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Paper Citation Record · LEDGER

Cosmological constraints on coupled dark energy

As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:1608.07039.

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

pith.paper-citation-record.v1
1608.07039 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 2026-08-15T06:32:42.880941+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T15:10:36.587280Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-14T15:10:36.832207Z

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 7431663c-3777-4440-9e1e-62796678ee9a · 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 Cosmological constraints on coupled dark energy

Reference 100

Resolution
verified exact
local_arxiv, observed 2026-08-14T15:10:36.840250Z

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.

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Observation 0ae0b10e-aff7-4691-933c-c6d3d8b1dec4 · 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 Cosmological constraints on coupled dark energy

Reference 202

Resolution
unresolved
no resolver link, observed 2026-08-14T13:51:08.981186Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T13:51:08.981186Z digest=sha256:9369451e630467046029c106c9171c4a0e252389a3e9907945b7027644fa9bdd

Observation 53bce818-c1f2-4acb-99aa-41edfa7df704 · 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 Cosmological constraints on coupled dark energy

Reference 48

Resolution
unresolved
no resolver link, observed 2026-08-06T18:14:13.571566Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T18:14:13.571566Z digest=sha256:639c39ddb537a2d097fccaf477612f2d879c1b8b5a68996d5a32698c49f64d65

Observation 06517b78-2724-45a4-b3ab-bdbf705a3dbc · 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 Cosmological constraints on coupled dark energy

Reference 38

Resolution
unresolved
no resolver link, observed 2026-08-05T16:03:01.194188Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-05T16:03:01.194188Z digest=sha256:58ca9f0db86acc629dd2883afa57644f52234d87f13e35088e014e7d729e457f