Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
NOTE: Explaining why the Uranian satellites have equatorial prograde orbits despite the large planetary obliquity
As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1208.4685.
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 2026-08-12T06:34:41.77262+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-11T23:13:10.690200Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-11T23:13:11.357547Z
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 f3c5eaf1-bcc7-42ee-873d-e0d61270724a · inbound
Accretion of Uranus and Neptune: confronting different giant impact scenarios cites this paper.
Accretion of Uranus and Neptune: confronting different giant impact scenarios NOTE: Explaining why the Uranian satellites have equatorial prograde orbits despite the large planetary obliquity
Reference 37
- Resolution
- malformed identifier
- local_arxiv, observed 2026-08-11T23:13:11.362056Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 8d89c949-0f97-4a2b-a977-6a25a64d9af5 · inbound
Dynamical formation of long-period exoplanets systems in evolving binary stars cites this paper.
Dynamical formation of long-period exoplanets systems in evolving binary stars NOTE: Explaining why the Uranian satellites have equatorial prograde orbits despite the large planetary obliquity
Reference 129
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T13:29:15.372796Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.