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Paper Citation Record · LEDGER

Brownian Motion of a Massive Binary

As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:astro-ph/0012264.

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

pith.paper-citation-record.v1
astro-ph/0012264 v2

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 2026-08-07T06:34:17.273281+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-04T00:54:09.269445Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-11T15:56:06.158350Z

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 ed09e7e0-27eb-47e8-b339-c1c983bef270 · inbound

Self-acceleration of Hardening Binaries cites this paper.

Self-acceleration of Hardening Binaries Brownian Motion of a Massive Binary

Reference 30

Resolution
verified exact
arxiv_id, observed 2026-07-04T16:17:47.120106Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=pdf_text observed=2026-05-09T19:04:20.072429Z digest=sha256:6daeda4f0327d4591fc34375d65e79d10ef4ed43ecfeea78e550471465f0db64

Observation ad11299b-fb24-4e67-b053-f05016de5c0a · inbound

On an empirical method to build near-equilibrium axisymmetric and triaxial galaxy models cites this paper.

On an empirical method to build near-equilibrium axisymmetric and triaxial galaxy models Brownian Motion of a Massive Binary

Reference 57

Resolution
unresolved
no resolver link, observed 2026-08-04T00:54:09.269445Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-04T00:54:09.269445Z digest=sha256:ba44e976729e041c6d8d2babd2de8a750e8f60bb303cdde296a302695dcf0f43