Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
The spin magnitude of stellar-mass binary black holes evolves with the mass: evidence from gravitational wave data
As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 22 inbound Pith citation observations for arXiv:2406.01679.
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 2026-08-09T06:31:02.800959+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-07T05:02:01.049503Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-08-05T02:28:24.338817Z
Reference resolution
0 of 0 outbound references displayed
- verified exact0
- verified fuzzy0
- unresolved0
- parse uncertain0
- malformed identifier0
- metadata mismatch0
External citation measurements
1
arxiv_reference, observed 2026-08-05T02:28:24.338817Z
Outbound references
No outbound reference observations are available for this paper version.
Pith citing papers
Observation 698ae5a4-1111-4906-9224-743d5353e82c · 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 spin magnitude of stellar-mass binary black holes evolves with the mass: evidence from gravitational wave data
Reference 57
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T05:02:01.049503Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation b1e33465-827b-440c-ac4c-9fb576b394dc · 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 spin magnitude of stellar-mass binary black holes evolves with the mass: evidence from gravitational wave data
Reference 113
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.390651Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 4bb227c1-0efb-44dd-aae3-0d203c412623 · 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 spin magnitude of stellar-mass binary black holes evolves with the mass: evidence from gravitational wave data
Reference 27
- Resolution
- verified exact
- arxiv_id, observed 2026-05-19T04:37:03.943680Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation a7794d3a-3591-46db-9fec-87817aff3073 · inbound
A new group of low-spin $50-70M_\odot$ Black Holes and the high pair-instability mass cutoff cites this paper.
A new group of low-spin $50-70M_\odot$ Black Holes and the high pair-instability mass cutoff The spin magnitude of stellar-mass binary black holes evolves with the mass: evidence from gravitational wave data
Reference 21
- Resolution
- verified exact
- arxiv_id, observed 2026-05-22T12:41:33.186007Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation 20c09e98-bd45-4990-9ae5-cc25d76860e0 · inbound
A new group of low-spin $50-70M_\odot$ Black Holes and the high pair-instability mass cutoff cites this paper.
A new group of low-spin $50-70M_\odot$ Black Holes and the high pair-instability mass cutoff The spin magnitude of stellar-mass binary black holes evolves with the mass: evidence from gravitational wave data
Reference 21
- Resolution
- unresolved
- no resolver link, observed 2026-08-04T08:07:40.094849Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 2043d560-299a-40d4-a35d-d6f2eef3e1ef · inbound
Population of Binary Black Holes Inferred from One Hundred and Fifty Gravitational Wave Signals cites this paper.
Population of Binary Black Holes Inferred from One Hundred and Fifty Gravitational Wave Signals The spin magnitude of stellar-mass binary black holes evolves with the mass: evidence from gravitational wave data
Reference 93
- Resolution
- unresolved
- no resolver link, observed 2026-08-04T07:34:45.375568Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation e580a02e-7595-48c0-b5eb-36a2165a683f · 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 The spin magnitude of stellar-mass binary black holes evolves with the mass: evidence from gravitational wave data
Reference 86
- Resolution
- verified exact
- arxiv_id, observed 2026-05-09T02:57:53.085370Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation 1f6c6dee-fd41-4e40-a268-35dacf944ca7 · 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 The spin magnitude of stellar-mass binary black holes evolves with the mass: evidence from gravitational wave data
Reference 86
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T11:02:35.622699Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 6b46471e-b77a-4750-846f-79e3be50c175 · inbound
Population Properties of Binary Black Holes with Eccentricity cites this paper.
Population Properties of Binary Black Holes with Eccentricity The spin magnitude of stellar-mass binary black holes evolves with the mass: evidence from gravitational wave data
Reference 68
- Resolution
- verified exact
- arxiv_id, observed 2026-05-16T02:30:31.782922Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation 8e9c2e74-06a1-4e16-a08e-ee522f8ae7d1 · inbound
Measurement prospects for the pair-instability mass cutoff with gravitational waves cites this paper.
Measurement prospects for the pair-instability mass cutoff with gravitational waves The spin magnitude of stellar-mass binary black holes evolves with the mass: evidence from gravitational wave data
Reference 53
- Resolution
- verified exact
- arxiv_id, observed 2026-05-16T05:37:24.017352Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation 2479d6da-88be-4dcc-9ccd-dc1cc1a0dc68 · 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 spin magnitude of stellar-mass binary black holes evolves with the mass: evidence from gravitational wave data
Reference 64
- Resolution
- metadata mismatch
- arxiv_id, observed 2026-05-11T11:51:01.543782Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation 88714451-afe2-4581-aed0-052d47469bef · inbound
How do the LIGO-Virgo-KAGRA's Heavy Black Holes Form? No evidence for core-collapse Intermediate-mass black holes in GWTC-4 cites this paper.
How do the LIGO-Virgo-KAGRA's Heavy Black Holes Form? No evidence for core-collapse Intermediate-mass black holes in GWTC-4 The spin magnitude of stellar-mass binary black holes evolves with the mass: evidence from gravitational wave data
Reference 143
- Resolution
- metadata mismatch
- arxiv_id, observed 2026-05-08T23:14:23.213676Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation 2e29eb1a-5056-4fb4-a84a-6feacf8cefde · inbound
Secondary-Mass Features improve Spectral-Siren $H_0$ Constraints cites this paper.
Secondary-Mass Features improve Spectral-Siren $H_0$ Constraints The spin magnitude of stellar-mass binary black holes evolves with the mass: evidence from gravitational wave data
Reference 62
- Resolution
- metadata mismatch
- arxiv_id, observed 2026-05-13T02:07:06.897977Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation f58b9072-681d-4cca-94bd-8f236373e2df · 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 The spin magnitude of stellar-mass binary black holes evolves with the mass: evidence from gravitational wave data
Reference 113
- Resolution
- verified exact
- arxiv_id, observed 2026-07-03T12:58:07.903189Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation f6ad4116-023c-4bc4-a1a8-ed99f33aa559 · inbound
The Chirp-Mass Ladder: A New Rung Emerges cites this paper.
The Chirp-Mass Ladder: A New Rung Emerges The spin magnitude of stellar-mass binary black holes evolves with the mass: evidence from gravitational wave data
Reference 214
- Resolution
- metadata mismatch
- arxiv_id, observed 2026-06-26T23:10:14.487868Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation 47daeefd-4736-470f-b9f5-416a7e0b44f3 · 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 spin magnitude of stellar-mass binary black holes evolves with the mass: evidence from gravitational wave data
Reference 120
- Resolution
- verified exact
- arxiv_id, observed 2026-06-30T14:34:46.195843Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation 90fe0f88-24ca-48ba-bb7d-b8080c3e9295 · inbound
Smoking-gun evidence for hierarchical black-hole mergers cites this paper.
Smoking-gun evidence for hierarchical black-hole mergers The spin magnitude of stellar-mass binary black holes evolves with the mass: evidence from gravitational wave data
Reference 19
- Resolution
- verified exact
- arxiv_id, observed 2026-07-02T07:26:45.436798Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation 70ecd4ea-1f78-49e5-a550-943b3e793f57 · inbound
No Evidence for Superradiant Axions in LIGO-Virgo-KAGRA GWTC-5 Binary Black Hole Spins cites this paper.
No Evidence for Superradiant Axions in LIGO-Virgo-KAGRA GWTC-5 Binary Black Hole Spins The spin magnitude of stellar-mass binary black holes evolves with the mass: evidence from gravitational wave data
Reference 104
- Resolution
- verified exact
- arxiv_id, observed 2026-07-03T19:58:53.906259Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation 4b3d1927-c28e-4cf3-9d2d-864647caceb9 · inbound
Periodic line-of-sight velocity-driven modulations to gravitational waves emitted by compact binaries in Keplerian outer orbits cites this paper.
Periodic line-of-sight velocity-driven modulations to gravitational waves emitted by compact binaries in Keplerian outer orbits The spin magnitude of stellar-mass binary black holes evolves with the mass: evidence from gravitational wave data
Reference 15
- Resolution
- unresolved
- no resolver link, observed 2026-07-13T01:31:57.131208Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 89e26f47-df39-4ad1-8a67-4137f59a2f34 · inbound
Periodic line-of-sight velocity-driven modulations to gravitational waves emitted by compact binaries in Keplerian outer orbits cites this paper.
Periodic line-of-sight velocity-driven modulations to gravitational waves emitted by compact binaries in Keplerian outer orbits The spin magnitude of stellar-mass binary black holes evolves with the mass: evidence from gravitational wave data
Reference 15
- Resolution
- unresolved
- no resolver link, observed 2026-08-02T07:36:04.813195Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 36c7a41f-2757-4947-b1d3-359e475de90b · inbound
Uncovering Hierarchical Sub-Population of Binary Black Holes cites this paper.
Uncovering Hierarchical Sub-Population of Binary Black Holes The spin magnitude of stellar-mass binary black holes evolves with the mass: evidence from gravitational wave data
Reference 67
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T23:27:58.928855Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 24d08f63-45d3-4c60-8dad-d6daab17939e · inbound
Assessing the waveform systematics from parameter estimation to population inference with eccentricity cites this paper.
Assessing the waveform systematics from parameter estimation to population inference with eccentricity The spin magnitude of stellar-mass binary black holes evolves with the mass: evidence from gravitational wave data
Reference 58
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T23:22:38.444289Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.