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Paper Citation Record · LEDGER

The dynamical evolution of massive black hole binaries - II. Self-consistent N-body integrations

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/9706298.

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

pith.paper-citation-record.v1
astro-ph/9706298 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 2026-08-04T00:54:09.539687Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-11T15:56:06.799668Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
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  • parse uncertain0
  • malformed identifier0
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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 1be03fdb-7e60-4ddb-9ce0-77efc992f8c3 · inbound

Self-acceleration of Hardening Binaries cites this paper.

Self-acceleration of Hardening Binaries The dynamical evolution of massive black hole binaries - II. Self-consistent N-body integrations

Reference 54

Resolution
verified exact
arxiv_id, observed 2026-07-04T16:03:05.450347Z

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=sha256:8d38793034e60360c1fa7c959cb3ec5c56f734cf30a70284960600bf4779d2e7

Observation 2ba7bbe5-24f1-4658-b293-c15383dc55a7 · 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 The dynamical evolution of massive black hole binaries - II. Self-consistent N-body integrations

Reference 60

Resolution
unresolved
no resolver link, observed 2026-08-04T00:54:09.539687Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-04T00:54:09.539687Z digest=sha256:7fa4318d94fff6bb522d411b887aabefacfeabfb50975d7ed7c3743d38374dea