activity
20042019
most citedDancing in the dark: galactic properties trace spin swings along the cosmic web

888 citations · 5.1k across the 30 of their papers we have counts for

collaborators

30 papers

cs.LG2019★ 4 cited

An empirical study of pretrained representations for few-shot classification

Tiago Ramalho, Thierry Sousbie, Stefano Peluchetti

Recent algorithms with state-of-the-art few-shot classification results start their procedure by computing data features output by a large pretrained model. In this paper we system…

astro-ph.CO2017★ 361 cited

Tracing the cosmic web

Noam I Libeskind, Rien van de Weygaert, Marius Cautun +27

The cosmic web is one of the most striking features of the distribution of galaxies and dark matter on the largest scales in the Universe. It is composed of dense regions packed fu…

astro-ph.GA2016★ 140 cited

The VIMOS Public Extragalactic Redshift Survey (VIPERS): Galaxy segregation inside filaments at

N. Malavasi, S. Arnouts, D. Vibert +42

We present the first quantitative detection of large-scale filamentary structure at in the large cosmological volume probed by the VIMOS Public Extragalactic Redshif…

physics.comp-ph2015★ 58 cited

ColDICE: a parallel Vlasov-Poisson solver using moving adaptive simplicial tessellation

Thierry Sousbie, Stéphane Colombi

Resolving numerically Vlasov-Poisson equations for initially cold systems can be reduced to following the evolution of a three-dimensional sheet evolving in six-dimensional phase-s…

astro-ph.CO2015★ 22 cited

Vlasov versus N-body: the Hénon sphere

S. Colombi, T. Sousbie, S. Peirani +2

We perform a detailed comparison of the phase-space density traced by the particle distribution in Gadget simulations to the result obtained with a spherical Vlasov solver using th…

astro-ph.CO2014★ 888 cited

Dancing in the dark: galactic properties trace spin swings along the cosmic web

Yohan Dubois, Christophe Pichon, Charlotte Welker +30

A large-scale hydrodynamical cosmological simulation, Horizon-AGN, is used to investigate the alignment between the spin of galaxies and the cosmic filaments above redshift 1.2. Th…