86 citations · 225 across the 14 of their papers we have counts for
14 papers
Euclid preparation. The shape of halo profiles in CDM and non-standard cosmologies
Euclid Collaboration, L. Pizzuti, G. Y. Ferron +304
We study the shape of three-dimensional and projected dark-matter halo profiles extracted from cosmological -body simulations in CDM and non-standard cosmologies, using the \…
cloelike: A Python Library for Cosmological Likelihood Inference in the Euclid Era
Marco Bonici, Guadalupe Cañas-Herrera, Pedro Carrilho +16
cloelike is a Python package providing modular, composable Gaussian likelihood classes for the main cosmological large-scale structure observables targeted by the ESA Euclid space…
cloelib: A Flexible Python Library for Computing Cosmological Observables in the Euclid Era
Marco Bonici, Guadalupe Cañas-Herrera, Pedro Carrilho +54
cloelib is a Python library developed to compute cosmological observables within the Cosmology Likelihood for Observables in Euclid (CLOE) ecosystem (cloe-org). As cosmology enters…
Euclid preparation: Testing multi-field inflation with galaxy power spectrum and bispectrum
Euclid Collaboration, D. Linde, A. Moradinezhad Dizgah +281
Primordial non-Gaussianity (PNG) is a powerful probe of the origin of cosmic structure. Stage-IV surveys like \Euclid will measure galaxy - and -point clustering at high sign…
Euclid preparation. XCV. Cosmology Likelihood for Observables in Euclid (CLOE). 2. Code implementation
Euclid Collaboration, S. Joudaki, V. Pettorino +345
We provide a description of the code implementation and structure of Cosmology Likelihood for Observables in Euclid (CLOE), developed by members of the Euclid Consortium. CLOE is a…
The simple way to measure evolving dark energy without prior-volume effects
Maria Tsedrik, Pedro Carrilho, Chiara Moretti
We present a simple yet effective method to resolve prior-volume effects, also known as projection effects, in full-shape analyses of the power spectrum multipoles within the Effec…
An implementation of nDGP gravity in Pinocchio
Yanling Song, Bin Hu, Chengzong Ruan +2
In this paper we investigate dark matter structure formation in the normal branch of the Dvali-Gabadadze-Porrati (nDGP) model using the PINOCCHIO algorithm. We first present 2nd or…
Probing solutions to the tension with galaxy clustering
Pedro Carrilho, Chiara Moretti, Maria Tsedrik
The current discrepancy between the CMB and weak lensing measurements of the amplitude of matter fluctuations, the so-called tension, has attracted a great deal of recent att…
Modified gravity and massive neutrinos: constraints from the full shape analysis of BOSS galaxies and forecasts for Stage IV surveys
Chiara Moretti, Maria Tsedrik, Pedro Carrilho +1
We constrain the growth index by performing a full-shape analysis of the power spectrum multipoles measured from the BOSS DR12 data. We adopt a theoretical model based on the E…
Euclid: Modelling massive neutrinos in cosmology -- a code comparison
J. Adamek, R. E. Angulo, C. Arnold +133
The measurement of the absolute neutrino mass scale from cosmological large-scale clustering data is one of the key science goals of the Euclid mission. Such a measurement relies o…
Cosmology with the EFTofLSS and BOSS: dark energy constraints and a note on priors
Pedro Carrilho, Chiara Moretti, Alkistis Pourtsidou
We analyse the BOSS DR12 galaxy power spectrum data jointly with BAO data for three models of dark energy. We use recent measurements using a windowless estimator, and an independe…
Interacting dark energy from the joint analysis of the power spectrum and bispectrum multipoles with the EFTofLSS
Maria Tsedrik, Chiara Moretti, Pedro Carrilho +2
Interacting dark energy models have been suggested as alternatives to the standard cosmological model, CDM. We focus on a phenomenologically interesting class of dark scattering…
The Halo Bispectrum Multipoles in Redshift Space
Federico Rizzo, Chiara Moretti, Kevin Pardede +5
We present the analysis of the halo bispectrum in redshift-space in terms of its multipoles, monopole, quadrupole and hexadecapole, measured from a large set of simulations. We fit…
Fast numerical method to generate halo catalogs in modified gravity (part I): second-order Lagrangian Perturbation Theory
Chiara Moretti, Simone Mozzon, Pierluigi Monaco +2
We present and test a new numerical method to determine second-order Lagrangian displacement fields in the context of modified gravity (MG) theories. We start from the extension of…