Paper Citation Record · LEDGER

Observational constraints on dynamical dark energy with pivoting redshift

As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:1811.06932.

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

pith.paper-citation-record.v1
1811.06932 v1

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measured 0 of 0 reference resolution

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measured 6 of 6 standing notices

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Source: scholarly_work_events, retraction_status_cache, observed 2026-08-08T06:32:00.761636+00:00

measured 6 of 6 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T18:51:43.896799Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-05-15T11:50:21.318234Z

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Outbound references

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Pith citing papers

Observation 218d8e2d-bbbe-4286-ac9e-5c7759aa2454 · inbound

In the Realm of the Hubble tension $-$ a Review of Solutions cites this paper.

In the Realm of the Hubble tension $-$ a Review of Solutions Observational constraints on dynamical dark energy with pivoting redshift

Reference 153

Resolution: verified exact; local_arxiv, observed 2026-05-15T11:50:21.319667Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation 0362ff81-b573-4933-8168-774871a26d4d · inbound

An overview of what current data can (and cannot yet) say about evolving dark energy cites this paper.

An overview of what current data can (and cannot yet) say about evolving dark energy Observational constraints on dynamical dark energy with pivoting redshift

Reference 170

Resolution: unresolved; no resolver link, observed 2026-08-07T18:51:43.896799Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 052957ce-e6c1-4d42-b0fd-011fe9294f54 · inbound

Constraints on Dark Energy Models Using Late Universe Probes cites this paper.

Constraints on Dark Energy Models Using Late Universe Probes Observational constraints on dynamical dark energy with pivoting redshift

Reference 71

Resolution: unresolved; no resolver link, observed 2026-08-07T00:54:44.684962Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 26204141-f37e-4def-827a-09dec82698f2 · inbound

Observational tests of \texorpdfstring{$\Lambda(t)$}{Lambda(t)} cosmology in light of DESI DR2 cites this paper.

Observational tests of \texorpdfstring{$\Lambda(t)$}{Lambda(t)} cosmology in light of DESI DR2 Observational constraints on dynamical dark energy with pivoting redshift

Reference 45

Resolution: verified exact; arxiv_id, observed 2026-05-10T07:32:00.149893Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation 880f0c3e-cdc2-4a4c-9aca-ed87180c1e4c · inbound

Impact of CMB low-$\ell$ EE polarization data on dark energy parameterizations cites this paper.

Impact of CMB low-$\ell$ EE polarization data on dark energy parameterizations Observational constraints on dynamical dark energy with pivoting redshift

Reference 42

Resolution: unresolved; no resolver link, observed 2026-08-03T02:10:40.515513Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7e11433c-0b8c-4e9b-8fd5-4d7cd0dcf5cb · inbound

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? cites this paper.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Observational constraints on dynamical dark energy with pivoting redshift

Reference 80

Resolution: unresolved; no resolver link, observed 2026-08-06T00:32:11.355467Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.