Paper Citation Record · LEDGER

$S_8$ increases with effective redshift in $\Lambda$CDM cosmology

As of 22 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 11 inbound Pith citation observations for arXiv:2303.06928.

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

pith.paper-citation-record.v1
2303.06928 v3

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measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

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measured 11 of 11 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-22T06:32:14.747728+00:00

measured 11 of 11 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-16T10:37:59.616369Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-03T12:58:08.191609Z

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External citation measurements

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Outbound references

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Pith citing papers

Observation bc32bf68-6e1b-40a0-8a3a-d974d234feac · inbound

$\Lambda_{\rm s}$CDM cosmology from a type-II minimally modified gravity cites this paper.

$\Lambda_{\rm s}$CDM cosmology from a type-II minimally modified gravity $S_8$ increases with effective redshift in $\Lambda$CDM cosmology

Reference 77

Resolution: verified exact; arxiv_id, observed 2026-05-24T03:53:54.089988Z

Source-reported events for the cited work

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Observation 591d8bb0-b357-4c77-9e6b-04224461f597 · inbound

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? cites this paper.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? $S_8$ increases with effective redshift in $\Lambda$CDM cosmology

Reference 39

Resolution: unresolved; no resolver link, observed 2026-08-11T13:41:23.721183Z

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Observation 598adc99-a678-4349-b523-7cf8d0d572d7 · inbound

Testing $\gamma\delta$CDM Model in the Redshift Bins cites this paper.

Testing $\gamma\delta$CDM Model in the Redshift Bins $S_8$ increases with effective redshift in $\Lambda$CDM cosmology

Reference 136

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Observation f521dd85-5535-4c7b-ae82-b30f825964b1 · inbound

Illustrating the consequences of a misuse of $\sigma_8$ in cosmology cites this paper.

Illustrating the consequences of a misuse of $\sigma_8$ in cosmology $S_8$ increases with effective redshift in $\Lambda$CDM cosmology

Reference 89

Resolution: unresolved; no resolver link, observed 2026-08-10T18:12:34.044006Z

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Observation e77e9879-1e24-4076-87a1-4410a9242f5c · inbound

Updated Constraints on Omnipotent Dark Energy: A Comprehensive Analysis with CMB and BAO Data cites this paper.

Updated Constraints on Omnipotent Dark Energy: A Comprehensive Analysis with CMB and BAO Data $S_8$ increases with effective redshift in $\Lambda$CDM cosmology

Reference 66

Resolution: unresolved; no resolver link, observed 2026-08-16T10:37:59.616369Z

Source-reported events for the cited work

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Observation 7f4066e5-4e8d-4590-8194-13ac36692316 · inbound

Challenging $\Lambda$CDM: 5$\sigma$ Evidence for a Dynamical Dark Energy Late-Time Transition cites this paper.

Challenging $\Lambda$CDM: 5$\sigma$ Evidence for a Dynamical Dark Energy Late-Time Transition $S_8$ increases with effective redshift in $\Lambda$CDM cosmology

Reference 41

Resolution: unresolved; no resolver link, observed 2026-08-16T05:27:54.198858Z

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Observation b82e2ea9-521d-4e26-8b42-92eb9ab2eb2b · inbound

Nonlinear Matter Power Spectrum from relativistic $N$-body Simulations: $\Lambda_{\rm s}$CDM versus $\Lambda$CDM cites this paper.

Nonlinear Matter Power Spectrum from relativistic $N$-body Simulations: $\Lambda_{\rm s}$CDM versus $\Lambda$CDM $S_8$ increases with effective redshift in $\Lambda$CDM cosmology

Reference 69

Resolution: verified exact; arxiv_id, observed 2026-05-18T04:50:54.861507Z

Source-reported events for the cited work

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Observation 3c034f92-11bb-42b7-8cfc-238abceea2f0 · inbound

New constraints on cosmic anisotropy from galaxy clusters using an improved dipole fitting method cites this paper.

New constraints on cosmic anisotropy from galaxy clusters using an improved dipole fitting method $S_8$ increases with effective redshift in $\Lambda$CDM cosmology

Reference 28

Resolution: verified exact; arxiv_id, observed 2026-05-16T02:27:10.981590Z

Source-reported events for the cited work

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Observation 01bf39f4-cffb-475f-87e9-9713d689bc57 · inbound

Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families cites this paper.

Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families $S_8$ increases with effective redshift in $\Lambda$CDM cosmology

Reference 30

Resolution: unresolved; no resolver link, observed 2026-07-15T12:01:04.317365Z

Source-reported events for the cited work

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Observation bd7b912e-d5fa-47c8-afe2-142af191a2d7 · inbound

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

Dark Matter with a Drag at Low Redshift $S_8$ increases with effective redshift in $\Lambda$CDM cosmology

Reference 13

Resolution: verified exact; arxiv_id, observed 2026-07-03T12:58:08.192944Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

Observation edff828b-ece6-46c3-9229-cbf293f8c3d3 · inbound

Testing Scale-Dependent Suppression of Structure Growth in the Linear Regime cites this paper.

Testing Scale-Dependent Suppression of Structure Growth in the Linear Regime $S_8$ increases with effective redshift in $\Lambda$CDM cosmology

Reference 87

Resolution: unresolved; no resolver link, observed 2026-08-04T12:59:01.716231Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.