Paper Citation Record · LEDGER

Cosmological structure formation in a homogeneous dark energy background

As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:astro-ph/0508156.

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

pith.paper-citation-record.v1
astro-ph/0508156 v4

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 2026-08-18T06:34:40.430872+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-12T12:45:53.163213Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-06-29T03:13:04.110227Z

Reference resolution

0 of 0 outbound references displayed

verified exact0
verified fuzzy0
unresolved0
parse uncertain0
malformed identifier0
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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 edc263df-437c-480c-b24a-3f85525195f0 · inbound

Super sample covariance and the volume scaling of galaxy survey covariance matrices cites this paper.

Super sample covariance and the volume scaling of galaxy survey covariance matrices Cosmological structure formation in a homogeneous dark energy background

Reference 75

Resolution: unresolved; no resolver link, observed 2026-08-12T12:45:53.163213Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e41bfba6-25e8-4384-8f74-4a691d2becae · inbound

Cosmo-Learn: code for learning cosmology using different methods and mock data cites this paper.

Cosmo-Learn: code for learning cosmology using different methods and mock data Cosmological structure formation in a homogeneous dark energy background

Reference 87

Resolution: unresolved; no resolver link, observed 2026-08-05T14:43:16.579694Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2d4a2bea-9e9b-4ed3-969a-b451352f653a · inbound

Large-scale structures of the Universe: physics, phenomenology, statistics cites this paper.

Large-scale structures of the Universe: physics, phenomenology, statistics Cosmological structure formation in a homogeneous dark energy background

Reference 93

Resolution: metadata mismatch; local_arxiv, observed 2026-06-29T03:13:04.111565Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation 372af385-9548-4041-b69a-289bdddbe015 · inbound

Decaying Dark Matter Halo Abundance from a Revised Spherical Collapse Model cites this paper.

Decaying Dark Matter Halo Abundance from a Revised Spherical Collapse Model Cosmological structure formation in a homogeneous dark energy background

Reference 94

Resolution: unresolved; no resolver link, observed 2026-08-01T13:07:58.367289Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.