KiDS-450 + 2dFLenS: Cosmological parameter constraints from weak gravitational lensing tomography and overlapping redshift-space galaxy clustering
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We perform a combined analysis of cosmic shear tomography, galaxy-galaxy lensing tomography, and redshift-space multipole power spectra (monopole and quadrupole) using 450 deg 2 of imaging data by the Kilo Degree Survey (KiDS-450) overlapping with two spectroscopic surveys: the 2-degree Field Lensing Survey (2dFLenS) and the Baryon Oscillation Spectroscopic Survey (BOSS).We restrict the galaxy-galaxy lensing and multipole power spectrum measurements to the overlapping regions with KiDS, and self-consistently compute the full covariance between the different observables using a large suite of N-body simulations.We methodically analyse different combinations of the observables, finding that the galaxy-galaxy lensing measurements are particularly useful in improving the constraint on the intrinsic alignment amplitude, while the multipole power spectra are useful in tightening the constraints along the lensing degeneracy direction.The fully combined constraint on S 8 ≡ σ 8 √ m /0.3 = 0.742 ± 0.035, which is an improvement by 20 per cent compared to KiDS alone, corresponds to a 2.6σ discordance with Planck, and is not significantly affected by fitting to a more conservative set of scales.Given the tightening of the parameter space, we are unable to resolve the discordance with an extended cosmology that is simultaneously favoured in a model selection sense, including the sum of neutrino masses, curvature, evolving dark energy and modified gravity.The complementarity of our observables allows for constraints on modified gravity degrees of freedom that are not simultaneously bounded with either probe alone, and up to a factor of three improvement in the S 8 constraint in the extended cosmology compared to KiDS alone.
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Joudaki et al. (2018) found that tightening constraints made the tension between large-scale constraints and Planck at the 2.6 sigma level.
“However, this tightening of constraints also made the tension between large-scale constraints and Planck at the 2.6 level.”
From Testing general relativity in cosmology (2019) · cites this paper as Joudaki et al. (2018)
Section 5.5 (page unavailable) reports that combining probes nearly halved the uncertainty in the large-scale constraint, but gives its discordance with Planck as 3.0σ, not 2.6σ. The 2.6σ value appears for the fiducial analysis in Table 5 and Section 6.1.2 (pages unavailable). (LLM, conf=0.88)
Experimental — accuracy not yet measuredFor the WL RSD combined analysis, Joudaki et al. (2018) find Sigma_2 and mu_2 values, while for KiDS only in Joudaki et al. (2017) Sigma_2 is constrained and mu_2 is unconstrained within its prior range; these and all other constraints on the six other modified gravity parameters are consistent with the GR values of unity.
“For this WL RSD combined analysis, they find and , while for KiDS only in Joudaki et al. (2017) and unconstrained within its prior range. These and all other constraints on the six other modified gravity parameters are all consistent with the GR values of unity.”
From Testing general relativity in cosmology (2019) · cites this paper as Joudaki et al. (2018)
Split into 2 atoms — 1 confirmed, 1 partially supported, 0 disputed, 0 misattributed, 0 unverifiable. Expand the claim to see per-atom verdicts.
Experimental — accuracy not yet measuredJoudaki et al. (2018) found that models with MG parameters could resolve the discordance in the linear/large-scale case but are not favored by model selection, and the same result stands for extended models with massive neutrinos, curvature or evolving dark energy.
“They found that models with MG parameters could resolve the discordance in the linear/large-scale case, but are not favored by model selection. The same result stands for extended models with massive neutrinos, curvature or evolving dark energy.”
From Testing general relativity in cosmology (2019) · cites this paper as Joudaki et al. (2018)
Sections 6.5.4 and 6.5.7 report that the large-scale modified-gravity analysis is concordant with Planck but not favored by model selection; the concordance is largely due to diminished constraining power. The Conclusions (§7) say that none of the extended models are both favored and able to resolve the discordance. They do not establish that the neutrino-mass, curvature, and evolving-dark-energy models share the large-scale modified-gravity result of resolving it. (LLM, conf=0.86)
Experimental — accuracy not yet measuredJoint analysis of shear-shear, galaxy-shear, and galaxy-galaxy correlation functions has become standard in analyses of precursor data sets.
“The joint analysis of shear -shear, galaxy -shear, and galaxy -galaxy correlation functions has become standard in analyses of precursor data sets ( e.g., DES Collaboration et al. 2018; Joudaki et al. 2018 ) .”
From LSST: From Science Drivers to Reference Design and Anticipated Data Products (2019) · cites this paper as Joudaki et al. 2018
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Constraints on intrinsic alignment contamination of weak lensing surveys using the MegaZ-LRG sample
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Joachimi, B., & Bridle, S. (2010) · Astronomy and Astrophysics · doi:10.1051/0004-6361/200913657 · Cited by 194 · see citing works
Quantifying the effect of baryon physics on weak lensing tomography
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Self-citationKiDS-450: The tomographic weak lensing power spectrum and constraints on cosmological parameters
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Self-citationCFHTLenS: testing the laws of gravity with tomographic weak lensing and redshift-space distortions
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Sellentin, E., & Heavens, A. (2015) · Monthly Notices of the Royal Astronomical Society Letters · doi:10.1093/mnrasl/slv190 · Cited by 182 · see citing works
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Massive Neutrinos and the Non-linear Matter Power SpectrumPreprint
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High-performance P3M N-body code: CUBEP3M
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Self-citationBayesian Measures of Model Complexity and Fit
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Non-linear cosmological power spectra in real and redshift space
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Cosmology from cosmic shear with Dark Energy Survey science verification data
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Measuring line-of-sight-dependent Fourier-space clustering using FFTs
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Precision calculations of the cosmic shear power spectrum projection
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Self-citationProbing modifications of general relativity using current cosmological observations
Zhao, G., Giannantonio, T., Pogosian, L., Silvestri, A., Bacon, D., Koyama, K., Nichol, R. C., & Song, Y. (2010) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.81.103510 · Cited by 143 · see citing works
Spergel, D. N., Flauger, R., & Hložek, R. (2015) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.91.023518 · Cited by 141 · see citing works
The Mira-Titan Universe. II. Matter Power Spectrum Emulation
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Galaxy alignments: An overview
Joachimi, B., Cacciato, M., Kitching, T., Leonard, A., Mandelbaum, R., Schuller, B., Sifón, C., Hoekstra, H., Kiessling, A., Kirk, D., et al. (2015) · KiltHub Repository · doi:10.1184/r1/6506831.v1 · Cited by 136 · see citing works
Self-citationThe third data release of the Kilo-Degree Survey and associated data products
de Jong, J. D., Kleijn, G. V. V., Erben, T., Hildebrandt, H., Kuijken, K., Sikkema, G., Brescia, M., Bilicki, M., Napolitano, N., Amaro, V., et al. (2017) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201730747 · Cited by 132 · see citing works
Self-citationCalibration of weak-lensing shear in the Kilo-Degree Survey
Conti, I. F., Herbonnet, R., Hoekstra, H., Merten, J., Miller, L., & Viola, M. (2016) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stx200 · Cited by 129 · see citing works
Self-citationGalaxy–galaxy lensing estimators and their covariance properties
Singh, S., Mandelbaum, R., Seljak, U., Slosar, A., & Vazquez, J. A. (2017) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stx1828 · Cited by 123 · see citing works
Joachimi, B., & Bridle, S. (2010) · Springer Link (Chiba Institute of Technology) · doi:10.1051/0004-6361/200913657/pdf · Cited by 123 · see citing works
On using angular cross-correlations to determine source redshift distributions
McQuinn, M., & White, M. J. (2013) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stt914 · Cited by 122 · see citing works
Pogosian, L., & Silvestri, A. (2016) · Physical Review D · doi:10.1103/physrevd.94.104014 · Cited by 112 · see citing works
Parejko, J. K., Sunayama, T., Padmanabhan, N., Wake, D. A., Berlind, A. A., Bizyaev, D., Blanton, M. R., Bolton, A. S., van den Bosch, F., Brinkmann, J., et al. (2012) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/sts314 · Cited by 108 · see citing works
Bayesian evidence as a tool for comparing datasets
Marshall, P. J., Rajguru, N., & Slosar, A. (2006) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.73.067302 · Cited by 105 · see citing works
Jee, M. J., Tyson, J. A., Hilbert, S., Schneider, M. D., Schmidt, S., & Wittman, D. (2016) · The Astrophysical Journal · doi:10.3847/0004-637x/824/2/77 · Cited by 98 · see citing works
Cosmological parameters from pre-planck cosmic microwave background measurements
Calabrese, E., Hložek, R., Battaglia, N., Battistelli, E. S., Bond, J. R., Chluba, J., Crichton, D., Das, S., Devlin, M. J., Dunkley, J., et al. (2013) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.87.103012 · Cited by 97 · see citing works
The 2-degree Field Lensing Survey: design and clustering measurements
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Self-citationComplementarity of weak lensing and peculiar velocity measurements in testing general relativity
Song, Y., Zhao, G., Bacon, D., Koyama, K., Nichol, R. C., & Pogosian, L. (2011) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.84.083523 · Cited by 83 · see citing works
Testing general relativity at cosmological scales: Implementation and parameter correlations
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Self-citationCosmological hints of modified gravity?
Valentino, E. D., MELCHIORRI, A., & Silk, J. I. (2016) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.93.023513 · Cited by 80 · see citing works
Tests of gravity from imaging and spectroscopic surveys
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Constraining gravity at the largest scales through CMB lensing and galaxy velocities
Pullen, A. R., Alam, S., He, S., & Ho, S. (2016) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stw1249 · Cited by 75 · see citing works
Harnois-Déraps, J., & Waerbeke, L. V. (2015) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stv794 · Cited by 73 · see citing works
Self-citationAre cosmological data sets consistent with each other within the Λ cold dark matter model?
Raveri, M. (2016) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.93.043522 · Cited by 73 · see citing works
Hikage, C., Mandelbaum, R., Takada, M., & Spergel, D. N. (2013) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stt1446 · Cited by 68 · see citing works
Spatial curvature and cosmological tests of general relativity
Dossett, J. N., & Ishak, M. (2012) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.86.103008 · Cited by 55 · see citing works
Joudaki, S., & Kaplinghat, M. (2012) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.86.023526 · Cited by 54 · see citing works
Self-citationJohnson, A., Blake, C., Dossett, J. N., Koda, J., Parkinson, D., & Joudaki, S. (2016) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stw447 · Cited by 51 · see citing works
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Cai, Y.-C., & Bernstein, G. M. (2012) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2012.20676.x · Cited by 49 · see citing works
Cosmological parameters from pre-Planck CMB measurements: A 2017 update
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Alam, S., Miyatake, H., More, S., Ho, S., & Mandelbaum, R. (2017) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stw3056 · Cited by 47 · see citing works
Dossett, J. N., Ishak, M., Parkinson, D., & Davis, T. M. (2015) · Physical Review D · doi:10.1103/physrevd.92.023003 · Cited by 44 · see citing works
Self-citationImpact of theoretical priors in cosmological analyses: The case of single field quintessence
Peirone, S., Martinelli, M., Raveri, M., & Silvestri, A. (2017) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.96.063524 · Cited by 40 · see citing works
A direct measurement of tomographic lensing power spectra from CFHTLenS
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Self-citationConstraints on neutrino mass and light degrees of freedom in extended cosmological parameter spaces
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Self-citationde Putter, R., Doré, O., & Das, S. (2013) · The Astrophysical Journal · doi:10.1088/0004-637x/780/2/185 · Cited by 23 · see citing works
Inference from the small scales of cosmic shear with current and future Dark Energy Survey data
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athena: Tree code for second-order correlation functions
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The Astro-WISE datacentric information system
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Combining spectroscopic and photometric surveys: Same or different sky?
Eriksen, M., & GAZTAÑAGA, E. (2015) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stv1093 · Cited by 15 · see citing works
The 2-degree Field Lensing Survey: photometric redshifts from a large new training sample tor < 19.5
Wolf, C., Johnson, A. S., Bilicki, M., Blake, C., Amon, A., Erben, T., Glazebrook, K., Heymans, C., Hildebrandt, H., Joudaki, S., et al. (2016) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stw3151 · Cited by 11 · see citing works
Self-citationThe Synergy between Weak Lensing and Galaxy Redshift SurveysPreprint
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Flagged first, then by citations
Research works printed but not linked: 4
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- Jeffreys H., 1961, Theory of Probability, 3rd edn, Oxford Classics series (reprinted 1998). Oxford University Press, Oxford, UK
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Cited by
Sorted by citations
LSST: From Science Drivers to Reference Design and Anticipated Data Products
Ivezić, Ž., Kahn, S. M., Tyson, J. A., Abel, B., Acosta, E., Allsman, R., Alonso, D., AlSayyad, Y., Anderson, S. F., Andrew, J., et al. (2019) · The Astrophysical Journal · doi:10.3847/1538-4357/ab042c · Cited by 4,357 · see citing works
Self-citationDark Energy Survey year 1 results: Cosmological constraints from galaxy clustering and weak lensing
Abbott, T. M. C., Abdalla, F. B., Alarcon, A., Aleksić, J., Allam, S., Allen, S., Amara, A., Annis, J., Asorey, J., Avila, S., et al. (2018) · Physical Review D · doi:10.1103/physrevd.98.043526 · Cited by 1,213 · see citing works
Self-citationDark Energy Survey Year 3 results: Cosmological constraints from galaxy clustering and weak lensing
Abbott, T. M. C., Aguena, M., Alarcon, A., Allam, S., Alves, O., Amon, A., Andrade-Oliveira, F., Annis, J., Avila, S., Bacon, D., et al. (2022) · Physical Review D · doi:10.1103/physrevd.105.023520 · Cited by 1,124 · see citing works
Self-citationHeymans, C., Tröster, T., Asgari, M., Blake, C., Hildebrandt, H., Joachimi, B., Kuijken, K., Lin, C.-A., Sánchez, A. G., van den Busch, J. L., et al. (2021) · Astronomy & Astrophysics · doi:10.1051/0004-6361/202039063 · Cited by 772 · see citing works
Self-citationTesting general relativity in cosmology
Ishak, M. (2019) · Living Reviews in Relativity · doi:10.1007/s41114-018-0017-4 · Cited by 449 · see citing works
Dark Energy Survey Year 3 results: Cosmology from cosmic shear and robustness to data calibration
Amon, A., Gruen, D., Troxel, M. A., MacCrann, N., Dodelson, S., Choi, A., Doux, C., Secco, L. F., Samuroff, S., Krause, E., et al. (2022) · Physical Review D · doi:10.1103/physrevd.105.023514 · Cited by 437 · see citing works
Self-citationWeak Lensing for Precision Cosmology
Mandelbaum, R. (2018) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev-astro-081817-051928 · Cited by 409 · see citing works
Exploring the Tension between Current Cosmic Microwave Background and Cosmic Shear Data
Di Valentino, E., & Bridle, S. (2018) · Symmetry · doi:10.3390/sym10110585 · Cited by 80 · see citing works
Abdalla, E., Abellán, G. F., Aboubrahim, A., Agnello, A., Akarsu, Ö., Akrami, Y., Alestas, G., Aloni, D., Amendola, L., Anchordoqui, L. A., et al. (2022) · Journal of High Energy Astrophysics · doi:10.1016/j.jheap.2022.04.002 · Cited by 37 · see citing works
Self-citation
- Authors
- Joudaki, S., Blake, C., Johnson, A., Amon, A., Asgari, M., Choi, A., Erben, T., Glazebrook, K., Harnois-Déraps, J., Heymans, C., Hildebrandt, H., Hoekstra, H., Klaes, D., Kuijken, K., Lidman, C., Mead, A., Miller, L., Parkinson, D., Poole, G. B., Schneider, P., Viola, M., & Wolf, C.
- Affiliations
- University of Oxford (GB)
- ARC Centre of Excellence for All-sky Astrophysics (AU)
- Royal Observatory (GB)
- The Ohio State University (US)
- University of Bonn (DE)
- Swinburne University of Technology (AU)
- Leiden University (NL)
- University of British Columbia (CA)
- The University of Queensland (AU)
- Australian National University (AU)
- Corresponding author
- Joudaki, Shahab
- ORCID
- Venue
- Monthly Notices of the Royal Astronomical Society
- Publisher
- Oxford University Press (OUP)
- Published
- 2017-10-31
- Volume
- 474
- Issue
- 4
- Pages
- 4894-4924
- ISSN
- 0035-8711 (ISSN-L)
- 1365-2966
- OpenAlex
- W2737954132
- Cited by
- 291
- References
- 142
- Citations by year
- 2026: 7 · 2025: 12 · 2024: 18 · 2023: 13 · 2022: 36 · 2021: 54 · 2020: 45 · 2019: 58 · 2018: 39 · 2017: 6 · 2016: 3
- FWCI
- 22.13
- Type
- journal article
- Language
- en
- Open access
- bronze
- doi.org
- Locations
- Monthly Notices of the Royal Astronomical Society (publishedVersion)
- arXiv (Cornell University) (acceptedVersion)
- ANU Open Research (Australian National University) (submittedVersion)
- Liverpool John Moores University (submittedVersion)
- Leiden Repository (Leiden University) (submittedVersion)
- Data Archiving and Networked Services (DANS) (submittedVersion, other-oa)
- Edinburgh Research Explorer (University of Edinburgh) (submittedVersion, other-oa)
- Swinburne figshare (Swinburne University of Technology) (submittedVersion)
- arXiv (Cornell University)
- Funders
- European Commission (656869)
- Science and Technology Facilities Council (ST/H002456/1, ST/N000919/1)
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Cosmology and Gravitation Theories
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Galaxies: Formation, Evolution, Phenomena
- Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Dark Matter and Cosmic Phenomena
- Keywords
- cosmological parameter constraints, cosmic shear tomography, KiDS-450, BOSS, S8 tension, Planck tension, modified gravity, dark energy, neutrino mass, cosmic curvature, covariance matrix, N-body simulations
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