Paper Citation Record · LEDGER

On Redshift Evolution & Negative Dark Energy Density in Pantheon+ Supernovae

As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 9 inbound Pith citation observations for arXiv:2301.12725.

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

pith.paper-citation-record.v1
2301.12725 v3

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 9 of 9 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-07T06:34:17.273281+00:00

measured 9 of 9 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-01T16:29:57.952451Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-24T03:53:54.564845Z

Reference resolution

0 of 0 outbound references displayed

verified exact0
verified fuzzy0
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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 7d7ba54e-21d6-4de1-99ce-5bff7677b823 · 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 On Redshift Evolution & Negative Dark Energy Density in Pantheon+ Supernovae

Reference 113

Resolution: verified exact; arxiv_id, observed 2026-05-24T03:53:54.567281Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 8175cef3-c140-48a2-b2a9-e1b50628cfd0 · 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 On Redshift Evolution & Negative Dark Energy Density in Pantheon+ Supernovae

Reference 179

Resolution: verified exact; arxiv_id, observed 2026-05-18T04:50:55.031411Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 392f4f09-2fd9-44cc-8911-692548b8198a · inbound

Revisiting the Matter Creation Process: Observational Constraints on Gravitationally Induced Dark Energy and the Hubble Tension cites this paper.

Revisiting the Matter Creation Process: Observational Constraints on Gravitationally Induced Dark Energy and the Hubble Tension On Redshift Evolution & Negative Dark Energy Density in Pantheon+ Supernovae

Reference 129

Resolution: verified exact; arxiv_id, observed 2026-05-16T12:17:52.223928Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation ff074e13-ac1d-48af-a45a-62ace48a4e49 · inbound

Probing Dynamical Dark Energy with Late-Time Data: Evidence, Tensions, and the Limits of the $w_0w_a$CDM Framework cites this paper.

Probing Dynamical Dark Energy with Late-Time Data: Evidence, Tensions, and the Limits of the $w_0w_a$CDM Framework On Redshift Evolution & Negative Dark Energy Density in Pantheon+ Supernovae

Reference 130

Resolution: verified exact; arxiv_id, observed 2026-05-21T13:30:12.223292Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation d9ac8dd8-5815-40e6-828b-698f780b754c · inbound

Redshift evolution of the Hubble constant: Constraints and new insights from an interacting dark energy model cites this paper.

Redshift evolution of the Hubble constant: Constraints and new insights from an interacting dark energy model On Redshift Evolution & Negative Dark Energy Density in Pantheon+ Supernovae

Reference 35

Resolution: verified exact; arxiv_id, observed 2026-05-15T19:30:17.137721Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 24963f8d-3c93-466b-bc5a-61856af07a35 · 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 On Redshift Evolution & Negative Dark Energy Density in Pantheon+ Supernovae

Reference 141

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

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7bf14a47-e96a-4797-bda8-77fc0294ce7c · inbound

Probing cosmic anisotropy with galaxy clusters and supernovae cites this paper.

Probing cosmic anisotropy with galaxy clusters and supernovae On Redshift Evolution & Negative Dark Energy Density in Pantheon+ Supernovae

Reference 61

Resolution: verified exact; arxiv_id, observed 2026-05-10T22:00:49.845066Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation f549d986-e6e6-43c9-99ff-4dc7469de6e3 · 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 On Redshift Evolution & Negative Dark Energy Density in Pantheon+ Supernovae

Reference 119

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 05f900e9-9814-42ae-90c8-f2f3c88933e2 · inbound

Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide cites this paper.

Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide On Redshift Evolution & Negative Dark Energy Density in Pantheon+ Supernovae

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-01T16:29:57.952451Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.