Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Modeling the 3--D Secular Planetary Three-Body Problem. Discussion on the outer ${\upsilon}$ Andromedae Planetary System
As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 1 inbound Pith citation observation for arXiv:astro-ph/0505169.
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 2026-08-19T06:32:44.657259+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-15T20:44:43.129912Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-15T20:44:43.456980Z
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 a47190e6-8875-457d-a59c-b048b6301abf · inbound
Dynamical regimes of two eccentric and mutually inclined giant planets cites this paper.
Dynamical regimes of two eccentric and mutually inclined giant planets Modeling the 3--D Secular Planetary Three-Body Problem. Discussion on the outer ${\upsilon}$ Andromedae Planetary System
Reference 2006
- Resolution
- verified exact
- local_arxiv, observed 2026-08-15T20:44:43.461629Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.