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20072026
most citedGalaxy formation in the Planck Cosmology - I. Matching the observed evolution of star formation rates, colours and stellar masses

680 citations · 8k across the 134 of their papers we have counts for

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Showing 2013 · astro-ph.COShow all

8 papers · 2 filters

astro-ph.CO2013★ 281 cited

The Mass-Concentration-Redshift Relation of Cold Dark Matter Halos

Aaron D. Ludlow, Julio F. Navarro, Raul E. Angulo +4

We use the Millennium Simulation series to investigate the mass and redshift dependence of the concentration of equilibrium cold dark matter (CDM) halos. We extend earlier work on…

astro-ph.CO2013★ 39 cited

Galaxy formation on the largest scales: The impact of astrophysics on the BAO peak

Raul E. Angulo, Simon D. M. White, Volker Springel +1

We investigate the effects of galaxy formation on the baryonic acoustic oscillations (BAO) peak by applying semi-analytic modelling techniques to the Millennium-XXL, a $3 \times 10…

astro-ph.CO2013★ 22 cited

Extending the halo mass resolution of -body simulations

Raul E. Angulo, Carlton M. Baugh, Carlos S. Frenk +1

We present a scheme to extend the halo mass resolution of N-body simulations of the hierarchical clustering of dark matter. The method uses the density field of the simulation to p…

astro-ph.CO2013★ 18 cited

Noiseless Gravitational Lensing Simulations

Raul E. Angulo, Ruizhu Chen, Stefan Hilbert +1

The microphysical properties of the DM particle can, in principle, be constrained by the properties and abundance of substructures in DM halos, as measured through strong gravitati…

astro-ph.CO2013★ 159 cited

The Warm DM halo mass function below the cut-off scale

Raul E. Angulo, Oliver Hahn, Tom Abel

Warm Dark Matter (WDM) cosmologies are a viable alternative to the Cold Dark Matter (CDM) scenario. Unfortunately, an accurate scrutiny of the WDM predictions with N-body simulatio…

astro-ph.CO2013★ 207 cited

The Mass Profile and Accretion History of Cold Dark Matter Halos

Aaron D. Ludlow, Julio F. Navarro, Michael Boylan-Kolchin +6

We use the Millennium Simulation series to study the relation between the accretion history (MAH) and mass profile of cold dark matter halos. We find that the mean density within t…

astro-ph.CO2013★ 57 cited

How closely do baryons follow dark matter on large scales?

Raul E. Angulo, Oliver Hahn, Tom Abel

We investigate the large-scale clustering and gravitational interaction of baryons and dark matter (DM) over cosmic time using a set of collisionless N-body simulations. Both compo…

astro-ph.CO2013★ 14 cited

Exploring the non-linear density field in the Millennium simulations with tessellations - I. The probability distribution function

Biswajit Pandey, Simon D. M. White, Volker Springel +1

We use the Delaunay Tessellation Field Estimator (DTFE) to study the one-point density distribution functions of the Millennium (MS) and Millennium-II (MS-II) simulations. The DTFE…