Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Disk induced binary precession: Implications for dynamics and multi-messenger observations of black hole binaries
As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2312.01805.
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 2026-08-11T06:34:44.6726+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-10T19:46:47.369850Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-06-29T01:02:56.189946Z
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 82a2a7b8-6e43-4622-b6de-1133e8d8f429 · inbound
Environmental effects in extreme mass ratio inspirals: perturbations to the environment in Kerr cites this paper.
Environmental effects in extreme mass ratio inspirals: perturbations to the environment in Kerr Disk induced binary precession: Implications for dynamics and multi-messenger observations of black hole binaries
Reference 38
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T19:46:47.369850Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 8663105c-05fa-44da-87ce-7c97dc0baa94 · inbound
Dissecting environmental effects with eccentric gravitational wave sources cites this paper.
Dissecting environmental effects with eccentric gravitational wave sources Disk induced binary precession: Implications for dynamics and multi-messenger observations of black hole binaries
Reference 29
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T05:02:46.059966Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 54620399-200f-4437-adcf-8c675d4a8d7e · inbound
GW231123: A Possible Primordial Black Hole Origin cites this paper.
GW231123: A Possible Primordial Black Hole Origin Disk induced binary precession: Implications for dynamics and multi-messenger observations of black hole binaries
Reference 137
- Resolution
- verified exact
- arxiv_id, observed 2026-05-18T22:56:53.660419Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 3562d5b0-2a9c-4715-bcdc-773e1ff11773 · inbound
January Food Benchmark (JFB): A Public Benchmark Dataset and Evaluation Suite for Multimodal Food Analysis cites this paper.
January Food Benchmark (JFB): A Public Benchmark Dataset and Evaluation Suite for Multimodal Food Analysis Disk induced binary precession: Implications for dynamics and multi-messenger observations of black hole binaries
Reference 139
- Resolution
- unresolved
- no resolver link, observed 2026-08-05T20:46:11.283718Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 91732bd7-73ce-4044-a78c-938aeb44e3e2 · inbound
Dynamics of Relativistic Binaries in Structured and Stochastic Environments: A Lagrange-Fourier-Hansen Framework cites this paper.
Dynamics of Relativistic Binaries in Structured and Stochastic Environments: A Lagrange-Fourier-Hansen Framework Disk induced binary precession: Implications for dynamics and multi-messenger observations of black hole binaries
Reference 104
- Resolution
- verified exact
- arxiv_id, observed 2026-06-29T01:02:56.191485Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.