activity
20182021
most citedCluster counts. II. Tensions, massive neutrinos, and modified gravity

13 citations · 13 across the 1 of their papers we have counts for

collaborators

7 papers

astro-ph.CO2021

An updated dark energy view of inflation

Sveva Castello, Stéphane Ilić, Martin Kunz

The present epoch of accelerated cosmic expansion is supposed to be driven by an unknown constituent called dark energy, which in the standard model takes the form of a cosmologica…

astro-ph.CO2020

Euclid: Forecast constraints on the cosmic distance duality relation with complementary external probes

M. Martinelli, C. J. A. P. Martins, S. Nesseris +82

In metric theories of gravity with photon number conservation, the luminosity and angular diameter distances are related via the Etherington relation, also known as the distance-du…

astro-ph.CO2020

Improvements in cosmological constraints from breaking growth degeneracy

Louis Perenon, Stéphane Ilić, Roy Maartens +1

The key probes of the growth of large-scale structure are its rate and amplitude . Redshift space distortions in the galaxy power spectrum allow us to measure only the com…

astro-ph.CO2020

Euclid: The importance of galaxy clustering and weak lensing cross-correlations within the photometric Euclid survey

I. Tutusaus, M. Martinelli, V. F. Cardone +87

The data from the Euclid mission will enable the measurement of the photometric redshifts, angular positions, and weak lensing shapes for over a billion galaxies. This large datase…

astro-ph.CO201913 cited

Cluster counts. II. Tensions, massive neutrinos, and modified gravity

Stéphane Ilić, Ziad Sakr, Alain Blanchard

The CDM concordance model is very successful at describing our Universe with high accuracy and few parameters. Despite its successes, a few tensions persist; most notably, the b…

astro-ph.CO2018

Cosmological cluster tension

A. Blanchard, Z. Sakr, S. IliĆ

The abundance of clusters is a classical cosmological probe sensitive to both the geometrical aspects and the growth rate of structures. The abundance of clusters of galaxies measu…