activity
20122026
most citedWSClean: an implementation of a fast, generic wide-field imager for radio astronomy

937 citations · 4.1k across the 35 of their papers we have counts for

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Showing 2015Show all

10 papers · 1 filter

astro-ph.IM2015★ 72 cited

Characterization of a Low-Frequency Radio Astronomy Prototype Array in Western Australia

A. T. Sutinjo, T. M. Colegate, R. B. Wayth +12

We report characterization results for an engineering prototype of a next-generation low-frequency radio astronomy array. This prototype, which we refer to as the Aperture Array Ve…

astro-ph.IM2015★ 20 cited

Murchison Widefield Array Observations of Anomalous Variability: A Serendipitous Night-time Detection of Interplanetary Scintillation

D. L. Kaplan, S. J. Tingay, P. K. Manoharan +33

We present observations of high-amplitude rapid (2 s) variability toward two bright, compact extragalactic radio sources out of several hundred of the brightest radio sources in on…

astro-ph.GA2015★ 89 cited

Broadband Spectral Modeling of the Extreme Gigahertz-Peaked Spectrum Radio Source PKS B0008-421

J. R. Callingham, B. M. Gaensler, R. D. Ekers +40

We present broadband observations and spectral modeling of PKS B0008-421, and identify it as an extreme gigahertz-peaked spectrum (GPS) source. PKS B0008-421 is characterized by th…

astro-ph.IM2015★ 18 cited

Ionospheric modelling using GPS to calibrate the MWA. 1: Comparison of first order ionospheric effects between GPS models and MWA observations

B. S. Arora, J. Morgan, S. M. Ord +56

We compare first order (refractive) ionospheric effects seen by the Murchison Widefield Array (MWA) with the ionosphere as inferred from Global Positioning System (GPS) data. The f…

astro-ph.CO2015★ 95 cited

Confirmation of Wide-Field Signatures in Redshifted 21 cm Power Spectra

Nithyanandan Thyagarajan, Daniel C. Jacobs, Judd D. Bowman +52

We confirm our recent prediction of the "pitchfork" foreground signature in power spectra of high-redshift 21 cm measurements where the interferometer is sensitive to large-scale s…

astro-ph.IM2015★ 38 cited

Power spectrum analysis of ionospheric fluctuations with the Murchison Widefield Array

Shyeh Tjing Loi, Cathryn M. Trott, Tara Murphy +45

Low-frequency, wide field-of-view (FoV) radio telescopes such as the Murchison Widefield Array (MWA) enable the ionosphere to be sampled at high spatial completeness. We present th…

astro-ph.SR2015★ 74 cited

Multiwavelength observations of a partially eruptive filament on 2011 September 8

Q. M. Zhang, Z. J. Ning, Y. Guo +5

In this paper, we report our multiwavelength observations of a partial filament eruption event in NOAA active region 11283 on 2011 September 8. A magnetic null point and the corres…

astro-ph.IM2015★ 161 cited

Foregrounds in Wide-Field Redshifted 21 cm Power Spectra

Nithyanandan Thyagarajan, Daniel C. Jacobs, Judd D. Bowman +61

Detection of 21~cm emission of HI from the epoch of reionization, at redshifts z>6, is limited primarily by foreground emission. We investigate the signatures of wide-field measure…

astro-ph.IM2015★ 42 cited

The Murchison Widefield Array Correlator

S. M. Ord, B. Crosse, D. Emrich +64

The Murchison Widefield Array (MWA) is a Square Kilometre Array (SKA) Precursor. The telescope is located at the Murchison Radio--astronomy Observatory (MRO) in Western Australia (…

astro-ph.IM2015★ 164 cited

The low-frequency environment of the Murchison Widefield Array: radio-frequency interference analysis and mitigation

A. R. Offringa, R. B. Wayth, N. Hurley-Walker +62

The Murchison Widefield Array (MWA) is a new low-frequency interferometric radio telescope built in Western Australia at one of the locations of the future Square Kilometre Array (…