J. Bel

First results from the IllustrisTNG simulations: matter and galaxy clustering

Large-scale galaxy bias

Non-local bias contribution to third-order galaxy correlations

Comparing halo bias from abundance and clustering

Linear and non-linear bias: predictions versus measurements

Measuring the growth of matter fluctuations with third-order galaxy correlations

Second-order matter fluctuations via higher order galaxy correlators

DEMNUni: the clustering of large-scale structures in the presence of massive neutrinos