Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Tidal dissipation in rotating and evolving giant planets with application to exoplanet systems
As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 1 inbound Pith citation observation for arXiv:2311.15815.
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 2026-08-10T06:31:04.303077+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-03T12:59:19.984006Z
A source-named dated measurement, never combined with another source.
Source: cited_works
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 7b0d742e-404e-4020-9cbe-06f1784ca226 · inbound
Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations cites this paper.
Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations Tidal dissipation in rotating and evolving giant planets with application to exoplanet systems
Reference 38
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T12:59:19.984006Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.