel Morales, Bryna Hazelton +48

We introduce the Fast Holographic Deconvolution method for analyzing interferometric radio data. Our new method is an extension of A-projection/software-holography/forward modeling…

astro-ph.IM2021

Characterization of the SKA1-Low prototype station Aperture Array Verification System 2

Giulia Macario, Giuseppe Pupillo, Gianni Bernardi +16

The low frequency component of the Square Kilometre Array (SKA1-Low) will be an aperture phased array located at the Murchison Radio-astronomy Observatory (MRO) site in Western Aus…

astro-ph.IM2026

A signal dedispersion algorithm for imaging-based transient searches

Cristian Di Pietrantonio, Marcin Sokolowski, Christopher Harris +2

Dedispersion is the computational process of correcting for the frequency-dependent time delay affecting a radio signal that propagates through the interstellar and intergalactic m…

astro-ph.CO2024

Strategy for mitigation of systematics for EoR experiments with the Murchison Widefield Array

Chuneeta D. Nunhokee, Dev Null, Cathryn M. Trott +4

Observations of the 21 cm signal face significant challenges due to bright astrophysical foregrounds that are several orders of magnitude higher than the brightness of the hydrogen…

astro-ph.IM2020

Controlling Rayleigh-Backscattering-Induced Distortion in Radio over Fiber Systems for Radioastronomic Applications

Jacopo Nanni, Andrea Giovannini, Muhammad Usman Hadi +6

Radio over Fiber (RoF) Systems exploiting a direct modulation of the laser source are presently utilized within important Radioastronomic scenarios. Due to the particular operating…

astro-ph.IM2025

BLINK: an End-To-End GPU High Time Resolution Imaging Pipeline for Fast Radio Burst Searches with the Murchison Widefield Array

Cristian Di Pietrantonio, Marcin Sokolowski, Christopher Harris +2

Petabytes of archival high time resolution observations have been captured with the Murchison Widefield Array. The search for Fast Radio Bursts within these using established softw…

astro-ph2008

The Sloan Lens ACS Survey. VII. Elliptical Galaxy Scaling Laws from Direct Observational Mass Measurements

Adam S. Bolton, Tommaso Treu, Leon V. E. Koopmans +5

We use a sample of 53 massive early-type strong gravitational lens galaxies with well-measured redshifts (ranging from z=0.06 to 0.36) and stellar velocity dispersions (between 175…

astro-ph2006

Field Deployment of Prototype Antenna Tiles for the Mileura Widefield Array--Low Frequency Demonstrator

Judd D. Bowman, David G. Barnes, Frank H. Briggs +22

Experiments were performed with prototype antenna tiles for the Mileura Widefield Array--Low Frequency Demonstrator (MWA-LFD) to better understand the widefield, wideband propertie…

astro-ph.CO2014

Overcoming real-world obstacles in 21 cm power spectrum estimation: A method demonstration and results from early Murchison Widefield Array data

Joshua S. Dillon, Adrian Liu, Christopher L. Williams +16

We present techniques for bridging the gap between idealized inverse covariance weighted quadratic estimation of 21 cm power spectra and the real-world challenges presented univers…

astro-ph.HE2026

50-250 MHz Pulsar Census with an SKA-Low prototype station: Spectra and Polarization

Pratik Kumar, Marcin Sokolowski, Randall Wayth

Low-frequency pulsar observations are crucial for understanding pulsar emission spectra and population physics, as well as for probing the interstellar medium (ISM) and Earth's ion…

astro-ph.GA2018

The MWA GLEAM 4-Jy (G4Jy) Sample

Sarah V. White, Thomas M. O. Franzen, O. Ivy Wong +15

Powerful radio-galaxies feature heavily in our understanding of galaxy evolution. However, when it comes to studying their properties as a function of redshift and/or environment,…

astro-ph.GA2020

The GLEAM 4-Jy (G4Jy) Sample: I. Definition and the catalogue

Sarah V. White, Thomas M. O. Franzen, Chris J. Riseley +21

The Murchison Widefield Array (MWA) has observed the entire southern sky (Declination, 30 deg) at low radio-frequencies, over the range 72-231 MHz. These observations constit…

astro-ph.CO2009

Strong gravitational lensing probes of the particle nature of dark matter

Leonidas A. Moustakas, Kevork Abazajian, Andrew Benson +44

There is a vast menagerie of plausible candidates for the constituents of dark matter, both within and beyond extensions of the Standard Model of particle physics. Each of these ca…

astro-ph.GA2020

The GLEAM 4-Jy (G4Jy) Sample: II. Host-galaxy identification for individual sources

Sarah V. White, Thomas M. O. Franzen, Chris J. Riseley +20

The entire southern sky (Declination, 30 deg) has been observed using the Murchison Widefield Array (MWA), which provides radio imaging of 2-arcmin resolution at low fr…

astro-ph.IM2022

DUG Insight: A software package for big-data analysis and visualisation, and its demonstration for passive radar space situational awareness using radio telescopes

Dylan Grigg, Steven Tingay, Marcin Sokolowski +1

As the demand for software to support the processing and analysis of massive radio astronomy datasets increases in the era of the SKA, we demonstrate the interactive workflow build…

astro-ph.IM2020

A survey of spatially and temporally resolved radio frequency interference in the FM band at the Murchison Radio-astronomy Observatory

Steven Tingay, Marcin Sokolowski, Randall Wayth +1

We present the first survey of radio frequency interference (RFI) at the future site of the low frequency Square Kilometre Array (SKA), the Murchison Radio-astronomy Observatory (M…

astro-ph2008

The Sloan Lens ACS Survey. V. The Full ACS Strong-Lens Sample

Adam S. Bolton, Scott Burles, Leon V. E. Koopmans +5

We present the definitive data for the full sample of 131 strong gravitational lens candidates observed with the Advanced Camera for Surveys (ACS) aboard the Hubble Space Telescope…

astro-ph.GA2017

A First Look for Molecules between 103 and 133 MHz using the Murchison Widefield Array

Chenoa Tremblay, Natasha Hurley-Walker, Maria Cunningham +4

We detail and present results from a pilot study to assess the feasibility of detecting molecular lines at low radio frequencies. We observed a 400 square degree region centred on…

astro-ph.IM2011

First geodetic observations using new VLBI stations ASKAP-29 and WARK12M

Leonid Petrov, Chris Phillips, Tasso Tzioumis +11

We report the results of a successful 7 hour 1.4 GHz VLBI experiment using two new stations, ASKAP-29 located in Western Australia and WARK12M located on the North Island of New Ze…

astro-ph.IM2025

Intrinsic Cross Polarization Ratio maps from all-sky observations with the SKA-Low prototype station Aperture Array Verification System 2

Giulia Macario, Giuseppe Pupillo, Gianni Bernardi +10

The low-frequency radio telescope of the Square Kilometre Array (SKA-Low), currently under construction in the remote Murchison shire in the Western Australia's outback, will obser…