680 citations · 8k across the 134 of their papers we have counts for
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Galaxy formation in the Planck cosmology - IV. Mass and environmental quenching, conformity and clustering
Bruno M. B. Henriques, Simon D. M. White, Peter A. Thomas +4
We study the quenching of star formation as a function of redshift, environment and stellar mass in the galaxy formation simulations of Henriques et al. (2015), which implement an…
Einasto Profiles and the Dark Matter Power Spectrum
Aaron D. Ludlow, Raul E. Angulo
We study the mass accretion histories (MAHs) and density profiles of dark matter halos using N-body simulations of self-similar gravitational clustering from scale-free power spect…
The effect of photometric redshift uncertainties on galaxy clustering and baryonic acoustic oscillations
Jonás Chaves-Montero, Raúl E. Angulo, Carlos Hernández-Monteagudo
In the upcoming era of high-precision galaxy surveys, it becomes necessary to understand the impact of redshift uncertainties on cosmological observables. In this paper we explore…
Very Massive Tracers and Higher Derivative Biases
Tomohiro Fujita, Valentin Mauerhofer, Leonardo Senatore +2
Most of the upcoming cosmological information will come from analyzing the clustering of the Large Scale Structures (LSS) of the universe through LSS or CMB observations. It is the…
Precise Clustering and Density Evolution of redMaPPer Galaxy Clusters versus MXXL Simulation
Pablo Jimeno, Tom Broadhurst, Ruth Lazkoz +4
We construct a large, redshift complete sample of distant galaxy clusters by correlating Sloan Digital Sky Survey (SDSS) Data Release 12 (DR12) redshifts with clusters identified w…
The Clustering of Galaxies in the Completed SDSS-III Baryon Oscillation Spectroscopic Survey: Cosmic Flows and Cosmic Web from Luminous Red Galaxies
Metin Ata, Francisco-Shu Kitaura, Chia-Hsun Chuang +31
We present a Bayesian phase-space reconstruction of the cosmic large-scale matter density and velocity fields from the SDSS-III Baryon Oscillations Spectroscopic Survey Data Releas…
Earth-mass haloes and the emergence of NFW density profiles
Raul E. Angulo, Oliver Hahn, Aaron Ludlow +1
We simulate neutralino dark matter (DM) haloes from their initial collapse, at earth mass, up to a few percent solar. Our results confirm that the density profiles of the…
Characterising Strong Lensing Galaxy Clusters using the Millennium-XXL and MOKA simulations
Carlo Giocoli, Mario Bonamigo, Marceau Limousin +5
In this paper we investigate the strong lensing statistics in galaxy clusters. We extract dark matter haloes from the Millennium-XXL simulation, compute their Einstein radius distr…
Cosmological -body simulations with suppressed variance
Raul E. Angulo, Andrew Pontzen
We present and test a method that dramatically reduces variance arising from the sparse sampling of wavemodes in cosmological simulations. The method uses two simulations which are…
The Mass-Concentration-Redshift Relation of Cold and Warm Dark Matter Halos
Aaron D. Ludlow, Sownak Bose, Raúl E. Angulo +5
We use a suite of cosmological simulations to study the mass-concentration-redshift relation, , of dark matter halos. Our simulations include standard -cold dark m…