Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Masses, Radii, and Orbits of Small Kepler Planets: The Transition from Gaseous to Rocky Planets
As of 5 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1401.4195.
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 2026-08-05T06:32:48.257954+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-01T13:29:14.723923Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-06-26T22:40:09.995517Z
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 10629055-f962-4160-afec-4595f841d3b1 · inbound
The Maximum Density of a Collisionally-Produced Planet is A Function of its Mass and Orbital Period cites this paper.
The Maximum Density of a Collisionally-Produced Planet is A Function of its Mass and Orbital Period Masses, Radii, and Orbits of Small Kepler Planets: The Transition from Gaseous to Rocky Planets
Reference 36
- Resolution
- verified exact
- local_arxiv, observed 2026-06-26T22:40:09.996741Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.
Observation 82fb67ab-6c22-4a31-8054-38c89bb7d234 · 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 Masses, Radii, and Orbits of Small Kepler Planets: The Transition from Gaseous to Rocky Planets
Reference 122
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T13:29:14.723923Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.