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Paper Citation Record · LEDGER

Eccentricity Evolution for Planets in Gaseous Disks

As of 14 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:astro-ph/0202462.

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

pith.paper-citation-record.v1
astro-ph/0202462 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 5 of 5 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-14T06:32:32.682623+00:00

measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-03T04:44:17.461176Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-03T18:58:50.111074Z

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 1b94ac1b-8a60-44f7-bfda-be40e41cbe99 · inbound

Understanding eccentric temperate giants: an in-depth study of the architecture and stellar obliquity of the TOI-2134 system cites this paper.

Understanding eccentric temperate giants: an in-depth study of the architecture and stellar obliquity of the TOI-2134 system Eccentricity Evolution for Planets in Gaseous Disks

Reference 103

Resolution
verified exact
local_arxiv, observed 2026-07-02T05:26:39.301983Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:6a58ed004b95d56095e80a41d3215341a4c26147f46a00faee23436b8fa17d49

Observation 9aa8cfb5-2669-4dc7-a720-1d5add6a3780 · inbound

Understanding eccentric temperate giants: an in-depth study of the architecture and stellar obliquity of the TOI-2134 system cites this paper.

Understanding eccentric temperate giants: an in-depth study of the architecture and stellar obliquity of the TOI-2134 system Eccentricity Evolution for Planets in Gaseous Disks

Reference 103

Resolution
verified exact
local_arxiv, observed 2026-07-03T18:58:50.112301Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:ec0e8e33d949ed51c0e62caa088aa56bb5b55efd72a38485e0d86c2ed9b91399

Observation 900b29ae-35ea-4ade-9b61-3bc1c20e5ee4 · inbound

Understanding eccentric temperate giants: an in-depth study of the architecture and stellar obliquity of the TOI-2134 system cites this paper.

Understanding eccentric temperate giants: an in-depth study of the architecture and stellar obliquity of the TOI-2134 system Eccentricity Evolution for Planets in Gaseous Disks

Reference 103

Resolution
unresolved
no resolver link, observed 2026-07-12T09:03:32.977007Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-12T09:03:32.977007Z digest=sha256:4beb71992b53caf555342a46154818be373a5fbc597ef0d9bf2ffc9fa73591b7

Observation 57b0fb29-2d0b-47d1-9705-32e850f2c806 · inbound

Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653 cites this paper.

Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653 Eccentricity Evolution for Planets in Gaseous Disks

Reference 52

Resolution
unresolved
no resolver link, observed 2026-08-01T12:49:01.575142Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T12:49:01.575142Z digest=sha256:522707e900c281241ab826e4ff5271048b9f0a6edd90db2293b1d1dafaa37436

Observation e3688d91-161c-44c9-998c-d3160925dd65 · inbound

Warm Sub-Saturns Orbiting Single Stars Are Spin-Orbit Aligned cites this paper.

Warm Sub-Saturns Orbiting Single Stars Are Spin-Orbit Aligned Eccentricity Evolution for Planets in Gaseous Disks

Reference 250

Resolution
unresolved
no resolver link, observed 2026-08-03T04:44:17.461176Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-03T04:44:17.461176Z digest=sha256:bbdfaf616110b76004151d7bfa98e12e9145b21c65aabf4e3491a3efc4c32e11