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Paper Citation Record · LEDGER

Evidence of Three Mechanisms Explaining the Radius Anomaly of Hot Jupiters

As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2009.04291.

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

pith.paper-citation-record.v1
2009.04291 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 3 of 3 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-09T06:31:02.800959+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-08T11:59:09.515077Z

measured 1 of 1 external citation measurements

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

Source: pith, 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

73
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 074f461a-605a-4d89-89fc-587888a827a9 · inbound

Phase-dependent chemistry of WASP-43 b revealed with a suite of one-, two-, and three-dimensional models cites this paper.

Phase-dependent chemistry of WASP-43 b revealed with a suite of one-, two-, and three-dimensional models Evidence of Three Mechanisms Explaining the Radius Anomaly of Hot Jupiters

Reference 128

Resolution
verified exact
local_arxiv, observed 2026-07-10T06:46:51.909552Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:b71e12c89048631be76184c0e697fbe1f777ddcaa0c4087126d423efd68e8e89

Observation 152baac3-5127-4088-99f5-657fad9298b6 · 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 of Three Mechanisms Explaining the Radius Anomaly of Hot Jupiters

Reference 286

Resolution
unresolved
no resolver link, observed 2026-07-31T17:15:23.985679Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-31T17:15:23.985679Z digest=sha256:f8f8219118a79ed7b9a3d0238c4921cb7c9c7ffd0b65d221ff53c2e43602748b

Observation 6c16fee9-551d-4e38-a97e-e71062dd660e · inbound

The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars cites this paper.

The TASSIE Program. II: Three Close-In Companions Orbiting Sun-Like Stars Evidence of Three Mechanisms Explaining the Radius Anomaly of Hot Jupiters

Reference 70

Resolution
unresolved
no resolver link, observed 2026-08-08T11:59:09.515077Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-08T11:59:09.515077Z digest=sha256:34ea97c66ef0423e3a88b5ec1cb78cf92cb2f055d47c7bc5e4a0bfd38f90e28a