Dark Energy Survey Year 3 results: cosmology with moments of weak lensing mass maps – validation on simulations

ABSTRACT We present a simulated cosmology analysis using the second and third moments of the weak lensing mass (convergence) maps. The second moment, or variances, of the convergence as a function of smoothing scale contains information similar to standard shear two-point statistics. The third momen...

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Published inMonthly notices of the Royal Astronomical Society Vol. 498; no. 3; pp. 4060 - 4087
Main Authors Gatti, M, Chang, C, Friedrich, O, Jain, B, Bacon, D, Crocce, M, DeRose, J, Ferrero, I, Fosalba, P, Gaztanaga, E, Gruen, D, Harrison, I, Jeffrey, N, MacCrann, N, McClintock, T, Secco, L, Whiteway, L, Abbott, T M C, Allam, S, Annis, J, Avila, S, Brooks, D, Buckley-Geer, E, Burke, D L, Carnero Rosell, A, Carrasco Kind, M, Carretero, J, Cawthon, R, da Costa, L N, De Vicente, J, Desai, S, Diehl, H T, Doel, P, Eifler, T F, Estrada, J, Everett, S, Evrard, A E, Frieman, J, García-Bellido, J, Gerdes, D W, Gruendl, R A, Gschwend, J, Gutierrez, G, James, D J, Johnson, M D, Krause, E, Kuehn, K, Lima, M, Maia, M A G, March, M, Marshall, J L, Melchior, P, Menanteau, F, Miquel, R, Palmese, A, Paz-Chinchón, F, Plazas, A A, Sánchez, C, Sanchez, E, Scarpine, V, Schubnell, M, Santiago, S, Sevilla-Noarbe, I, Smith, M, Soares-Santos, M, Suchyta, E, Swanson, M E C, Tarle, G, Thomas, D, Troxel, M A, Zuntz, J
Format Journal Article
LanguageEnglish
Norwegian
Published United Kingdom Oxford University Press 01.11.2020
Royal Astronomical Society
Subjects
ASTRONOMY AND ASTROPHYSICS
cosmology: observations
gravitational lensing: weak
large-scale structure of Universe
gravitational lensing: weak
cosmology: observations
large-scale structure of Universe
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Abstract ABSTRACT We present a simulated cosmology analysis using the second and third moments of the weak lensing mass (convergence) maps. The second moment, or variances, of the convergence as a function of smoothing scale contains information similar to standard shear two-point statistics. The third moment, or the skewness, contains additional non-Gaussian information. The analysis is geared towards the third year (Y3) data from the Dark Energy Survey (DES), but the methodology can be applied to other weak lensing data sets. We present the formalism for obtaining the convergence maps from the measured shear and for obtaining the second and third moments of these maps given partial sky coverage. We estimate the covariance matrix from a large suite of numerical simulations. We test our pipeline through a simulated likelihood analyses varying 5 cosmological parameters and 10 nuisance parameters and identify the scales where systematic or modelling uncertainties are not expected to affect the cosmological analysis. Our simulated likelihood analysis shows that the combination of second and third moments provides a 1.5 per cent constraint on S8 ≡ σ8(Ωm/0.3)0.5 for DES Year 3 data. This is 20 per cent better than an analysis using a simulated DES Y3 shear two-point statistics, owing to the non-Gaussian information captured by the inclusion of higher order statistics. This paper validates our methodology for constraining cosmology with DES Year 3 data, which will be presented in a subsequent paper.
AbstractList ABSTRACT We present a simulated cosmology analysis using the second and third moments of the weak lensing mass (convergence) maps. The second moment, or variances, of the convergence as a function of smoothing scale contains information similar to standard shear two-point statistics. The third moment, or the skewness, contains additional non-Gaussian information. The analysis is geared towards the third year (Y3) data from the Dark Energy Survey (DES), but the methodology can be applied to other weak lensing data sets. We present the formalism for obtaining the convergence maps from the measured shear and for obtaining the second and third moments of these maps given partial sky coverage. We estimate the covariance matrix from a large suite of numerical simulations. We test our pipeline through a simulated likelihood analyses varying 5 cosmological parameters and 10 nuisance parameters and identify the scales where systematic or modelling uncertainties are not expected to affect the cosmological analysis. Our simulated likelihood analysis shows that the combination of second and third moments provides a 1.5 per cent constraint on S8 ≡ σ8(Ωm/0.3)0.5 for DES Year 3 data. This is 20 per cent better than an analysis using a simulated DES Y3 shear two-point statistics, owing to the non-Gaussian information captured by the inclusion of higher order statistics. This paper validates our methodology for constraining cosmology with DES Year 3 data, which will be presented in a subsequent paper.
We present a simulated cosmology analysis using the second and third moments of the weak lensing mass (convergence) maps. The second moment, or variances, of the convergence as a function of smoothing scale contains information similar to standard shear two-point statistics. The third moment, or the skewness, contains additional non-Gaussian information. The analysis is geared towards the third year (Y3) data from the Dark Energy Survey (DES), but the methodology can be applied to other weak lensing data sets. We present the formalism for obtaining the convergence maps from the measured shear and for obtaining the second and third moments of these maps given partial sky coverage. We estimate the covariance matrix from a large suite of numerical simulations. We test our pipeline through a simulated likelihood analyses varying 5 cosmological parameters and 10 nuisance parameters and identify the scales where systematic or modelling uncertainties are not expected to affect the cosmological analysis. Our simulated likelihood analysis shows that the combination of second and third moments provides a 1.5 percent constraint on S8 ≡ σ8(Ωm/0.3)0.5 for DES Year 3 data. This is 20 percent better than an analysis using a simulated DES Y3 shear two-point statistics, owing to the non-Gaussian information captured by the inclusion of higher order statistics. This paper validates our methodology for constraining cosmology with DES Year 3 data, which will be presented in a subsequent paper.
Author Annis, J
Gruendl, R A
Avila, S
Marshall, J L
MacCrann, N
Estrada, J
Fosalba, P
Sánchez, C
Frieman, J
Palmese, A
Gerdes, D W
García-Bellido, J
Miquel, R
Harrison, I
Melchior, P
Carnero Rosell, A
Santiago, S
Troxel, M A
Schubnell, M
Gaztanaga, E
Diehl, H T
Krause, E
Tarle, G
Jain, B
Gruen, D
McClintock, T
Kuehn, K
Bacon, D
Burke, D L
Buckley-Geer, E
Menanteau, F
Suchyta, E
Sanchez, E
Carretero, J
Soares-Santos, M
Gschwend, J
Secco, L
Paz-Chinchón, F
da Costa, L N
Cawthon, R
Chang, C
James, D J
Carrasco Kind, M
Swanson, M E C
Whiteway, L
Eifler, T F
Zuntz, J
Scarpine, V
Brooks, D
Doel, P
Smith, M
Crocce, M
Plazas, A A
Thomas, D
Ferrero, I
De Vicente, J
Desai, S
Gutierrez, G
Maia, M A G
Evrard, A E
Jeffrey, N
Abbott, T M C
Allam, S
March, M
Friedrich, O
DeRose, J
Sevilla-Noarbe, I
Johnson, M D
Lima, M
Everett, S
Gatti, M
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Fermi National Accelerator Laboratory (FNAL), Batavia, IL (United States)
Oak Ridge National Laboratory (ORNL), Oak Ridge, TN (United States)
SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States)
Univ. of Michigan, Ann Arbor, MI (United States)
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IEDL.DBID TOX
ISSN 0035-8711
IngestDate Mon Apr 01 04:56:13 EDT 2024
Sat Apr 29 05:40:50 EDT 2023
Thu Sep 12 17:55:21 EDT 2024
Wed Aug 28 03:20:15 EDT 2024
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Issue 3
Keywords gravitational lensing: weak
cosmology: observations
large-scale structure of Universe
Language English
Norwegian
License This article is published and distributed under the terms of the Oxford University Press, Standard Journals Publication Model (https://academic.oup.com/journals/pages/open_access/funder_policies/chorus/standard_publication_model)
LinkModel DirectLink
MergedId FETCHMERGED-LOGICAL-c364t-1669efde31d5c9563416b1bc43b9e3a27f5b69595dcada16c56b2d955f3b387d3
Notes NFR/287772
AC02-07CH11359; SC0019193; AC05-00OR22725
USDOE Office of Science (SC), High Energy Physics (HEP)
FERMILAB-PUB-19-576-A-AD-AE-SCD; arXiv:1911.05568
ORCID 0000-0002-6011-0530
0000-0002-7887-0896
0000-0001-6082-8529
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OpenAccessLink http://hdl.handle.net/10852/80172
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oup_primary_10_1093_mnras_staa2680
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Snippet ABSTRACT We present a simulated cosmology analysis using the second and third moments of the weak lensing mass (convergence) maps. The second moment, or...
We present a simulated cosmology analysis using the second and third moments of the weak lensing mass (convergence) maps. The second moment, or variances, of...
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SubjectTerms ASTRONOMY AND ASTROPHYSICS
cosmology: observations
gravitational lensing: weak
large-scale structure of Universe
Title Dark Energy Survey Year 3 results: cosmology with moments of weak lensing mass maps – validation on simulations
URI http://hdl.handle.net/10852/80172
https://www.osti.gov/biblio/1668095
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