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Semantic Scholar Open Access 2024 2 sitasi

Euclid: Improving the efficiency of weak lensing shear bias calibration. Pixel noise cancellation and the response method on trial

H. Jansen M. Tewes T. Schrabback N. Aghanim A. Amara +424 lainnya
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Abstrak

To obtain an accurate cosmological inference from upcoming weak lensing surveys such as the one conducted by the shear measurement requires calibration using galaxy image simulations. As it typically requires millions of simulated galaxy images and consequently a substantial computational effort, seeking methods to speed the calibration up is valuable. We study the efficiency of different noise cancellation methods that aim at reducing the simulation volume required to reach a given precision in the shear measurement. The more efficient a method is, the faster we can estimate the relevant biases up to a required precision level. Explicitly, we compared fit methods with different noise cancellations and a method based on responses. We used to simulate galaxies both on a grid and at random positions in larger scenes. Placing the galaxies at random positions requires their detection, which we performed with On the grid, we neglected the detection step and, therefore, the potential detection bias arising from it. The shear of the simulated images was measured with the fast moment-based method for which we note deviations from purely linear shear measurement biases. For the estimation of uncertainties, we used bootstrapping as an empirical method. We extended the response-based approach to work on a wider range of shears and provide accurate estimates of selection biases. We find that each method we studied on top of shape noise cancellation can further increase the efficiency of calibration simulations. The improvement depends on the considered shear amplitude range and the type of simulations (grid-based or random positions). The response method on a grid for small shears provides the biggest improvement. Here the runtime for the estimation of multiplicative biases can be lowered by a factor of $145$ compared to the benchmark simulations without any cancellation. In the more realistic case of randomly positioned galaxies, we still find an improvement factor of $70$ for small shears using the response method. Alternatively, the runtime can be lowered by a factor of 7 already using pixel noise cancellation on top of shape noise cancellation. Furthermore, we demonstrate that the efficiency of shape noise cancellation can be enhanced in the presence of blending if entire scenes are rotated instead of individual galaxies.

Topik & Kata Kunci

Physics

Penulis (429)

H

H. Jansen

M

M. Tewes

T

T. Schrabback

N

N. Aghanim

A

A. Amara

S

S. Andreon

N

N. Auricchio

M

M. Baldi

E

E. Branchini

M

M. Brescia

J

J. Brinchmann

S

S. Camera

V

V. Capobianco

C

C. Carbone

V

V. Cardone

J

J. Carretero

S

S. Casas

M

M. Castellano

S

S. Cavuoti

A

A. Cimatti

G

G. Congedo

L

L. Conversi

Y

Y. Copin

L

L. Corcione

F

F. Courbin

H

H. Courtois

A

A. Silva

H

H. Degaudenzi

J

J. Dinis

F

F. Dubath

X

X. Dupac

M

M. Farina

S

S. Farrens

S

S. Ferriol

M

M. Frailis

E

E. Franceschi

M

M. Fumana

S

S. Galeotta

B

B. Gillis

C

C. Giocoli

A

A. Grazian

F

F. Grupp

S

S. Haugan

H

H. Hoekstra

W

W. Holmes

F

F. Hormuth

A

A. Hornstrup

P

P. Hudelot

K

K. Jahnke

B

B. Joachimi

S

S. Kermiche

A

A. Kiessling

M

M. Kilbinger

T

T. Kitching

B

B. Kubik

H

H. Kurki-Suonio

S

S. Ligori

P

P. Lilje

V

V. Lindholm

I

I. Lloro

E

E. Maiorano

O

O. Mansutti

O

O. Marggraf

K

K. Markovič

N

N. Martinet

F

F. Marulli

R

R. Massey

E

E. Medinaceli

S

S. Mei

M

M. Melchior

Y

Y. Mellier

M

M. Meneghetti

E

E. Merlin

G

G. Meylan

L

L. Miller

M

Michele Moresco

L

L. Moscardini

E

E. Munari

R

R. Nakajima

S

S. Niemi

C

C. Padilla

S

S. Paltani

F

F. Pasian

K

K. Pedersen

V

V. Pettorino

S

S. Pires

G

G. Polenta

M

M. Poncet

F

F. Raison

A

A. Renzi

J

J. Rhodes

G

G. Riccio

E

E. Romelli

M

M. Roncarelli

E

E. Rossetti

R

R. Saglia

D

D. Sapone

B

B. Sartoris

P

P. Schneider

A

A. Secroun

G

G. Seidel

S

S. Serrano

C

C. Sirignano

G

G. Sirri

J

J. Skottfelt

L

L. Stanco

P

P. Tallada-Cresp'i

I

I. Tereno

R

R. Toledo-Moreo

F

F. Torradeflot

I

I. Tutusaus

E

E. Valentijn

L

L. Valenziano

T

T. Vassallo

A

A. Veropalumbo

Y

Y. Wang

J

J. Weller

G

G. Zamorani

J

J. Zoubian

C

C. Colodro-Conde

V

V. S. U. Bonn

A

Argelander Institut fur Astronomie

7

71 AufdemHugel

5

53121 Bonn

G

Germany

U

U. Innsbruck

I

Institut fur Teilchenphysik

T

Technikerstr. 258

6

6020 Innsbruck

M

M Austria

U

Universit'e Paris-Saclay

C

Cnrs

I

I. D. Spatiale

9

91405

O

Orsay

F

France

I

Institute of Cosmology

G

Gravitation

U

U. Portsmouth

P

PO1 3FX

U

Uk

I

Inaf Brera

2

28 ViaBrera

2

20133 Milano

I

Italy

I

I. Bologna

V

V. G. 933

4

40129 Bologna

D

D. Astronomia

U

U. Bologna

V

V. G. 932

I

I. Bologna

6

62 vialeBertiPichat

4

40129 Bologna

D

D. Fisica

U

U. Genova

3

33 viaDodecaneso

1

16146

G

Genova

I

I. Genova

D

Department of PhysicsE. Pancini

U

U. Federico

6

6. ViaCinthia

8

80126

N

Napoli

I

I. -. Capodimonte

1

16 viaMoiariello

8

80131 Napoli

I

I. D. A. E. C. D. Espacco

U

U. Porto

C

Caup

R

Rua das Estrelas

P

P. Porto

P

Portugal

U

U. Torino

1

1. ViaP.Giuria

1

10125 Torino

I

I. Torino

I

I. Torino

2

20 viaOsservatorio

1

1. P. Torinese

I

Inaf-Iasf Milano

1

12 ViaAlfonsoCorti

2

20133 Milano

I

I. Roma

3

33 viaFrascati

0

00078 Monte Porzio Catone

I

I. Roma

P

P. A. Moro

2

2. -. C. D. D. Fisica

E

Edificio G. Marconi

0

00133 Roma

I

Institut de F'isica d'Altes Energies

T

T. Z. F. O. Science

T

Technology

C

Campus Uab

0

08193 Bellaterra

S

Spain.

P

Port d'Informaci'o Cient'ifica

C

C. Sn

I

I. F. Physics

C

Cosmology

R

Rwth Aachen University

5

52056 Aachen

I

I. Naples

D

D. Bologna

I

Institute for Astronomy

U

U. Edinburgh

R

R. Observatory

B

B. Hill

E

Edinburgh EH9 3HJ

E

European Space AgencyESRIN

1

1. LargoGalileoGalilei

0

00044 Frascati

R

Roma

E

Esacesa

C

Camino Bajo de Castillo

S

Sn

U

Urb. Villafranca del Castillo

2

28692 Villanueva de la Canada

M

Madrid

U

U. Lyon

1

1. UnivClaudeBernardLyon

C

CNRSIN2p3

I

I. Lyon

U

Umr 5822

6

69622 Villeurbanne

I

I. O. Physics

L

Laboratory of Astrophysics

E

E. P. F. Lausanne

O

Observatoire de Sauverny

1

1290 Versoix

S

Switzerland.

1

1. UCBLyon

I

Iuf

4

4. R. E. Fermi

D

Departament de F'isica

F

F. Ciencias

U

Universidade Tecnica de Lisboa

C

C8 Edif'icio

C

C. Grande

P

P. Lisboa

1

1049-001 Lisboa

D

D. O. Astronomy

U

U. Geneva

1

16 ch.d'Ecogia

I

I. D. A. E. P. Spaziali

V

V. Cavaliere

1

100

0

00133 Roma

U

Universit'e de Paris Cit'e

C

Cea

A

Aim

9

91191

G

Gif-sur-Yvette

I

Inaf Trieste

1

11 ViaG.B.Tiepolo

3

34127 Trieste

I

Inaf - Padova

5

5. Viadell'Osservatorio

3

35131 Padova

M

M. F. P. Physics

1

1. Giessenbachstr.

8

85748 Garching

U

University Observatory

F

F. O. Physics

L

Ludwig-Maximilians-Universitat

1

1. Scheinerstr.

8

81679 Munich

I

I. Astrophysics

U

U. Oslo

P

P. O. B. 1. Blindern

0

0315 Oslo

N

Norway.

L

L. Observatory

L

Leiden University

2

2. NielsBohrweg

2

2333 CA Leiden

T

The Netherlands.

J

Jet propulsion Laboratory

C

C. I. O. Technology.

4

4800 Oak Grove Drive

P

Pasadena

C

Ca

9

91109

U

Usa

v

von Hoerner Sulger GmbH

8

8. Schlossplatz

6

68723 Schwetzingen

T

T. Denmark

E

Elektrovej 327

2

2800 Kgs. Lyngby

D

Denmark.

C

Cosmic Dawn Center

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I. Paris

U

Umr 7095

S

Sorbonne Universit'e

9

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7

7. Paris

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M. Astronomie

1

17 Konigstuhl

6

69117 Heidelberg

D

D. Physics

A

Astronomy

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U. London

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Gower Street

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London WC1E 6BT

A

A. Universit'e

C

Cppm

M

Marseille

A

Astrophysique

I

Instrumentation et Mod'elisation Paris-Saclay

9

91191 Gif-sur-Yvette

M

Mullard Space Science Laboratory

H

Holmbury St. Mary

D

Dorking

S

Surrey RH5 6NT

6

64 P.O.Box

0

0. Helsinki

F

Finland.

H

H. I. O. Physics

2

2. GustafHallstrominkatu

U

U. Helsinki

H

Helsinki

N

Nova Optical IR Instrumentation Group at Astron

4

4. OudeHoogeveensedijk

7

7991PD

D

Dwingeloo

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Cnes

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Lam

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V. G. 932

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Institute for Computational Cosmology

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D. University

S

South Road

D

DH1 3LE

A

Astroparticule et Cosmologie

7

7. Paris

U

U. Sciences

A

A. Switzerland

S

School of Electrical Engineering

5

5210 Windisch

9

98 bis boulevard Arago

7

75014

P

Paris

C

C. Saclay

D

Dfrirfu

S

S. d’Astrophysique

B

Bat. 709

O

O. University

K

Keble Road

O

O. 3RH

E

European Space AgencyESTEC

1

1. Keplerlaan

2

2. Noordwijk

U

U. Aarhus

N

Ny Munkegade 120

C

C. DK-8000Aarhus

S

S. Center

I

Italian Space Agency

v

via del Politecnico snc

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00133 Roma

C

C. Toulouse

1

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9

9. 31401ToulouseCedex

D

D. Galilei'

U

U. Padova

8

8. viaMarzolo

3

35131 Padova

I

INFN-Padova

U

Universitatssternwarte Munchen

F

F. Physik

L

Ludwig-Maximilians-Universitat Munchen

1

1. Scheinerstrasse

8

8. Munchen

F

Fcfm

U

U. D. Chile

B

Blanco Encalada 2008

S

Santiago

C

Chile

I

I. D. E. D. Catalunya

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Carrer Gran Capit'a 2-4

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08193 Barcelona

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Carrer de Can Magrans

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Sn

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08193 Barcelona

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Satlantis

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U. Park

S

Sede Bld 48940

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Leioa-Bilbao

C

Centre for Medical Imaging

O

Open University

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W. Hall

M

Milton Keynes

M

MK76AA

C

Centro de Investigaciones Energ'eticas

M

Medioambientales y Tecnol'ogicas

4

40 AvenidaComplutense

2

28014 Madrid

T

Tapada da Ajuda

1

1049-001 Lisboa

U

Universidad Polit'ecnica de Cartagena

D

D. D. E. Y. T. D. Computadoras

1

1. PlazadelHospital

3

30202 Cartagena

I

Institut de Recherche en Astrophysique et Plan'etologie

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U. Toulouse

U

Ups

1

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3

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K

K. Institute

U

U. Groningen

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PO Box 800

9

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I

INFN-Bologna

4

46 ViaIrnerio

4

40129 Bologna

I

Infrared Processing

A

A. Center

C

CA 91125

I

Instituto de Astrof'isica de Canarias

C

C. V. L. sn

3

38204

S

San Crist'obal de La Laguna

T

Tenerife

J

Junia

E

Epa department

4

41 Bd Vauban

5

59000 Lille

Format Sitasi

APA MLA BibTeX
Jansen, H., Tewes, M., Schrabback, T., Aghanim, N., Amara, A., Andreon, S. et al. (2024). Euclid: Improving the efficiency of weak lensing shear bias calibration. Pixel noise cancellation and the response method on trial. https://doi.org/10.1051/0004-6361/202347833

Akses Cepat

Lihat di Sumber doi.org/10.1051/0004-6361/202347833
Informasi Jurnal
Tahun Terbit
2024
Bahasa
en
Total Sitasi
2×
Sumber Database
Semantic Scholar
DOI
10.1051/0004-6361/202347833
Akses
Open Access ✓