Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Giant exoplanet composition: Why do the hydrogen-helium equation of state and interior structure matter?
As of 23 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2410.21382.
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 2026-08-23T06:30:58.430688+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-12T13:30:09.189178Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-05-23T05:37:36.833581Z
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 613a1a7a-89e3-48da-a916-0d01846f1666 · inbound
The bulk metallicity of giant planets around M stars cites this paper.
The bulk metallicity of giant planets around M stars Giant exoplanet composition: Why do the hydrogen-helium equation of state and interior structure matter?
Reference 29
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T13:30:09.189178Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 52800d2d-4fd8-4930-9f20-af7258411ad6 · inbound
A Denser Hydrogen Inferred from First-Principles Simulations Challenges Jupiter's Interior Models cites this paper.
A Denser Hydrogen Inferred from First-Principles Simulations Challenges Jupiter's Interior Models Giant exoplanet composition: Why do the hydrogen-helium equation of state and interior structure matter?
Reference 14
- Resolution
- verified exact
- arxiv_id, observed 2026-05-23T05:37:36.836042Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.
Observation cb32e249-1fc8-4c9a-a62b-57347c8822e2 · inbound
The influence of composition gradients on giant planet radii cites this paper.
The influence of composition gradients on giant planet radii Giant exoplanet composition: Why do the hydrogen-helium equation of state and interior structure matter?
Reference 6
- Resolution
- unresolved
- no resolver link, observed 2026-07-12T02:17:19.814114Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.