Paper Citation Record · LEDGER

No evidence that the majority of black holes in binaries have zero spin

As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 10 inbound Pith citation observations for arXiv:2205.08574.

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

pith.paper-citation-record.v1
2205.08574 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 10 of 10 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-18T06:34:40.430872+00:00

measured 10 of 10 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T05:02:01.034693Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-09T20:56:34.367485Z

Reference resolution

0 of 0 outbound references displayed

verified exact0
verified fuzzy0
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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 916257fd-4483-4e0f-8e16-bb48968b9a31 · inbound

Parameter inference of millilensed gravitational waves using neural spline flows cites this paper.

Parameter inference of millilensed gravitational waves using neural spline flows No evidence that the majority of black holes in binaries have zero spin

Reference 71

Resolution: verified exact; arxiv_id, observed 2026-05-19T13:22:18.717847Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation 71ab6b3a-1b75-436a-b90e-5e2ab4b925c1 · inbound

Inferring the pair-instability mass gap from gravitational wave data cites this paper.

Inferring the pair-instability mass gap from gravitational wave data No evidence that the majority of black holes in binaries have zero spin

Reference 50

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:01.034693Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1640bced-ed1a-4c2d-9edd-9caae61634c1 · inbound

Disentangling spinning and nonspinning binary black hole populations with spin sorting cites this paper.

Disentangling spinning and nonspinning binary black hole populations with spin sorting No evidence that the majority of black holes in binaries have zero spin

Reference 44

Resolution: verified exact; arxiv_id, observed 2026-05-19T02:22:56.268909Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation 460def42-9d47-4037-8098-bc0b85a5da16 · inbound

When (not) to trust Monte Carlo approximations for hierarchical Bayesian inference cites this paper.

When (not) to trust Monte Carlo approximations for hierarchical Bayesian inference No evidence that the majority of black holes in binaries have zero spin

Reference 95

Resolution: unresolved; no resolver link, observed 2026-08-04T22:42:34.780779Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 09ac02c9-1967-4d01-b826-7586e5bb6ce4 · inbound

Posterior Predictive Checks for Gravitational-wave Populations: Limitations and Improvements cites this paper.

Posterior Predictive Checks for Gravitational-wave Populations: Limitations and Improvements No evidence that the majority of black holes in binaries have zero spin

Reference 92

Resolution: verified exact; arxiv_id, observed 2026-05-10T23:25:50.767622Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation d4b35f98-af58-4eb2-a770-48620c116904 · inbound

Second-Generation Mass Peak in the Gravitational-Wave Population as a Probe of Globular Clusters cites this paper.

Second-Generation Mass Peak in the Gravitational-Wave Population as a Probe of Globular Clusters No evidence that the majority of black holes in binaries have zero spin

Reference 105

Resolution: verified exact; arxiv_id, observed 2026-05-11T06:11:02.708208Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation c5e9a5cf-4952-4ed9-aa25-7ba1463e1eed · 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 No evidence that the majority of black holes in binaries have zero spin

Reference 249

Resolution: unresolved; no resolver link, observed 2026-08-02T12:20:54.134630Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b9f1de26-4276-4e46-a20c-370ac3a18a80 · inbound

Identifying lensed gravitational waves with physics-informed posterior learning cites this paper.

Identifying lensed gravitational waves with physics-informed posterior learning No evidence that the majority of black holes in binaries have zero spin

Reference 25

Resolution: unresolved; no resolver link, observed 2026-07-11T23:16:00.672720Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 92313198-4d1d-457e-84e6-807e6508f498 · inbound

Testing General Relativity with GWTC-4.0 through mixture models cites this paper.

Testing General Relativity with GWTC-4.0 through mixture models No evidence that the majority of black holes in binaries have zero spin

Reference 50

Resolution: verified exact; local_arxiv, observed 2026-07-09T20:56:34.368819Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation 7d5bc5d6-febc-4427-a726-22726d2a8dae · inbound

Modes in Transitional Millisecond Pulsars: Evidence of Pulsar Wind-Induced Disk Heating from GRMHD and Radiative Transfer cites this paper.

Modes in Transitional Millisecond Pulsars: Evidence of Pulsar Wind-Induced Disk Heating from GRMHD and Radiative Transfer No evidence that the majority of black holes in binaries have zero spin

Reference 213

Resolution: unresolved; no resolver link, observed 2026-08-01T13:29:47.353376Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.