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Euclid preparation. L. Calibration of the halo linear bias in Lambda(u)CDM cosmologies

Euclid Collaboration T. Castro A. Fumagalli R. E. Angulo S. Bocquet S. Borgani +495 lainnya
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The mission, designed to map the geometry of the dark Universe, presents an unprecedented opportunity for advancing our understanding of the cosmos through its photometric galaxy cluster survey. Central to this endeavor is the accurate calibration of the mass- and redshift-dependent halo bias (HB), which is the focus of this paper. Our aim is to enhance the precision of HB predictions, which is crucial for deriving cosmological constraints from the clustering of galaxy clusters. Our study is based on the peak-background split (PBS) model linked to the halo mass function (HMF), and it extends it with a parametric correction to precisely align with results from an extended set of $N$-body simulations carried out with the code. Employing simulations with fixed and paired initial conditions, we meticulously analyzed the matter-halo cross-spectrum and modeled its covariance using a large number of mock catalogs generated with Lagrangian perturbation theory simulations with the code. This ensures a comprehensive understanding of the uncertainties in our HB calibration. Our findings indicate that the calibrated HB model is remarkably resilient against changes in cosmological parameters, including those involving massive neutrinos. The robustness and adaptability of our calibrated HB model provide an important contribution to the cosmological exploitation of the cluster surveys to be provided by the mission. This study highlights the necessity of continuously refining the calibration of cosmological tools such as the HB to match the advancing quality of observational data. As we project the impact of our calibrated model on cosmological constraints, we find that given the sensitivity of the survey, a miscalibration of the HB could introduce biases in cluster cosmology analysis. Our work fills this critical gap, ensuring the HB calibration matches the expected precision of the survey.

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Physics

Penulis (500)

E

Euclid Collaboration T. Castro

A

A. Fumagalli

R

R. E. Angulo

S

S. Bocquet

S

S. Borgani

M

M. Costanzi

J

J. Dakin

K

K. Dolag

P

P. Monaco

A

A. Saro

E

E. Sefusatti

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N. Aghanim

L

L. Amendola

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S. Andreon

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C. Baccigalupi

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M. Baldi

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C. Bodendorf

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D. Bonino

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E. Branchini

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M. Brescia

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A. Caillat

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S. Camera

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V. Capobianco

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C. Carbone

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J. Carretero

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S. Casas

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M. Castellano

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G. Castignani

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S. Cavuoti

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A. Cimatti

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C. Colodro-Conde

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G. Congedo

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C. Conselice

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L. Conversi

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Y. Copin

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A. Costille

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F. Courbin

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H. Courtois

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A. Silva

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H. Degaudenzi

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G. Lucia

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A. Giorgio

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M. Douspis

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X. Dupac

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S. Dusini

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M. Farina

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S. Farrens

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S. Ferriol

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P. Fosalba

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M. Frailis

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E. Franceschi

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M. Fumana

S

S. Galeotta

B

B. Gillis

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C. Giocoli

P

P. G'omez-Alvarez

A

A. Grazian

F

F. Grupp

L

L. Guzzo

S

S. Haugan

W

W. Holmes

F

F. Hormuth

A

A. Hornstrup

S

S. Ili'c

K

K. Jahnke

M

M. Jhabvala

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B. Joachimi

E

E. Keihanen

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S. Kermiche

A

A. Kiessling

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M. Kilbinger

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B. Kubik

M

M. Kunz

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H. Kurki-Suonio

P

P. Lilje

V

V. Lindholm

I

I. Lloro

E

E. Maiorano

O

O. Mansutti

O

O. Marggraf

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K. Markovič

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M. Martinelli

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N. Martinet

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F. Marulli

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R. Massey

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S. Maurogordato

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E. Medinaceli

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M. Melchior

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Y. Mellier

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M. Meneghetti

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E. Merlin

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G. Meylan

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L. Moscardini

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E. Munari

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S. Niemi

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C. Padilla

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S. Paltani

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F. Pasian

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K. Pedersen

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W. Percival

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V. Pettorino

S

S. Pires

G

G. Polenta

M

M. Poncet

L

L. Popa

L

L. Pozzetti

F

F. Raison

A

A. Renzi

G

G. Riccio

E

E. Romelli

M

M. Roncarelli

R

R. Saglia

Z

Z. Sakr

J

J. Salvignol

A

A. S'anchez

D

D. Sapone

B

B. Sartoris

M

M. Schirmer

A

A. Secroun

S

S. Serrano

C

C. Sirignano

G

G. Sirri

L

L. Stanco

J

J. Steinwagner

P

P. Tallada-Cresp'i

A

A. Taylor

I

I. Tereno

R

R. Toledo-Moreo

F

F. Torradeflot

I

I. Tutusaus

L

L. Valenziano

T

T. Vassallo

G

G. Kleijn

Y

Y. Wang

J

J. Weller

A

A. Zacchei

G

G. Zamorani

E

E. Zucca

A

A. Biviano

M

M. Bolzonella

E

E. Bozzo

C

C. Burigana

M

M. Calabrese

D

D. Ferdinando

J

J. Vigo

F

F. Finelli

J

J. Graciá-Carpio

S

S. Matthew

N

N. Mauri

A

A. Pezzotta

M

M. Pontinen

C

C. Porciani

V

V. Scottez

M

M. Tenti

M

M. Viel

M

M. Wiesmann

Y

Y. Akrami

V

V. Allevato

S

S. Anselmi

M

M. Archidiacono

F

F. Atrio-Barandela

A

A. Balaguera-Antolínez

M

M. Ballardini

D

D. Bertacca

M

M. Béthermin

A

A. Blanchard

L

L. Blot

H

H. Bohringer

S

S. Bruton

R

R. Cabanac

A

A. Calabró

G

G. Cañas-Herrera

A

A. Cappi

F

F. Caro

C

C. Carvalho

K

K. Chambers

A

A. Cooray

B

B. Caro

S

S. D. Torre

G

G. Desprez

A

A. D'iaz-S'anchez

J

J. Diaz

S

S. Domizio

H

H. Dole

S

S. Escoffier

A

A. Ferrari

P

P. G. Ferreira

I

I. Ferrero

A

A. Finoguenov

A

A. Fontana

F

F. Fornari

L

L. Gabarra

K

K. Ganga

J

J. Garc'ia-Bellido

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T. Gasparetto

V

V. Gautard

E

E. Gaztañaga

F

F. Giacomini

F

F. Gianotti

G

G. Gozaliasl

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A

A. Hall

H

H. Hildebrandt

J

J. Hjorth

A

A. Muñoz

J

J. Kajava

V

Vanshika Kansal

D

D. Karagiannis

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C. Kirkpatrick

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A. Brun

J

J. L. Graet

L

L. Legrand

J

J. Lesgourgues

T

T. Liaudat

A

A. Loureiro

G

G. Maggio

M

M. Magliocchetti

F

F. Mannucci

R

R. Maoli

C

C. Martins

L

L. Maurin

R

R. B. Metcalf

M

M. Miluzio

A

A. Montoro

A

A. Mora

C

C. Moretti

G

G. Morgante

S

S. Nadathur

N

N. A. Walton

L

L. Pagano

L

L. Patrizii

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V. Popa

D

D. Potter

I

I. Risso

P

P. Rocci

M

M. Sahl'en

E

E. Sarpa

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A. Schneider

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A

A. Mancini

J

J. Stadel

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K. Tanidis

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C. Tao

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G. Testera

R

R. Teyssier

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S. Toft

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S. Tosi

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A. Troja

M

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C. Valieri

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J. Valiviita

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D. Vergani

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G. Verza

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P. V. I. A. D. Trieste

1

11 ViaG.B.Tiepolo

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34127 Trieste

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Italy

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I. -. C. N. D. R. I. H. P. Computing

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Bologna

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81679 Munich

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Germany

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P. M. Lardizábal

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20018

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Donostia-San Sebasti'an

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Guipuzkoa

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Spain.

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Ikerbasque

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Basque Foundation for Science

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48013

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Bilbao

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Orsay

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U. Heidelberg

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20133 Milano

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V. G. 932

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40129 Bologna

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I. Bologna

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80126

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Campus Uab

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08193 Bellaterra

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52056 Aachen

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D. Bologna

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Instituto de Astrof'isica de Canarias

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38204

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Tenerife

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U. Edinburgh

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B. Hill

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Departament de F'isica

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Portugal

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U. Milano

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U. Oslo

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Format Sitasi

APA MLA BibTeX
Castro, E.C.T., Fumagalli, A., Angulo, R.E., Bocquet, S., Borgani, S., Costanzi, M. et al. (2024). Euclid preparation. L. Calibration of the halo linear bias in Lambda(u)CDM cosmologies. https://doi.org/10.1051/0004-6361/202451230

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Informasi Jurnal
Tahun Terbit
2024
Bahasa
en
Total Sitasi
1×
Sumber Database
Semantic Scholar
DOI
10.1051/0004-6361/202451230
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Open Access ✓