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20072026
most citedWSClean: an implementation of a fast, generic wide-field imager for radio astronomy

937 citations · 7.3k across the 150 of their papers we have counts for

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Showing 2018Show all

8 papers · 1 filter

astro-ph.GA2018★ 44 cited

Source counts and confusion at 72-231 MHz in the MWA GLEAM survey

T. M. O. Franzen, T. Vernstrom, C. A. Jackson +5

The GaLactic and Extragalactic All-sky MWA survey (GLEAM) is a radio continuum survey at 72-231 MHz of the whole sky south of declination +30 deg, carried out with the Murchison Wi…

astro-ph.GA2018★ 2 cited

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.GA2018★ 37 cited

The POlarised GLEAM Survey (POGS) I: First Results from a Low-Frequency Radio Linear Polarisation Survey of the Southern Sky

C. J. Riseley, E. Lenc, C. L. Van Eck +7

The low-frequency polarisation properties of radio sources are poorly studied, particularly in statistical samples. However, the new generation of low-frequency telescopes, such as…

astro-ph.IM2018★ 1 cited

De-distorting ionospheric effects in the image plane

N. Hurley-Walker, P. J. Hancock

The Earth's ionosphere refracts radio waves incident on an interferometer, resulting in shifts to the measured positions of radio sources. We present a method to smoothly remove th…

astro-ph.GA2018★ 19 cited

Galactic synchrotron distribution derived from 152 HII region absorption features in the full GLEAM survey

H. Su, J. P. Macquart, N. Hurley-Walker +22

We derive the synchrotron distribution in the Milky Way disk from HII region absorption observations over -40° < l < 40° at six frequencies of 76.2, 83.8, 91.5, 99.2, 106.9, and 11…

astro-ph.GA2018★ 2 cited

Low-Frequency Carbon Recombination Lines in the Orion Molecular Cloud Complex

Chenoa D. Tremblay, Christopher H. Jordan, Maria Cunningham +2

We detail tentative detections of low-frequency carbon radio recombination lines from within the Orion molecular cloud complex observed at 99-129 MHz. These tentative detections in…