Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Key drivers of the preference for dynamic dark energy
As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2405.03983.
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 2026-08-10T06:31:04.303077+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-10T22:00:59.764065Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-05-19T05:22:06.250398Z
Reference resolution
0 of 0 outbound references displayed
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- 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 3c0ccfa2-5377-414b-bba3-9781a2d0351b · inbound
Is excess smoothing of Planck CMB ansiotropy data partially responsible for evidence for dark energy dynamics in other $w(z)$CDM parametrizations? cites this paper.
Is excess smoothing of Planck CMB ansiotropy data partially responsible for evidence for dark energy dynamics in other $w(z)$CDM parametrizations? Key drivers of the preference for dynamic dark energy
Reference 21
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T22:00:59.764065Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation d019e1fb-6651-4ded-9756-9f46efe8e655 · inbound
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae cites this paper.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae Key drivers of the preference for dynamic dark energy
Reference 70
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:12:26.195708Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 19ae6e2f-0629-439e-aa2d-117227d075be · inbound
New Insights into Dark Energy from DESI DR2 with CMB and SNIa cites this paper.
New Insights into Dark Energy from DESI DR2 with CMB and SNIa Key drivers of the preference for dynamic dark energy
Reference 51
- Resolution
- verified exact
- arxiv_id, observed 2026-05-19T05:22:06.253083Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.