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Paper Citation Record · LEDGER

Distinguishing black-hole spin-orbit resonances by their gravitational-wave signatures

As of 21 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.

pith.paper-citation-record.v1
1403.7147 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 5 of 5 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-21T06:32:19.484+00:00

measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T15:36:24.689343Z

measured 0 of 1 external citation measurements

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

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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 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.

source=pdf_text observed=2026-08-07T15:36:24.689343Z digest=sha256:e7533359088ce12ddb80993f3f396bec4b6747a34cec8f0de3a4d13178d7523e

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.

source=pdf_text observed=2026-08-04T17:49:18.630456Z digest=sha256:042e9010881beb8b781325aea744faf83c336e5b8438c8bf39c597451abb4353

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 2026-08-21T06:32:19.484+00:00.

source=pdf_text observed=2026-07-11T11:50:26.030339Z digest=sha256:4994cd16cb62c9bc629dd84e027275764dfd47df779a22074437032f9d3a06ca

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.

source=pdf_text observed=2026-08-02T12:20:52.227527Z digest=sha256:32ad42808667fa99c0e33c16d5a323bc0b19b71b6bb7e33ac88fb3649e043ce0

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 2026-08-21T06:32:19.484+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:076a12d1e2505f8353f106041f887b2dce971ae1454ab408e572b1fbffb4bb66