Paper Citation Record · LEDGER

Implications of the possible 21-cm line excess at cosmic dawn on dynamics of interacting dark energy

As of 16 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 8 inbound Pith citation observations for arXiv:1904.02458.

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

pith.paper-citation-record.v1
1904.02458 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 8 of 8 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-16T06:30:59.297886+00:00

measured 8 of 8 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T14:30:02.155652Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-01T16:45:51.042661Z

Reference resolution

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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 782e4524-c99f-4838-90e3-fc6d50fc6318 · inbound

Quantifying the impacts of future gravitational-wave data on constraining interacting dark energy cites this paper.

Quantifying the impacts of future gravitational-wave data on constraining interacting dark energy Implications of the possible 21-cm line excess at cosmic dawn on dynamics of interacting dark energy

Reference 98

Resolution: unresolved; no resolver link, observed 2026-08-14T14:30:02.155652Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6fa1fc81-f1c1-43fc-89d1-1077d47965e4 · inbound

Improving cosmological parameter estimation with the future 21 cm observation from SKA cites this paper.

Improving cosmological parameter estimation with the future 21 cm observation from SKA Implications of the possible 21-cm line excess at cosmic dawn on dynamics of interacting dark energy

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-14T14:07:51.314442Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 621378cd-112b-4cb5-9604-19ae1ad9ad2c · inbound

Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions cites this paper.

Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions Implications of the possible 21-cm line excess at cosmic dawn on dynamics of interacting dark energy

Reference 227

Resolution: unresolved; no resolver link, observed 2026-08-14T13:51:09.072544Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation dd712609-d650-41d2-98b5-f88c33510e5e · inbound

Interacting phantom dark energy: new accelerating scaling attractors cites this paper.

Interacting phantom dark energy: new accelerating scaling attractors Implications of the possible 21-cm line excess at cosmic dawn on dynamics of interacting dark energy

Reference 82

Resolution: unresolved; no resolver link, observed 2026-08-12T11:29:07.746475Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation bab54569-4475-4c6e-b9b4-7ea617c51724 · inbound

Solving an Interacting Quintessence Model with a Sound Horizon Initial Condition and its Observational Constraints cites this paper.

Solving an Interacting Quintessence Model with a Sound Horizon Initial Condition and its Observational Constraints Implications of the possible 21-cm line excess at cosmic dawn on dynamics of interacting dark energy

Reference 65

Resolution: unresolved; no resolver link, observed 2026-08-06T18:14:14.231693Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0fbf7205-c399-47bc-9032-b23d0b3361cf · inbound

Accelerating scaling solutions from dark matter particle creation cites this paper.

Accelerating scaling solutions from dark matter particle creation Implications of the possible 21-cm line excess at cosmic dawn on dynamics of interacting dark energy

Reference 51

Resolution: malformed identifier; arxiv_id, observed 2026-05-11T14:36:08.102301Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

Observation 34852ca0-461d-4a78-9df3-8bdbd82718e2 · inbound

Accelerating scaling solutions from dark matter particle creation cites this paper.

Accelerating scaling solutions from dark matter particle creation Implications of the possible 21-cm line excess at cosmic dawn on dynamics of interacting dark energy

Reference 45

Resolution: unresolved; no resolver link, observed 2026-07-12T18:37:05.978670Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 80dccf93-3b68-4bf3-a572-8c57b4850cfa · inbound

Unifying Early and Late Dark Energy: Dynamical Requirements and Obstructions cites this paper.

Unifying Early and Late Dark Energy: Dynamical Requirements and Obstructions Implications of the possible 21-cm line excess at cosmic dawn on dynamics of interacting dark energy

Reference 163

Resolution: verified exact; arxiv_id, observed 2026-07-01T16:45:51.044337Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.