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Paper Citation Record · LEDGER

Late-time suppression of structure growth as a solution for the $S_8$ tension

As of 16 August 2026, this Paper Citation Record lists 70 of 70 outbound references and 1 inbound Pith citation observation for arXiv:2505.09176.

A citation records a reference. It does not transfer a finding from one paper to another.

pith.paper-citation-record.v1
2505.09176 v1

Coverage vector

measured 70 of 70 reference resolution

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Source: paper_references, paper_reference_links, observed 2026-08-15T21:42:04.947836Z

measured 71 of 71 standing notices

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measured 1 of 1 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-06-27T08:39:40.656848Z

measured 0 of 1 external citation measurements

A source-named dated measurement, never combined with another source.

Source: arxiv_reference, observed 2026-07-03T12:58:08.292069Z

Reference resolution

70 of 70 outbound references displayed

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Outbound references

Observation 36fbd004-e444-465d-b5e9-887ab8d98afa · outbound

This paper cites Observational Probes of Cosmic Acceleration.

Late-time suppression of structure growth as a solution for the $S_8$ tension Observational Probes of Cosmic Acceleration

Reference 1

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Observation 935b1778-bc8f-4499-be68-5487fd8cfd0f · outbound

This paper cites Dark Energy Tracking Growth (DETG) model.

Late-time suppression of structure growth as a solution for the $S_8$ tension Dark Energy Tracking Growth (DETG) model

Reference 2

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Observation 5fe9803d-faa4-4106-8818-5ea1c8c2f96d · outbound

This paper cites For the fiducialΛCDM model, we assumeM ν = 0.06eV for the total neutrino mass, corresponding to the lower bound of the normal mass hierarchy [e.g., 33].

Late-time suppression of structure growth as a solution for the $S_8$ tension For the fiducialΛCDM model, we assumeM ν = 0.06eV for the total neutrino mass, corresponding to the lower bound of the normal mass hierarchy [e.g., 33]

Reference 3

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Observation 0a60eafd-69a5-4150-a800-34b944b81a57 · outbound

This paper cites ij” denote tomographic bins; e.g. “ij.

Late-time suppression of structure growth as a solution for the $S_8$ tension ij” denote tomographic bins; e.g. “ij

Reference 4

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Observation 95fd8a5f-c6ec-444c-8470-a6c2135d1f95 · outbound

This paper cites Dodelson and F.

Late-time suppression of structure growth as a solution for the $S_8$ tension Dodelson and F

Reference 5

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Observation 1afd67d7-85b9-4503-900a-d28944e239f8 · outbound

This paper cites Cosmology Intertwined: A Review of the Particle Physics, Astrophysics, and Cosmology Associated with the Cosmological Tensions and Anomalies.

Late-time suppression of structure growth as a solution for the $S_8$ tension Cosmology Intertwined: A Review of the Particle Physics, Astrophysics, and Cosmology Associated with the Cosmological Tensions and Anomalies

Reference 6

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Observation 664677f1-7426-4f71-9352-3ccb45d5e222 · outbound

This paper cites Hyper Suprime-Cam Year 3 Results: Cosmology from Cosmic Shear Two-point Correlation Functions.

Late-time suppression of structure growth as a solution for the $S_8$ tension Hyper Suprime-Cam Year 3 Results: Cosmology from Cosmic Shear Two-point Correlation Functions

Reference 7

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Observation 897ee4b4-1ef0-445b-aa7a-f7587db0c3c4 · outbound

This paper cites Hyper Suprime-Cam Year 3 Results: Cosmology from Cosmic Shear Power Spectra.

Late-time suppression of structure growth as a solution for the $S_8$ tension Hyper Suprime-Cam Year 3 Results: Cosmology from Cosmic Shear Power Spectra

Reference 8

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Observation e095ced6-3da6-47c5-8f7b-4cf13108ca39 · outbound

This paper cites KiDS-1000 Cosmology: Cosmic shear constraints and comparison between two point statistics.

Late-time suppression of structure growth as a solution for the $S_8$ tension KiDS-1000 Cosmology: Cosmic shear constraints and comparison between two point statistics

Reference 9

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Observation 6905ddf4-97ad-474e-8dfa-0c7e7a10159b · outbound

This paper cites Dark Energy Survey Year 3 Results: Cosmology from Cosmic Shear and Robustness to Modeling Uncertainty.

Late-time suppression of structure growth as a solution for the $S_8$ tension Dark Energy Survey Year 3 Results: Cosmology from Cosmic Shear and Robustness to Modeling Uncertainty

Reference 10

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Observation 87fa81c5-57e2-4cdb-a032-f917f32a6282 · outbound

This paper cites Hyper Suprime-Cam Year 3 Results: Cosmology from Galaxy Clustering and Weak Lensing with HSC and SDSS using the Emulator Based Halo Model.

Late-time suppression of structure growth as a solution for the $S_8$ tension Hyper Suprime-Cam Year 3 Results: Cosmology from Galaxy Clustering and Weak Lensing with HSC and SDSS using the Emulator Based Halo Model

Reference 11

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Observation 4903026a-0297-417e-9142-e13a397307da · outbound

This paper cites Hyper Suprime-Cam Year 3 Results: Cosmology from Galaxy Clustering and Weak Lensing with HSC and SDSS using the Minimal Bias Model.

Late-time suppression of structure growth as a solution for the $S_8$ tension Hyper Suprime-Cam Year 3 Results: Cosmology from Galaxy Clustering and Weak Lensing with HSC and SDSS using the Minimal Bias Model

Reference 12

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Observation 8838f200-a6f5-459d-a705-f640a802ea44 · outbound

This paper cites KiDS-1000 Cosmology: Multi-probe weak gravitational lensing and spectroscopic galaxy clustering constraints.

Late-time suppression of structure growth as a solution for the $S_8$ tension KiDS-1000 Cosmology: Multi-probe weak gravitational lensing and spectroscopic galaxy clustering constraints

Reference 13

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Observation 7806374d-84d4-4c86-96e0-499032a8d1c2 · outbound

This paper cites Dark Energy Survey Year 3 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing.

Late-time suppression of structure growth as a solution for the $S_8$ tension Dark Energy Survey Year 3 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing

Reference 14

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Observation 13e8e740-86f2-43b6-a95a-c426540c1e09 · outbound

This paper cites Cosmological Parameters from the BOSS Galaxy Power Spectrum.

Late-time suppression of structure growth as a solution for the $S_8$ tension Cosmological Parameters from the BOSS Galaxy Power Spectrum

Reference 15

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Observation 525a0fc6-3893-475c-b487-57634a02ff22 · outbound

This paper cites A new analysis of galaxy 2-point functions in the BOSS survey, including full-shape information and post-reconstruction BAO.

Late-time suppression of structure growth as a solution for the $S_8$ tension A new analysis of galaxy 2-point functions in the BOSS survey, including full-shape information and post-reconstruction BAO

Reference 16

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Observation 9941453f-3979-459a-85b9-78e860fed4f3 · outbound

This paper cites Full-shape cosmology analysis of SDSS-III BOSS galaxy power spectrum using emulator-based halo model: a $5\%$ determination of $\sigma_8$.

Late-time suppression of structure growth as a solution for the $S_8$ tension Full-shape cosmology analysis of SDSS-III BOSS galaxy power spectrum using emulator-based halo model: a $5\%$ determination of $\sigma_8$

Reference 17

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Observation 1812261b-225d-49f4-8ac1-04e4fa0604ad · outbound

This paper cites Testing small-scale modifications in the primordial power spectrum with Subaru HSC cosmic shear, primary CMB and CMB lensing.

Late-time suppression of structure growth as a solution for the $S_8$ tension Testing small-scale modifications in the primordial power spectrum with Subaru HSC cosmic shear, primary CMB and CMB lensing

Reference 18

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Observation b706da79-b412-449c-bf3e-4f09d92f0181 · outbound

This paper cites Evidence for suppression of structure growth in the concordance cosmological model.

Late-time suppression of structure growth as a solution for the $S_8$ tension Evidence for suppression of structure growth in the concordance cosmological model

Reference 19

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Observation 8a9fb9f7-84d8-4b5f-9676-3a38611ba037 · outbound

This paper cites Late Time Modification of Structure Growth and the S8 Tension.

Late-time suppression of structure growth as a solution for the $S_8$ tension Late Time Modification of Structure Growth and the S8 Tension

Reference 20

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Observation 810bfec3-f6f9-47df-816b-7c689dbaf17e · outbound

This paper cites The SRG/eROSITA All-Sky Survey : Constraints on the structure growth from cluster number counts.

Late-time suppression of structure growth as a solution for the $S_8$ tension The SRG/eROSITA All-Sky Survey : Constraints on the structure growth from cluster number counts

Reference 21

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Observation 3d663a05-f5e0-4319-ba04-30851484a629 · outbound

This paper cites Cosmic Growth History and Expansion History.

Late-time suppression of structure growth as a solution for the $S_8$ tension Cosmic Growth History and Expansion History

Reference 22

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This paper cites The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: RSD measurement from the power spectrum and bispectrum of the DR12 BOSS galaxies.

Late-time suppression of structure growth as a solution for the $S_8$ tension The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: RSD measurement from the power spectrum and bispectrum of the DR12 BOSS galaxies

Reference 23

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Observation 4691a2d4-a200-4dce-90ab-fbecda63d4a6 · outbound

This paper cites The impact of baryons on the matter power spectrum from the Horizon-AGN cosmological hydrodynamical simulation.

Late-time suppression of structure growth as a solution for the $S_8$ tension The impact of baryons on the matter power spectrum from the Horizon-AGN cosmological hydrodynamical simulation

Reference 24

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Observation b568619f-2639-4c9d-a92e-0bd7bbec1457 · outbound

This paper cites Constraining Baryonic Physics with DES Y1 and Planck data -- Combining Galaxy Clustering, Weak Lensing, and CMB Lensing.

Late-time suppression of structure growth as a solution for the $S_8$ tension Constraining Baryonic Physics with DES Y1 and Planck data -- Combining Galaxy Clustering, Weak Lensing, and CMB Lensing

Reference 25

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This paper cites Exploring the baryonic effect signature in the Hyper Suprime-Cam Year 3 cosmic shear two-point correlations on small scales: the $S_8$ tension remains present.

Late-time suppression of structure growth as a solution for the $S_8$ tension Exploring the baryonic effect signature in the Hyper Suprime-Cam Year 3 cosmic shear two-point correlations on small scales: the $S_8$ tension remains present

Reference 26

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Late-time suppression of structure growth as a solution for the $S_8$ tension Reconstructing the shape of the non-linear matter power spectrum using CMB lensing and cosmic shear

Reference 27

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This paper cites A Unified Catalog-level Reanalysis of Stage-III Cosmic Shear Surveys.

Late-time suppression of structure growth as a solution for the $S_8$ tension A Unified Catalog-level Reanalysis of Stage-III Cosmic Shear Surveys

Reference 28

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Late-time suppression of structure growth as a solution for the $S_8$ tension Quantifying the effect of baryon physics on weak lensing tomography

Reference 29

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Late-time suppression of structure growth as a solution for the $S_8$ tension Modelling baryonic feedback for survey cosmology

Reference 30

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Late-time suppression of structure growth as a solution for the $S_8$ tension HMcode-2020: Improved modelling of non-linear cosmological power spectra with baryonic feedback

Reference 31

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This paper cites A non-linear solution to the $S_8$ tension?.

Late-time suppression of structure growth as a solution for the $S_8$ tension A non-linear solution to the $S_8$ tension?

Reference 32

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Late-time suppression of structure growth as a solution for the $S_8$ tension DES Y3 cosmic shear down to small scales: constraints on cosmology and baryons

Reference 33

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Late-time suppression of structure growth as a solution for the $S_8$ tension Unresolved cited work

Reference 34

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Observation 7cba3a04-892a-4a52-bac8-3381149304fc · outbound

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Late-time suppression of structure growth as a solution for the $S_8$ tension Weighing Neutrinos with Galaxy Surveys

Reference 35

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Observation f3a78e60-325b-4b3a-a444-228a7be82843 · outbound

This paper cites Cosmology with High-redshift Galaxy Survey: Neutrino Mass and Inflation.

Late-time suppression of structure growth as a solution for the $S_8$ tension Cosmology with High-redshift Galaxy Survey: Neutrino Mass and Inflation

Reference 36

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Observation 8c62eb6b-1474-44fd-8c47-dbfbc3571818 · outbound

This paper cites Accurate halo-model matter power spectra with dark energy, massive neutrinos and modified gravitational forces.

Late-time suppression of structure growth as a solution for the $S_8$ tension Accurate halo-model matter power spectra with dark energy, massive neutrinos and modified gravitational forces

Reference 37

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Observation 7bc66076-df19-4f20-9ba4-c9ace375640b · outbound

This paper cites An accurate halo model for fitting non-linear cosmological power spectra and baryonic feedback models.

Late-time suppression of structure growth as a solution for the $S_8$ tension An accurate halo model for fitting non-linear cosmological power spectra and baryonic feedback models

Reference 38

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Observation 19aca4a4-4d20-4800-bc76-05d58a05db87 · outbound

This paper cites KiDS-1000 Methodology: Modelling and inference for joint weak gravitational lensing and spectroscopic galaxy clustering analysis.

Late-time suppression of structure growth as a solution for the $S_8$ tension KiDS-1000 Methodology: Modelling and inference for joint weak gravitational lensing and spectroscopic galaxy clustering analysis

Reference 39

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Observation 560997a6-6e34-4cdf-a18b-432be4f62bfe · outbound

This paper cites Towards a realistic population of simulated galaxy groups and clusters.

Late-time suppression of structure growth as a solution for the $S_8$ tension Towards a realistic population of simulated galaxy groups and clusters

Reference 40

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Observation 85e4134f-e3d6-4d91-abeb-fb7bf30ee011 · outbound

This paper cites Weak lensing combined with the kinetic Sunyaev Zel'dovich effect: A study of baryonic feedback.

Late-time suppression of structure growth as a solution for the $S_8$ tension Weak lensing combined with the kinetic Sunyaev Zel'dovich effect: A study of baryonic feedback

Reference 41

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Observation ebb896a6-979b-408f-942c-10bd9600dc57 · outbound

This paper cites The Structure of Cold Dark Matter Halos.

Late-time suppression of structure growth as a solution for the $S_8$ tension The Structure of Cold Dark Matter Halos

Reference 42

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Observation 8d81fed9-f4b0-40e0-a139-d77c3377ace8 · outbound

This paper cites an unresolved cited work.

Late-time suppression of structure growth as a solution for the $S_8$ tension Unresolved cited work

Reference 43

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Observation 04ec5fc6-4ecc-4c02-a3b5-bffb5542a0b2 · outbound

This paper cites an unresolved cited work.

Late-time suppression of structure growth as a solution for the $S_8$ tension Unresolved cited work

Reference 44

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Observation a21388f9-4a72-45f7-a97e-28f8c7b744dd · outbound

This paper cites A new method to quantify the effects of baryons on the matter power spectrum.

Late-time suppression of structure growth as a solution for the $S_8$ tension A new method to quantify the effects of baryons on the matter power spectrum

Reference 45

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Observation aa87d072-b9ae-4334-8295-81f1c4e0fc96 · outbound

This paper cites Quantifying baryon effects on the matter power spectrum and the weak lensing shear correlation.

Late-time suppression of structure growth as a solution for the $S_8$ tension Quantifying baryon effects on the matter power spectrum and the weak lensing shear correlation

Reference 46

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Observation 4d52bfa9-401d-4390-ba63-e4d5543158b2 · outbound

This paper cites The BAHAMAS project: the CMB--large-scale structure tension and the roles of massive neutrinos and galaxy formation.

Late-time suppression of structure growth as a solution for the $S_8$ tension The BAHAMAS project: the CMB--large-scale structure tension and the roles of massive neutrinos and galaxy formation

Reference 47

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Observation 6820e78f-512b-4790-b8ed-9c4c5a349913 · outbound

This paper cites Simba: Cosmological Simulations with Black Hole Growth and Feedback.

Late-time suppression of structure growth as a solution for the $S_8$ tension Simba: Cosmological Simulations with Black Hole Growth and Feedback

Reference 48

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Observation 6dc9a33a-9775-4154-8687-167687bf5271 · outbound

This paper cites Introducing the Illustris Project: Simulating the coevolution of dark and visible matter in the Universe.

Late-time suppression of structure growth as a solution for the $S_8$ tension Introducing the Illustris Project: Simulating the coevolution of dark and visible matter in the Universe

Reference 49

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Observation 0103fcf4-14d4-4002-adab-d82dc04129ae · outbound

This paper cites First results from the IllustrisTNG simulations: matter and galaxy clustering.

Late-time suppression of structure growth as a solution for the $S_8$ tension First results from the IllustrisTNG simulations: matter and galaxy clustering

Reference 50

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Observation 0f6000ac-52c8-47e5-a8b0-035428e75cf2 · outbound

This paper cites The EAGLE project: Simulating the evolution and assembly of galaxies and their environments.

Late-time suppression of structure growth as a solution for the $S_8$ tension The EAGLE project: Simulating the evolution and assembly of galaxies and their environments

Reference 51

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Observation 0305f68c-883b-4ea5-ae66-9185e5e3d39c · outbound

This paper cites Mitigating baryon feedback bias in cosmic shear through a theoretical error covariance in the matter power spectrum.

Late-time suppression of structure growth as a solution for the $S_8$ tension Mitigating baryon feedback bias in cosmic shear through a theoretical error covariance in the matter power spectrum

Reference 52

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Observation 94c9b274-84db-4654-9fc6-e5372a4964ee · outbound

This paper cites Impact of massive neutrinos on nonlinear matter power spectrum.

Late-time suppression of structure growth as a solution for the $S_8$ tension Impact of massive neutrinos on nonlinear matter power spectrum

Reference 53

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Observation 5de12671-6121-4dc0-8b93-8757b63d77f3 · outbound

This paper cites Efficient Computation of CMB anisotropies in closed FRW models.

Late-time suppression of structure growth as a solution for the $S_8$ tension Efficient Computation of CMB anisotropies in closed FRW models

Reference 54

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Observation 5b887db6-1795-4ab5-a242-f15f9618914b · outbound

This paper cites Sweeping Horndeski Canvas: New Growth-Rate Parameterization for Modified-Gravity Theories.

Late-time suppression of structure growth as a solution for the $S_8$ tension Sweeping Horndeski Canvas: New Growth-Rate Parameterization for Modified-Gravity Theories

Reference 55

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Observation d66c1828-6fb6-4bad-96b3-08dcb6cf7160 · outbound

This paper cites Separate universe approach to evaluate nonlinear matter power spectrum for non-flat $\Lambda$CDM model.

Late-time suppression of structure growth as a solution for the $S_8$ tension Separate universe approach to evaluate nonlinear matter power spectrum for non-flat $\Lambda$CDM model

Reference 56

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Observation e8e29c1c-fe77-4058-a2f4-ed7fbf9d8d3a · outbound

This paper cites 2D-FFTLog: Efficient computation of real space covariance matrices for galaxy clustering and weak lensing.

Late-time suppression of structure growth as a solution for the $S_8$ tension 2D-FFTLog: Efficient computation of real space covariance matrices for galaxy clustering and weak lensing

Reference 57

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Observation 9302fa01-dce0-4573-82c9-ebda2cffcdad · outbound

This paper cites Planck 2018 results. VI. Cosmological parameters.

Late-time suppression of structure growth as a solution for the $S_8$ tension Planck 2018 results. VI. Cosmological parameters

Reference 58

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source=pdf_text observed=2026-08-15T21:42:04.893192Z digest=sha256:61ebf592f11a8c0523c429e4f0bccf62b3902dae276831943998d751f73fe428

Observation 3df56915-890d-42f5-9031-84b4f619cb83 · outbound

This paper cites The Atacama Cosmology Telescope: A Measurement of the DR6 CMB Lensing Power Spectrum and its Implications for Structure Growth.

Late-time suppression of structure growth as a solution for the $S_8$ tension The Atacama Cosmology Telescope: A Measurement of the DR6 CMB Lensing Power Spectrum and its Implications for Structure Growth

Reference 59

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Observation 7e7d48f0-8743-4640-909e-187ed527cfa7 · outbound

This paper cites The Atacama Cosmology Telescope: DR6 Gravitational Lensing Map and Cosmological Parameters.

Late-time suppression of structure growth as a solution for the $S_8$ tension The Atacama Cosmology Telescope: DR6 Gravitational Lensing Map and Cosmological Parameters

Reference 60

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Observation 48c6dd4b-72e5-41b7-8d62-1e8f57b9a4b4 · outbound

This paper cites DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations.

Late-time suppression of structure growth as a solution for the $S_8$ tension DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations

Reference 61

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Observation a4bc39d5-c42a-4b9b-9ed4-a43901f98287 · outbound

This paper cites The three-year shear catalog of the Subaru Hyper Suprime-Cam SSP Survey.

Late-time suppression of structure growth as a solution for the $S_8$ tension The three-year shear catalog of the Subaru Hyper Suprime-Cam SSP Survey

Reference 62

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Observation 2e4084e5-149c-42f8-9ada-e2638ecaab0c · outbound

This paper cites MultiNest: an efficient and robust Bayesian inference tool for cosmology and particle physics.

Late-time suppression of structure growth as a solution for the $S_8$ tension MultiNest: an efficient and robust Bayesian inference tool for cosmology and particle physics

Reference 63

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Observation 88aaec05-35ea-4f09-a105-ec990105f813 · outbound

This paper cites Cosmological inference from the emulator based halo model II: Joint analysis of galaxy-galaxy weak lensing and galaxy clustering from HSC-Y1 and SDSS.

Late-time suppression of structure growth as a solution for the $S_8$ tension Cosmological inference from the emulator based halo model II: Joint analysis of galaxy-galaxy weak lensing and galaxy clustering from HSC-Y1 and SDSS

Reference 64

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Observation c1fb2121-9343-4e88-a26f-c655b95044a6 · outbound

This paper cites GetDist: a Python package for analysing Monte Carlo samples.

Late-time suppression of structure growth as a solution for the $S_8$ tension GetDist: a Python package for analysing Monte Carlo samples

Reference 65

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Observation 6316a80f-77eb-471f-8470-018426f80158 · outbound

This paper cites Jeffreys,The Theory of Probability(1961).

Late-time suppression of structure growth as a solution for the $S_8$ tension Jeffreys,The Theory of Probability(1961)

Reference 66

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Observation e5d2b751-55e0-45a9-8529-2f118598b170 · outbound

This paper cites Cosmological constraints from the tomographic cross-correlation of DESI Luminous Red Galaxies and Planck CMB lensing.

Late-time suppression of structure growth as a solution for the $S_8$ tension Cosmological constraints from the tomographic cross-correlation of DESI Luminous Red Galaxies and Planck CMB lensing

Reference 67

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Observation 93c1c915-0016-4bc8-b7fd-debc86e7c11f · outbound

This paper cites Cosmological constraints from the cross-correlation of DESI Luminous Red Galaxies with CMB lensing from Planck PR4 and ACT DR6.

Late-time suppression of structure growth as a solution for the $S_8$ tension Cosmological constraints from the cross-correlation of DESI Luminous Red Galaxies with CMB lensing from Planck PR4 and ACT DR6

Reference 68

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Observation 4bc35cd7-efb2-46f6-a713-84bf4ec9c07f · outbound

This paper cites The growth of density perturbations in the last $\sim$10 billion years from tomographic large-scale structure data.

Late-time suppression of structure growth as a solution for the $S_8$ tension The growth of density perturbations in the last $\sim$10 billion years from tomographic large-scale structure data

Reference 69

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Observation 7b86bd34-cd82-4469-8b6f-d24a65af2543 · outbound

This paper cites DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints.

Late-time suppression of structure growth as a solution for the $S_8$ tension DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints

Reference 70

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Pith citing papers

Observation 626f2149-585f-4a36-a6d8-c38d0347ed59 · inbound

Dark Matter with a Drag at Low Redshift cites this paper.

Dark Matter with a Drag at Low Redshift Late-time suppression of structure growth as a solution for the $S_8$ tension

Reference 11

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