Consistent lensing and clustering in a low-S8Universe with BOSS, des Year 3, HSC Year 1, and KiDS-1000

A. Amon; N. C. Robertson; H. Miyatake; C. Heymans; M. White; J. Derose; S. Yuan; R. H. Wechsler; T. N. Varga; S. Bocquet; A. Dvornik; S. More; A. J. Ross; H. Hoekstra; A. Alarcon; M. Asgari; J. Blazek; A. Campos; R. Chen; A. Choi; M. Crocce; H. T. Diehl; C. Doux; K. Eckert; J. Elvin-Poole; S. Everett; A. Ferté; M. Gatti; G. Giannini; D. Gruen; R. A. Gruendl; W. G. Hartley; K. Herner; H. Hildebrandt; S. Huang; E. M. Huff; B. Joachimi; S. Lee; N. MacCrann; J. Myles; A. Navarro-Alsina; T. Nishimichi; J. Prat; L. F. Secco; I. Sevilla-Noarbe; E. Sheldon; T. Shin; T. Tröster; M. A. Troxel; I. Tutusaus; A. H. Wright; B. Yin; M. Aguena; S. Allam; J. Annis; D. Bacon; M. Bilicki; D. Brooks; D. L. Burke; A. Carnero Rosell; J. Carretero; F. J. Castander; R. Cawthon; M. Costanzi; L. N. Da Costa; M. E.S. Pereira; J. De Jong; J. De Vicente; S. Desai; J. P. Dietrich; P. Doel; I. Ferrero; J. Frieman; J. García-Bellido; D. W. Gerdes; J. Gschwend; G. Gutierrez; S. R. Hinton; D. L. Hollowood; K. Honscheid; D. Huterer; A. Kannawadi; K. Kuehn; N. Kuropatkin; O. Lahav; M. Lima; M. A.G. Maia; J. L. Marshall; F. Menanteau; R. Miquel; J. J. Mohr; R. Morgan; J. Muir; F. Paz-Chinchón; A. Pieres; A. A. Plazas Malagón; A. Porredon; M. Rodriguez-Monroy; A. Roodman; E. Sanchez; S. Serrano; H. Shan; E. Suchyta; M. E.C. Swanson; G. Tarle; D. Thomas; C. To; Y. Zhang

doi:10.1093/mnras/stac2938

Consistent lensing and clustering in a low-S₈Universe with BOSS, des Year 3, HSC Year 1, and KiDS-1000

A. Amon, N. C. Robertson, H. Miyatake, C. Heymans, M. White, J. Derose, S. Yuan, R. H. Wechsler, T. N. Varga, S. Bocquet, A. Dvornik, S. More, A. J. Ross, H. Hoekstra, A. Alarcon, M. Asgari, J. Blazek, A. Campos, R. Chen, A. ChoiM. Crocce, H. T. Diehl, C. Doux, K. Eckert, J. Elvin-Poole, S. Everett, A. Ferté, M. Gatti, G. Giannini, D. Gruen, R. A. Gruendl, W. G. Hartley, K. Herner, H. Hildebrandt, S. Huang, E. M. Huff, B. Joachimi, S. Lee, N. MacCrann, J. Myles, A. Navarro-Alsina, T. Nishimichi, J. Prat, L. F. Secco, I. Sevilla-Noarbe, E. Sheldon, T. Shin, T. Tröster, M. A. Troxel, I. Tutusaus, A. H. Wright, B. Yin, M. Aguena, S. Allam, J. Annis, D. Bacon, M. Bilicki, D. Brooks, D. L. Burke, A. Carnero Rosell, J. Carretero, F. J. Castander, R. Cawthon, M. Costanzi, L. N. Da Costa, M. E.S. Pereira, J. De Jong, J. De Vicente, S. Desai, J. P. Dietrich, P. Doel, I. Ferrero, J. Frieman, J. García-Bellido, D. W. Gerdes, J. Gschwend, G. Gutierrez, S. R. Hinton, D. L. Hollowood, K. Honscheid, D. Huterer, A. Kannawadi, K. Kuehn, N. Kuropatkin, O. Lahav, M. Lima, M. A.G. Maia, J. L. Marshall, F. Menanteau, R. Miquel, J. J. Mohr, R. Morgan, J. Muir, F. Paz-Chinchón, A. Pieres, A. A. Plazas Malagón, A. Porredon, M. Rodriguez-Monroy, A. Roodman, E. Sanchez, S. Serrano, H. Shan, E. Suchyta, M. E.C. Swanson, G. Tarle, D. Thomas, C. To, Y. Zhang

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Abstract

We evaluate the consistency between lensing and clustering based on measurements from Baryon Oscillation Spectroscopic Survey combined with galaxy-galaxy lensing from Dark Energy Survey (DES) Year 3, Hyper Suprime-Cam Subaru Strategic Program (HSC) Year 1, and Kilo-Degree Survey (KiDS)-1000. We find good agreement between these lensing data sets. We model the observations using the Dark Emulator and fit the data at two fixed cosmologies: Planck (S8 = 0.83), and a Lensing cosmology (S8 = 0.76). For a joint analysis limited to large scales, we find that both cosmologies provide an acceptable fit to the data. Full utilization of the higher signal-to-noise small-scale measurements is hindered by uncertainty in the impact of baryon feedback and assembly bias, which we account for with a reasoned theoretical error budget. We incorporate a systematic inconsistency parameter for each redshift bin, A, that decouples the lensing and clustering. With a wide range of scales, we find different results for the consistency between the two cosmologies. Limiting the analysis to the bins for which the impact of the lens sample selection is expected to be minimal, for the Lensing cosmology, the measurements are consistent with A = 1; A = 0.91 ± 0.04 (A = 0.97 ± 0.06) using DES+KiDS (HSC). For the Planck case, we find a discrepancy: A = 0.79 ± 0.03 (A = 0.84 ± 0.05) using DES+KiDS (HSC). We demonstrate that a kinematic Sunyaev-Zeldovich-based estimate for baryonic effects alleviates some of the discrepancy in the Planck cosmology. This analysis demonstrates the statistical power of small-scale measurements; however, caution is still warranted given modelling uncertainties and foreground sample selection effects.

Original language	English
Pages (from-to)	477-503
Number of pages	27
Journal	Monthly Notices of the Royal Astronomical Society
Volume	518
Issue number	1
DOIs	https://doi.org/10.1093/mnras/stac2938
State	Published - Jan 1 2023

Funding

AA acknowledges financial support from the award of a Kavli Institute Fellowship at KIPAC and at KICC. HM and TN are supported by JSPS KAKENHI Grant Number 19H00677, by Japan Science and Technology Agency (JST) CREST JPMHCR1414, and by JST AIP Network Lab Acceleration Research Grant Number JP20317829. HM is supported by JSPS KAKENHI Grant Numbers 20H01932 and 21H05456, and by JSPS Core-to-Core Program Grant Numbers JPJSCCA20200002 and JPJSCCA20210003. CH, MA, and TT acknowledge support from the European Research Council under grant number 647112. CH also acknowledges support from the Max Planck Society and the Alexander von Humboldt Foundation in the framework of the Max Planck-Humboldt Research Award endowed by the Federal Ministry of Education and Research. TN is supported in part by MEXT/JSPS KAKENHI Grant Numbers JP20H05861 and JP21H01081. MB is supported by the Polish National Science Centre through grant numbers 2020/38/E/ST9/00395, 2018/30/E/ST9/00698, 2018/31/G/ST9/03388, and 2020/39/B/ST9/03494, and by the Polish Ministry of Science and Higher Education through grant DIR/WK/2018/12. JdJ is supported by the Netherlands Organisation for Scientific Research (NWO) through grant 621.016.402. HHi is supported by a Heisenberg grant of the Deutsche Forschungsge-meinschaft (Hi 1495/5-1), and AD and AW acknowledge support from an ERC Consolidator Grant (No. 770935). HHo acknowledges support from Vici grant 639.043.512, financed by the Netherlands Organisation for Scientific Research (NWO). HYS acknowledges the support from CMS-CSST-2021-A01 and CMS-CSST-2021-B01, NSFC of China under grant 11973070, the Shanghai Committee of Science and Technology grant No. 19ZR1466600, and Key Research Program of Frontier Science, Chinese Academy of Sciences, Grant No. ZDBS-LY-7013. TT acknowledges support from the Leverhulme Trust. Funding for the DES Projects has been provided by the U.S. Department of Energy, the U.S. National Science Foundation, the Ministry of Science and Education of Spain, the Science and Technology Facilities Council of the United Kingdom, the Higher Education Funding Council for England, the National Center for Supercomputing Applications at the University of Illinois at Urbana-Champaign, the Kavli Institute of Cosmological Physics at the University of Chicago, the Center for Cosmology and Astro-Particle Physics at the Ohio State University, the Mitchell Institute for Fundamental Physics and Astronomy at Te xas A&M Univ ersity, Financiadora de Estudos e Projetos, Funda\u00E7\u00E3o Carlos Chagas Filho de Amparo \u00E0 Pesquisa do Estado do Rio de Janeiro, Conselho Nacional de Desenvolvimento Cient\u00EDfico e Tecnol\u00F3gico and the Minist\u00E9rio da Ci\u00EAncia, Tecnologiae Inova\u00E7\u00E3o, the Deutsche Forschungsgemeinschaft, and the collaborating institutions in the Dark Energy Survey. The DES data management system is supported by the National Science Foundation under Grant Numbers AST-1138766 and AST-1536171. The DES participants from Spanish institutions are partially supported by MICINN under grants ESP2017-89838, PGC2018-094773, PGC2018-102021, SEV-2016-0588, SEV-2016-0597, and MDM-2015-0509, some of which include ERDF funds from the European Union. IFAE is partially funded by the CERCA program of the Generalitat de Catalunya. Research leading to these results has received funding from the European Research Council under the European Union's Seventh Frame work Program (FP7/2007-2013) including ERC grant agreements 240672, 291329, and 306478. We acknowledge support from the Brazilian Instituto Nacional de Ci\u00EAncia e Tecnologia (INCT) do Universo Online (CNPq grant 465376/2014-2). This manuscript has been authored by Fermi Research Alliance, LLC under Contract No. DE-AC02-07CH11359 with the U.S. Department of Energy, Office of Science, Office of High Energy Physics.

Funders	Funder number
Kavli Institute
Brazilian Instituto Nacional de Ciência e Tecnologia
High Energy Physics
KIPAC
Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro
Leverhulme Trust
Ohio State University
University of Chicago
Generalitat de Catalunya
Higher Education Funding Council for England
Financiadora de Estudos e Projetos
Tecnologiae Inovação
Max-Planck-Gesellschaft
Bundesministerium für Bildung und Forschung
Ministry of Education and Science of Ukraine
European Commission
Instituto Nacional de Ciência e Tecnologia para Excitotoxicidade e Neuroproteção
European Union's Seventh Frame work Program
U.S. Department of Energy
Mitchell Institute for Fundamental Physics and Astronomy at Te xas A&M Univ ersity
Science and Technology Facilities Council of the United Kingdom
Ministério da Ciência
Office of Science
National Centre for Supercomputing Applications
European Regional Development Fund
Alexander von Humboldt-Stiftung
Key Research Program of Frontier Science, Chinese Academy of Sciences	ZDBS-LY-7013
Key Research Program of Frontier Science, Chinese Academy of Sciences
Narodowe Centrum Nauki	2020/39/B/ST9/03494, 2018/30/E/ST9/00698, 2020/38/E/ST9/00395, 2018/31/G/ST9/03388
Narodowe Centrum Nauki
Ministry of Education, Culture, Sports, Science and Technology	JP21H01081, JP20H05861
Ministry of Education, Culture, Sports, Science and Technology
Ministerio de Ciencia e Innovación	SEV-2016-0588, SEV-2016-0597, MDM-2015-0509, PGC2018-094773, PGC2018-102021, ESP2017-89838
Ministerio de Ciencia e Innovación
Fermi Research Alliance, LLC	DE-AC02-07CH11359
Seventh Framework Programme	240672, 306478, 291329
Seventh Framework Programme
Deutsche Forschungsgemeinschaft	Hi 1495/5-1
Deutsche Forschungsgemeinschaft
Nederlandse Organisatie voor Wetenschappelijk Onderzoek	621.016.402
Nederlandse Organisatie voor Wetenschappelijk Onderzoek
Japan Science and Technology Agency	CREST JPMHCR1414
Japan Science and Technology Agency
Ministerstwo Edukacji i Nauki	DIR/WK/2018/12
Ministerstwo Edukacji i Nauki
European Research Council	CMS-CSST-2021-A01, CMS-CSST-2021-B01, 639.043.512
European Research Council
National Natural Science Foundation of China	11973070
National Natural Science Foundation of China
Science and Technology Commission of Shanghai Municipality	19ZR1466600
Science and Technology Commission of Shanghai Municipality
Conselho Nacional de Desenvolvimento Científico e Tecnológico	465376/2014-2
Conselho Nacional de Desenvolvimento Científico e Tecnológico
Japan Society for the Promotion of Science	20H01932
Japan Society for the Promotion of Science
Horizon 2020 Framework Programme	770935, 647112
Horizon 2020 Framework Programme
JST AIP Network Lab Acceleration Research	21H05456, JPJSCCA20200002, JPJSCCA20210003, JP20317829
National Science Foundation	AST-1138766, AST-1536171
National Science Foundation
Japan Society for the Promotion of Science London	19H00677
Japan Society for the Promotion of Science London

Keywords

cosmology: observations
gravitational lensing: weak
large-scale structure of Universe

Access to Document

10.1093/mnras/stac2938

Cite this

Amon, A., Robertson, N. C., Miyatake, H., Heymans, C., White, M., Derose, J., Yuan, S., Wechsler, R. H., Varga, T. N., Bocquet, S., Dvornik, A., More, S., Ross, A. J., Hoekstra, H., Alarcon, A., Asgari, M., Blazek, J., Campos, A., Chen, R., ... Zhang, Y. (2023). Consistent lensing and clustering in a low-S₈Universe with BOSS, des Year 3, HSC Year 1, and KiDS-1000. Monthly Notices of the Royal Astronomical Society, 518(1), 477-503. https://doi.org/10.1093/mnras/stac2938

@article{db48720b4fd741e795f4fc9f44fdf5d1,

title = "Consistent lensing and clustering in a low-S8Universe with BOSS, des Year 3, HSC Year 1, and KiDS-1000",

abstract = "We evaluate the consistency between lensing and clustering based on measurements from Baryon Oscillation Spectroscopic Survey combined with galaxy-galaxy lensing from Dark Energy Survey (DES) Year 3, Hyper Suprime-Cam Subaru Strategic Program (HSC) Year 1, and Kilo-Degree Survey (KiDS)-1000. We find good agreement between these lensing data sets. We model the observations using the Dark Emulator and fit the data at two fixed cosmologies: Planck (S8 = 0.83), and a Lensing cosmology (S8 = 0.76). For a joint analysis limited to large scales, we find that both cosmologies provide an acceptable fit to the data. Full utilization of the higher signal-to-noise small-scale measurements is hindered by uncertainty in the impact of baryon feedback and assembly bias, which we account for with a reasoned theoretical error budget. We incorporate a systematic inconsistency parameter for each redshift bin, A, that decouples the lensing and clustering. With a wide range of scales, we find different results for the consistency between the two cosmologies. Limiting the analysis to the bins for which the impact of the lens sample selection is expected to be minimal, for the Lensing cosmology, the measurements are consistent with A = 1; A = 0.91 ± 0.04 (A = 0.97 ± 0.06) using DES+KiDS (HSC). For the Planck case, we find a discrepancy: A = 0.79 ± 0.03 (A = 0.84 ± 0.05) using DES+KiDS (HSC). We demonstrate that a kinematic Sunyaev-Zeldovich-based estimate for baryonic effects alleviates some of the discrepancy in the Planck cosmology. This analysis demonstrates the statistical power of small-scale measurements; however, caution is still warranted given modelling uncertainties and foreground sample selection effects.",

keywords = "cosmology: observations, gravitational lensing: weak, large-scale structure of Universe",

author = "A. Amon and Robertson, {N. C.} and H. Miyatake and C. Heymans and M. White and J. Derose and S. Yuan and Wechsler, {R. H.} and Varga, {T. N.} and S. Bocquet and A. Dvornik and S. More and Ross, {A. J.} and H. Hoekstra and A. Alarcon and M. Asgari and J. Blazek and A. Campos and R. Chen and A. Choi and M. Crocce and Diehl, {H. T.} and C. Doux and K. Eckert and J. Elvin-Poole and S. Everett and A. Fert{\'e} and M. Gatti and G. Giannini and D. Gruen and Gruendl, {R. A.} and Hartley, {W. G.} and K. Herner and H. Hildebrandt and S. Huang and Huff, {E. M.} and B. Joachimi and S. Lee and N. MacCrann and J. Myles and A. Navarro-Alsina and T. Nishimichi and J. Prat and Secco, {L. F.} and I. Sevilla-Noarbe and E. Sheldon and T. Shin and T. Tr{\"o}ster and Troxel, {M. A.} and I. Tutusaus and Wright, {A. H.} and B. Yin and M. Aguena and S. Allam and J. Annis and D. Bacon and M. Bilicki and D. Brooks and Burke, {D. L.} and {Carnero Rosell}, A. and J. Carretero and Castander, {F. J.} and R. Cawthon and M. Costanzi and {Da Costa}, {L. N.} and Pereira, {M. E.S.} and {De Jong}, J. and {De Vicente}, J. and S. Desai and Dietrich, {J. P.} and P. Doel and I. Ferrero and J. Frieman and J. Garc{\'i}a-Bellido and Gerdes, {D. W.} and J. Gschwend and G. Gutierrez and Hinton, {S. R.} and Hollowood, {D. L.} and K. Honscheid and D. Huterer and A. Kannawadi and K. Kuehn and N. Kuropatkin and O. Lahav and M. Lima and Maia, {M. A.G.} and Marshall, {J. L.} and F. Menanteau and R. Miquel and Mohr, {J. J.} and R. Morgan and J. Muir and F. Paz-Chinch{\'o}n and A. Pieres and {Plazas Malag{\'o}n}, {A. A.} and A. Porredon and M. Rodriguez-Monroy and A. Roodman and E. Sanchez and S. Serrano and H. Shan and E. Suchyta and Swanson, {M. E.C.} and G. Tarle and D. Thomas and C. To and Y. Zhang",

note = "Publisher Copyright: {\textcopyright} 2022 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society.",

year = "2023",

month = jan,

day = "1",

doi = "10.1093/mnras/stac2938",

language = "English",

volume = "518",

pages = "477--503",

journal = "Monthly Notices of the Royal Astronomical Society",

issn = "0035-8711",

publisher = "Oxford University Press",

number = "1",

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Amon, A, Robertson, NC, Miyatake, H, Heymans, C, White, M, Derose, J, Yuan, S, Wechsler, RH, Varga, TN, Bocquet, S, Dvornik, A, More, S, Ross, AJ, Hoekstra, H, Alarcon, A, Asgari, M, Blazek, J, Campos, A, Chen, R, Choi, A, Crocce, M, Diehl, HT, Doux, C, Eckert, K, Elvin-Poole, J, Everett, S, Ferté, A, Gatti, M, Giannini, G, Gruen, D, Gruendl, RA, Hartley, WG, Herner, K, Hildebrandt, H, Huang, S, Huff, EM, Joachimi, B, Lee, S, MacCrann, N, Myles, J, Navarro-Alsina, A, Nishimichi, T, Prat, J, Secco, LF, Sevilla-Noarbe, I, Sheldon, E, Shin, T, Tröster, T, Troxel, MA, Tutusaus, I, Wright, AH, Yin, B, Aguena, M, Allam, S, Annis, J, Bacon, D, Bilicki, M, Brooks, D, Burke, DL, Carnero Rosell, A, Carretero, J, Castander, FJ, Cawthon, R, Costanzi, M, Da Costa, LN, Pereira, MES, De Jong, J, De Vicente, J, Desai, S, Dietrich, JP, Doel, P, Ferrero, I, Frieman, J, García-Bellido, J, Gerdes, DW, Gschwend, J, Gutierrez, G, Hinton, SR, Hollowood, DL, Honscheid, K, Huterer, D, Kannawadi, A, Kuehn, K, Kuropatkin, N, Lahav, O, Lima, M, Maia, MAG, Marshall, JL, Menanteau, F, Miquel, R, Mohr, JJ, Morgan, R, Muir, J, Paz-Chinchón, F, Pieres, A, Plazas Malagón, AA, Porredon, A, Rodriguez-Monroy, M, Roodman, A, Sanchez, E, Serrano, S, Shan, H, Suchyta, E, Swanson, MEC, Tarle, G, Thomas, D, To, C & Zhang, Y 2023, 'Consistent lensing and clustering in a low-S₈Universe with BOSS, des Year 3, HSC Year 1, and KiDS-1000', Monthly Notices of the Royal Astronomical Society, vol. 518, no. 1, pp. 477-503. https://doi.org/10.1093/mnras/stac2938

TY - JOUR

T1 - Consistent lensing and clustering in a low-S8Universe with BOSS, des Year 3, HSC Year 1, and KiDS-1000

AU - Amon, A.

AU - Robertson, N. C.

AU - Miyatake, H.

AU - Heymans, C.

AU - White, M.

AU - Derose, J.

AU - Yuan, S.

AU - Wechsler, R. H.

AU - Varga, T. N.

AU - Bocquet, S.

AU - Dvornik, A.

AU - More, S.

AU - Ross, A. J.

AU - Hoekstra, H.

AU - Alarcon, A.

AU - Asgari, M.

AU - Blazek, J.

AU - Campos, A.

AU - Chen, R.

AU - Choi, A.

AU - Crocce, M.

AU - Diehl, H. T.

AU - Doux, C.

AU - Eckert, K.

AU - Elvin-Poole, J.

AU - Everett, S.

AU - Ferté, A.

AU - Gatti, M.

AU - Giannini, G.

AU - Gruen, D.

AU - Gruendl, R. A.

AU - Hartley, W. G.

AU - Herner, K.

AU - Hildebrandt, H.

AU - Huang, S.

AU - Huff, E. M.

AU - Joachimi, B.

AU - Lee, S.

AU - MacCrann, N.

AU - Myles, J.

AU - Navarro-Alsina, A.

AU - Nishimichi, T.

AU - Prat, J.

AU - Secco, L. F.

AU - Sevilla-Noarbe, I.

AU - Sheldon, E.

AU - Shin, T.

AU - Tröster, T.

AU - Troxel, M. A.

AU - Tutusaus, I.

AU - Wright, A. H.

AU - Yin, B.

AU - Aguena, M.

AU - Allam, S.

AU - Annis, J.

AU - Bacon, D.

AU - Bilicki, M.

AU - Brooks, D.

AU - Burke, D. L.

AU - Carnero Rosell, A.

AU - Carretero, J.

AU - Castander, F. J.

AU - Cawthon, R.

AU - Costanzi, M.

AU - Da Costa, L. N.

AU - Pereira, M. E.S.

AU - De Jong, J.

AU - De Vicente, J.

AU - Desai, S.

AU - Dietrich, J. P.

AU - Doel, P.

AU - Ferrero, I.

AU - Frieman, J.

AU - García-Bellido, J.

AU - Gerdes, D. W.

AU - Gschwend, J.

AU - Gutierrez, G.

AU - Hinton, S. R.

AU - Hollowood, D. L.

AU - Honscheid, K.

AU - Huterer, D.

AU - Kannawadi, A.

AU - Kuehn, K.

AU - Kuropatkin, N.

AU - Lahav, O.

AU - Lima, M.

AU - Maia, M. A.G.

AU - Marshall, J. L.

AU - Menanteau, F.

AU - Miquel, R.

AU - Mohr, J. J.

AU - Morgan, R.

AU - Muir, J.

AU - Paz-Chinchón, F.

AU - Pieres, A.

AU - Plazas Malagón, A. A.

AU - Porredon, A.

AU - Rodriguez-Monroy, M.

AU - Roodman, A.

AU - Sanchez, E.

AU - Serrano, S.

AU - Shan, H.

AU - Suchyta, E.

AU - Swanson, M. E.C.

AU - Tarle, G.

AU - Thomas, D.

AU - To, C.

AU - Zhang, Y.

PY - 2023/1/1

Y1 - 2023/1/1

N2 - We evaluate the consistency between lensing and clustering based on measurements from Baryon Oscillation Spectroscopic Survey combined with galaxy-galaxy lensing from Dark Energy Survey (DES) Year 3, Hyper Suprime-Cam Subaru Strategic Program (HSC) Year 1, and Kilo-Degree Survey (KiDS)-1000. We find good agreement between these lensing data sets. We model the observations using the Dark Emulator and fit the data at two fixed cosmologies: Planck (S8 = 0.83), and a Lensing cosmology (S8 = 0.76). For a joint analysis limited to large scales, we find that both cosmologies provide an acceptable fit to the data. Full utilization of the higher signal-to-noise small-scale measurements is hindered by uncertainty in the impact of baryon feedback and assembly bias, which we account for with a reasoned theoretical error budget. We incorporate a systematic inconsistency parameter for each redshift bin, A, that decouples the lensing and clustering. With a wide range of scales, we find different results for the consistency between the two cosmologies. Limiting the analysis to the bins for which the impact of the lens sample selection is expected to be minimal, for the Lensing cosmology, the measurements are consistent with A = 1; A = 0.91 ± 0.04 (A = 0.97 ± 0.06) using DES+KiDS (HSC). For the Planck case, we find a discrepancy: A = 0.79 ± 0.03 (A = 0.84 ± 0.05) using DES+KiDS (HSC). We demonstrate that a kinematic Sunyaev-Zeldovich-based estimate for baryonic effects alleviates some of the discrepancy in the Planck cosmology. This analysis demonstrates the statistical power of small-scale measurements; however, caution is still warranted given modelling uncertainties and foreground sample selection effects.

AB - We evaluate the consistency between lensing and clustering based on measurements from Baryon Oscillation Spectroscopic Survey combined with galaxy-galaxy lensing from Dark Energy Survey (DES) Year 3, Hyper Suprime-Cam Subaru Strategic Program (HSC) Year 1, and Kilo-Degree Survey (KiDS)-1000. We find good agreement between these lensing data sets. We model the observations using the Dark Emulator and fit the data at two fixed cosmologies: Planck (S8 = 0.83), and a Lensing cosmology (S8 = 0.76). For a joint analysis limited to large scales, we find that both cosmologies provide an acceptable fit to the data. Full utilization of the higher signal-to-noise small-scale measurements is hindered by uncertainty in the impact of baryon feedback and assembly bias, which we account for with a reasoned theoretical error budget. We incorporate a systematic inconsistency parameter for each redshift bin, A, that decouples the lensing and clustering. With a wide range of scales, we find different results for the consistency between the two cosmologies. Limiting the analysis to the bins for which the impact of the lens sample selection is expected to be minimal, for the Lensing cosmology, the measurements are consistent with A = 1; A = 0.91 ± 0.04 (A = 0.97 ± 0.06) using DES+KiDS (HSC). For the Planck case, we find a discrepancy: A = 0.79 ± 0.03 (A = 0.84 ± 0.05) using DES+KiDS (HSC). We demonstrate that a kinematic Sunyaev-Zeldovich-based estimate for baryonic effects alleviates some of the discrepancy in the Planck cosmology. This analysis demonstrates the statistical power of small-scale measurements; however, caution is still warranted given modelling uncertainties and foreground sample selection effects.

KW - cosmology: observations

KW - gravitational lensing: weak

KW - large-scale structure of Universe

UR - http://www.scopus.com/inward/record.url?scp=85145928509&partnerID=8YFLogxK

U2 - 10.1093/mnras/stac2938

DO - 10.1093/mnras/stac2938

M3 - Article

AN - SCOPUS:85145928509

SN - 0035-8711

VL - 518

SP - 477

EP - 503

JO - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

IS - 1

ER -