Paper Citation Record · LEDGER

Measuring the effective complexity of cosmological models

As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:astro-ph/0602378.

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

pith.paper-citation-record.v1
astro-ph/0602378 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 6 of 6 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-09T06:31:02.800959+00:00

measured 6 of 6 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T00:32:11.995298Z

measured 1 of 1 external citation measurements

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

Source: pith, observed 2026-08-05T02:28:24.338817Z

Reference resolution

0 of 0 outbound references displayed

verified exact0
verified fuzzy0
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External citation measurements

161
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 0629cc1e-514f-461c-b309-1fed7ff9b0cb · inbound

A barotropic alternative to Early Dark Energy for alleviating the $H_0$ tension cites this paper.

A barotropic alternative to Early Dark Energy for alleviating the $H_0$ tension Measuring the effective complexity of cosmological models

Reference 70

Resolution: verified exact; arxiv_id, observed 2026-05-11T12:11:05.546707Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation a8625b01-f423-4dd1-8d9e-e35390b977e0 · inbound

KiDS+VIKING-450 cosmology with Bayesian hierarchical model redshift distributions cites this paper.

KiDS+VIKING-450 cosmology with Bayesian hierarchical model redshift distributions Measuring the effective complexity of cosmological models

Reference 159

Resolution: verified exact; local_arxiv, observed 2026-05-15T03:24:53.404717Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 94c3093b-4383-4495-803f-b23247e91306 · inbound

Bounding the Effect of HOD Assumptions on Small-Scale Clustering Constraints cites this paper.

Bounding the Effect of HOD Assumptions on Small-Scale Clustering Constraints Measuring the effective complexity of cosmological models

Reference 83

Resolution: verified exact; local_arxiv, observed 2026-06-27T11:10:52.089961Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 23169784-7b16-478a-8d5a-14af7270e548 · inbound

Impact of CMB low-$\ell$ EE polarization data on dark energy parameterizations cites this paper.

Impact of CMB low-$\ell$ EE polarization data on dark energy parameterizations Measuring the effective complexity of cosmological models

Reference 74

Resolution: unresolved; no resolver link, observed 2026-08-03T02:10:44.122626Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 71fe9f14-7362-469b-8981-4ef253190cdc · inbound

The macroscopic precession model of quasi-periodic oscillations for rotating compact objects cites this paper.

The macroscopic precession model of quasi-periodic oscillations for rotating compact objects Measuring the effective complexity of cosmological models

Reference 20

Resolution: unresolved; no resolver link, observed 2026-08-01T05:11:58.554486Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 441b6466-e4d6-4953-8d59-28e0c456c57d · inbound

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? cites this paper.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Measuring the effective complexity of cosmological models

Reference 99

Resolution: unresolved; no resolver link, observed 2026-08-06T00:32:11.995298Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.