activity
20232026
most citedEuclid. I. Overview of the Euclid mission

550 citations · 571 across the 11 of their papers we have counts for

collaborators

12 papers

gr-qc2026

Beyond ΛCDM with the SKA Observatory -- I: Probing Gravity on Cosmological Scales

S. Camera, C. Addis, S. L. Guedezounme +26

General relativity (GR) is currently the best description of the gravitational interaction at our disposal and is one of the foundations of the concordance cosmological model. For…

astro-ph.CO2026

Late-time reconstruction of non-minimally coupled gravity with a smoothness prior

Gen Ye, Anton Chudaykin, Camille Bonvin +1

We present a non-parametric, model-independent reconstruction of the cosmological background and perturbation dynamics in non-minimally coupled theories of gravity. Within the Effe…

astro-ph.CO2026

Kinematic cosmic dipole from a large sample of strong lenses

Martin Millon, Charles Dalang, Thomas Collett +1

Measurements of the kinematic cosmic dipole continue to show an intriguing tension between the value inferred from the CMB and that obtained from high-redshift source number counts…

astro-ph.CO2026★ 1 cited

Testing the Equivalence Principle in Galaxy Clusters

Enea Di Dio, Sveva Castello, Camille Bonvin

Clusters of galaxies have been used to measure a subtle effect predicted by Einstein: gravitational redshift. This signal encodes pristine information about our Universe, since it…

astro-ph.CO2025

Euclid preparation. Review of forecast constraints on dark energy and modified gravity

Euclid Collaboration, N. Frusciante, M. Martinelli +326

The Euclid mission has been designed to provide, as one of its main deliverables, information on the nature of the gravitational interaction, which determines the expansion of the…

astro-ph.CO2025

Gravitational redshift from large-scale structure: nonlinearities, antisymmetries, and the dipole

Lawrence Dam, Camille Bonvin

Gravitational redshift imprints a slight asymmetry in the observed clustering of galaxies, producing odd multipoles (e.g. the dipole) in the cross-correlation function. But there a…

astro-ph.CO2025★ 2 cited

Reconstructing the dark energy density in light of DESI BAO observations

Maria Berti, Emilio Bellini, Camille Bonvin +3

In light of the evidence for dynamical dark energy (DE) found from the most recent Dark Energy Spectroscopic Instrument (DESI) baryon acoustic oscillation (BAO) measurements, we pe…

astro-ph.CO2025★ 2 cited

Gravitational Redshift from Galaxy Clusters -- a Relativistic Approach

Enea Di Dio, Sveva Castello, Camille Bonvin

The light that we receive from clusters of galaxies is redshifted by the presence of the clusters' gravitational potential. This effect, known as gravitational redshift, was first…

astro-ph.CO2024★ 10 cited

Testing the equivalence principle across the Universe: a model-independent approach with galaxy multi-tracing

Sveva Castello, Ziyang Zheng, Camille Bonvin +1

We present a test of the equivalence principle on cosmological scales. This cornerstone of general relativity has been tested with high precision for standard matter, but its valid…

astro-ph.CO2024★ 6 cited

Euclid: Relativistic effects in the dipole of the 2-point correlation function

F. Lepori, S. Schulz, I. Tutusaus +130

Gravitational redshift and Doppler effects give rise to an antisymmetric component of the galaxy correlation function when cross-correlating two galaxy populations or two different…

astro-ph.CO2024★ 550 cited

Euclid. I. Overview of the Euclid mission

Euclid Collaboration, Y. Mellier, Abdurro'uf +1134

The current standard model of cosmology successfully describes a variety of measurements, but the nature of its main ingredients, dark matter and dark energy, remains unknown. Eucl…

astro-ph.CO2023

Euclid Preparation. TBD. Impact of magnification on spectroscopic galaxy clustering

Euclid Collaboration, G. Jelic-Cizmek, F. Sorrenti +226

In this paper we investigate the impact of lensing magnification on the analysis of Euclid's spectroscopic survey, using the multipoles of the 2-point correlation function for gala…