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Paper Citation Record · LEDGER

Observational Constraints on Axion(s) Dark Energy with a Cosmological Constant

As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2005.08813.

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

pith.paper-citation-record.v1
2005.08813 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 5 of 5 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 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T21:35:00.500599Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-21T13:30:12.109351Z

Reference resolution

0 of 0 outbound references displayed

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  • 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 4452c86f-2946-478e-bda6-d2e1379d1c79 · inbound

The Lifespan of our Universe cites this paper.

The Lifespan of our Universe Observational Constraints on Axion(s) Dark Energy with a Cosmological Constant

Reference 28

Resolution
unresolved
no resolver link, observed 2026-08-06T21:35:00.500599Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:35:00.500599Z digest=sha256:20ccaf5b9e433de395de84d07922c8c7125d2f25f5849023b25d39d95390ace1

Observation da13ac63-2030-4ff2-92aa-253e2b5a4bc3 · 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 Observational Constraints on Axion(s) Dark Energy with a Cosmological Constant

Reference 159

Resolution
verified exact
arxiv_id, observed 2026-05-18T04:50:54.986846Z

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.

source=pdf_text observed=2026-05-18T04:46:14.832965Z digest=sha256:db848847017a2e95fdfdc5c02383b11857905d8b3e4abe83f13fc15c74b88a9c

Observation f6a16551-f260-4398-8363-c9aa28e65402 · 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 Observational Constraints on Axion(s) Dark Energy with a Cosmological Constant

Reference 113

Resolution
verified exact
arxiv_id, observed 2026-05-21T13:30:12.111144Z

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.

source=pdf_text observed=2026-05-21T13:29:05.147292Z digest=sha256:ca890bbcb02b5ddd384c5f64160805738250301c22421140f517917c329209d1

Observation 5df79d28-a96e-4abd-9b10-8722ac515932 · 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 Observational Constraints on Axion(s) Dark Energy with a Cosmological Constant

Reference 123

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

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-15T12:01:04.317365Z digest=sha256:f99c94eea624e04d0b67ad50cb5b07dcb099b72a6361c3d52b7613f7700547e0

Observation 219b86d6-a50b-49d4-8451-6b103ab792e2 · 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 Observational Constraints on Axion(s) Dark Energy with a Cosmological Constant

Reference 101

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

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-11T09:40:49.196932Z digest=sha256:abac513da075c0b514f88b511c1d6588216d1b16b02d9745702020c6fd5af626