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Paper Citation Record · LEDGER

Analytical Treatment of Planetary Resonances

As of 21 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1305.6513.

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

pith.paper-citation-record.v1
1305.6513 v1

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 2026-08-21T06:32:19.484+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-07-13T01:25:33.763066Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-10T05:46:49.951652Z

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 bd18bba1-b492-4bde-bcd4-60a0b429b7bb · inbound

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

How to measure tidal dissipation in long resonant chains Analytical Treatment of Planetary Resonances

Reference 32

Resolution
verified exact
local_arxiv, observed 2026-07-10T05:46:49.953162Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:ab5713861a5330395560cb5984d76806d7b72a54f983b4f38c4824d543f292b7

Observation 10f5ac54-8923-4bf7-9ff9-968d25bc4008 · 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 Analytical Treatment of Planetary Resonances

Reference 109

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

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-13T01:25:33.763066Z digest=sha256:903087de31f3a0182fa4c70216b2ebe0ea38043a0db3424483d2610dff0df3f8