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Paper Citation Record · LEDGER

Floating binary planets from ejections during close stellar encounters

As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2310.06016.

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

pith.paper-citation-record.v1
2310.06016 v3

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 2026-08-12T06:34:41.77262+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-10T15:41:26.258685Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-06T17:11:32.476409Z

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 5fe3f6b6-56f3-4d2c-91f1-17692ec83d0a · inbound

Exoplanet Occurrence Rate with Age for FGK Stars in Kepler cites this paper.

Exoplanet Occurrence Rate with Age for FGK Stars in Kepler Floating binary planets from ejections during close stellar encounters

Reference 95

Resolution
unresolved
no resolver link, observed 2026-08-10T15:41:26.258685Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T15:41:26.258685Z digest=sha256:922315493095fd9abe00fadfce3a3890711388f017890c42ea3856281c63e460

Observation 2760aa20-cffa-46b5-9946-0f7833aafac5 · inbound

Why Wide Jupiter-Mass Binary-Objects Cannot Form cites this paper.

Why Wide Jupiter-Mass Binary-Objects Cannot Form Floating binary planets from ejections during close stellar encounters

Reference 2

Resolution
metadata mismatch
local_arxiv, observed 2026-08-06T17:11:32.481680Z

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.

source=pdf_text observed=2026-08-06T17:11:32.073625Z digest=sha256:c51919d15aaa8d9ecb69493e9fded469da8399cde79d763874b9429847b557ee