Dark Energy Survey Year 1 Results: Methodology and Projections for Joint Analysis of Galaxy Clustering, Galaxy Lensing, and CMB Lensing Two-point Functions
International audience Optical imaging surveys measure both the galaxy density and the gravitational lensing-induced shear fields across the sky. Recently, the Dark Energy Survey (DES) Collaboration used a joint fit to two-point correlations between these observables to place tight constraints on co...
Published in: | Physical Review D |
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Format: | Article in Journal/Newspaper |
Language: | English |
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Online Access: | https://hal.science/hal-01724844 https://hal.science/hal-01724844/document https://hal.science/hal-01724844/file/10.1103PhysRevD.99.023508.pdf https://doi.org/10.1103/PhysRevD.99.023508 |
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ftinsu:oai:HAL:hal-01724844v1 2024-04-14T08:19:47+00:00 Dark Energy Survey Year 1 Results: Methodology and Projections for Joint Analysis of Galaxy Clustering, Galaxy Lensing, and CMB Lensing Two-point Functions Baxter, E.J. Omori, Y. Chang, C. Giannantonio, T. Kirk, D. Krause, E. Blazek, J. Bleem, L. Choi, A. Crawford, T.M. Dodelson, S. Eifler, T.F. Friedrich, O. Gruen, D. Holder, G.P. Jain, B. Jarvis, M. Maccrann, N. Nicola, A. Pandey, S. Prat, J. Reichardt, C.L. Samuroff, S. Sánchez, C. Secco, L.F. Sheldon, E. Troxel, M.A. Zuntz, J. Abbott, T.M.C. Abdalla, F.B. Annis, J. Avila, S. Bechtol, K. Benson, B.A. Bertin, E. Brooks, D. Buckley-Geer, E. Burke, D.L. Carnero Rosell, A. Carrasco Kind, M. Carretero, J. Castander, F.J. Cawthon, R. Cunha, C.E. d'Andrea, C.B. da Costa, L.N. Davis, C. de Vicente, J. Depoy, D.L. Diehl, H.T. Doel, P. Estrada, J. Evrard, A.E. Flaugher, B. Fosalba, P. Frieman, J. García-Bellido, J. Gaztanaga, E. Gerdes, D.W. Gruendl, R.A. Gschwend, J. Gutierrez, G. Hartley, W.G. Hollowood, D. Hoyle, B. James, D.J. Kent, S. Kuehn, K. Kuropatkin, N. Lahav, O. Lima, M. Maia, M.A.G. March, M. Marshall, J.L. Melchior, P. Menanteau, F. Miquel, R. Plazas, A.A. Roodman, A. Rykoff, E.S. Sanchez, E. Schindler, R. Schubnell, M. Sevilla-Noarbe, I. Smith, M. Smith, R.C. Soares-Santos, M. Sobreira, F. Suchyta, E. Swanson, M.E.C. Tarle, G. Walker, A.R. Wu, W.L.K. Weller, J. Institut d'Astrophysique de Paris (IAP) Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS) DES 2019 https://hal.science/hal-01724844 https://hal.science/hal-01724844/document https://hal.science/hal-01724844/file/10.1103PhysRevD.99.023508.pdf https://doi.org/10.1103/PhysRevD.99.023508 en eng HAL CCSD info:eu-repo/semantics/altIdentifier/arxiv/1802.05257 info:eu-repo/semantics/altIdentifier/doi/10.1103/PhysRevD.99.023508 hal-01724844 https://hal.science/hal-01724844 https://hal.science/hal-01724844/document https://hal.science/hal-01724844/file/10.1103PhysRevD.99.023508.pdf ARXIV: 1802.05257 doi:10.1103/PhysRevD.99.023508 INSPIRE: 1654991 info:eu-repo/semantics/OpenAccess Phys.Rev.D https://hal.science/hal-01724844 Phys.Rev.D, 2019, 99 (2), pp.023508. ⟨10.1103/PhysRevD.99.023508⟩ Cosmology [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] info:eu-repo/semantics/article Journal articles 2019 ftinsu https://doi.org/10.1103/PhysRevD.99.023508 2024-03-21T17:06:29Z International audience Optical imaging surveys measure both the galaxy density and the gravitational lensing-induced shear fields across the sky. Recently, the Dark Energy Survey (DES) Collaboration used a joint fit to two-point correlations between these observables to place tight constraints on cosmology (T. M. C. Abbott (Dark Energy Survey Collaboration), Phys. Rev. D 98, 043526 (2018)PRVDAQ2470-001010.1103/PhysRevD.98.043526). In this work, we develop the methodology to extend the DES Year 1 joint probes analysis to include cross-correlations of the optical survey observables with gravitational lensing of the cosmic microwave background as measured by the South Pole Telescope (SPT) and Planck. Using simulated analyses, we show how the resulting set of five two-point functions increases the robustness of the cosmological constraints to systematic errors in galaxy lensing shear calibration. Additionally, we show that contamination of the SPT+Planck cosmic microwave background lensing map by the thermal Sunyaev-Zel’dovich effect is a potentially large source of systematic error for two-point function analyses but show that it can be reduced to acceptable levels in our analysis by masking clusters of galaxies and imposing angular scale cuts on the two-point functions. The methodology developed here will be applied to the analysis of data from the DES, the SPT, and Planck in a companion work. Article in Journal/Newspaper South pole Institut national des sciences de l'Univers: HAL-INSU Abbott ENVELOPE(-62.133,-62.133,-64.100,-64.100) South Pole Physical Review D 99 2 |
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Institut national des sciences de l'Univers: HAL-INSU |
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ftinsu |
language |
English |
topic |
Cosmology [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] |
spellingShingle |
Cosmology [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] Baxter, E.J. Omori, Y. Chang, C. Giannantonio, T. Kirk, D. Krause, E. Blazek, J. Bleem, L. Choi, A. Crawford, T.M. Dodelson, S. Eifler, T.F. Friedrich, O. Gruen, D. Holder, G.P. Jain, B. Jarvis, M. Maccrann, N. Nicola, A. Pandey, S. Prat, J. Reichardt, C.L. Samuroff, S. Sánchez, C. Secco, L.F. Sheldon, E. Troxel, M.A. Zuntz, J. Abbott, T.M.C. Abdalla, F.B. Annis, J. Avila, S. Bechtol, K. Benson, B.A. Bertin, E. Brooks, D. Buckley-Geer, E. Burke, D.L. Carnero Rosell, A. Carrasco Kind, M. Carretero, J. Castander, F.J. Cawthon, R. Cunha, C.E. d'Andrea, C.B. da Costa, L.N. Davis, C. de Vicente, J. Depoy, D.L. Diehl, H.T. Doel, P. Estrada, J. Evrard, A.E. Flaugher, B. Fosalba, P. Frieman, J. García-Bellido, J. Gaztanaga, E. Gerdes, D.W. Gruendl, R.A. Gschwend, J. Gutierrez, G. Hartley, W.G. Hollowood, D. Hoyle, B. James, D.J. Kent, S. Kuehn, K. Kuropatkin, N. Lahav, O. Lima, M. Maia, M.A.G. March, M. Marshall, J.L. Melchior, P. Menanteau, F. Miquel, R. Plazas, A.A. Roodman, A. Rykoff, E.S. Sanchez, E. Schindler, R. Schubnell, M. Sevilla-Noarbe, I. Smith, M. Smith, R.C. Soares-Santos, M. Sobreira, F. Suchyta, E. Swanson, M.E.C. Tarle, G. Walker, A.R. Wu, W.L.K. Weller, J. Dark Energy Survey Year 1 Results: Methodology and Projections for Joint Analysis of Galaxy Clustering, Galaxy Lensing, and CMB Lensing Two-point Functions |
topic_facet |
Cosmology [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] |
description |
International audience Optical imaging surveys measure both the galaxy density and the gravitational lensing-induced shear fields across the sky. Recently, the Dark Energy Survey (DES) Collaboration used a joint fit to two-point correlations between these observables to place tight constraints on cosmology (T. M. C. Abbott (Dark Energy Survey Collaboration), Phys. Rev. D 98, 043526 (2018)PRVDAQ2470-001010.1103/PhysRevD.98.043526). In this work, we develop the methodology to extend the DES Year 1 joint probes analysis to include cross-correlations of the optical survey observables with gravitational lensing of the cosmic microwave background as measured by the South Pole Telescope (SPT) and Planck. Using simulated analyses, we show how the resulting set of five two-point functions increases the robustness of the cosmological constraints to systematic errors in galaxy lensing shear calibration. Additionally, we show that contamination of the SPT+Planck cosmic microwave background lensing map by the thermal Sunyaev-Zel’dovich effect is a potentially large source of systematic error for two-point function analyses but show that it can be reduced to acceptable levels in our analysis by masking clusters of galaxies and imposing angular scale cuts on the two-point functions. The methodology developed here will be applied to the analysis of data from the DES, the SPT, and Planck in a companion work. |
author2 |
Institut d'Astrophysique de Paris (IAP) Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS) DES |
format |
Article in Journal/Newspaper |
author |
Baxter, E.J. Omori, Y. Chang, C. Giannantonio, T. Kirk, D. Krause, E. Blazek, J. Bleem, L. Choi, A. Crawford, T.M. Dodelson, S. Eifler, T.F. Friedrich, O. Gruen, D. Holder, G.P. Jain, B. Jarvis, M. Maccrann, N. Nicola, A. Pandey, S. Prat, J. Reichardt, C.L. Samuroff, S. Sánchez, C. Secco, L.F. Sheldon, E. Troxel, M.A. Zuntz, J. Abbott, T.M.C. Abdalla, F.B. Annis, J. Avila, S. Bechtol, K. Benson, B.A. Bertin, E. Brooks, D. Buckley-Geer, E. Burke, D.L. Carnero Rosell, A. Carrasco Kind, M. Carretero, J. Castander, F.J. Cawthon, R. Cunha, C.E. d'Andrea, C.B. da Costa, L.N. Davis, C. de Vicente, J. Depoy, D.L. Diehl, H.T. Doel, P. Estrada, J. Evrard, A.E. Flaugher, B. Fosalba, P. Frieman, J. García-Bellido, J. Gaztanaga, E. Gerdes, D.W. Gruendl, R.A. Gschwend, J. Gutierrez, G. Hartley, W.G. Hollowood, D. Hoyle, B. James, D.J. Kent, S. Kuehn, K. Kuropatkin, N. Lahav, O. Lima, M. Maia, M.A.G. March, M. Marshall, J.L. Melchior, P. Menanteau, F. Miquel, R. Plazas, A.A. Roodman, A. Rykoff, E.S. Sanchez, E. Schindler, R. Schubnell, M. Sevilla-Noarbe, I. Smith, M. Smith, R.C. Soares-Santos, M. Sobreira, F. Suchyta, E. Swanson, M.E.C. Tarle, G. Walker, A.R. Wu, W.L.K. Weller, J. |
author_facet |
Baxter, E.J. Omori, Y. Chang, C. Giannantonio, T. Kirk, D. Krause, E. Blazek, J. Bleem, L. Choi, A. Crawford, T.M. Dodelson, S. Eifler, T.F. Friedrich, O. Gruen, D. Holder, G.P. Jain, B. Jarvis, M. Maccrann, N. Nicola, A. Pandey, S. Prat, J. Reichardt, C.L. Samuroff, S. Sánchez, C. Secco, L.F. Sheldon, E. Troxel, M.A. Zuntz, J. Abbott, T.M.C. Abdalla, F.B. Annis, J. Avila, S. Bechtol, K. Benson, B.A. Bertin, E. Brooks, D. Buckley-Geer, E. Burke, D.L. Carnero Rosell, A. Carrasco Kind, M. Carretero, J. Castander, F.J. Cawthon, R. Cunha, C.E. d'Andrea, C.B. da Costa, L.N. Davis, C. de Vicente, J. Depoy, D.L. Diehl, H.T. Doel, P. Estrada, J. Evrard, A.E. Flaugher, B. Fosalba, P. Frieman, J. García-Bellido, J. Gaztanaga, E. Gerdes, D.W. Gruendl, R.A. Gschwend, J. Gutierrez, G. Hartley, W.G. Hollowood, D. Hoyle, B. James, D.J. Kent, S. Kuehn, K. Kuropatkin, N. Lahav, O. Lima, M. Maia, M.A.G. March, M. Marshall, J.L. Melchior, P. Menanteau, F. Miquel, R. Plazas, A.A. Roodman, A. Rykoff, E.S. Sanchez, E. Schindler, R. Schubnell, M. Sevilla-Noarbe, I. Smith, M. Smith, R.C. Soares-Santos, M. Sobreira, F. Suchyta, E. Swanson, M.E.C. Tarle, G. Walker, A.R. Wu, W.L.K. Weller, J. |
author_sort |
Baxter, E.J. |
title |
Dark Energy Survey Year 1 Results: Methodology and Projections for Joint Analysis of Galaxy Clustering, Galaxy Lensing, and CMB Lensing Two-point Functions |
title_short |
Dark Energy Survey Year 1 Results: Methodology and Projections for Joint Analysis of Galaxy Clustering, Galaxy Lensing, and CMB Lensing Two-point Functions |
title_full |
Dark Energy Survey Year 1 Results: Methodology and Projections for Joint Analysis of Galaxy Clustering, Galaxy Lensing, and CMB Lensing Two-point Functions |
title_fullStr |
Dark Energy Survey Year 1 Results: Methodology and Projections for Joint Analysis of Galaxy Clustering, Galaxy Lensing, and CMB Lensing Two-point Functions |
title_full_unstemmed |
Dark Energy Survey Year 1 Results: Methodology and Projections for Joint Analysis of Galaxy Clustering, Galaxy Lensing, and CMB Lensing Two-point Functions |
title_sort |
dark energy survey year 1 results: methodology and projections for joint analysis of galaxy clustering, galaxy lensing, and cmb lensing two-point functions |
publisher |
HAL CCSD |
publishDate |
2019 |
url |
https://hal.science/hal-01724844 https://hal.science/hal-01724844/document https://hal.science/hal-01724844/file/10.1103PhysRevD.99.023508.pdf https://doi.org/10.1103/PhysRevD.99.023508 |
long_lat |
ENVELOPE(-62.133,-62.133,-64.100,-64.100) |
geographic |
Abbott South Pole |
geographic_facet |
Abbott South Pole |
genre |
South pole |
genre_facet |
South pole |
op_source |
Phys.Rev.D https://hal.science/hal-01724844 Phys.Rev.D, 2019, 99 (2), pp.023508. ⟨10.1103/PhysRevD.99.023508⟩ |
op_relation |
info:eu-repo/semantics/altIdentifier/arxiv/1802.05257 info:eu-repo/semantics/altIdentifier/doi/10.1103/PhysRevD.99.023508 hal-01724844 https://hal.science/hal-01724844 https://hal.science/hal-01724844/document https://hal.science/hal-01724844/file/10.1103PhysRevD.99.023508.pdf ARXIV: 1802.05257 doi:10.1103/PhysRevD.99.023508 INSPIRE: 1654991 |
op_rights |
info:eu-repo/semantics/OpenAccess |
op_doi |
https://doi.org/10.1103/PhysRevD.99.023508 |
container_title |
Physical Review D |
container_volume |
99 |
container_issue |
2 |
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1796297902376615936 |