Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Solving the Hubble tension at intermediate redshifts with dynamical dark energy
As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2311.16862.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-12T06:34:41.77262+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-12T04:57:06.700643Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-07-03T21:58:58.799998Z
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 9e065f8f-59e2-41bf-8a59-ff742b040c96 · inbound
Exploring cosmological imprints of phantom crossing with dynamical dark energy in Horndeski gravity cites this paper.
Exploring cosmological imprints of phantom crossing with dynamical dark energy in Horndeski gravity Solving the Hubble tension at intermediate redshifts with dynamical dark energy
Reference 18
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T04:57:06.700643Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation b8951f4b-bb97-4572-8a9d-a2652a97ae46 · inbound
The case for a low dark matter density in dynamical dark energy model from local probes cites this paper.
The case for a low dark matter density in dynamical dark energy model from local probes Solving the Hubble tension at intermediate redshifts with dynamical dark energy
Reference 24
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T20:19:23.872647Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 07c369e3-4f64-4702-8fe9-500e2e03ef01 · inbound
New constraints on cosmic anisotropy from galaxy clusters using an improved dipole fitting method cites this paper.
New constraints on cosmic anisotropy from galaxy clusters using an improved dipole fitting method Solving the Hubble tension at intermediate redshifts with dynamical dark energy
Reference 33
- Resolution
- verified exact
- arxiv_id, observed 2026-05-16T02:27:09.979872Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation f3862169-179c-4e27-8322-88c2c8d41188 · inbound
Alleviating the Hubble tension with the $\Lambda_{\omega_s}$CDM model cites this paper.
Alleviating the Hubble tension with the $\Lambda_{\omega_s}$CDM model Solving the Hubble tension at intermediate redshifts with dynamical dark energy
Reference 21
- Resolution
- verified exact
- arxiv_id, observed 2026-07-03T21:58:58.801691Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 5274031f-5d09-4608-a1fe-d62adee0ab53 · inbound
Growth, geometry, and early-universe split of the matter density parameter $\Omega_{\rm m}$ cites this paper.
Growth, geometry, and early-universe split of the matter density parameter $\Omega_{\rm m}$ Solving the Hubble tension at intermediate redshifts with dynamical dark energy
Reference 118
- Resolution
- unresolved
- no resolver link, observed 2026-07-31T11:14:47.055670Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.