Paper Citation Record · LEDGER

Gravitational waves from cosmological compact binaries

As of 22 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:astro-ph/0002055.

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

pith.paper-citation-record.v1
astro-ph/0002055 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 2 of 2 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 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T14:30:02.404226Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-12T04:42:53.137407Z

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 cdfd2aaa-8bf4-4986-bfe7-a64f91868406 · inbound

Quantifying the impacts of future gravitational-wave data on constraining interacting dark energy cites this paper.

Quantifying the impacts of future gravitational-wave data on constraining interacting dark energy Gravitational waves from cosmological compact binaries

Reference 149

Resolution: unresolved; no resolver link, observed 2026-08-14T14:30:02.404226Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8deb56dc-003f-4e6e-857f-e4225d253241 · inbound

Estimating the gravitational wave background anisotropy: a Bayesian approach boosted by cross-correlation angular power spectrum cites this paper.

Estimating the gravitational wave background anisotropy: a Bayesian approach boosted by cross-correlation angular power spectrum Gravitational waves from cosmological compact binaries

Reference 8

Resolution: verified exact; local_arxiv, observed 2026-08-12T04:42:53.141704Z

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.