Paper Citation Record · LEDGER

The binary black hole spin distribution likely broadens with redshift

As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 11 inbound Pith citation observations for arXiv:2204.01578.

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

pith.paper-citation-record.v1
2204.01578 v2

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measured 0 of 0 reference resolution

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measured 11 of 11 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-10T06:31:04.303077+00:00

measured 11 of 11 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-09T04:41:35.373964Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-06-30T14:44:45.666677Z

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Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 711f5504-66f8-4fdb-be95-cc1511d59387 · inbound

Population Synthesis of Gravitational Wave Sources cites this paper.

Population Synthesis of Gravitational Wave Sources The binary black hole spin distribution likely broadens with redshift

Reference 31

Resolution: unresolved; no resolver link, observed 2026-08-09T04:41:35.373964Z

Source-reported events for the cited work

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Observation 77243710-0934-4cbf-b521-83e265272af8 · 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 The binary black hole spin distribution likely broadens with redshift

Reference 41

Resolution: unresolved; no resolver link, observed 2026-08-07T15:36:23.221235Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c68e8c3b-f25f-4721-88e6-9d302bb72652 · inbound

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

Parameter inference of millilensed gravitational waves using neural spline flows The binary black hole spin distribution likely broadens with redshift

Reference 72

Resolution: verified exact; arxiv_id, observed 2026-05-19T13:22:18.766223Z

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Observation 440237e4-df85-47fe-b5de-e40dd3a29811 · inbound

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

Inferring the pair-instability mass gap from gravitational wave data The binary black hole spin distribution likely broadens with redshift

Reference 72

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:01.115118Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7747956f-1fd5-4fe6-ad5f-3772a92d4231 · inbound

Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop cites this paper.

Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop The binary black hole spin distribution likely broadens with redshift

Reference 106

Resolution: unresolved; no resolver link, observed 2026-08-06T22:52:12.371598Z

Source-reported events for the cited work

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Observation 61f74bc7-da2d-4029-9520-06d18224a138 · inbound

The fault in our sirens: Hierarchical diagnosis of waveform systematics in Hubble-Lema\^itre constant measurements cites this paper.

The fault in our sirens: Hierarchical diagnosis of waveform systematics in Hubble-Lema\^itre constant measurements The binary black hole spin distribution likely broadens with redshift

Reference 48

Resolution: unresolved; no resolver link, observed 2026-08-06T17:20:18.299801Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6862254d-84d3-4094-aa08-13ce6187282b · inbound

Comparing astrophysical models to gravitational-wave data in the observable space cites this paper.

Comparing astrophysical models to gravitational-wave data in the observable space The binary black hole spin distribution likely broadens with redshift

Reference 23

Resolution: verified exact; arxiv_id, observed 2026-05-19T04:37:03.983989Z

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 d6ad557d-2f08-4b51-aa71-03e0d6c085b0 · inbound

Emergent structure in the binary black hole mass distribution and implications for population-based cosmology cites this paper.

Emergent structure in the binary black hole mass distribution and implications for population-based cosmology The binary black hole spin distribution likely broadens with redshift

Reference 63

Resolution: metadata mismatch; arxiv_id, observed 2026-05-11T11:51:01.429840Z

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 0985470e-c321-4e9b-9d56-157ff9d93d3f · 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 The binary black hole spin distribution likely broadens with redshift

Reference 271

Resolution: unresolved; no resolver link, observed 2026-08-02T12:20:55.500731Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c0c2d5f1-f49c-4940-ad1f-225bf8310d31 · inbound

Joint population and strong-lensing inference for resolved gravitational-wave events probes the black-hole merger rate beyond the peak of star formation cites this paper.

Joint population and strong-lensing inference for resolved gravitational-wave events probes the black-hole merger rate beyond the peak of star formation The binary black hole spin distribution likely broadens with redshift

Reference 118

Resolution: verified exact; arxiv_id, observed 2026-06-30T14:44:45.668431Z

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 f085d14b-2e08-4b5a-951f-0c51aa0f71d4 · inbound

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

Identifying lensed gravitational waves with physics-informed posterior learning The binary black hole spin distribution likely broadens with redshift

Reference 23

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

Source-reported events for the cited work

Unavailable: canonical work link unavailable.