Paper Citation Record · LEDGER

The Prevalence of Resonance Among Young, Close-in Planets

As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:2406.06885.

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

pith.paper-citation-record.v1
2406.06885 v3

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 6 of 6 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-10T06:31:04.303077+00:00

measured 6 of 6 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-09T14:15:05.046600Z

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
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External citation measurements

1
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation e998c51c-d138-41bd-bd4f-b38f124debbd · inbound

Amplifying Resonant Repulsion with Inflated Young Planets, Overlooked Inner Planets, and Non-zero Initial $\Delta$ cites this paper.

Amplifying Resonant Repulsion with Inflated Young Planets, Overlooked Inner Planets, and Non-zero Initial $\Delta$ The Prevalence of Resonance Among Young, Close-in Planets

Reference 19

Resolution: unresolved; no resolver link, observed 2026-08-09T14:15:05.046600Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f6b55931-c847-4124-8f87-ba17826b7187 · inbound

JWST unveils a high mean molecular weight atmosphere for mini-Neptune TOI-1130b: Evidence for formation beyond the water ice line cites this paper.

JWST unveils a high mean molecular weight atmosphere for mini-Neptune TOI-1130b: Evidence for formation beyond the water ice line The Prevalence of Resonance Among Young, Close-in Planets

Reference 289

Resolution: verified exact; arxiv_id, observed 2026-05-08T19:19:04.628887Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation 028ed720-1fb6-41e3-974c-81470a1e893c · inbound

Stellar Obliquities of Young Systems, Atmospheres Undergoing Contraction and Escape (SOYSAUCE) II: a 135 Myr planet on an aligned orbit with transit timing variations cites this paper.

Stellar Obliquities of Young Systems, Atmospheres Undergoing Contraction and Escape (SOYSAUCE) II: a 135 Myr planet on an aligned orbit with transit timing variations The Prevalence of Resonance Among Young, Close-in Planets

Reference 19

Resolution: verified exact; arxiv_id, observed 2026-06-27T14:51:01.714289Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation 27ec9eaf-c072-4eb2-a078-3bc18d3930e5 · inbound

How to measure tidal dissipation in long resonant chains cites this paper.

How to measure tidal dissipation in long resonant chains The Prevalence of Resonance Among Young, Close-in Planets

Reference 157

Resolution: metadata mismatch; local_arxiv, observed 2026-07-10T05:46:50.151657Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation 702308f4-013a-4af3-9bae-c0ba543130dc · inbound

HD 148797: A bright F-type star with two moderate-period low-density sub-Jovian planets. Compact multi-planet architectures are common in the Neptunian savanna cites this paper.

HD 148797: A bright F-type star with two moderate-period low-density sub-Jovian planets. Compact multi-planet architectures are common in the Neptunian savanna The Prevalence of Resonance Among Young, Close-in Planets

Reference 125

Resolution: unresolved; no resolver link, observed 2026-07-13T01:25:33.763066Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e166f621-9c3e-4e4f-b1b0-e4f5d1e9de1f · inbound

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

Dynamically Selected Mass-Radius Relationship for Low Mass Exoplanets The Prevalence of Resonance Among Young, Close-in Planets

Reference 122

Resolution: unresolved; no resolver link, observed 2026-08-01T12:14:31.412632Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.