Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Interpreting the atmospheric composition of exoplanets: sensitivity to planet formation assumptions
As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2204.13714.
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 2026-08-02T00:06:48.655345Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-07-10T06:46:51.887899Z
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 74a440d7-5400-4ee4-8ed7-c40adf81177a · inbound
Phase-dependent chemistry of WASP-43 b revealed with a suite of one-, two-, and three-dimensional models cites this paper.
Phase-dependent chemistry of WASP-43 b revealed with a suite of one-, two-, and three-dimensional models Interpreting the atmospheric composition of exoplanets: sensitivity to planet formation assumptions
Reference 104
- Resolution
- verified exact
- local_arxiv, observed 2026-07-10T06:46:51.889101Z
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.
Observation 38d4d3f9-ba05-4648-bd3b-a0c0f78f27bf · inbound
The majority of hot Jupiters formed beyond the water ice line cites this paper.
The majority of hot Jupiters formed beyond the water ice line Interpreting the atmospheric composition of exoplanets: sensitivity to planet formation assumptions
Reference 16
- Resolution
- unresolved
- no resolver link, observed 2026-08-02T00:06:48.655345Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.