Paper Citation Record · LEDGER

Dynamical Origin of Extrasolar Planet Eccentricity Distribution

As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 9 inbound Pith citation observations for arXiv:astro-ph/0703160.

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

pith.paper-citation-record.v1
astro-ph/0703160 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 9 of 9 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-12T06:34:41.77262+00:00

measured 9 of 9 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-02T00:06:51.293492Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-03T18:58:49.843854Z

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 cbd95c3d-b42c-445b-a483-329233dbd353 · inbound

Planet-Planet Secular Migration Predicts a Stellar Obliquity-Period Anti-Correlation cites this paper.

Planet-Planet Secular Migration Predicts a Stellar Obliquity-Period Anti-Correlation Dynamical Origin of Extrasolar Planet Eccentricity Distribution

Reference 248

Resolution: verified exact; local_arxiv, observed 2026-06-26T15:29:33.381010Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation 5fe4502b-2164-4d59-8ff3-1eeba522e5a5 · inbound

Observing a 542-day transiting giant with large TTVs: The 2025 transit of HIP 41378 f and new constraints on the outer system cites this paper.

Observing a 542-day transiting giant with large TTVs: The 2025 transit of HIP 41378 f and new constraints on the outer system Dynamical Origin of Extrasolar Planet Eccentricity Distribution

Reference 241

Resolution: verified exact; local_arxiv, observed 2026-06-26T07:19:07.910460Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation 9518f668-8b70-438d-9809-13f50ad0eadf · inbound

Observing a 542-day transiting giant with large TTVs: The 2025 transit of HIP 41378 f and new constraints on the outer system cites this paper.

Observing a 542-day transiting giant with large TTVs: The 2025 transit of HIP 41378 f and new constraints on the outer system Dynamical Origin of Extrasolar Planet Eccentricity Distribution

Reference 241

Resolution: verified exact; local_arxiv, observed 2026-06-30T10:24:35.561606Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation 662f2d3e-1f90-42d5-9105-7b70b120803a · 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 Dynamical Origin of Extrasolar Planet Eccentricity Distribution

Reference 93

Resolution: verified exact; local_arxiv, observed 2026-07-02T05:26:39.291678Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation 0a911fd2-a77d-4f5b-9395-578cd1352721 · 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 Dynamical Origin of Extrasolar Planet Eccentricity Distribution

Reference 93

Resolution: verified exact; local_arxiv, observed 2026-07-03T18:58:49.845268Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation b0d83ac6-3492-480b-8e2b-ae8a1d89e0cd · 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 Dynamical Origin of Extrasolar Planet Eccentricity Distribution

Reference 93

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

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d95c906f-0d2c-4216-bf8e-bf0cc0115d74 · inbound

The majority of hot Jupiters formed beyond the water ice line cites this paper.

The majority of hot Jupiters formed beyond the water ice line Dynamical Origin of Extrasolar Planet Eccentricity Distribution

Reference 53

Resolution: unresolved; no resolver link, observed 2026-08-02T00:06:51.293492Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6fc61bb5-c22e-432a-bd77-3153074623a3 · inbound

Dynamical formation of long-period exoplanets systems in evolving binary stars cites this paper.

Dynamical formation of long-period exoplanets systems in evolving binary stars Dynamical Origin of Extrasolar Planet Eccentricity Distribution

Reference 197

Resolution: unresolved; no resolver link, observed 2026-08-01T13:29:21.780329Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation fb058453-383d-48ed-ac41-65515a4f13cf · 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 Dynamical Origin of Extrasolar Planet Eccentricity Distribution

Reference 78

Resolution: unresolved; no resolver link, observed 2026-08-01T12:49:04.668717Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.