Paper Citation Record · LEDGER

Comparison of dark energy models using late-universe observations

As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 8 inbound Pith citation observations for arXiv:2504.09054.

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

pith.paper-citation-record.v1
2504.09054 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 8 of 8 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 8 of 8 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T00:54:46.931376Z

measured 1 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-08-05T02:28:24.338817Z

Reference resolution

0 of 0 outbound references displayed

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External citation measurements

0
arxiv_reference, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation a6fe9f65-3225-4a26-92f9-973498ff587b · inbound

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

Constraints on Dark Energy Models Using Late Universe Probes Comparison of dark energy models using late-universe observations

Reference 100

Resolution: unresolved; no resolver link, observed 2026-08-07T00:54:46.931376Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 038d66db-ecd9-4637-b5f0-ce489aa9ab78 · inbound

Interacting Scalar Fields as Dark Energy and Dark Matter in Einstein scalar Gauss Bonnet Gravity cites this paper.

Interacting Scalar Fields as Dark Energy and Dark Matter in Einstein scalar Gauss Bonnet Gravity Comparison of dark energy models using late-universe observations

Reference 35

Resolution: verified exact; arxiv_id, observed 2026-05-19T05:57:07.833219Z

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 0724a701-c628-4b3b-9954-07bca7a0d438 · inbound

Exploring non-cold dark matter in a scenario of dynamical dark energy with DESI DR2 data cites this paper.

Exploring non-cold dark matter in a scenario of dynamical dark energy with DESI DR2 data Comparison of dark energy models using late-universe observations

Reference 39

Resolution: unresolved; no resolver link, observed 2026-08-06T18:36:59.481657Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation cf9440c0-6646-4f4e-a8cb-7f5175104bc1 · inbound

Cosmological preference for a positive neutrino mass at 2.7$\sigma$: A joint analysis of DESI DR2, DESY5, and DESY1 data cites this paper.

Cosmological preference for a positive neutrino mass at 2.7$\sigma$: A joint analysis of DESI DR2, DESY5, and DESY1 data Comparison of dark energy models using late-universe observations

Reference 26

Resolution: unresolved; no resolver link, observed 2026-08-06T15:12:33.766556Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation cac0d362-af4e-424e-8f08-6033254f75b1 · inbound

Interacting $k$-essence field with non-pressureless Dark Matter: Cosmological Dynamics and Observational Constraints cites this paper.

Interacting $k$-essence field with non-pressureless Dark Matter: Cosmological Dynamics and Observational Constraints Comparison of dark energy models using late-universe observations

Reference 44

Resolution: verified exact; arxiv_id, observed 2026-05-18T18:16:43.647616Z

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 483df286-2842-4726-85c7-7cd4e30435db · inbound

Synergy between CSST and third-generation gravitational-wave detectors: Inferring cosmological parameters using cross-correlation of dark sirens and galaxies cites this paper.

Synergy between CSST and third-generation gravitational-wave detectors: Inferring cosmological parameters using cross-correlation of dark sirens and galaxies Comparison of dark energy models using late-universe observations

Reference 23

Resolution: verified exact; arxiv_id, observed 2026-05-18T04:50:53.864596Z

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 1592ad51-49af-4c1d-bf4b-df448f280822 · inbound

Model-independent late-universe measurements of $H_0$ and $\Omega_K$ with the parametrization based on cosmic age-improved inverse distance ladder cites this paper.

Model-independent late-universe measurements of $H_0$ and $\Omega_K$ with the parametrization based on cosmic age-improved inverse distance ladder Comparison of dark energy models using late-universe observations

Reference 97

Resolution: unresolved; no resolver link, observed 2026-08-04T07:19:40.282572Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d89aea2e-eafa-409d-82aa-f51ab3f36bcf · inbound

Evidence for deviation in gravitational light deflection from general relativity at cosmological scales with KiDS-Legacy and CMB lensing cites this paper.

Evidence for deviation in gravitational light deflection from general relativity at cosmological scales with KiDS-Legacy and CMB lensing Comparison of dark energy models using late-universe observations

Reference 88

Resolution: verified exact; arxiv_id, observed 2026-05-16T08:17:35.562592Z

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.