activity
19972025
most citedThe Phase II Murchison Widefield Array: Design Overview

240 citations · 709 across the 15 of their papers we have counts for

collaborators

15 papers

astro-ph.GA2025

Stellar Mass-Dispersion Measure Correlations Constrain Baryonic Feedback in Fast Radio Burst Host Galaxies

Calvin Leung, Sunil Simha, Isabel Medlock +20

Low redshift fast radio bursts (FRBs) provide robust measurements of the host-galaxy contribution to the dispersion measure (DM), which can constrain the circumgalactic medium (CGM…

astro-ph.HE2020★ 91 cited

Detection of Repeating FRB 180916.J0158+65 Down to Frequencies of 300 MHz

P. Chawla, B. C. Andersen, M. Bhardwaj +37

We report on the detection of seven bursts from the periodically active, repeating fast radio burst (FRB) source FRB 180916.J0158+65 in the 300-400-MHz frequency range with the Gre…

astro-ph.IM2018★ 240 cited

The Phase II Murchison Widefield Array: Design Overview

Randall B. Wayth, Steven J. Tingay, Cathryn M. Trott +26

We describe the motivation and design details of the "Phase II" upgrade of the Murchison Widefield Array (MWA) radio telescope. The expansion doubles to 256 the number of antenna t…

astro-ph.IM2016

Limits of noise and confusion in the MWA GLEAM year 1 survey

T. M. O. Franzen, C. A. Jackson, J. R. Callingham +21

The GaLactic and Extragalactic All-sky MWA survey (GLEAM) is a new relatively low resolution, contiguous 72-231 MHz survey of the entire sky south of declination +25 deg. In this p…

astro-ph.GA2016

The MWA GLEAM 4Jy Sample; a new large, bright radio source sample at 151 MHz

C A Jackson, T M O Franzen, N Seymour +25

This paper outlines how the new GaLactic and Extragalactic All-sky MWA Survey (GLEAM, Wayth et al. 2015), observed by the Murchison Widefield Array covering the frequency range 72…

astro-ph.GA2013★ 5 cited

A Precision Multi-Band Two-Epoch Photometric Catalog of 44 Million Sources in the Northern Sky from Combination of the USNO-B and Sloan Digital Sky Survey Catalogs

G. J. Madsen, B. M. Gaensler

A key science driver for the next generation of wide-field optical and radio surveys is the exploration of the time variable sky. These surveys will have unprecedented sensitivity…