Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
The dynamical evolution of massive black hole binaries - I. Hardening in a fixed stellar background
As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:astro-ph/9601092.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-07T06:34:17.273281+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-04T00:54:09.432858Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-05-11T15:51:44.978333Z
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 1bdd8ba8-69f7-44e8-b245-e866c432f5ab · inbound
Probing Supermassive Black Hole Mergers with Pulsar Timing Arrays cites this paper.
Probing Supermassive Black Hole Mergers with Pulsar Timing Arrays The dynamical evolution of massive black hole binaries - I. Hardening in a fixed stellar background
Reference 13
- Resolution
- verified exact
- arxiv_id, observed 2026-07-04T17:52:08.173835Z
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.
Observation d797bdb6-387c-4fee-88be-0d885d656a17 · inbound
Self-acceleration of Hardening Binaries cites this paper.
Self-acceleration of Hardening Binaries The dynamical evolution of massive black hole binaries - I. Hardening in a fixed stellar background
Reference 21
- Resolution
- verified exact
- arxiv_id, observed 2026-07-04T17:52:08.173835Z
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.
Observation 23527f20-d3a4-4a58-b504-2cdba210fa9e · 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 - I. Hardening in a fixed stellar background
Reference 59
- Resolution
- unresolved
- no resolver link, observed 2026-08-04T00:54:09.432858Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.