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Cosmology Likelihood for Observables in \Euclid (CLOE). 1. Theoretical recipe

Euclid Collaboration V. F. Cardone S. Joudaki L. Blot M. Bonici S. Camera +495 lainnya
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As the statistical precision of cosmological measurements increases, the accuracy of the theoretical description of these measurements needs to increase correspondingly in order to infer the underlying cosmology that governs the Universe. To this end, we have created the Cosmology Likelihood for Observables in Euclid (CLOE), which is a novel cosmological parameter inference pipeline developed within the Euclid Consortium to translate measurements and covariances into cosmological parameter constraints. In this first in a series of six papers, we describe the theoretical recipe of this code for the Euclid primary probes. These probes are composed of the photometric 3x2pt observables of cosmic shear, galaxy-galaxy lensing, and galaxy clustering, along with spectroscopic galaxy clustering. We provide this description in both Fourier and configuration space for standard and extended summary statistics, including the wide range of systematic uncertainties that affect them. This includes systematic uncertainties such as intrinsic galaxy alignments, baryonic feedback, photometric and spectroscopic redshift uncertainties, shear calibration uncertainties, sample impurities, photometric and spectroscopic galaxy biases, as well as magnification bias. The theoretical descriptions are further able to accommodate both Gaussian and non-Gaussian likelihoods and extended cosmologies with non-zero curvature, massive neutrinos, evolving dark energy, and simple forms of modified gravity. These theoretical descriptions that underpin CLOE will form a crucial component in revealing the true nature of the Universe with next-generation cosmological surveys such as Euclid.

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Physics

Penulis (500)

E

Euclid Collaboration V. F. Cardone

S

S. Joudaki

L

L. Blot

M

M. Bonici

S

S. Camera

G

G. Cañas-Herrera

P

P. Carrilho

S

S. Casas

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S. Davini

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S. Domizio

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S. Farrens

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S. G. Beauchamps

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S. Ili'c

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F. Keil

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A. Brun

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M. Martinelli

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C. Moretti

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V. Pettorino

A

A. Pezzotta

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Z. Sakr

D

D. Sciotti

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K. Tanidis

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I. Tutusaus

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V. Ajani

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M. Crocce

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C. Giocoli

L

L. Legrand

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M. Lembo

G

G. Lesci

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D. N. Girones

A

A. Nouri-Zonoz

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S. Pamuk

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M. Tsedrik

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C. Carbone

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C. Duncan

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M. Kilbinger

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F. Lacasa

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M. Lattanzi

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D. Sapone

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E. Sellentin

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P. Taylor

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N. Aghanim

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B. Altieri

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Edificio G. Marconi

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00133 Roma

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PO1 3FX

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Japan.

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Observatoire de Paris

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Universit'e Psl

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Sorbonne Universit'e

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Cnrs

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92190 Meudon

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France

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Inaf-Iasf Milano

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European Space AgencyESTEC

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2. Noordwijk

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The Netherlands.

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Institute Lorentz

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Leiden University

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2. NielsBohrweg

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L. Observatory

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55 Einsteinweg

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Institute for Astronomy

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U. Edinburgh

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R. Observatory

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B. Hill

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Cosmology

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Rwth Aachen University

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52056 Aachen

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Germany

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16146

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Genova

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U. Genova

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Cea

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Aim

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91191

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Barcelona

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Campus Uab

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Carrer de Can Magrans

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08193 Barcelona

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IJCLab

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Ups

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Cnes

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31400 Toulouse

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Sissa

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International School for Advanced Studies

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Via Bonomea 265

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Cambridge

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Format Sitasi

APA MLA BibTeX
Cardone, E.C.V.F., Joudaki, S., Blot, L., Bonici, M., Camera, S., Cañas-Herrera, G. et al. (2025). Cosmology Likelihood for Observables in \Euclid (CLOE). 1. Theoretical recipe. https://www.semanticscholar.org/paper/67af3cf747096c1f96999fa9e46630e970d902e2

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