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Paper Citation Record · LEDGER

Giant exoplanet composition: Why do the hydrogen-helium equation of state and interior structure matter?

As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2410.21382.

A citation records a reference. It does not transfer a finding from one paper to another.

pith.paper-citation-record.v1
2410.21382 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 2 of 2 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-07T06:34:17.273281+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-07-12T02:17:19.814114Z

measured 0 of 1 external citation measurements

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

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  • verified fuzzy0
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  • malformed identifier0
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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 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 2026-08-07T06:34:17.273281+00:00.

source=pdf_text observed=2026-05-23T05:35:55.037502Z digest=sha256:e666bdbae9667768de5acfc714e347fc8cab5036b908c1ddd6b3f245407f135a

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.

source=arxiv_source observed=2026-07-12T02:17:19.814114Z digest=sha256:df83577fa286baba745b0693e9007bf70ee51127a1400f36d9c4d72fc155c70c