activity
19982023
most citedThe broken hierarchy of galaxy formation

2.5k citations · 15.5k across the 168 of their papers we have counts for

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Showing 2017Show all

9 papers · 1 filter

astro-ph.GA2017★ 31 cited

Cosmic CARNage I: on the calibration of galaxy formation models

Alexander Knebe, Frazer R. Pearce, Violeta Gonzalez-Perez +31

We present a comparison of nine galaxy formation models, eight semi-analytical and one halo occupation distribution model, run on the same underlying cold dark matter simulation (c…

astro-ph.GA2017★ 78 cited

MultiDark-Galaxies: data release and first results

Alexander Knebe, Doris Stoppacher, Francisco Prada +18

We present the public release of the MultiDark-Galaxies: three distinct galaxy catalogues derived from one of the Planck cosmology MultiDark simulations (i.e. MDPL2, with a volume…

astro-ph.GA2017★ 44 cited

Predicting Hα emission line galaxy counts for future galaxy redshift surveys

Alexander Merson, Yun Wang, Andrew Benson +4

Knowledge of the number density of H emitting galaxies is vital for assessing the scientific impact of the Euclid and WFIRST missions. In this work we present predictions from a…

astro-ph.IM2017★ 21 cited

DESCQA: An Automated Validation Framework for Synthetic Sky Catalogs

Yao-Yuan Mao, Eve Kovacs, Katrin Heitmann +24

The use of high-quality simulated sky catalogs is essential for the success of cosmological surveys. The catalogs have diverse applications, such as investigating signatures of fun…

astro-ph.GA2017★ 17 cited

Quantifying the Origin and Distribution of Intracluster Light in a Fornax-like Cluster

Kathryn A. Harris, Victor P. Debattista, Fabio Governato +9

Using a cosmological -body simulation, we investigate the origin and distribution of stars in the intracluster light (ICL) of a Fornax-like cluster. In a dark matter only simula…

astro-ph.GA2017★ 19 cited

Constraining the Noise-Free Distribution of Halo Spin Parameters

Andrew J. Benson

Any measurement made using an N-body simulation is subject to noise due to the finite number of particles used to sample the dark matter distribution function, and the lack of stru…