Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Distinguishing black-hole spin-orbit resonances by their gravitational-wave signatures
As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:1403.7147.
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 2026-08-10T06:31:04.303077+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-07T15:36:24.689343Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-07-09T08:05:16.230513Z
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 cdeea92e-8aa8-462e-8aa2-a275d81eefbd · inbound
The Long Road to Alignment: Measuring Black Hole Spin Orientation with Expanding Gravitational-Wave Datasets cites this paper.
The Long Road to Alignment: Measuring Black Hole Spin Orientation with Expanding Gravitational-Wave Datasets Distinguishing black-hole spin-orbit resonances by their gravitational-wave signatures
Reference 53
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T15:36:24.689343Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 0526dc8b-f06e-4723-9048-d356980ff0bc · inbound
Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency cites this paper.
Detecting regular precession using a new gravitational waveform model directly parameterized by both precession amplitude and frequency Distinguishing black-hole spin-orbit resonances by their gravitational-wave signatures
Reference 63
- Resolution
- unresolved
- no resolver link, observed 2026-08-04T17:49:18.630456Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 220362fb-ef96-4dd2-ae9f-7168d8e9254f · inbound
The first decade of gravitational-wave measurements of black hole spins cites this paper.
The first decade of gravitational-wave measurements of black hole spins Distinguishing black-hole spin-orbit resonances by their gravitational-wave signatures
Reference 186
- Resolution
- verified exact
- local_arxiv, observed 2026-06-28T00:21:27.864833Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation 10bede8a-bb17-409b-80f7-a79d83c7da03 · inbound
The first decade of gravitational-wave measurements of black hole spins cites this paper.
The first decade of gravitational-wave measurements of black hole spins Distinguishing black-hole spin-orbit resonances by their gravitational-wave signatures
Reference 186
- Resolution
- unresolved
- no resolver link, observed 2026-08-02T12:20:52.227527Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 4761b340-475f-4586-a2cf-069a08fe68ca · inbound
Modern tidal interaction models for rapid binary population synthesis: II. Binary black hole formation, mergers, and spins cites this paper.
Modern tidal interaction models for rapid binary population synthesis: II. Binary black hole formation, mergers, and spins Distinguishing black-hole spin-orbit resonances by their gravitational-wave signatures
Reference 146
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-06-26T17:49:41.049326Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.