Joint analysis of Dark Energy Survey Year 3 data and CMB lensing from SPT and Planck. I. Construction of CMB lensing maps and modeling choices
Joint analyses of cross-correlations between measurements of galaxy positions, galaxy lensing, and lensing of the cosmic microwave background (CMB) offer powerful constraints on the large-scale structure of the Universe. In a forthcoming analysis, we will present cosmological constraints from the an...
Published in: | Physical Review D |
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Main Authors: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
Format: | Article in Journal/Newspaper |
Language: | English |
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2023
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Online Access: | https://researchers.mq.edu.au/en/publications/f52aaf4a-de66-4caa-b126-d4f31dbe16de https://doi.org/10.1103/PhysRevD.107.023529 http://www.scopus.com/inward/record.url?scp=85147523490&partnerID=8YFLogxK http://purl.org/au-research/grants/arc/DP200101068 |
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Joint analyses of cross-correlations between measurements of galaxy positions, galaxy lensing, and lensing of the cosmic microwave background (CMB) offer powerful constraints on the large-scale structure of the Universe. In a forthcoming analysis, we will present cosmological constraints from the analysis of such cross-correlations measured using Year 3 data from the Dark Energy Survey (DES), and CMB data from the South Pole Telescope (SPT) and Planck. Here we present two key ingredients of this analysis: (1) an improved CMB lensing map in the SPT-SZ survey footprint and (2) the analysis methodology that will be used to extract cosmological information from the cross-correlation measurements. Relative to previous lensing maps made from the same CMB observations, we have implemented techniques to remove contamination from the thermal Sunyaev Zel'dovich effect, enabling the extraction of cosmological information from smaller angular scales of the cross-correlation measurements than in previous analyses with DES Year 1 data. We describe our model for the cross-correlations between these maps and DES data, and validate our modeling choices to demonstrate the robustness of our analysis. We then forecast the expected cosmological constraints from the galaxy survey-CMB lensing auto and cross-correlations. We find that the galaxy-CMB lensing and galaxy shear-CMB lensing correlations will on their own provide a constraint on S 8 = σ 8 √Ω m /0.3 at the few percent level, providing a powerful consistency check for the DES-only constraints. We explore scenarios where external priors on shear calibration are removed, finding that the joint analysis of CMB lensing cross-correlations can provide constraints on the shear calibration amplitude at the 5% to 10% level. |
format |
Article in Journal/Newspaper |
author |
Omori, Y. Baxter, E. J. Chang, C. Friedrich, O. Alarcon, A. Alves, O. Amon, A. Andrade-Oliveira, F. Bechtol, K. Becker, M. R. Bernstein, G. M. Blazek, J. Bleem, L. E. Camacho, H. Campos, A. Carnero Rosell, A. Carrasco Kind, M. Cawthon, R. Chen, R. Choi, A. Cordero, J. Crawford, T. M. Crocce, M. Davis, C. DeRose, J. Dodelson, S. Doux, C. Drlica-Wagner, A. Eckert, K. Eifler, T. F. Elsner, F. Elvin-Poole, J. Everett, S. Fang, X. Ferté, A. Fosalba, P. Gatti, M. Giannini, G. Gruen, D. Gruendl, R. A. Harrison, I. Herner, K. Huang, H. Huff, E. M. Huterer, D. Jarvis, M. Krause, E. Kuropatkin, N. Leget, P.-F. Lemos, P. Liddle, A. R. MacCrann, N. McCullough, J. Muir, J. Myles, J. Navarro-Alsina, A. Pandey, S. Park, Y. Porredon, A. Prat, J. Raveri, M. Rollins, R. P. Roodman, A. Rosenfeld, R. Ross, A. J. Rykoff, E. S. Sánchez, C. Sanchez, J. Secco, L. F. Sevilla-Noarbe, I. Sheldon, E. Shin, T. Troxel, M. A. Tutusaus, I. Varga, T. N. Weaverdyck, N. Wechsler, R. H. Wu, W. L. K. Yanny, B. Yin, B. Zhang, Y. Zuntz, J. Abbott, T. M. C. Aguena, M. Allam, S. Annis, J. Bacon, D. Benson, B. A. Bertin, E. Bocquet, S. Brooks, D. Burke, D. L. Carlstrom, J. E. Carretero, J. Chang, C. L. Chown, R. Costanzi, M. da Costa, L. N. Crites, A. T. Pereira, M. E. S. de Haan, T. De Vicente, J. Desai, S. Diehl, H. T. Dobbs, M. A. Doel, P. Everett, W. Ferrero, I. Flaugher, B. Friedel, D. Frieman, J. García-Bellido, J. Gaztanaga, E. George, E. M. Giannantonio, T. Halverson, N. W. Hinton, S. R. Holder, G. P. Hollowood, D. L. Holzapfel, W. L. Honscheid, K. Hrubes, J. D. James, D. J. Knox, L. Kuehn, K. Lahav, O. Lee, A. T. Lima, M. Luong-Van, D. March, M. McMahon, J. J. Melchior, P. Menanteau, F. Meyer, S. S. Miquel, R. Mocanu, L. Mohr, J. J. Morgan, R. Natoli, T. Padin, S. Palmese, A. Paz-Chinchón, F. Pieres, A. Plazas Malagón, A. A. Pryke, C. Reichardt, C. L. Romer, A. K. Ruhl, J. E. Sanchez, E. Schaffer, K. K. Schubnell, M. Serrano, S. Shirokoff, E. Smith, M. Staniszewski, Z. Stark, A. A. Suchyta, E. Tarle, G. Thomas, D. To, C. Vieira, J. D. Weller, J. Williamson, R. |
spellingShingle |
Omori, Y. Baxter, E. J. Chang, C. Friedrich, O. Alarcon, A. Alves, O. Amon, A. Andrade-Oliveira, F. Bechtol, K. Becker, M. R. Bernstein, G. M. Blazek, J. Bleem, L. E. Camacho, H. Campos, A. Carnero Rosell, A. Carrasco Kind, M. Cawthon, R. Chen, R. Choi, A. Cordero, J. Crawford, T. M. Crocce, M. Davis, C. DeRose, J. Dodelson, S. Doux, C. Drlica-Wagner, A. Eckert, K. Eifler, T. F. Elsner, F. Elvin-Poole, J. Everett, S. Fang, X. Ferté, A. Fosalba, P. Gatti, M. Giannini, G. Gruen, D. Gruendl, R. A. Harrison, I. Herner, K. Huang, H. Huff, E. M. Huterer, D. Jarvis, M. Krause, E. Kuropatkin, N. Leget, P.-F. Lemos, P. Liddle, A. R. MacCrann, N. McCullough, J. Muir, J. Myles, J. Navarro-Alsina, A. Pandey, S. Park, Y. Porredon, A. Prat, J. Raveri, M. Rollins, R. P. Roodman, A. Rosenfeld, R. Ross, A. J. Rykoff, E. S. Sánchez, C. Sanchez, J. Secco, L. F. Sevilla-Noarbe, I. Sheldon, E. Shin, T. Troxel, M. A. Tutusaus, I. Varga, T. N. Weaverdyck, N. Wechsler, R. H. Wu, W. L. K. Yanny, B. Yin, B. Zhang, Y. Zuntz, J. Abbott, T. M. C. Aguena, M. Allam, S. Annis, J. Bacon, D. Benson, B. A. Bertin, E. Bocquet, S. Brooks, D. Burke, D. L. Carlstrom, J. E. Carretero, J. Chang, C. L. Chown, R. Costanzi, M. da Costa, L. N. Crites, A. T. Pereira, M. E. S. de Haan, T. De Vicente, J. Desai, S. Diehl, H. T. Dobbs, M. A. Doel, P. Everett, W. Ferrero, I. Flaugher, B. Friedel, D. Frieman, J. García-Bellido, J. Gaztanaga, E. George, E. M. Giannantonio, T. Halverson, N. W. Hinton, S. R. Holder, G. P. Hollowood, D. L. Holzapfel, W. L. Honscheid, K. Hrubes, J. D. James, D. J. Knox, L. Kuehn, K. Lahav, O. Lee, A. T. Lima, M. Luong-Van, D. March, M. McMahon, J. J. Melchior, P. Menanteau, F. Meyer, S. S. Miquel, R. Mocanu, L. Mohr, J. J. Morgan, R. Natoli, T. Padin, S. Palmese, A. Paz-Chinchón, F. Pieres, A. Plazas Malagón, A. A. Pryke, C. Reichardt, C. L. Romer, A. K. Ruhl, J. E. Sanchez, E. Schaffer, K. K. Schubnell, M. Serrano, S. Shirokoff, E. Smith, M. Staniszewski, Z. Stark, A. A. Suchyta, E. Tarle, G. Thomas, D. To, C. Vieira, J. D. Weller, J. Williamson, R. Joint analysis of Dark Energy Survey Year 3 data and CMB lensing from SPT and Planck. I. Construction of CMB lensing maps and modeling choices |
author_facet |
Omori, Y. Baxter, E. J. Chang, C. Friedrich, O. Alarcon, A. Alves, O. Amon, A. Andrade-Oliveira, F. Bechtol, K. Becker, M. R. Bernstein, G. M. Blazek, J. Bleem, L. E. Camacho, H. Campos, A. Carnero Rosell, A. Carrasco Kind, M. Cawthon, R. Chen, R. Choi, A. Cordero, J. Crawford, T. M. Crocce, M. Davis, C. DeRose, J. Dodelson, S. Doux, C. Drlica-Wagner, A. Eckert, K. Eifler, T. F. Elsner, F. Elvin-Poole, J. Everett, S. Fang, X. Ferté, A. Fosalba, P. Gatti, M. Giannini, G. Gruen, D. Gruendl, R. A. Harrison, I. Herner, K. Huang, H. Huff, E. M. Huterer, D. Jarvis, M. Krause, E. Kuropatkin, N. Leget, P.-F. Lemos, P. Liddle, A. R. MacCrann, N. McCullough, J. Muir, J. Myles, J. Navarro-Alsina, A. Pandey, S. Park, Y. Porredon, A. Prat, J. Raveri, M. Rollins, R. P. Roodman, A. Rosenfeld, R. Ross, A. J. Rykoff, E. S. Sánchez, C. Sanchez, J. Secco, L. F. Sevilla-Noarbe, I. Sheldon, E. Shin, T. Troxel, M. A. Tutusaus, I. Varga, T. N. Weaverdyck, N. Wechsler, R. H. Wu, W. L. K. Yanny, B. Yin, B. Zhang, Y. Zuntz, J. Abbott, T. M. C. Aguena, M. Allam, S. Annis, J. Bacon, D. Benson, B. A. Bertin, E. Bocquet, S. Brooks, D. Burke, D. L. Carlstrom, J. E. Carretero, J. Chang, C. L. Chown, R. Costanzi, M. da Costa, L. N. Crites, A. T. Pereira, M. E. S. de Haan, T. De Vicente, J. Desai, S. Diehl, H. T. Dobbs, M. A. Doel, P. Everett, W. Ferrero, I. Flaugher, B. Friedel, D. Frieman, J. García-Bellido, J. Gaztanaga, E. George, E. M. Giannantonio, T. Halverson, N. W. Hinton, S. R. Holder, G. P. Hollowood, D. L. Holzapfel, W. L. Honscheid, K. Hrubes, J. D. James, D. J. Knox, L. Kuehn, K. Lahav, O. Lee, A. T. Lima, M. Luong-Van, D. March, M. McMahon, J. J. Melchior, P. Menanteau, F. Meyer, S. S. Miquel, R. Mocanu, L. Mohr, J. J. Morgan, R. Natoli, T. Padin, S. Palmese, A. Paz-Chinchón, F. Pieres, A. Plazas Malagón, A. A. Pryke, C. Reichardt, C. L. Romer, A. K. Ruhl, J. E. Sanchez, E. Schaffer, K. K. Schubnell, M. Serrano, S. Shirokoff, E. Smith, M. Staniszewski, Z. Stark, A. A. Suchyta, E. Tarle, G. Thomas, D. To, C. Vieira, J. D. Weller, J. Williamson, R. |
author_sort |
Omori, Y. |
title |
Joint analysis of Dark Energy Survey Year 3 data and CMB lensing from SPT and Planck. I. Construction of CMB lensing maps and modeling choices |
title_short |
Joint analysis of Dark Energy Survey Year 3 data and CMB lensing from SPT and Planck. I. Construction of CMB lensing maps and modeling choices |
title_full |
Joint analysis of Dark Energy Survey Year 3 data and CMB lensing from SPT and Planck. I. Construction of CMB lensing maps and modeling choices |
title_fullStr |
Joint analysis of Dark Energy Survey Year 3 data and CMB lensing from SPT and Planck. I. Construction of CMB lensing maps and modeling choices |
title_full_unstemmed |
Joint analysis of Dark Energy Survey Year 3 data and CMB lensing from SPT and Planck. I. Construction of CMB lensing maps and modeling choices |
title_sort |
joint analysis of dark energy survey year 3 data and cmb lensing from spt and planck. i. construction of cmb lensing maps and modeling choices |
publishDate |
2023 |
url |
https://researchers.mq.edu.au/en/publications/f52aaf4a-de66-4caa-b126-d4f31dbe16de https://doi.org/10.1103/PhysRevD.107.023529 http://www.scopus.com/inward/record.url?scp=85147523490&partnerID=8YFLogxK http://purl.org/au-research/grants/arc/DP200101068 |
geographic |
South Pole |
geographic_facet |
South Pole |
genre |
South pole |
genre_facet |
South pole |
op_source |
Omori , Y , Baxter , E J , Chang , C , Friedrich , O , Alarcon , A , Alves , O , Amon , A , Andrade-Oliveira , F , Bechtol , K , Becker , M R , Bernstein , G M , Blazek , J , Bleem , L E , Camacho , H , Campos , A , Carnero Rosell , A , Carrasco Kind , M , Cawthon , R , Chen , R , Choi , A , Cordero , J , Crawford , T M , Crocce , M , Davis , C , DeRose , J , Dodelson , S , Doux , C , Drlica-Wagner , A , Eckert , K , Eifler , T F , Elsner , F , Elvin-Poole , J , Everett , S , Fang , X , Ferté , A , Fosalba , P , Gatti , M , Giannini , G , Gruen , D , Gruendl , R A , Harrison , I , Herner , K , Huang , H , Huff , E M , Huterer , D , Jarvis , M , Krause , E , Kuropatkin , N , Leget , P-F , Lemos , P , Liddle , A R , MacCrann , N , McCullough , J , Muir , J , Myles , J , Navarro-Alsina , A , Pandey , S , Park , Y , Porredon , A , Prat , J , Raveri , M , Rollins , R P , Roodman , A , Rosenfeld , R , Ross , A J , Rykoff , E S , Sánchez , C , Sanchez , J , Secco , L F , Sevilla-Noarbe , I , Sheldon , E , Shin , T , Troxel , M A , Tutusaus , I , Varga , T N , Weaverdyck , N , Wechsler , R H , Wu , W L K , Yanny , B , Yin , B , Zhang , Y , Zuntz , J , Abbott , T M C , Aguena , M , Allam , S , Annis , J , Bacon , D , Benson , B A , Bertin , E , Bocquet , S , Brooks , D , Burke , D L , Carlstrom , J E , Carretero , J , Chang , C L , Chown , R , Costanzi , M , da Costa , L N , Crites , A T , Pereira , M E S , de Haan , T , De Vicente , J , Desai , S , Diehl , H T , Dobbs , M A , Doel , P , Everett , W , Ferrero , I , Flaugher , B , Friedel , D , Frieman , J , García-Bellido , J , Gaztanaga , E , George , E M , Giannantonio , T , Halverson , N W , Hinton , S R , Holder , G P , Hollowood , D L , Holzapfel , W L , Honscheid , K , Hrubes , J D , James , D J , Knox , L , Kuehn , K , Lahav , O , Lee , A T , Lima , M , Luong-Van , D , March , M , McMahon , J J , Melchior , P , Menanteau , F , Meyer , S S , Miquel , R , Mocanu , L , Mohr , J J , Morgan , R , Natoli , T , Padin , S , P |
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info:eu-repo/semantics/closedAccess |
op_doi |
https://doi.org/10.1103/PhysRevD.107.023529 |
container_title |
Physical Review D |
container_volume |
107 |
container_issue |
2 |
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1802650213251284992 |
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ftmacquarieunicr:oai:https://researchers.mq.edu.au:publications/f52aaf4a-de66-4caa-b126-d4f31dbe16de 2024-06-23T07:56:51+00:00 Joint analysis of Dark Energy Survey Year 3 data and CMB lensing from SPT and Planck. I. Construction of CMB lensing maps and modeling choices Omori, Y. Baxter, E. J. Chang, C. Friedrich, O. Alarcon, A. Alves, O. Amon, A. Andrade-Oliveira, F. Bechtol, K. Becker, M. R. Bernstein, G. M. Blazek, J. Bleem, L. E. Camacho, H. Campos, A. Carnero Rosell, A. Carrasco Kind, M. Cawthon, R. Chen, R. Choi, A. Cordero, J. Crawford, T. M. Crocce, M. Davis, C. DeRose, J. Dodelson, S. Doux, C. Drlica-Wagner, A. Eckert, K. Eifler, T. F. Elsner, F. Elvin-Poole, J. Everett, S. Fang, X. Ferté, A. Fosalba, P. Gatti, M. Giannini, G. Gruen, D. Gruendl, R. A. Harrison, I. Herner, K. Huang, H. Huff, E. M. Huterer, D. Jarvis, M. Krause, E. Kuropatkin, N. Leget, P.-F. Lemos, P. Liddle, A. R. MacCrann, N. McCullough, J. Muir, J. Myles, J. Navarro-Alsina, A. Pandey, S. Park, Y. Porredon, A. Prat, J. Raveri, M. Rollins, R. P. Roodman, A. Rosenfeld, R. Ross, A. J. Rykoff, E. S. Sánchez, C. Sanchez, J. Secco, L. F. Sevilla-Noarbe, I. Sheldon, E. Shin, T. Troxel, M. A. Tutusaus, I. Varga, T. N. Weaverdyck, N. Wechsler, R. H. Wu, W. L. K. Yanny, B. Yin, B. Zhang, Y. Zuntz, J. Abbott, T. M. C. Aguena, M. Allam, S. Annis, J. Bacon, D. Benson, B. A. Bertin, E. Bocquet, S. Brooks, D. Burke, D. L. Carlstrom, J. E. Carretero, J. Chang, C. L. Chown, R. Costanzi, M. da Costa, L. N. Crites, A. T. Pereira, M. E. S. de Haan, T. De Vicente, J. Desai, S. Diehl, H. T. Dobbs, M. A. Doel, P. Everett, W. Ferrero, I. Flaugher, B. Friedel, D. Frieman, J. García-Bellido, J. Gaztanaga, E. George, E. M. Giannantonio, T. Halverson, N. W. Hinton, S. R. Holder, G. P. Hollowood, D. L. Holzapfel, W. L. Honscheid, K. Hrubes, J. D. James, D. J. Knox, L. Kuehn, K. Lahav, O. Lee, A. T. Lima, M. Luong-Van, D. March, M. McMahon, J. J. Melchior, P. Menanteau, F. Meyer, S. S. Miquel, R. Mocanu, L. Mohr, J. J. Morgan, R. Natoli, T. Padin, S. Palmese, A. Paz-Chinchón, F. Pieres, A. Plazas Malagón, A. A. Pryke, C. Reichardt, C. L. Romer, A. K. Ruhl, J. E. Sanchez, E. Schaffer, K. K. Schubnell, M. Serrano, S. Shirokoff, E. Smith, M. Staniszewski, Z. Stark, A. A. Suchyta, E. Tarle, G. Thomas, D. To, C. Vieira, J. D. Weller, J. Williamson, R. 2023-01-15 https://researchers.mq.edu.au/en/publications/f52aaf4a-de66-4caa-b126-d4f31dbe16de https://doi.org/10.1103/PhysRevD.107.023529 http://www.scopus.com/inward/record.url?scp=85147523490&partnerID=8YFLogxK http://purl.org/au-research/grants/arc/DP200101068 eng eng info:eu-repo/semantics/closedAccess Omori , Y , Baxter , E J , Chang , C , Friedrich , O , Alarcon , A , Alves , O , Amon , A , Andrade-Oliveira , F , Bechtol , K , Becker , M R , Bernstein , G M , Blazek , J , Bleem , L E , Camacho , H , Campos , A , Carnero Rosell , A , Carrasco Kind , M , Cawthon , R , Chen , R , Choi , A , Cordero , J , Crawford , T M , Crocce , M , Davis , C , DeRose , J , Dodelson , S , Doux , C , Drlica-Wagner , A , Eckert , K , Eifler , T F , Elsner , F , Elvin-Poole , J , Everett , S , Fang , X , Ferté , A , Fosalba , P , Gatti , M , Giannini , G , Gruen , D , Gruendl , R A , Harrison , I , Herner , K , Huang , H , Huff , E M , Huterer , D , Jarvis , M , Krause , E , Kuropatkin , N , Leget , P-F , Lemos , P , Liddle , A R , MacCrann , N , McCullough , J , Muir , J , Myles , J , Navarro-Alsina , A , Pandey , S , Park , Y , Porredon , A , Prat , J , Raveri , M , Rollins , R P , Roodman , A , Rosenfeld , R , Ross , A J , Rykoff , E S , Sánchez , C , Sanchez , J , Secco , L F , Sevilla-Noarbe , I , Sheldon , E , Shin , T , Troxel , M A , Tutusaus , I , Varga , T N , Weaverdyck , N , Wechsler , R H , Wu , W L K , Yanny , B , Yin , B , Zhang , Y , Zuntz , J , Abbott , T M C , Aguena , M , Allam , S , Annis , J , Bacon , D , Benson , B A , Bertin , E , Bocquet , S , Brooks , D , Burke , D L , Carlstrom , J E , Carretero , J , Chang , C L , Chown , R , Costanzi , M , da Costa , L N , Crites , A T , Pereira , M E S , de Haan , T , De Vicente , J , Desai , S , Diehl , H T , Dobbs , M A , Doel , P , Everett , W , Ferrero , I , Flaugher , B , Friedel , D , Frieman , J , García-Bellido , J , Gaztanaga , E , George , E M , Giannantonio , T , Halverson , N W , Hinton , S R , Holder , G P , Hollowood , D L , Holzapfel , W L , Honscheid , K , Hrubes , J D , James , D J , Knox , L , Kuehn , K , Lahav , O , Lee , A T , Lima , M , Luong-Van , D , March , M , McMahon , J J , Melchior , P , Menanteau , F , Meyer , S S , Miquel , R , Mocanu , L , Mohr , J J , Morgan , R , Natoli , T , Padin , S , P article 2023 ftmacquarieunicr https://doi.org/10.1103/PhysRevD.107.023529 2024-06-12T23:47:26Z Joint analyses of cross-correlations between measurements of galaxy positions, galaxy lensing, and lensing of the cosmic microwave background (CMB) offer powerful constraints on the large-scale structure of the Universe. In a forthcoming analysis, we will present cosmological constraints from the analysis of such cross-correlations measured using Year 3 data from the Dark Energy Survey (DES), and CMB data from the South Pole Telescope (SPT) and Planck. Here we present two key ingredients of this analysis: (1) an improved CMB lensing map in the SPT-SZ survey footprint and (2) the analysis methodology that will be used to extract cosmological information from the cross-correlation measurements. Relative to previous lensing maps made from the same CMB observations, we have implemented techniques to remove contamination from the thermal Sunyaev Zel'dovich effect, enabling the extraction of cosmological information from smaller angular scales of the cross-correlation measurements than in previous analyses with DES Year 1 data. We describe our model for the cross-correlations between these maps and DES data, and validate our modeling choices to demonstrate the robustness of our analysis. We then forecast the expected cosmological constraints from the galaxy survey-CMB lensing auto and cross-correlations. We find that the galaxy-CMB lensing and galaxy shear-CMB lensing correlations will on their own provide a constraint on S 8 = σ 8 √Ω m /0.3 at the few percent level, providing a powerful consistency check for the DES-only constraints. We explore scenarios where external priors on shear calibration are removed, finding that the joint analysis of CMB lensing cross-correlations can provide constraints on the shear calibration amplitude at the 5% to 10% level. Article in Journal/Newspaper South pole Macquarie University Research Portal South Pole Physical Review D 107 2 |