Paper Citation Record · LEDGER

Most Black Holes are Born Very Slowly Rotating

As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 21 inbound Pith citation observations for arXiv:1907.03714.

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

pith.paper-citation-record.v1
1907.03714 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 21 of 21 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-08T06:32:00.761636+00:00

measured 21 of 21 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T05:02:01.151490Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-08T17:55:20.691430Z

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 ef297591-bf83-4f7f-9120-a17f32c77408 · inbound

GWTC-2.1: Deep Extended Catalog of Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run cites this paper.

GWTC-2.1: Deep Extended Catalog of Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run Most Black Holes are Born Very Slowly Rotating

Reference 242

Resolution: metadata mismatch; arxiv_id, observed 2026-05-16T07:47:32.887016Z

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 e9a15041-33fe-4f9c-823d-ea55ec7269eb · inbound

GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo During the Second Part of the Third Observing Run cites this paper.

GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo During the Second Part of the Third Observing Run Most Black Holes are Born Very Slowly Rotating

Reference 63

Resolution: verified exact; arxiv_id, observed 2026-05-11T09:30:26.333140Z

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 762385e9-1873-44c7-8f71-f35690167b70 · inbound

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

Inferring the pair-instability mass gap from gravitational wave data Most Black Holes are Born Very Slowly Rotating

Reference 87

Resolution: unresolved; no resolver link, observed 2026-08-07T05:02:01.151490Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ce8b326c-d61b-4469-9ca0-03ed611e6e73 · 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 Most Black Holes are Born Very Slowly Rotating

Reference 141

Resolution: unresolved; no resolver link, observed 2026-08-06T22:52:12.465484Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d580c930-7749-4027-a5a4-98f6fd17a09e · inbound

Potential science with GW250114 -- the loudest binary black hole merger detected to date cites this paper.

Potential science with GW250114 -- the loudest binary black hole merger detected to date Most Black Holes are Born Very Slowly Rotating

Reference 23

Resolution: unresolved; no resolver link, observed 2026-08-06T18:15:44.396834Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ee1d24de-f39e-43fa-bf27-d941a553e95f · 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 Most Black Holes are Born Very Slowly Rotating

Reference 14

Resolution: verified exact; arxiv_id, observed 2026-05-19T02:22:56.091485Z

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 f0b454d8-dd95-44fb-bc84-1c3a7516ff77 · inbound

Aligned Hierarchical Black Hole Mergers in Active-Galactic-Nuclei Disks Revealed by GWTC-4 cites this paper.

Aligned Hierarchical Black Hole Mergers in Active-Galactic-Nuclei Disks Revealed by GWTC-4 Most Black Holes are Born Very Slowly Rotating

Reference 10

Resolution: unresolved; no resolver link, observed 2026-08-04T14:43:52.891461Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 86848a23-9bd4-4a68-b96c-168112a1a57e · inbound

Stable mass transfer in massive binaries leading to merging black holes cites this paper.

Stable mass transfer in massive binaries leading to merging black holes Most Black Holes are Born Very Slowly Rotating

Reference 165

Resolution: unresolved; no resolver link, observed 2026-08-03T14:34:39.695783Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 34f9ef30-4622-4d79-8e32-5ba861974d21 · inbound

Signatures of a subpopulation of hierarchical mergers in the GWTC-4 gravitational-wave dataset cites this paper.

Signatures of a subpopulation of hierarchical mergers in the GWTC-4 gravitational-wave dataset Most Black Holes are Born Very Slowly Rotating

Reference 66

Resolution: verified exact; arxiv_id, observed 2026-05-09T02:57:52.243691Z

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 e52d4e9e-dd26-4a15-9915-3423cd0e4bdb · inbound

Signatures of a subpopulation of hierarchical mergers in the GWTC-4 gravitational-wave dataset cites this paper.

Signatures of a subpopulation of hierarchical mergers in the GWTC-4 gravitational-wave dataset Most Black Holes are Born Very Slowly Rotating

Reference 66

Resolution: unresolved; no resolver link, observed 2026-08-03T11:02:35.425149Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 86040e0a-7f80-43d4-ae7f-adbb613954e8 · inbound

The impact of waveform systematics and Gaussian noise on the interpretation of GW231123 cites this paper.

The impact of waveform systematics and Gaussian noise on the interpretation of GW231123 Most Black Holes are Born Very Slowly Rotating

Reference 11

Resolution: verified exact; arxiv_id, observed 2026-05-16T14:33:00.381601Z

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 2e22ce7c-dedf-42b7-89b3-9cf19dbdb081 · inbound

The Black Hole Mass Gap as a New Probe of Millicharged Particles cites this paper.

The Black Hole Mass Gap as a New Probe of Millicharged Particles Most Black Holes are Born Very Slowly Rotating

Reference 44

Resolution: verified exact; arxiv_id, observed 2026-05-13T21:03:19.639856Z

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 64a471b4-9bb5-4cc6-952e-99a0fc2ffc39 · inbound

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

Posterior Predictive Checks for Gravitational-wave Populations: Limitations and Improvements Most Black Holes are Born Very Slowly Rotating

Reference 54

Resolution: verified exact; arxiv_id, observed 2026-05-10T23:25:50.666409Z

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 cf4f3aa1-41ef-4fe5-809f-17f145ae75d2 · 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 Most Black Holes are Born Very Slowly Rotating

Reference 84

Resolution: verified exact; arxiv_id, observed 2026-05-11T06:11:02.303633Z

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 bb92b2a0-60a4-4849-bdbd-01b27de9a746 · 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 Most Black Holes are Born Very Slowly Rotating

Reference 59

Resolution: unresolved; no resolver link, observed 2026-08-02T12:20:51.688740Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9a6f4eef-4f8b-4929-8d25-538aeafe6d8d · inbound

Evidence for additional structure in the effective spin distribution hints at multiple formation pathways in GWTC-5.0 cites this paper.

Evidence for additional structure in the effective spin distribution hints at multiple formation pathways in GWTC-5.0 Most Black Holes are Born Very Slowly Rotating

Reference 27

Resolution: verified exact; arxiv_id, observed 2026-07-03T12:58:07.872579Z

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 eb1a8cec-4489-4ef5-9d60-2cfd9eeee946 · inbound

Formation of rotating supergiants via stellar mergers in dense clusters: Implications for black hole natal spins cites this paper.

Formation of rotating supergiants via stellar mergers in dense clusters: Implications for black hole natal spins Most Black Holes are Born Very Slowly Rotating

Reference 92

Resolution: unresolved; no resolver link, observed 2026-07-11T06:51:42.465920Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6326e20e-cd1c-4643-98b4-faa885d45a71 · inbound

A Possible Triple Formation Scenario of Binary Black Hole Merge With One In Pair-instability Supernova Mass Gap cites this paper.

A Possible Triple Formation Scenario of Binary Black Hole Merge With One In Pair-instability Supernova Mass Gap Most Black Holes are Born Very Slowly Rotating

Reference 86

Resolution: verified exact; local_arxiv, observed 2026-07-08T17:55:20.692650Z

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 24bbeddd-e5cc-41e5-94a3-0eeb5193ffdb · inbound

Black-Hole Spin Measurements from X-ray Reflection Spectroscopy: Quality Criteria and Community Recommendations cites this paper.

Black-Hole Spin Measurements from X-ray Reflection Spectroscopy: Quality Criteria and Community Recommendations Most Black Holes are Born Very Slowly Rotating

Reference 2

Resolution: unresolved; no resolver link, observed 2026-08-02T02:20:50.832872Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d5a5a55d-697a-4887-9e6c-37105556b06d · inbound

Assessing the Impact of Instrumental Requirements on the Scientific Performance of the Einstein Telescope cites this paper.

Assessing the Impact of Instrumental Requirements on the Scientific Performance of the Einstein Telescope Most Black Holes are Born Very Slowly Rotating

Reference 109

Resolution: unresolved; no resolver link, observed 2026-08-01T09:38:55.155465Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c2792199-b497-4683-a44c-783d2764f6e8 · inbound

A Four-dimensional Model-agnostic Probe into the Astrophysical Origins of Binary Black Hole Subpopulations cites this paper.

A Four-dimensional Model-agnostic Probe into the Astrophysical Origins of Binary Black Hole Subpopulations Most Black Holes are Born Very Slowly Rotating

Reference 64

Resolution: unresolved; no resolver link, observed 2026-07-31T01:54:12.303640Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.