Paper Citation Record · LEDGER

Inferring $S_8(z)$ and $\gamma(z)$ with cosmic growth rate measurements using machine learning

As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 10 inbound Pith citation observations for arXiv:2201.07829.

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

pith.paper-citation-record.v1
2201.07829 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 10 of 10 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-09T06:31:02.800959+00:00

measured 10 of 10 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T12:25:52.322289Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-04T22:30:10.240988Z

Reference resolution

0 of 0 outbound references displayed

verified exact0
verified fuzzy0
unresolved0
parse uncertain0
malformed identifier0
metadata mismatch0

External citation measurements

No source-named external measurement is stored.

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 068b7339-8499-4ebd-a1f3-eee74a166bfb · inbound

Revisiting the temperature evolution law of the CMB with gaussian processes cites this paper.

Revisiting the temperature evolution law of the CMB with gaussian processes Inferring $S_8(z)$ and $\gamma(z)$ with cosmic growth rate measurements using machine learning

Reference 56

Resolution: unresolved; no resolver link, observed 2026-08-07T12:25:52.322289Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a9d5f381-30fc-416b-aa4c-8ca68ff91277 · inbound

Is $\omega_0 \omega_a$CDM a good model for the clumpy Universe? cites this paper.

Is $\omega_0 \omega_a$CDM a good model for the clumpy Universe? Inferring $S_8(z)$ and $\gamma(z)$ with cosmic growth rate measurements using machine learning

Reference 6

Resolution: unresolved; no resolver link, observed 2026-08-06T21:15:08.344531Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8cc2143c-1c19-4bcd-bf6d-63653694831d · inbound

Cosmological tensions in Proca-Nuevo theory cites this paper.

Cosmological tensions in Proca-Nuevo theory Inferring $S_8(z)$ and $\gamma(z)$ with cosmic growth rate measurements using machine learning

Reference 102

Resolution: unresolved; no resolver link, observed 2026-08-03T20:12:23.728018Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 684a1bea-36a5-4333-8113-f2ba1016684f · inbound

Observational constraints on 3-forms dark energy cites this paper.

Observational constraints on 3-forms dark energy Inferring $S_8(z)$ and $\gamma(z)$ with cosmic growth rate measurements using machine learning

Reference 119

Resolution: unresolved; no resolver link, observed 2026-08-03T17:24:59.437102Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 975df5a2-9ad0-4745-be28-47d0faf8fa6c · inbound

Effective field theory interpretation of ATLAS measurements involving the Higgs boson, electroweak bosons and the top quark cites this paper.

Effective field theory interpretation of ATLAS measurements involving the Higgs boson, electroweak bosons and the top quark Inferring $S_8(z)$ and $\gamma(z)$ with cosmic growth rate measurements using machine learning

Reference 107

Resolution: verified exact; arxiv_id, observed 2026-07-04T22:30:10.242766Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 72161d11-a513-44b7-8ae7-574e9434d37a · inbound

Saturation Mechanisms in the Interacting Dark Sector cites this paper.

Saturation Mechanisms in the Interacting Dark Sector Inferring $S_8(z)$ and $\gamma(z)$ with cosmic growth rate measurements using machine learning

Reference 108

Resolution: verified exact; arxiv_id, observed 2026-05-11T18:41:12.928744Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 1cbd1456-ca17-467f-ac04-57050fac1d2b · inbound

Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus cites this paper.

Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus Inferring $S_8(z)$ and $\gamma(z)$ with cosmic growth rate measurements using machine learning

Reference 190

Resolution: unresolved; no resolver link, observed 2026-07-11T09:40:49.196932Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 10f8fe34-dfad-45b5-b79d-5e8875cc8027 · inbound

Breaking the Dark Sector Degeneracy with Nonparametric Expansion--Growth Reconstruction cites this paper.

Breaking the Dark Sector Degeneracy with Nonparametric Expansion--Growth Reconstruction Inferring $S_8(z)$ and $\gamma(z)$ with cosmic growth rate measurements using machine learning

Reference 66

Resolution: unresolved; no resolver link, observed 2026-07-14T03:00:21.146194Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 117809a8-a131-44ac-ab68-7d219a15e035 · inbound

Hubble tension: the shape wall cites this paper.

Hubble tension: the shape wall Inferring $S_8(z)$ and $\gamma(z)$ with cosmic growth rate measurements using machine learning

Reference 246

Resolution: unresolved; no resolver link, observed 2026-08-01T08:08:57.841958Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9ae4a1ff-5daf-43ec-8251-69128cde77bb · inbound

Early- and late-time constraints on Wald-Gauss-Bonnet topological dark energy and implications for the $H_0$ and $S_8$ tensions cites this paper.

Early- and late-time constraints on Wald-Gauss-Bonnet topological dark energy and implications for the $H_0$ and $S_8$ tensions Inferring $S_8(z)$ and $\gamma(z)$ with cosmic growth rate measurements using machine learning

Reference 114

Resolution: unresolved; no resolver link, observed 2026-08-01T02:46:23.113917Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.