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Paper Citation Record · LEDGER

Dynamics of a Massive Black Hole at the Center of a Dense Stellar System

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/0107287.

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

pith.paper-citation-record.v1
astro-ph/0107287 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 2026-08-04T00:54:09.043213Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-11T15:51:44.868443Z

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 fd0b9844-d670-48f4-8b50-6f7ba81c2438 · inbound

Self-acceleration of Hardening Binaries cites this paper.

Self-acceleration of Hardening Binaries Dynamics of a Massive Black Hole at the Center of a Dense Stellar System

Reference 36

Resolution
verified exact
arxiv_id, observed 2026-07-04T16:23:42.867597Z

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=sha256:0193c3602711870365603f70400d5d4dcc7ff36f52b42dc7fbf296c71f3c5866

Observation 3ea52d38-08c7-45ae-afdb-16a5b7f92fb1 · 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 Dynamics of a Massive Black Hole at the Center of a Dense Stellar System

Reference 54

Resolution
unresolved
no resolver link, observed 2026-08-04T00:54:09.043213Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-04T00:54:09.043213Z digest=sha256:a4299483521eea80a1ed56f735c395fe23a5158bd58808989eb2698857336bd3