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20152026
most citedEuclid. III. The NISP Instrument

114 citations · 1.9k across the 269 of their papers we have counts for

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Showing 2021Show all

13 papers · 1 filter

astro-ph.CO2021★ 34 cited

Cosmological Constraints on sub-horizon scales modified gravity theories with MGCLASS II

Ziad Sakr, Matteo Martinelli

In this paper we introduce a new public Einstein-Boltzmann solver, \texttt{MGCLASS II}, built as a modification to the publicly available \texttt{CLASS} code, that allows to obtain…

astro-ph.CO2021★ 29 cited

Can varying the gravitational constant alleviate the tensions ?

Ziad Sakr, Domenico Sapone

Constraints on the cosmological concordance model parameters from observables at different redshifts are usually obtained using the locally measured value of the gravitational cons…

astro-ph.CO2021★ 15 cited

Cluster counts III. CDM extensions and the cluster tension

Ziad Sakr, Stephane Ilic, Alain Blanchard

In this work, we examine whether further extensions to the CDM model could alleviate the tension. For that, we derive constraints on the parameters subject of the discrepa…

astro-ph.CO2021★ 29 cited

Euclid: Forecast constraints on consistency tests of the CDM model

S. Nesseris, D. Sapone, M. Martinelli +112

The standard cosmological model is based on the fundamental assumptions of a spatially homogeneous and isotropic universe on large scales. An observational detection of a violation…

astro-ph.CO2021★ 56 cited

Euclid preparation: XIX. Impact of magnification on photometric galaxy clustering

F. Lepori, I. Tutusaus, C. Viglione +183

We investigate the importance of lensing magnification for estimates of galaxy clustering and its cross-correlation with shear for the photometric sample of Euclid. Using updated s…

astro-ph.CO2021★ 17 cited

Impact of survey geometry and super-sample covariance on future photometric galaxy surveys

S. Gouyou Beauchamps, F. Lacasa, I. Tutusaus +4

Photometric galaxy surveys probe the late-time Universe where the density field is highly non-Gaussian. A consequence is the emergence of the super-sample covariance (SSC), a non-G…

astro-ph.CO2021★ 68 cited

Euclid: Forecasts from redshift-space distortions and the Alcock-Paczynski test with cosmic voids

N. Hamaus, M. Aubert, A. Pisani +127

Euclid is poised to survey galaxies across a cosmological volume of unprecedented size, providing observations of more than a billion objects distributed over a third of the full s…

astro-ph.CO2021★ 33 cited

The Copernican principle in light of the latest cosmological data

David Camarena, Valerio Marra, Ziad Sakr +1

We pursue a program to confront observations with inhomogeneous extensions of the FLRW metric. The main idea is to test the Copernican principle rather than assuming it a priori. W…

astro-ph.CO2021★ 78 cited

preparation: XV. Forecasting cosmological constraints for the and CMB joint analysis

Euclid Collaboration, S. Ilić, N. Aghanim +207

The combination and cross-correlation of the upcoming data with cosmic microwave background (CMB) measurements is a source of great expectation since it will provide the l…

astro-ph.CO2021★ 30 cited

Euclid: constraining dark energy coupled to electromagnetism using astrophysical and laboratory data

M. Martinelli, C. J. A. P. Martins, S. Nesseris +92

In physically realistic scalar-field based dynamical dark energy models (including, e.g., quintessence) one naturally expects the scalar field to couple to the rest of the model's…

astro-ph.CO2021★ 26 cited

Euclid preparation: XII. Optimizing the photometric sample of the Euclid survey for galaxy clustering and galaxy-galaxy lensing analyses

Euclid Collaboration, A. Pocino, I. Tutusaus +157

The accuracy of photometric redshifts (photo-zs) particularly affects the results of the analyses of galaxy clustering with photometrically-selected galaxies (GCph) and weak lensin…

astro-ph.CO2021★ 7 cited

Gravitation And the Universe from large Scale-Structures: The GAUSS mission concept

Alain Blanchard, Aubourg Éric, Philippe Brax +25

Today, thanks in particular to the results of the ESA Planck mission, the concordance cosmological model appears to be the most robust to describe the evolution and content of the…

astro-ph.CO2021

Euclid preparation: XI. Mean redshift determination from galaxy redshift probabilities for cosmic shear tomography

Euclid Collaboration, O. Ilbert, S. de la Torre +162

The analysis of weak gravitational lensing in wide-field imaging surveys is considered to be a major cosmological probe of dark energy. Our capacity to constrain the dark energy eq…