Pith. sign in

Paper Citation Record · LEDGER

Brownian Motion in Gravitationally-Interacting Systems

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/0202257.

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

pith.paper-citation-record.v1
astro-ph/0202257 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 2026-08-07T06:34:17.273281+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-04T00:54:09.102181Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-11T15:51:44.970529Z

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 e1eab51b-3002-425a-b70b-d05f54310ecf · inbound

Self-acceleration of Hardening Binaries cites this paper.

Self-acceleration of Hardening Binaries Brownian Motion in Gravitationally-Interacting Systems

Reference 37

Resolution
verified exact
arxiv_id, observed 2026-07-04T16:29:24.074666Z

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:fc099bbcb754e96df6389f9b1bfff5598055b906c0b148923e09662ae4b321bf

Observation fb2f874f-241f-4094-adb4-581fc214e5a4 · 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 in Gravitationally-Interacting Systems

Reference 55

Resolution
unresolved
no resolver link, observed 2026-08-04T00:54:09.102181Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-04T00:54:09.102181Z digest=sha256:29e80403d8c990c1a24a4ea803a56575977caff77496747ebe911854df9991d4