activity
19972024
most citedCold streams in early massive hot haloes as the main mode of galaxy formation

1.7k citations · 13.5k across the 186 of their papers we have counts for

collaborators
Showing 2008 · astro-phShow all

10 papers · 2 filters

astro-ph2008★ 85 cited

The Local Theory of the Cosmic Skeleton

D. Pogosyan, C. Pichon, C. Gay +4

The local theory of the critical lines of 2D and 3D Gaussian fields that underline the cosmic structures is presented. In the context of cosmological matter distribution the subset…

astro-ph2008★ 23 cited

Phase-space structures I: A comparison of 6D density estimators

M. Maciejewski, S. Colombi, C. Alard +2

This paper reviews and analyses methods used to identify neighbours in 6D space and estimate the corresponding phase-space density. It compares SPH methods to 6D Delaunay tessellat…

astro-ph2008★ 70 cited

The fully connected N-dimensional skeleton: probing the evolution of the cosmic web

T. Sousbie, S. Colombi, C. Pichon

A method to compute the full hierarchy of the critical subsets of a density field is presented. It is based on a watershed technique and uses a probability propagation scheme to im…

astro-ph2008★ 1.7k cited

Cold streams in early massive hot haloes as the main mode of galaxy formation

A. Dekel, Y. Birnboim, G. Engel +7

The massive galaxies in the young universe, ten billion years ago, formed stars at surprising intensities. Although this is commonly attributed to violent mergers, the properties o…

astro-ph2008★ 134 cited

Full-Sky Weak Lensing Simulation with 70 Billion Particles

Romain Teyssier, Sandrine Pires, Simon Prunet +7

We have performed a 70 billion dark-matter particles N-body simulation in a 2 Gpc periodic box, using the concordance, cosmological model as favored by the latest WMAP3 re…

astro-ph2008★ 177 cited

Initial Conditions for Large Cosmological Simulations

S. Prunet, C. Pichon, D. Aubert +3

This technical paper describes a software package that was designed to produce initial conditions for large cosmological simulations in the context of the Horizon collaboration. Th…

astro-ph2008★ 19 cited

Numerical investigation of lenses with substructures using the perturbative method

Sébastien Peirani, Christophe Alard, Christophe Pichon +2

We present a statistical study of the effects induced by substructures on the deflection potential of dark matter halos in the strong lensing regime. This investigation is based on…

astro-ph2008★ 19 cited

On the Onset of Stochasticity in CDM Cosmological Simulations

Jerome Thiebaut, Christophe Pichon, Thierry Sousbie +2

The onset of stochasticity is measured in CDM cosmological simulations using a set of classical observables. It is quantified as the local derivative of the logarithm of the dis…

astro-ph2008★ 343 cited

Bimodal gas accretion in the Horizon-MareNostrum galaxy formation simulation

P. Ocvirk, C. Pichon, R. Teyssier

(abridged) The physics of diffuse gas accretion and the properties of the cold and hot modes of accretion onto proto-galaxies between z=2 and z=5.4 is investigated using the large…

astro-ph2008

Recovering the topology of the IGM at z~2

S. Caucci, S. Colombi, C. Pichon +3

We investigate how well the 3D density field of neutral hydrogen in the Intergalactic Medium (IGM) can be reconstructed using the Lyman-alpha absorptions observed along lines of si…