activity
20142019
most citedThe Case for Electron Re-Acceleration at Galaxy Cluster Shocks

203 citations · 984 across the 16 of their papers we have counts for

collaborators

16 papers

astro-ph.GA201933 cited

The kiloparsec-scale gas kinematics in two star-forming galaxies at seen with ALMA and VLT-SINFONI

J. Molina, Edo Ibar, I. Smail +5

We present Atacama Large Millimeter/submillimeter Array (ALMA) CO() observations of two main-sequence star-forming galaxies at taken from the High-Z Emission Lin…

astro-ph.GA2019

The energetics of starburst-driven outflows at z=1 from KMOS

Mark Swinbank, Chris Harrison, Alfie Tiley +12

We present an analysis of the gas outflow energetics of 529 main-sequence star-forming galaxies at z~1 using KMOS observations of the broad, underlying H-alpha and forbidden lines…

astro-ph.GA201960 cited

Rejuvenation in quiescent galaxies in LEGA-C

Priscilla Chauke, Arjen van der Wel, Camilla Pacifici +12

We use reconstructed star-formation histories (SFHs) of quiescent galaxies at in the LEGA-C survey to identify secondary star-formation episodes that, after an initial pe…

astro-ph.HE2017203 cited

The Case for Electron Re-Acceleration at Galaxy Cluster Shocks

Reinout J. van Weeren, Felipe Andrade-Santos, William A. Dawson +16

On the largest scales, the Universe consists of voids and filaments making up the cosmic web. Galaxy clusters are located at the knots in this web, at the intersection of filaments…

astro-ph.GA201651 cited

SINFONI-HiZELS: The dynamics, merger rates & metallicity gradients of `typical' star-forming galaxies at = 0.8-2.2

J. Molina, E. Ibar, A. M. Swinbank +5

We present adaptive optics (AO) assisted SINFONI integral field unit (IFU) spectroscopy of eleven H emitting galaxies selected from the High-Z Emission Line Survey (HiZELS). We…

astro-ph.GA201645 cited

A large H survey of star formation in relaxed and merging galaxy cluster environments at

Andra Stroe, David Sobral, Ana Afonso +4

We present the first results from the largest H survey of star formation and AGN activity in galaxy clusters. Using 9 different narrow band filters, we select H emitt…