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Paper Citation Record · LEDGER

Main-sequence systems: orbital stability in stellar binaries

As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2407.13901.

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

pith.paper-citation-record.v1
2407.13901 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 2026-08-11T06:34:44.6726+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-10T21:20:40.914830Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-06T15:02:07.215059Z

Reference resolution

0 of 0 outbound references displayed

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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 a048b3c5-9acc-41e2-99d0-5b0e2b99df08 · inbound

Planet formation and long-term stability in a very eccentric stellar binary cites this paper.

Planet formation and long-term stability in a very eccentric stellar binary Main-sequence systems: orbital stability in stellar binaries

Reference 17

Resolution
unresolved
no resolver link, observed 2026-08-10T21:20:40.914830Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T21:20:40.914830Z digest=sha256:02b0078c58d52f6fbce1286df390b648c79941c98049d98921fd720a48248136

Observation 0e7198d6-fc70-4a92-9e6c-e7334c9b89dd · inbound

Orbital Stability of Hierarchical 3 and 4-Body Systems with Inclination: Results for Kepler-1625, 1708, and HD 23079 cites this paper.

Orbital Stability of Hierarchical 3 and 4-Body Systems with Inclination: Results for Kepler-1625, 1708, and HD 23079 Main-sequence systems: orbital stability in stellar binaries

Reference 37

Resolution
unresolved
no resolver link, observed 2026-08-10T17:25:36.541817Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T17:25:36.541817Z digest=sha256:e8511362ff067dcf930511efec7745842377e3e33f89027a1c40fc87f11ff172

Observation 815d6cec-038a-4621-a25b-b9aa4de9157f · inbound

Secular Resonances in Planet-Hosting Binary Stars. I. General Theory cites this paper.

Secular Resonances in Planet-Hosting Binary Stars. I. General Theory Main-sequence systems: orbital stability in stellar binaries

Reference 12

Resolution
verified exact
local_arxiv, observed 2026-08-06T15:02:07.221027Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

source=arxiv_source observed=2026-08-06T15:02:07.184268Z digest=sha256:34e96d297d5d95deee05f013966ec65e9e96b9e65f3e2dd3066f74bde97f88db