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20072021
most citedEMU: Evolutionary Map of the Universe

430 citations · 1.2k across the 29 of their papers we have counts for

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Showing astro-ph.GAShow all

10 papers · 1 filter

astro-ph.GA2020★ 17 cited

Magnetic fields in elliptical galaxies: an observational probe of the fluctuation dynamo action

Amit Seta, Luiz Felippe S. Rodrigues, Christoph Federrath +1

Fluctuation dynamos are thought to play an essential role in magnetized galaxy evolution, saturating within Gyr and thus potentially acting as seeds for large-scale dyna…

astro-ph.GA2020★ 2 cited

SuperCLASS -- II: Photometric Redshifts and Characteristics of Spatially-Resolved Jy Radio Sources

Sinclaire M. Manning, Caitlin M. Casey, Chao-Ling Hung +12

We present optical and near-infrared imaging covering a 1.53 deg region in the Super-Cluster Assisted Shear Survey (SuperCLASS) field, which aims to make the first robust…

astro-ph.GA2020★ 6 cited

SuperCLASS -- I. The Super CLuster Assisted Shear Survey: Project overview and Data Release 1

Richard A. Battye, Michael L. Brown, Caitlin M. Casey +24

The SuperCLuster Assisted Shear Survey (SuperCLASS) is a legacy programme using the e-MERLIN interferometric array. The aim is to observe the sky at L-band (1.4 GHz) to a r.m.s. of…

astro-ph.GA2017★ 2 cited

AMI-LA Observations of the SuperCLASS Super-cluster

C. J. Riseley, K. J. B. Grainge, Y. C. Perrott +21

We present a deep survey of the SuperCLASS super-cluster - a region of sky known to contain five Abell clusters at redshift - performed using the Arcminute Microkelvin I…

astro-ph.GA2016★ 12 cited

Deep observations of the Super-CLASS super-cluster at 325 MHz with the GMRT: the low-frequency source catalogue

C. J. Riseley, A. M. M. Scaife, C. A. Hales +12

We present the results of 325 MHz GMRT observations of a super-cluster field, known to contain five Abell clusters at redshift . We achieve a nominal sensitivity of $34…

astro-ph.GA2016★ 120 cited

Highest Redshift Image of Neutral Hydrogen in Emission: A CHILES Detection of a Starbursting Galaxy at z=0.376

Ximena Fernández, Hansung B. Gim, J. H. van Gorkom +32

Our current understanding of galaxy evolution still has many uncertainties associated with the details of accretion, processing, and removal of gas across cosmic time. The next gen…