output
20082025
most citedWSClean: an implementation of a fast, generic wide-field imager for radio astronomy

937 citations

Showing 2017Show all

40 papers · 1 filter

astro-ph.IM2017★ 240 cited

Faceting for direction-dependent spectral deconvolution

C. Tasse, B. Hugo, M. Mirmont +7

The new generation of radio interferometers is characterized by high sensitivity, wide fields of view and large fractional bandwidth. To synthesize the deepest images enabled by th…

astro-ph.GA2017★ 71 cited

Painting galaxies into dark matter halos using machine learning

Shankar Agarwal, Romeel Davé, Bruce A. Bassett

We develop a machine learning (ML) framework to populate large dark matter-only simulations with baryonic galaxies. Our ML framework takes input halo properties including halo mass…

astro-ph.GA2017★ 28 cited

The jet/wind outflow in Centaurus A: a local laboratory for AGN feedback

B. McKinley, S. J. Tingay, E. Carretti +20

We present new radio and optical images of the nearest radio galaxy Centaurus A and its host galaxy NGC 5128. We focus our investigation on the northern transition region, where en…

astro-ph.CO2017★ 122 cited

Statistical 21-cm Signal Separation via Gaussian Process Regression Analysis

F. G. Mertens, A. Ghosh, L. V. E. Koopmans

Detecting and characterizing the Epoch of Reionization and Cosmic Dawn via the redshifted 21-cm hyperfine line of neutral hydrogen will revolutionize the study of the formation of…

astro-ph.IM2017★ 58 cited

Detection of Bars in Galaxies using a Deep Convolutional Neural Network

Sheelu Abraham, Arun Aniyan, Ajit K. Kembhavi +2

We present an automated method for the detection of bar structure in optical images of galaxies using a deep convolutional neural network which is easy to use and provides good acc…

astro-ph.CO2017★ 31 cited

Model-independent curvature determination with 21cm intensity mapping experiments

Amadeus Witzemann, Philip Bull, Chris Clarkson +3

Recent precision cosmological parameter constraints imply that the spatial curvature of the Universe is essentially dynamically negligible - but only if relatively strong assumptio…