Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
How Post-Newtonian Dynamics Shape the Distribution of Stationary Binary Black Hole LISA Sources in nearby Globular Clusters
As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1807.08864.
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 2026-08-15T06:32:42.880941+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-14T10:21:19.234195Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-05-23T03:25:20.748667Z
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 0d71c420-1372-44f1-ae82-e775fa92f4c5 · inbound
The Missing Link in Gravitational-Wave Astronomy: Discoveries waiting in the decihertz range cites this paper.
The Missing Link in Gravitational-Wave Astronomy: Discoveries waiting in the decihertz range How Post-Newtonian Dynamics Shape the Distribution of Stationary Binary Black Hole LISA Sources in nearby Globular Clusters
Reference 114
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T10:21:19.234195Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation b0144443-4dc7-484c-b77e-4e73de103d0f · inbound
Analytic Waveforms for Eccentric Gravitational Wave Bursts cites this paper.
Analytic Waveforms for Eccentric Gravitational Wave Bursts How Post-Newtonian Dynamics Shape the Distribution of Stationary Binary Black Hole LISA Sources in nearby Globular Clusters
Reference 23
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T05:05:21.435701Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 853bc731-f3b8-46a3-97da-9b139f4c1638 · inbound
Non-adiabatic dynamics of eccentric black-hole binaries in post-Newtonian theory cites this paper.
Non-adiabatic dynamics of eccentric black-hole binaries in post-Newtonian theory How Post-Newtonian Dynamics Shape the Distribution of Stationary Binary Black Hole LISA Sources in nearby Globular Clusters
Reference 5
- Resolution
- verified exact
- local_arxiv, observed 2026-05-23T03:25:20.751031Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.