Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
The Heavy Element Composition of Disk Instability Planets Can Range From Sub- to Super-Nebular
As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1104.0939.
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 2026-08-02T01:07:57.162737Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-06-26T13:09:29.702505Z
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 393aa16e-e0a8-49ff-81ce-0213087d7f6c · inbound
The panchromatic JWST dayside spectrum of WASP-121 b reveals a refractory-rich formation cites this paper.
The panchromatic JWST dayside spectrum of WASP-121 b reveals a refractory-rich formation The Heavy Element Composition of Disk Instability Planets Can Range From Sub- to Super-Nebular
Reference 85
- Resolution
- verified exact
- local_arxiv, observed 2026-06-26T13:09:29.703850Z
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 256e7f35-63bc-4cfd-b726-8ca9c99a08e6 · inbound
Dust Growth in Binary Systems: Inhibition of dust settling and growth in circumbinary discs cites this paper.
Dust Growth in Binary Systems: Inhibition of dust settling and growth in circumbinary discs The Heavy Element Composition of Disk Instability Planets Can Range From Sub- to Super-Nebular
Reference 285
- Resolution
- unresolved
- no resolver link, observed 2026-08-02T01:07:57.162737Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.