activity
20082025
most citedAustralian Square Kilometre Array Pathfinder: I. System Description

293 citations · 2.8k across the 77 of their papers we have counts for

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45 papers · 1 filter

astro-ph.GA2025★ 20 cited

The Evolutionary Map of the Universe: A new radio atlas for the southern hemisphere sky

A. M. Hopkins, A. Kapinska, J. Marvil +70

We present the Evolutionary Map of the Universe (EMU) survey conducted with the Australian Square Kilometre Array Pathfinder (ASKAP). EMU aims to deliver the touchstone radio atlas…

astro-ph.GA2023★ 25 cited

MIGHTEE-HI: The first MeerKAT HI mass function from an untargeted interferometric survey

Anastasia A. Ponomareva, Matt J. Jarvis, Hengxing Pan +17

We present the first measurement of the HI mass function (HIMF) using data from MeerKAT, based on 276 direct detections from the MIGHTEE Survey Early Science data covering a period…

astro-ph.GA2023★ 18 cited

Radio spectral properties of star-forming galaxies between 150-5000MHz in the ELAIS-N1 field

Fangxia An, M. Vaccari, P. N. Best +9

By combining high-sensitivity LOFAR 150MHz, uGMRT 400MHz and 1,250MHz, GMRT 610MHz, and VLA 5GHz data in the ELAIS-N1 field, we study the radio spectral properties of radio-detecte…

astro-ph.GA2022★ 34 cited

MIGHTEE: Deep 1.4 GHz Source Counts and the Sky Temperature Contribution of Star Forming Galaxies and Active Galactic Nuclei

C. L. Hale, I. H. Whittam, M. J. Jarvis +22

We present deep 1.4 GHz source counts from 5 deg of the continuum Early Science data release of the MeerKAT International Gigahertz Tiered Extragalactic Exploration (MIGH…

astro-ph.GA2022★ 19 cited

MIGHTEE-HI: The HI mass-stellar mass relation over the last billion years

Hengxing Pan, Matt J. Jarvis, Mario G. Santos +19

We study the relation over the last billion years using the MIGHTEE-HI sample. We first model the upper envelope of the relation with…

astro-ph.GA2022★ 9 cited

Collimation of the kiloparsec-scale radio jets in NGC 2663

Velibor Velović, M. D. Filipović, L. Barnes +25

We present the discovery of highly-collimated radio jets spanning a total of 355 kpc around the nearby elliptical galaxy NGC 2663, and the possible first detection of recollimation…

astro-ph.GA2022★ 33 cited

MIGHTEE-HI: Evolution of HI scaling relations of star-forming galaxies at

Francesco Sinigaglia, Giulia Rodighiero, Ed Elson +33

We present the first measurements of HI galaxy scaling relations from a blind survey at . We perform spectral stacking of 9023 spectra of star-forming galaxies undetected i…

astro-ph.GA2022★ 38 cited

Radio fossils, relics, and haloes in Abell 3266: cluster archaeology with ASKAP-EMU and the ATCA

C. J. Riseley, E. Bonnassieux, T. Vernstrom +21

Abell 3266 is a massive and complex merging galaxy cluster that exhibits significant substructure. We present new, highly sensitive radio continuum observations of Abell 3266 perfo…

astro-ph.GA2022★ 52 cited

MIGHTEE: the nature of the radio-loud AGN population

I. H. Whittam, M. J. Jarvis, C. L. Hale +24

We study the nature of the faint radio source population detected in the MeerKAT International GHz Tiered Extragalactic Exploration (MIGHTEE) Early Science data in the COSMOS field…

astro-ph.GA2022★ 12 cited

LADUMA: Discovery of a luminous OH megamaser at

Marcin Glowacki, Jordan D. Collier, Amir Kazemi-Moridani +65

In the local Universe, OH megamasers (OHMs) are detected almost exclusively in infrared-luminous galaxies, with a prevalence that increases with IR luminosity, suggesting that they…

astro-ph.GA2022★ 50 cited

MeerKAT uncovers the physics of an Odd Radio Circle

Ray P. Norris, J. D. Collier, Roland M. Crocker +14

Odd Radio Circles (ORCs) are recently-discovered faint diffuse circles of radio emission, of unknown cause, surrounding galaxies at moderate redshift ($z ~ 0.2-0.6). Here we presen…

astro-ph.GA2022★ 24 cited

MIGHTEE-HI: the HI Size-Mass relation over the last billion years

Sambatriniaina H. A. Rajohnson, Bradley S. Frank, Anastasia A. Ponomareva +15

We present the observed HI size-mass relation of galaxies from the MIGHTEE Survey Early Science data. The high sensitivity of MeerKAT allows us to detect galaxies spanning mo…

astro-ph.GA2021

High-resolution observations of low-luminosity peaked spectrum sources

Jordan D Collier

Although radio observations have been historically seen as less valuable than optical observations, today's broadband radio spectra of peaked spectrum sources reveal detailed physi…

astro-ph.GA2021

MIGHTEE: total intensity radio continuum imaging and the COSMOS / XMM-LSS Early Science fields

I. Heywood, M. J. Jarvis, C. L. Hale +23

MIGHTEE is a galaxy evolution survey using simultaneous radio continuum, spectro-polarimetry, and spectral line observations from the South African MeerKAT telescope. When complete…

astro-ph.GA2021★ 50 cited

MIGHTEE-HI: The baryonic Tully-Fisher relation over the last billion years

Anastasia A. Ponomareva, Wanga Mulaudzi, Natasha Maddox +17

Using a sample of 67 galaxies from the MIGHTEE Survey Early Science data we study the HI-based baryonic Tully-Fisher relation (bTFr), covering a period of one billion years (…

astro-ph.GA2021★ 44 cited

Radio spectral properties of star-forming galaxies in the MIGHTEE-COSMOS field and their impact on the far-infrared-radio correlation

Fangxia An, M. Vaccari, Ian Smail +17

We study the radio spectral properties of 2,094 star-forming galaxies (SFGs) by combining our early science data from the MeerKAT International GHz Tiered Extragalactic Exploration…

astro-ph.GA2021★ 8 cited

Radio Continuum Sources behind the Large Magellanic Cloud

M. D. Filipović, I. S. Bojičić, K. R. Grieve +38

We present a comprehensive multi-frequency catalogue of radio sources behind the Large Magellanic Cloud between 0.2 and 20 GHz, gathered from a combination of new and legacy radio…

astro-ph.GA2021★ 8 cited

MIGHTEE-HI: Discovery of an HI-rich galaxy group at z = 0.044 with MeerKAT

Shilpa Ranchod, Roger P. Deane, Anastasia A. Ponomareva +13

We present the serendipitous discovery of a galaxy group in the XMM-LSS field with MIGHTEE Early Science observations. Twenty galaxies are detected in HI in this group…

astro-ph.GA2021★ 32 cited

The ASKAP-EMU Early Science Project: 888 MHz Radio Continuum Survey of the Large Magellanic Cloud

Clara M. Pennock, Jacco Th. van Loon, Miroslav D. Filipovic +28

We present an analysis of a new 120 deg radio continuum image of the Large Magellanic Cloud (LMC) at 888 MHz with a bandwidth of 288 MHz and beam size of $13\rlap{.}^{\prime\…

astro-ph.GA2021★ 31 cited

Remnant Radio Galaxies Discovered in a Multi-frequency Survey

B. Quici, N. Hurley-Walker, N. Seymour +20

The remnant phase of a radio galaxy begins when the jets launched from an active galactic nucleus are switched off. To study the fraction of radio galaxies in a remnant phase, we t…

astro-ph.GA2021★ 14 cited

Evolutionary Map of the Universe (EMU):Compact radio sources in the SCORPIO field towards the Galactic plane

S. Riggi, G. Umana, C. Trigilio +26

We present observations of a region of the Galactic plane taken during the Early Science Program of the Australian Square Kilometre Array Pathfinder (ASKAP). In this context, we ob…

astro-ph.GA2020★ 45 cited

MIGHTEE: Are giant radio galaxies more common than we thought?

J. Delhaize, I. Heywood, M. Prescott +31

We report the discovery of two new giant radio galaxies (GRGs) using the MeerKAT International GHz Tiered Extragalactic Exploration (MIGHTEE) survey. Both GRGs were found within a…

astro-ph.GA2020★ 96 cited

MIGHTEE-HI: The HI emission project of the MeerKAT MIGHTEE survey

Natasha Maddox, Bradley S. Frank, A. A. Ponomareva +19

We present the HI emission project within the MIGHTEE survey, currently being carried out with the newly commissioned MeerKAT radio telescope. This is one of the first deep, blind,…

astro-ph.GA2020★ 130 cited

The infrared-radio correlation of star-forming galaxies is strongly M-dependent but nearly redshift-invariant since z4

I. Delvecchio, E. Daddi, M. T. Sargent +25

Several works in the past decade have used the ratio between total (rest 8-1000m) infrared and radio (rest 1.4~GHz) luminosity in star-forming galaxies (q), often referre…