Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
On the evolution of a twisted thin accretion disc in eccentric inclined supermassive binary black holes
As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2401.01317.
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 2026-08-06T17:18:50.361705Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-05-12T06:01:24.659030Z
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 fdae8f54-a974-4d82-917d-869ae82134aa · inbound
The evolution of a supermassive binary black hole in an non-spherical nuclear star cluster cites this paper.
The evolution of a supermassive binary black hole in an non-spherical nuclear star cluster On the evolution of a twisted thin accretion disc in eccentric inclined supermassive binary black holes
Reference 68
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T17:18:50.361705Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 5bb50ee0-d8c5-4f4e-8d9d-4af2550abb8f · inbound
A low viscosity relatively thick twisted disk in a supermassive binary black hole as a potential model of OJ 287 cites this paper.
A low viscosity relatively thick twisted disk in a supermassive binary black hole as a potential model of OJ 287 On the evolution of a twisted thin accretion disc in eccentric inclined supermassive binary black holes
Reference 23
- Resolution
- verified exact
- arxiv_id, observed 2026-05-12T06:01:24.664889Z
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.