Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Carbon-rich Sub-Neptune Interiors Are Compatible with JWST Observations
As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2508.15117.
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 2026-08-07T06:34:17.273281+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-05T12:09:29.378936Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-07-12T06:48:33.961171Z
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 d5a6a4e7-60ec-4d97-b7a6-24ba86d8b0e0 · inbound
An Analysis of the Radius Gap in a Sample of Kepler, K2 and TESS exoplanets orbiting M Dwarf Stars cites this paper.
An Analysis of the Radius Gap in a Sample of Kepler, K2 and TESS exoplanets orbiting M Dwarf Stars Carbon-rich Sub-Neptune Interiors Are Compatible with JWST Observations
Reference 83
- Resolution
- unresolved
- no resolver link, observed 2026-08-05T12:09:29.378936Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation f80f8aca-6e3b-4ed3-9090-1901a3f14b6d · inbound
Uniform Metallicity Measurements of M Dwarf Planet Hosts Support Metallicity-Dependent Sub-Neptune Formation cites this paper.
Uniform Metallicity Measurements of M Dwarf Planet Hosts Support Metallicity-Dependent Sub-Neptune Formation Carbon-rich Sub-Neptune Interiors Are Compatible with JWST Observations
Reference 254
- Resolution
- verified exact
- local_arxiv, observed 2026-07-12T06:48:33.963261Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.