activity
20192026
most citedCOVMOS: a new Monte Carlo approach for galaxy clustering analysis

17 citations · 49 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.CO2026

Euclid preparation. CII. Non-Gaussianity of 2-pt statistics likelihood: Parameter inference with a non-Gaussian likelihood in Fourier and configuration space

Euclid Collaboration, S. Gouyou Beauchamps, J. Bel +277

In this work we account for this skewness in parameter inference by modelling the likelihood through an Edgeworth expansion which involves the complete skewness tensor, composed of…

astro-ph.CO2025★ 1 cited

Euclid preparation: LXXXVII. Non-Gaussianity of 2-point statistics likelihood: Precise analysis of the matter power spectrum distribution

Euclid Collaboration, J. Bel, S. Gouyou Beauchamps +281

We investigate the non-Gaussian features in the distribution of the matter power spectrum multipoles. Using the COVMOS method, we generate 100\,000 mock realisations of dark matter…

astro-ph.CO2023★ 8 cited

Euclid preparation. LII. Forecast impact of super-sample covariance on 3x2pt analysis with Euclid

Euclid Collaboration, D. Sciotti, S. Gouyou Beauchamps +221

Deviations from Gaussianity in the distribution of the fields probed by large-scale structure surveys generate additional terms in the data covariance matrix, increasing the uncert…

astro-ph.CO2023★ 5 cited

Cosmological inference including massive neutrinos from the matter power spectrum: biases induced by uncertainties in the covariance matrix

S. Gouyou Beauchamps, P. Baratta, S. Escoffier +4

Data analysis from upcoming large galaxy redshift surveys, such as Euclid and DESI will significantly improve constraints on cosmological parameters. To optimally extract the infor…

astro-ph.CO2022★ 17 cited

COVMOS: a new Monte Carlo approach for galaxy clustering analysis

Philippe Baratta, Julien Bel, Sylvain Gouyou Beauchamps +1

We validate the COVMOS method introduced in Baratta et al. (2019) allowing for the fast simulation of catalogues of different cosmological field tracers (e.g. dark matter particles…

astro-ph.CO2022★ 7 cited

Efficient computation of the super-sample covariance for stage IV galaxy surveys

Fabien Lacasa, Marie Aubert, Philippe Baratta +6

Super-sample covariance (SSC) is an important effect for cosmological analyses that use the deep structure of the cosmic web; it may, however, be nontrivial to include it practical…

astro-ph.CO2019★ 11 cited

High-precision Monte-Carlo modelling of galaxy distribution

Philippe Baratta, Julien Bel, Stephane Plaszczynski +1

We revisit the case of fast Monte-Carlo simulations of galaxy positions for a non-gaussian field. More precisely we address the question of generating a 3D field with a given one-p…