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Title: Dark Energy Survey Year 1 Results: Cosmological Constraints from Cluster Abundances, Weak Lensing, and Galaxy Correlations

Abstract

We present the first joint analysis of cluster abundances and auto or cross-correlations of three cosmic tracer fields: galaxy density, weak gravitational lensing shear, and cluster density split by optical richness. From a joint analysis (4×2pt+N) of cluster abundances, three cluster cross-correlations, and the auto correlations of the galaxy density measured from the first year data of the Dark Energy Survey, we obtain Ωm=$$0.305^{+0.055}_{-0.038}$$ and σ8=$$0.783^{+0.064}_{-0.054}$$. This result is consistent with constraints from the DES-Y1 galaxy clustering and weak lensing two-point correlation functions for the flat νΛCDM model. Consequently, we combine cluster abundances and all two-point correlations from across all three cosmic tracer fields (6×2pt+N) and find improved constraints on cosmological parameters as well as on the cluster observable-mass scaling relation. This analysis is an important advance in both optical cluster cosmology and multiprobe analyses of upcoming wide imaging surveys.

Authors:
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Publication Date:
Research Org.:
Oak Ridge National Lab. (ORNL), Oak Ridge, TN (United States); SLAC National Accelerator Lab., Menlo Park, CA (United States); Argonne National Lab. (ANL), Argonne, IL (United States); Univ. of Michigan, Ann Arbor, MI (United States)
Sponsoring Org.:
USDOE Office of Science (SC), Advanced Scientific Computing Research (ASCR); National Science Foundation (NSF)
Contributing Org.:
DES Collaboration
OSTI Identifier:
1807206
Alternate Identifier(s):
OSTI ID: 1810564; OSTI ID: 1839686; OSTI ID: 1872399
Grant/Contract Number:  
AC05-00OR22725; AC02-06CH11357; SC0020247; AC02-76SF00515; SC0009913; SC0015975; 465376/2014-2; SEV-2016-0588; SEV-2016-0597; MDM-2015-0509; PGC2018-094773; PGC2018-102021; ESP2017-89838; AST-1536171; AST-1138766; AST-1516997; 291329; 240672; 306478; AC02-07CH11359; SC0019193
Resource Type:
Accepted Manuscript
Journal Name:
Physical Review Letters
Additional Journal Information:
Journal Volume: 126; Journal Issue: 14; Journal ID: ISSN 0031-9007
Publisher:
American Physical Society (APS)
Country of Publication:
United States
Language:
English
Subject:
79 ASTRONOMY AND ASTROPHYSICS; Cosmological parameters; Cosmology; Dark energy; Dark matter; Galaxy cluster count; Large-scale structure of the universe

Citation Formats

To, C., Krause, E., Rozo, E., Wu, H., Gruen, D., Wechsler, R.  H., Eifler, T.  F., Rykoff, E.  S., Costanzi, M., Becker, M.  R., Bernstein, G.  M., Blazek, J., Bocquet, S., Bridle, S.  L., Cawthon, R., Choi, A., Crocce, M., Davis, C., DeRose, J., Drlica-Wagner, A., Elvin-Poole, J., Fang, X., Farahi, A., Friedrich, O., Gatti, M., Gaztanaga, E., Giannantonio, T., Hartley, W.  G., Hoyle, B., Jarvis, M., MacCrann, N., McClintock, T., Miranda, V., Pereira, M.  E. S., Park, Y., Porredon, A., Prat, J., Rau, M.  M., Ross, A.  J., Samuroff, S., Sánchez, C., Sevilla-Noarbe, I., Sheldon, E., Troxel, M.  A., Varga, T.  N., Vielzeuf, P., Zhang, Y., Zuntz, J., Abbott, T.  M. C., Aguena, M., Amon, A., Annis, J., Avila, S., Bertin, E., Bhargava, S., Brooks, D., Burke, D.  L., Carnero Rosell, A., Carrasco Kind, M., Carretero, J., Chang, C., Conselice, C., da Costa, L.  N., Davis, T.  M., Desai, S., Diehl, H.  T., Dietrich, J.  P., Everett, S., Evrard, A.  E., Ferrero, I., Flaugher, B., Fosalba, P., Frieman, J., García-Bellido, J., Gruendl, R.  A., Gutierrez, G., Hinton, S.  R., Hollowood, D.  L., Honscheid, K., Huterer, D., James, D.  J., Jeltema, T., Kron, R., Kuehn, K., Kuropatkin, N., Lima, M., Maia, M.  A. G., Marshall, J.  L., Menanteau, F., Miquel, R., Morgan, R., Muir, J., Myles, J., Palmese, A., Paz-Chinchón, F., Plazas, A.  A., Romer, A.  K., Roodman, A., Sanchez, E., Santiago, B., Scarpine, V., Serrano, S., Smith, M., Suchyta, E., Swanson, M.  E. C., Tarle, G., Thomas, D., Tucker, D.  L., Weller, J., Wester, W., and Wilkinson, R.  D. Dark Energy Survey Year 1 Results: Cosmological Constraints from Cluster Abundances, Weak Lensing, and Galaxy Correlations. United States: N. p., 2021. Web. doi:10.1103/physrevlett.126.141301.
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To, C., Krause, E., Rozo, E., Wu, H., Gruen, D., Wechsler, R.  H., Eifler, T.  F., Rykoff, E.  S., Costanzi, M., Becker, M.  R., Bernstein, G.  M., Blazek, J., Bocquet, S., Bridle, S.  L., Cawthon, R., Choi, A., Crocce, M., Davis, C., DeRose, J., Drlica-Wagner, A., Elvin-Poole, J., Fang, X., Farahi, A., Friedrich, O., Gatti, M., Gaztanaga, E., Giannantonio, T., Hartley, W.  G., Hoyle, B., Jarvis, M., MacCrann, N., McClintock, T., Miranda, V., Pereira, M.  E. S., Park, Y., Porredon, A., Prat, J., Rau, M.  M., Ross, A.  J., Samuroff, S., Sánchez, C., Sevilla-Noarbe, I., Sheldon, E., Troxel, M.  A., Varga, T.  N., Vielzeuf, P., Zhang, Y., Zuntz, J., Abbott, T.  M. C., Aguena, M., Amon, A., Annis, J., Avila, S., Bertin, E., Bhargava, S., Brooks, D., Burke, D.  L., Carnero Rosell, A., Carrasco Kind, M., Carretero, J., Chang, C., Conselice, C., da Costa, L.  N., Davis, T.  M., Desai, S., Diehl, H.  T., Dietrich, J.  P., Everett, S., Evrard, A.  E., Ferrero, I., Flaugher, B., Fosalba, P., Frieman, J., García-Bellido, J., Gruendl, R.  A., Gutierrez, G., Hinton, S.  R., Hollowood, D.  L., Honscheid, K., Huterer, D., James, D.  J., Jeltema, T., Kron, R., Kuehn, K., Kuropatkin, N., Lima, M., Maia, M.  A. G., Marshall, J.  L., Menanteau, F., Miquel, R., Morgan, R., Muir, J., Myles, J., Palmese, A., Paz-Chinchón, F., Plazas, A.  A., Romer, A.  K., Roodman, A., Sanchez, E., Santiago, B., Scarpine, V., Serrano, S., Smith, M., Suchyta, E., Swanson, M.  E. C., Tarle, G., Thomas, D., Tucker, D.  L., Weller, J., Wester, W., & Wilkinson, R.  D. Dark Energy Survey Year 1 Results: Cosmological Constraints from Cluster Abundances, Weak Lensing, and Galaxy Correlations. United States. https://doi.org/10.1103/physrevlett.126.141301
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To, C., Krause, E., Rozo, E., Wu, H., Gruen, D., Wechsler, R.  H., Eifler, T.  F., Rykoff, E.  S., Costanzi, M., Becker, M.  R., Bernstein, G.  M., Blazek, J., Bocquet, S., Bridle, S.  L., Cawthon, R., Choi, A., Crocce, M., Davis, C., DeRose, J., Drlica-Wagner, A., Elvin-Poole, J., Fang, X., Farahi, A., Friedrich, O., Gatti, M., Gaztanaga, E., Giannantonio, T., Hartley, W.  G., Hoyle, B., Jarvis, M., MacCrann, N., McClintock, T., Miranda, V., Pereira, M.  E. S., Park, Y., Porredon, A., Prat, J., Rau, M.  M., Ross, A.  J., Samuroff, S., Sánchez, C., Sevilla-Noarbe, I., Sheldon, E., Troxel, M.  A., Varga, T.  N., Vielzeuf, P., Zhang, Y., Zuntz, J., Abbott, T.  M. C., Aguena, M., Amon, A., Annis, J., Avila, S., Bertin, E., Bhargava, S., Brooks, D., Burke, D.  L., Carnero Rosell, A., Carrasco Kind, M., Carretero, J., Chang, C., Conselice, C., da Costa, L.  N., Davis, T.  M., Desai, S., Diehl, H.  T., Dietrich, J.  P., Everett, S., Evrard, A.  E., Ferrero, I., Flaugher, B., Fosalba, P., Frieman, J., García-Bellido, J., Gruendl, R.  A., Gutierrez, G., Hinton, S.  R., Hollowood, D.  L., Honscheid, K., Huterer, D., James, D.  J., Jeltema, T., Kron, R., Kuehn, K., Kuropatkin, N., Lima, M., Maia, M.  A. G., Marshall, J.  L., Menanteau, F., Miquel, R., Morgan, R., Muir, J., Myles, J., Palmese, A., Paz-Chinchón, F., Plazas, A.  A., Romer, A.  K., Roodman, A., Sanchez, E., Santiago, B., Scarpine, V., Serrano, S., Smith, M., Suchyta, E., Swanson, M.  E. C., Tarle, G., Thomas, D., Tucker, D.  L., Weller, J., Wester, W., and Wilkinson, R.  D. Tue . "Dark Energy Survey Year 1 Results: Cosmological Constraints from Cluster Abundances, Weak Lensing, and Galaxy Correlations". United States. https://doi.org/10.1103/physrevlett.126.141301. https://www.osti.gov/servlets/purl/1807206.
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@article{osti_1807206,
title = {Dark Energy Survey Year 1 Results: Cosmological Constraints from Cluster Abundances, Weak Lensing, and Galaxy Correlations},
author = {To, C. and Krause, E. and Rozo, E. and Wu, H. and Gruen, D. and Wechsler, R.  H. and Eifler, T.  F. and Rykoff, E.  S. and Costanzi, M. and Becker, M.  R. and Bernstein, G.  M. and Blazek, J. and Bocquet, S. and Bridle, S.  L. and Cawthon, R. and Choi, A. and Crocce, M. and Davis, C. and DeRose, J. and Drlica-Wagner, A. and Elvin-Poole, J. and Fang, X. and Farahi, A. and Friedrich, O. and Gatti, M. and Gaztanaga, E. and Giannantonio, T. and Hartley, W.  G. and Hoyle, B. and Jarvis, M. and MacCrann, N. and McClintock, T. and Miranda, V. and Pereira, M.  E. S. and Park, Y. and Porredon, A. and Prat, J. and Rau, M.  M. and Ross, A.  J. and Samuroff, S. and Sánchez, C. and Sevilla-Noarbe, I. and Sheldon, E. and Troxel, M.  A. and Varga, T.  N. and Vielzeuf, P. and Zhang, Y. and Zuntz, J. and Abbott, T.  M. C. and Aguena, M. and Amon, A. and Annis, J. and Avila, S. and Bertin, E. and Bhargava, S. and Brooks, D. and Burke, D.  L. and Carnero Rosell, A. and Carrasco Kind, M. and Carretero, J. and Chang, C. and Conselice, C. and da Costa, L.  N. and Davis, T.  M. and Desai, S. and Diehl, H.  T. and Dietrich, J.  P. and Everett, S. and Evrard, A.  E. and Ferrero, I. and Flaugher, B. and Fosalba, P. and Frieman, J. and García-Bellido, J. and Gruendl, R.  A. and Gutierrez, G. and Hinton, S.  R. and Hollowood, D.  L. and Honscheid, K. and Huterer, D. and James, D.  J. and Jeltema, T. and Kron, R. and Kuehn, K. and Kuropatkin, N. and Lima, M. and Maia, M.  A. G. and Marshall, J.  L. and Menanteau, F. and Miquel, R. and Morgan, R. and Muir, J. and Myles, J. and Palmese, A. and Paz-Chinchón, F. and Plazas, A.  A. and Romer, A.  K. and Roodman, A. and Sanchez, E. and Santiago, B. and Scarpine, V. and Serrano, S. and Smith, M. and Suchyta, E. and Swanson, M.  E. C. and Tarle, G. and Thomas, D. and Tucker, D.  L. and Weller, J. and Wester, W. and Wilkinson, R.  D.},
abstractNote = {We present the first joint analysis of cluster abundances and auto or cross-correlations of three cosmic tracer fields: galaxy density, weak gravitational lensing shear, and cluster density split by optical richness. From a joint analysis (4×2pt+N) of cluster abundances, three cluster cross-correlations, and the auto correlations of the galaxy density measured from the first year data of the Dark Energy Survey, we obtain Ωm=$0.305^{+0.055}_{-0.038}$ and σ8=$0.783^{+0.064}_{-0.054}$. This result is consistent with constraints from the DES-Y1 galaxy clustering and weak lensing two-point correlation functions for the flat νΛCDM model. Consequently, we combine cluster abundances and all two-point correlations from across all three cosmic tracer fields (6×2pt+N) and find improved constraints on cosmological parameters as well as on the cluster observable-mass scaling relation. This analysis is an important advance in both optical cluster cosmology and multiprobe analyses of upcoming wide imaging surveys.},
doi = {10.1103/physrevlett.126.141301},
journal = {Physical Review Letters},
number = 14,
volume = 126,
place = {United States},
year = {Tue Apr 06 00:00:00 EDT 2021},
month = {Tue Apr 06 00:00:00 EDT 2021}
}
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