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Paper Citation Record · LEDGER

Evidence for the volatile-rich composition of a 1.5-$R_\oplus$ planet

As of 5 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2212.08477.

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

pith.paper-citation-record.v1
2212.08477 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 2026-08-05T06:32:48.257954+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-01T12:14:31.135939Z

measured 0 of 1 external citation measurements

A source-named dated measurement, never combined with another source.

Source: cited_works

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 ac6ae1cb-b7c0-4b65-a32e-b6aa00629fdb · inbound

Dynamically Selected Mass-Radius Relationship for Low Mass Exoplanets cites this paper.

Dynamically Selected Mass-Radius Relationship for Low Mass Exoplanets Evidence for the volatile-rich composition of a 1.5-$R_\oplus$ planet

Reference 24

Resolution
unresolved
no resolver link, observed 2026-08-01T12:14:31.135939Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T12:14:31.135939Z digest=sha256:9ba4105d1806cdffcb93834d06d08de85d6a6fa78fc2ca4d52c5afcbe64b61e1

Observation 22db41be-06f0-42fd-b0e8-7a253471f864 · inbound

Characterizing the oxidation state of rocky exoplanets with the Large Interferometer for Exoplanets (LIFE) cites this paper.

Characterizing the oxidation state of rocky exoplanets with the Large Interferometer for Exoplanets (LIFE) Evidence for the volatile-rich composition of a 1.5-$R_\oplus$ planet

Reference 126

Resolution
unresolved
no resolver link, observed 2026-07-31T17:15:21.816340Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-31T17:15:21.816340Z digest=sha256:a257f334596cf528b88a70c30df66021b0d679605935d950ec69b52433022ded