activity
20172026
most citedImprints of relativistic effects on the asymmetry of the halo cross-correlation function: from linear to non-linear scales

60 citations · 219 across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph.CO2026

PySCo-EFT and ECOSMOG-EFT: a tandem of N-body simulation codes for the Effective Field Theory of Dark Energy

Himanish Ganjoo, Yann Rasera, Emilio Bellini +18

Modified gravity theories constitute viable alternatives to the standard cosmological model for explaining the observed late-time accelerated expansion of the Universe. The Effecti…

astro-ph.CO2021★ 8 cited

Cosmological test of local position invariance from the asymmetric galaxy clustering

Shohei Saga, Atsushi Taruya, Michel-Andrès Breton +1

The local position invariance (LPI) is one of the three major pillars of Einstein equivalence principle, ensuring the space-time independence on the outcomes of local experiments.…

astro-ph.CO2021★ 15 cited

The RayGalGroupSims cosmological simulation suite for the study of relativistic effects: an application to lensing-matter clustering statistics

Y. Rasera, M-A. Breton, P-S. Corasaniti +8

General Relativistic effects on the clustering of matter in the universe provide a sensitive probe of cosmology and gravity theories that can be tested with the upcoming generation…

astro-ph.CO2021★ 7 cited

Magrathea-Pathfinder: A 3D adaptive-mesh code for geodesic ray tracing in -body simulations

Michel-Andrès Breton, Vincent Reverdy

We introduce Magrathea-Pathfinder, a relativistic ray-tracing framework that can reconstruct the past light cone of observers in cosmological simulations. The code directly compute…

astro-ph.CO2021★ 5 cited

Impact of lensing magnification on the analysis of galaxy clustering in redshift space

Michel-Andrès Breton, Sylvain de la Torre, Jade Piat

We study the impact of lensing magnification on the observed three-dimensional galaxy clustering in redshift space. We used the RayGal suite of N-body simulations, from which we ex…

astro-ph.CO2021★ 23 cited

Detectability of the gravitational redshift effect from the asymmetric galaxy clustering

Shohei Saga, Atsushi Taruya, Michel-Andrès Breton +1

It has been recently recognized that the observational relativistic effects, mainly arising from the light propagation in an inhomogeneous universe, induce the dipole asymmetry in…

astro-ph.CO2020★ 18 cited

Theoretical and numerical perspectives on cosmic distance averages

Michel-Andrès Breton, Pierre Fleury

The interpretation of cosmological observations relies on a notion of an average Universe, which is usually considered as the homogeneous and isotropic Friedmann-Lemaître-Robertson…

astro-ph.CO2020★ 8 cited

Fast analytical calculation of the random pair counts for realistic survey geometry

Michel-Andrès Breton, Sylvain de la Torre

Galaxy clustering is a standard cosmological probe that is commonly analysed through two-point statistics. In observations, the estimation of the two-point correlation function cru…

astro-ph.CO2020★ 20 cited

Modelling the asymmetry of the halo cross-correlation function with relativistic effects at quasi-linear scales

Shohei Saga, Atsushi Taruya, Michel-Andrès Breton +1

The observed galaxy distribution via galaxy redshift surveys appears distorted due to redshift-space distortions (RSD). While one dominant contribution to RSD comes from the Dopple…

astro-ph.CO2019★ 27 cited

Wide-angle redshift-space distortions at quasi-linear scales: cross-correlation functions from Zel'dovich approximation

Atsushi Taruya, Shohei Saga, Michel-Andrès Breton +2

Redshift-space distortions (RSD) in galaxy redshift surveys generally break both the isotropy and homogeneity of galaxy distribution. While the former aspect is particularly highli…

astro-ph.CO2018★ 60 cited

Imprints of relativistic effects on the asymmetry of the halo cross-correlation function: from linear to non-linear scales

Michel-Andrès Breton, Yann Rasera, Atsushi Taruya +2

The apparent distribution of large-scale structures in the universe is sensitive to the velocity/potential of the sources as well as the potential along the line-of-sight through t…

astro-ph.CO2017★ 28 cited

Probing Cosmology with Dark Matter Halo Sparsity Using X-ray Cluster Mass Measurements

P. S. Corasaniti, S. Ettori, Y. Rasera +5

We present a new cosmological probe for galaxy clusters, the halo sparsity. This characterises halos in terms of the ratio of halo masses measured at two different radii and carrie…