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Paper Citation Record · LEDGER

Confronting interacting dark radiation scenarios with cosmological data

As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2212.13264.

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

pith.paper-citation-record.v1
2212.13264 v2

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 2026-08-18T06:34:40.430872+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-15T14:31:27.087502Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-20T04:08:02.987961Z

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 3ff149f6-d48b-4fa1-aefa-68743c42259b · inbound

Atomic Dark Matter, Interacting Dark Radiation, and the Hubble Tension cites this paper.

Atomic Dark Matter, Interacting Dark Radiation, and the Hubble Tension Confronting interacting dark radiation scenarios with cosmological data

Reference 31

Resolution
unresolved
no resolver link, observed 2026-08-12T22:01:20.758616Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 6e132ca9-d551-494d-b754-2d29e40ba34a · inbound

BAO miscalibration cannot rescue late-time solutions to the Hubble tension cites this paper.

BAO miscalibration cannot rescue late-time solutions to the Hubble tension Confronting interacting dark radiation scenarios with cosmological data

Reference 53

Resolution
unresolved
no resolver link, observed 2026-08-04T12:53:36.552997Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T12:53:36.552997Z digest=sha256:2765704f9c9c8d71521f4bc235fb71b96953146cbf81f1f7fa97579a1042d97e

Observation d963a69b-daf8-47ca-ab5a-e52b60428a27 · inbound

Dark Matter Interpretation of the Super-Kamiokande Antineutrino Excess and Predictions for JUNO cites this paper.

Dark Matter Interpretation of the Super-Kamiokande Antineutrino Excess and Predictions for JUNO Confronting interacting dark radiation scenarios with cosmological data

Reference 64

Resolution
verified exact
arxiv_id, observed 2026-05-20T04:08:02.991379Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-05-20T04:04:42.736350Z digest=sha256:bbca4f0759e27fffbaa488156b53b5f1243d17e6446063ea5743634a6a0bb918

Observation fce7a7ca-88ed-4ddd-b9b2-b7dc5739d6c2 · inbound

Sensitivity of Next-Generation CMB Surveys to Neutrinos and Other Light Relics cites this paper.

Sensitivity of Next-Generation CMB Surveys to Neutrinos and Other Light Relics Confronting interacting dark radiation scenarios with cosmological data

Reference 230

Resolution
unresolved
no resolver link, observed 2026-08-15T14:31:27.087502Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-15T14:31:27.087502Z digest=sha256:cb80cacd90ebdb7d310864aac372b11f5575cb4493929b75330bceea0a4e9e59