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20092021
most citedThe Cluster-EAGLE project: global properties of simulated clusters with resolved galaxies

243 citations · 2.4k across the 46 of their papers we have counts for

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Showing astro-ph.GAShow all

18 papers · 1 filter

astro-ph.GA2020★ 52 cited

The splashback boundary of haloes in hydrodynamic simulations

Stephanie O'Neil, David J. Barnes, Mark Vogelsberger +1

The splashback radius, , is a physically motivated halo boundary that separates infalling and collapsed matter of haloes. We study in the hydrodynamic and…

astro-ph.GA2020★ 40 cited

Is there enough star formation in simulated protoclusters?

Seunghwan Lim, Douglas Scott, Arif Babul +5

As progenitors of the most massive objects, protoclusters are key to tracing the evolution and star-formation history of the Universe, and are responsible for per c…

astro-ph.GA2020★ 91 cited

First Light And Reionisation Epoch Simulations (FLARES) II: The Photometric Properties of High-Redshift Galaxies

Aswin P. Vijayan, Christopher C. Lovell, Stephen M. Wilkins +5

We present the photometric properties of galaxies in the First Light and Reionisation Epoch Simulations (FLARES). The simulations trace the evolution of galaxies in a range of over…

astro-ph.GA2020★ 37 cited

Properties of the ionized CGM and IGM: a comparison of galaxy formation models via the Sunyaev-Zel'dovich effect

S. H. Lim, David Barnes, Mark Vogelsberger +5

We present a comparison of the physical properties of the ionized gas in the circumgalactic (CGM) and intergalactic (IGM) media at between observations and four cosmologic…

astro-ph.GA2020★ 138 cited

First Light And Reionisation Epoch Simulations (FLARES) I: Environmental Dependence of High-Redshift Galaxy Evolution

Christopher C. Lovell, Aswin P. Vijayan, Peter A. Thomas +4

We introduce the First Light And Reionisation Epoch Simulations (FLARES), a suite of zoom simulations using the EAGLE model. We resimulate a range of overdensities during the Epoch…

astro-ph.GA2020★ 71 cited

The intra-cluster light as a tracer of the total matter density distribution: a view from simulations

Isaac Alonso Asensio, Claudio Dalla Vecchia, Yannick M. Bahé +2

By using deep observations of clusters of galaxies, it has been recently found that the projected stellar mass density closely follows the projected total (dark and baryonic) mass…