Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Absence of the predicted 2022 October outburst of OJ 287 and implications for binary SMBH scenarios
As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2302.11646.
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 2026-08-06T17:18:50.238102Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-05-12T06:01:24.625528Z
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 97cef153-9726-411a-9f80-33555a3d062f · 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 Absence of the predicted 2022 October outburst of OJ 287 and implications for binary SMBH scenarios
Reference 67
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T17:18:50.238102Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 776c1abc-55e5-473c-b469-cb3e8ee63a9e · 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 Absence of the predicted 2022 October outburst of OJ 287 and implications for binary SMBH scenarios
Reference 21
- Resolution
- verified exact
- arxiv_id, observed 2026-05-12T06:01:24.628006Z
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.