activity
20172020
most citedFirst Season MWA Phase II EoR Power Spectrum Results at Redshift 7

98 citations · 212 across the 7 of their papers we have counts for

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7 papers · 1 filter

astro-ph.IM20209 cited

Calibration database for the Murchison Widefield Array All-Sky Virtual Observatory

M. Sokolowski, C. H. Jordan, G. Sleap +11

We present a calibration component for the Murchison Widefield Array All-Sky Virtual Observatory (MWA ASVO) utilising a newly developed PostgreSQL database of calibration solutions…

astro-ph.IM201935 cited

Science with the Murchison Widefield Array: Phase I Results and Phase II Opportunities

A. P. Beardsley, M. Johnston-Hollitt, C. M. Trott +56

The Murchison Widefield Array (MWA) is an open access telescope dedicated to studying the low frequency (80300 MHz) southern sky. Since beginning operations in mid 2013, the MWA…

astro-ph.IM201910 cited

A VOEvent based automatic trigger system for the Murchison Widefield Array

P. J. Hancock, G. E. Anderson, A. Williams +22

The Murchison Widefield Array (MWA) is an electronically steered low frequency (\,MHz) radio interferometer, with a `slew' time less than 8seconds. Low frequency (\…

astro-ph.IM2018

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.IM2018

In situ measurement of MWA primary beam variation using ORBCOMM

J. L. B. Line, B. McKinley, J. Rasti +21

We provide the first in situ measurements of antenna element (tile) beam shapes of the Murchison Widefield Array (MWA), a low radio-frequency interferometer and an SKA precursor. M…

astro-ph.IM2018

Comparing Redundant and Sky Model Based Interferometric Calibration: A First Look with Phase II of the MWA

W. Li, J. C. Pober, B. J. Hazelton +53

Interferometric arrays seeking to measure the 21 cm signal from the Epoch of Reionization must contend with overwhelmingly bright emission from foreground sources. Accurate recover…