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Paper Citation Record · LEDGER

$\Lambda$CDM model against cosmography: A possible deviation after DESI 2024

As of 22 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:2408.10704.

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

pith.paper-citation-record.v1
2408.10704 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 6 of 6 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-22T06:32:14.747728+00:00

measured 6 of 6 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-15T17:14:14.408010Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-10T07:32:00.084823Z

Reference resolution

0 of 0 outbound references displayed

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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 49175ee4-5c6c-424d-a9cf-2e671a098038 · 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? $\Lambda$CDM model against cosmography: A possible deviation after DESI 2024

Reference 84

Resolution
unresolved
no resolver link, observed 2026-08-11T13:41:23.874531Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-11T13:41:23.874531Z digest=sha256:ea270c1f8910b099b9ee0391c881edf4842a3561a73bdd004a389ebca686e2d5

Observation f6fcb6af-7a6a-47aa-9ad0-e0307c521048 · 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? $\Lambda$CDM model against cosmography: A possible deviation after DESI 2024

Reference 45

Resolution
unresolved
no resolver link, observed 2026-08-10T22:00:59.850724Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T22:00:59.850724Z digest=sha256:9dab629ba6faa5fe90b485477ce400b6f2684761e8a3be7b0486da2454f50152

Observation 90e94442-b9ae-442a-a0d3-7cd9fc6fd8e2 · inbound

Testing $\gamma\delta$CDM Model in the Redshift Bins cites this paper.

Testing $\gamma\delta$CDM Model in the Redshift Bins $\Lambda$CDM model against cosmography: A possible deviation after DESI 2024

Reference 115

Resolution
unresolved
no resolver link, observed 2026-08-10T20:48:22.802368Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T20:48:22.802368Z digest=sha256:227d817f7e3d58a6c09bcc13cb870652592ae1d69e4a962806ff2ef54cd42423

Observation d7e8f505-2cef-488a-82fc-6492d39a90e7 · inbound

Sign Switching in Dark Sector Coupling Interactions as a Candidate for Resolving Cosmological Tensions cites this paper.

Sign Switching in Dark Sector Coupling Interactions as a Candidate for Resolving Cosmological Tensions $\Lambda$CDM model against cosmography: A possible deviation after DESI 2024

Reference 41

Resolution
unresolved
no resolver link, observed 2026-08-10T19:20:16.580865Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T19:20:16.580865Z digest=sha256:e4fcf243b7ccb410d26bc816aff16792615e5eaf793ea647f5a50a6a0ba1510e

Observation 561719ee-248b-4d56-9bfe-8ca0349db6a0 · inbound

Exact Solutions for a Teleparallel Cosmological Model with Vector Field via Noether Symmetry cites this paper.

Exact Solutions for a Teleparallel Cosmological Model with Vector Field via Noether Symmetry $\Lambda$CDM model against cosmography: A possible deviation after DESI 2024

Reference 69

Resolution
unresolved
no resolver link, observed 2026-08-15T17:14:14.408010Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-15T17:14:14.408010Z digest=sha256:d926c2fc923e08ce8331703ac9234612703177cf0624ebeea39b79136d62bd1c

Observation 04107a0e-8786-478b-b1a0-834c37931016 · inbound

Observational tests of \texorpdfstring{$\Lambda(t)$}{Lambda(t)} cosmology in light of DESI DR2 cites this paper.

Observational tests of \texorpdfstring{$\Lambda(t)$}{Lambda(t)} cosmology in light of DESI DR2 $\Lambda$CDM model against cosmography: A possible deviation after DESI 2024

Reference 18

Resolution
verified exact
arxiv_id, observed 2026-05-10T07:32:00.087872Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

source=pdf_text observed=2026-05-10T07:29:51.699632Z digest=sha256:759d6bdd0eeb22566055e817fcbb16afe03fea7f80885afd6112e7ad65e83f00