Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
The binary black hole spin distribution likely broadens with redshift
As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 10 inbound Pith citation observations for arXiv:2204.01578.
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 2026-08-08T06:32:00.761636+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-07T15:36:23.221235Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-06-30T14:44:45.666677Z
Reference resolution
0 of 0 outbound references displayed
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- 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 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
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.
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
Unavailable: canonical work link unavailable.
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 2026-08-08T06:32:00.761636+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 2026-08-08T06:32:00.761636+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 2026-08-08T06:32:00.761636+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.