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Paper Citation Record · LEDGER

CMB distance priors revisited: effects of dark energy dynamics, spatial curvature, primordial power spectrum, and neutrino parameters

As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 10 inbound Pith citation observations for arXiv:1912.04921.

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

pith.paper-citation-record.v1
1912.04921 v3

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 10 of 10 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-18T06:34:40.430872+00:00

measured 10 of 10 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T18:15:34.161432Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-03T23:09:01.429977Z

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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 99c89cf8-8d12-486e-8b5c-094aa0f73f12 · inbound

Improving cosmological constraints via galaxy intrinsic alignment in full-shape analysis cites this paper.

Improving cosmological constraints via galaxy intrinsic alignment in full-shape analysis CMB distance priors revisited: effects of dark energy dynamics, spatial curvature, primordial power spectrum, and neutrino parameters

Reference 120

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Observation c457d27f-c50d-4ce7-b820-396faa304647 · inbound

A comprehensive numerical study on four categories of holographic dark energy models cites this paper.

A comprehensive numerical study on four categories of holographic dark energy models CMB distance priors revisited: effects of dark energy dynamics, spatial curvature, primordial power spectrum, and neutrino parameters

Reference 127

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no resolver link, observed 2026-08-11T17:28:35.790645Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 8b558ec4-1c64-425a-b8b8-97783167432c · inbound

Controlled Tension Forecasting: Quantifying Cross-Probe Biases in $\omega_0\omega_a$CDM cites this paper.

Controlled Tension Forecasting: Quantifying Cross-Probe Biases in $\omega_0\omega_a$CDM CMB distance priors revisited: effects of dark energy dynamics, spatial curvature, primordial power spectrum, and neutrino parameters

Reference 56

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Observation 9dd99d24-c2f1-438d-8218-8e727dd6817b · inbound

Redshift evolution of the Hubble constant: Constraints and new insights from an interacting dark energy model cites this paper.

Redshift evolution of the Hubble constant: Constraints and new insights from an interacting dark energy model CMB distance priors revisited: effects of dark energy dynamics, spatial curvature, primordial power spectrum, and neutrino parameters

Reference 99

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verified exact
arxiv_id, observed 2026-05-15T19:30:17.263669Z

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Observation 29d8ab33-9f4f-4d45-bfe9-7e5a9c026559 · inbound

Cosmological constraints on the big bang quantum cosmology model cites this paper.

Cosmological constraints on the big bang quantum cosmology model CMB distance priors revisited: effects of dark energy dynamics, spatial curvature, primordial power spectrum, and neutrino parameters

Reference 72

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arxiv_id, observed 2026-05-14T23:43:18.327145Z

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Observation d7adf64a-f91b-42e2-8d03-4f6680f6c65e · inbound

Forecasting neutrino mass constraints from the Nancy Grace Roman Space Telescope cites this paper.

Forecasting neutrino mass constraints from the Nancy Grace Roman Space Telescope CMB distance priors revisited: effects of dark energy dynamics, spatial curvature, primordial power spectrum, and neutrino parameters

Reference 98

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arxiv_id, observed 2026-05-10T10:49:57.158821Z

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Observation 7736d859-33f7-49e1-bcc8-63dc6ad7681e · inbound

No evidence for phantom crossing: local goodness-of-fit improvements do not persist under global Bayesian model comparison cites this paper.

No evidence for phantom crossing: local goodness-of-fit improvements do not persist under global Bayesian model comparison CMB distance priors revisited: effects of dark energy dynamics, spatial curvature, primordial power spectrum, and neutrino parameters

Reference 25

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Observation a400d70b-ab33-479b-a848-79330f4f2094 · inbound

No evidence for phantom crossing: local goodness-of-fit improvements do not persist under global Bayesian model comparison cites this paper.

No evidence for phantom crossing: local goodness-of-fit improvements do not persist under global Bayesian model comparison CMB distance priors revisited: effects of dark energy dynamics, spatial curvature, primordial power spectrum, and neutrino parameters

Reference 29

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arxiv_id, observed 2026-05-21T08:19:52.308177Z

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Observation b515bc6f-0201-4804-8872-eee927118411 · inbound

CMBComp: A Simple and Accurate Compressed CMB Likelihood for Dark Energy, Curvature, and Massive Neutrinos cites this paper.

CMBComp: A Simple and Accurate Compressed CMB Likelihood for Dark Energy, Curvature, and Massive Neutrinos CMB distance priors revisited: effects of dark energy dynamics, spatial curvature, primordial power spectrum, and neutrino parameters

Reference 10

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arxiv_id, observed 2026-07-03T23:09:01.431940Z

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Observation 7f597b46-0acb-49f1-b6de-7083e594c454 · inbound

Modified Cosmology from Mass-to-Horizon Relation: Observational Bounds cites this paper.

Modified Cosmology from Mass-to-Horizon Relation: Observational Bounds CMB distance priors revisited: effects of dark energy dynamics, spatial curvature, primordial power spectrum, and neutrino parameters

Reference 36

Resolution
unresolved
no resolver link, observed 2026-08-01T15:16:19.844192Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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