Paper Citation Record · LEDGER

Quantifying dimensionality: Bayesian cosmological model complexities

As of 13 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:1903.06682.

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

pith.paper-citation-record.v1
1903.06682 v3

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measured 0 of 0 reference resolution

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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 2026-08-13T06:32:02.005865+00:00

measured 6 of 6 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-10T22:01:00.028422Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-21T11:34:09.179081Z

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External citation measurements

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Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 6494e9f6-24aa-46d6-a05c-f066cc2adb92 · 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? Quantifying dimensionality: Bayesian cosmological model complexities

Reference 90

Resolution: unresolved; no resolver link, observed 2026-08-10T22:01:00.028422Z

Source-reported events for the cited work

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Observation 4507d298-4226-4daf-98a7-012dfced9301 · inbound

Approximating non-Gaussian Bayesian partitions with normalising flows: statistics, inference and application to cosmology cites this paper.

Approximating non-Gaussian Bayesian partitions with normalising flows: statistics, inference and application to cosmology Quantifying dimensionality: Bayesian cosmological model complexities

Reference 4

Resolution: unresolved; no resolver link, observed 2026-08-10T21:29:10.517448Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2ad91111-a33e-4698-b5e2-eed33d2e6d0a · inbound

Updated observational constraints on $\phi$CDM dynamical dark energy cosmological models cites this paper.

Updated observational constraints on $\phi$CDM dynamical dark energy cosmological models Quantifying dimensionality: Bayesian cosmological model complexities

Reference 77

Resolution: unresolved; no resolver link, observed 2026-08-04T13:43:12.348243Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation fcfe5364-351f-4b39-8a87-cbfb6e1be59f · inbound

unimpeded: A Public Grid of Nested Sampling Chains for Cosmological Model Comparison and Tension Analysis cites this paper.

unimpeded: A Public Grid of Nested Sampling Chains for Cosmological Model Comparison and Tension Analysis Quantifying dimensionality: Bayesian cosmological model complexities

Reference 24

Resolution: unresolved; no resolver link, observed 2026-08-03T23:41:00.508538Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9a45bc4f-fd1f-4e0b-bbc8-b2035498b0fb · inbound

The Bayesian view of DESI DR2 with unimpeded: Evidence and tension in a combined analysis with CMB and supernovae across cosmological models cites this paper.

The Bayesian view of DESI DR2 with unimpeded: Evidence and tension in a combined analysis with CMB and supernovae across cosmological models Quantifying dimensionality: Bayesian cosmological model complexities

Reference 20

Resolution: verified exact; arxiv_id, observed 2026-05-21T11:34:09.181284Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

Observation e7a3d29c-4a34-40b8-ad9b-3dbd6a0d3953 · inbound

Is the $w_0w_a$CDM cosmological parameterization evidence for dark energy dynamics partially caused by the excess smoothing of Planck PR4 CMB anisotropy data? cites this paper.

Is the $w_0w_a$CDM cosmological parameterization evidence for dark energy dynamics partially caused by the excess smoothing of Planck PR4 CMB anisotropy data? Quantifying dimensionality: Bayesian cosmological model complexities

Reference 87

Resolution: verified exact; arxiv_id, observed 2026-05-13T17:38:03.053781Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.