Paper Citation Record · LEDGER

Galactic Binaries as Sources of Gravitational Waves

As of 24 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:astro-ph/0310800.

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

pith.paper-citation-record.v1
astro-ph/0310800 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 2026-08-23T06:30:58.430688+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-07-11T11:50:26.030339Z

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
unresolved0
parse uncertain0
malformed identifier0
metadata mismatch0

External citation measurements

16
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation dad8e3f8-c73d-4d5a-a750-f2ae17f7316f · inbound

Massquerade: Impacts of Mass Ratio Reversals on Binary Black Hole Merger Rates and Mass Distributions cites this paper.

Massquerade: Impacts of Mass Ratio Reversals on Binary Black Hole Merger Rates and Mass Distributions Galactic Binaries as Sources of Gravitational Waves

Reference 228

Resolution: verified exact; local_arxiv, observed 2026-05-22T09:31:21.402716Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

Observation 334363e5-8f9c-460e-88c4-0bc527eb6920 · inbound

Improving the resolution of double white dwarf systems with spaceborne gravitational wave observatories using a robust astrophysical prior cites this paper.

Improving the resolution of double white dwarf systems with spaceborne gravitational wave observatories using a robust astrophysical prior Galactic Binaries as Sources of Gravitational Waves

Reference 24

Resolution: verified exact; local_arxiv, observed 2026-07-01T21:36:15.843010Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.