Paper Citation Record · LEDGER

Cosmological model selection

As of 22 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:astro-ph/0608184.

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

pith.paper-citation-record.v1
astro-ph/0608184 v1

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 2026-08-22T06:32:14.747728+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-12T13:51:30.616909Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-05-18T10:46:16.350751Z

Reference resolution

0 of 0 outbound references displayed

verified exact0
verified fuzzy0
unresolved0
parse uncertain0
malformed identifier0
metadata mismatch0

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 8f6c2812-e4a9-4ef9-bb75-c3e17ff27a69 · inbound

General parametrization for energy density of quintessence field cites this paper.

General parametrization for energy density of quintessence field Cosmological model selection

Reference 58

Resolution: unresolved; no resolver link, observed 2026-08-12T13:51:30.616909Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6c6eb350-e156-42bf-9128-3699b9da906c · inbound

Beyond CPL: Evidence for dynamical dark energy in three-parameter models cites this paper.

Beyond CPL: Evidence for dynamical dark energy in three-parameter models Cosmological model selection

Reference 101

Resolution: verified exact; local_arxiv, observed 2026-05-18T10:46:16.353310Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

Observation 1d8a79ab-a6a8-41d8-815a-372a246ee840 · inbound

Probing the sensitivity of dark energy dynamics to equation of state parametrization flexibility cites this paper.

Probing the sensitivity of dark energy dynamics to equation of state parametrization flexibility Cosmological model selection

Reference 33

Resolution: verified exact; local_arxiv, observed 2026-05-16T21:18:32.683826Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

Observation da4c5a74-dda3-41d1-a0ec-3aa3f2f5f921 · inbound

Observational constraints on early time non-phantom behaviour of dynamical dark energy cites this paper.

Observational constraints on early time non-phantom behaviour of dynamical dark energy Cosmological model selection

Reference 113

Resolution: unresolved; no resolver link, observed 2026-08-03T14:40:55.597286Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.