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Paper Citation Record · LEDGER

Tidally Heated Sub-Neptunes, Refined Planetary Compositions, and Confirmation of a Third Planet in the TOI-1266 System

As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2409.16374.

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

pith.paper-citation-record.v1
2409.16374 v3

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 2026-08-01T12:14:31.173012Z

measured 1 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-08-05T02:28:24.338817Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
  • unresolved0
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

External citation measurements

0
arxiv_reference, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 056557b6-3278-4adf-a905-9c84f8804fc5 · inbound

The mass of TOI-1883 b: A low density super-Neptune in the ridge regime transiting an early-M dwarf cites this paper.

The mass of TOI-1883 b: A low density super-Neptune in the ridge regime transiting an early-M dwarf Tidally Heated Sub-Neptunes, Refined Planetary Compositions, and Confirmation of a Third Planet in the TOI-1266 System

Reference 120

Resolution
verified exact
arxiv_id, observed 2026-06-27T21:21:16.646097Z

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=arxiv_source observed=2026-06-27T21:18:48.013062Z digest=sha256:20aa3b0b680beb3f06e8b610c6998275c493cca56bbab14b743be447eafd7be9

Observation 7cb929fb-b725-4c36-9a22-5d9be2a92195 · inbound

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

Dynamically Selected Mass-Radius Relationship for Low Mass Exoplanets Tidally Heated Sub-Neptunes, Refined Planetary Compositions, and Confirmation of a Third Planet in the TOI-1266 System

Reference 36

Resolution
unresolved
no resolver link, observed 2026-08-01T12:14:31.173012Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T12:14:31.173012Z digest=sha256:9e5db32c058f57e066acb189765659e348dd3647b939833ebfce7154108a2cfa