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 4 inbound Pith citation observations for arXiv:2405.03983.

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

pith.paper-citation-record.v1
2405.03983 v4

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 4 of 4 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-11T06:34:44.6726+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T13:41:23.970701Z

measured 0 of 1 external citation measurements

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

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 d4c8e8af-36bc-4673-901a-7f99a3a4a0d3 · inbound

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? cites this paper.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? Key drivers of the preference for dynamic dark energy

Reference 110

Resolution: unresolved; no resolver link, observed 2026-08-11T13:41:23.970701Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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 2026-08-11T06:34:44.6726+00:00.