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Paper Citation Record · LEDGER

The Gravitational Million-Body Problem

As of 21 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:astro-ph/0111045.

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

pith.paper-citation-record.v1
astro-ph/0111045 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 3 of 3 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-21T06:32:19.484+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-09T22:57:34.059504Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-10T12:15:01.137692Z

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 7a18d42b-e7fb-49c0-9b66-03b25e7467a4 · inbound

Localizing Dynamically-Formed Black Hole Binaries in Milky Way Globular Clusters with LISA cites this paper.

Localizing Dynamically-Formed Black Hole Binaries in Milky Way Globular Clusters with LISA The Gravitational Million-Body Problem

Reference 47

Resolution
unresolved
no resolver link, observed 2026-08-09T22:57:34.059504Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-09T22:57:34.059504Z digest=sha256:f1416614105cd57441bbc933ce581535b557b63fc19658a37d410d3c7ac8b044

Observation eee052ed-0523-434e-a990-ab6760da2a4d · inbound

Stellar Dynamics in Open Clusters Increases the Binary Fraction and Mass Ratios: Evidence from Photometric Binaries in 35 Open Clusters cites this paper.

Stellar Dynamics in Open Clusters Increases the Binary Fraction and Mass Ratios: Evidence from Photometric Binaries in 35 Open Clusters The Gravitational Million-Body Problem

Reference 28

Resolution
unresolved
no resolver link, observed 2026-08-06T22:44:27.732934Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T22:44:27.732934Z digest=sha256:09077b933601b56b05a12cb4a0e82688db4a345e002b6ec9824e8a0814f9168b

Observation 7fb68b4b-beda-4e22-a639-ae6d53da7e0a · inbound

Solving Inverse Problems of Chaotic Systems with Bidirectional Conditional Flow Matching cites this paper.

Solving Inverse Problems of Chaotic Systems with Bidirectional Conditional Flow Matching The Gravitational Million-Body Problem

Reference 55

Resolution
metadata mismatch
local_arxiv, observed 2026-06-25T23:18:40.514679Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

source=pdf_text observed=2026-06-25T23:18:24.145654Z digest=sha256:71bd18075189513344bb4f0d7ad8314840ec78c039cddac7e0cf849ce7fd3a0d