Paper Citation Record · LEDGER

Tracking and coupled dark energy as seen by WMAP

As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:astro-ph/0303228.

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

pith.paper-citation-record.v1
astro-ph/0303228 v2

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measured 0 of 0 reference resolution

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measured 6 of 6 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-15T06:32:42.880941+00:00

measured 6 of 6 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T15:10:35.748933Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-02T10:36:52.154802Z

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Outbound references

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Pith citing papers

Observation ef43ca48-8422-4c13-baf3-9b6d040aae19 · inbound

Probing the independence within the dark sector in the fluid approximation cites this paper.

Probing the independence within the dark sector in the fluid approximation Tracking and coupled dark energy as seen by WMAP

Reference 13

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:35.748933Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation bccac7f2-d393-490e-a83d-9b441954e930 · inbound

Fractional Dark Matter decay: cosmological imprints and observational constraints cites this paper.

Fractional Dark Matter decay: cosmological imprints and observational constraints Tracking and coupled dark energy as seen by WMAP

Reference 41

Resolution: unresolved; no resolver link, observed 2026-08-14T14:43:27.487949Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7d7bea9b-7406-440f-b9e4-376a71f58a17 · 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 Tracking and coupled dark energy as seen by WMAP

Reference 132

Resolution: unresolved; no resolver link, observed 2026-08-14T13:51:08.726848Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5c0f2508-622e-4bb6-86e9-a1a83f1d5732 · 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 Tracking and coupled dark energy as seen by WMAP

Reference 25

Resolution: unresolved; no resolver link, observed 2026-08-06T18:14:10.571847Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4dd5e589-ad4b-4f1f-950f-51505e0ddc3d · inbound

Dark Energy Is Not That Into You: Variable Couplings after DESI DR2 BAO cites this paper.

Dark Energy Is Not That Into You: Variable Couplings after DESI DR2 BAO Tracking and coupled dark energy as seen by WMAP

Reference 2

Resolution: unresolved; no resolver link, observed 2026-08-05T16:03:01.077423Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f454a2b0-70e7-4523-b21d-5d02acd660f2 · inbound

Dissipative Dark Energy can explain the DESI phantom crossing cites this paper.

Dissipative Dark Energy can explain the DESI phantom crossing Tracking and coupled dark energy as seen by WMAP

Reference 38

Resolution: verified exact; local_arxiv, observed 2026-07-02T10:36:52.156049Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.