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Paper Citation Record · LEDGER

Disk eccentricity and embedded planets

As of 13 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:astro-ph/0510393.

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

pith.paper-citation-record.v1
astro-ph/0510393 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 2026-08-13T06:32:02.005865+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-02T01:07:57.187521Z

measured 0 of 1 external citation measurements

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

Source: cited_works

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 e89dc551-7050-44cd-83ec-e5b3de7590ca · inbound

Dust Growth in Binary Systems: Inhibition of dust settling and growth in circumbinary discs cites this paper.

Dust Growth in Binary Systems: Inhibition of dust settling and growth in circumbinary discs Disk eccentricity and embedded planets

Reference 291

Resolution
unresolved
no resolver link, observed 2026-08-02T01:07:57.187521Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T01:07:57.187521Z digest=sha256:2aaa66cf85533d23aca81a0dbfdf615931b1d1922790e32287fbf9dc163746f1

Observation f220336b-1bbb-45c3-9245-49b3b8796577 · 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 Disk eccentricity and embedded planets

Reference 51

Resolution
unresolved
no resolver link, observed 2026-08-02T00:06:51.284768Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T00:06:51.284768Z digest=sha256:f703c27e99d8450c2b5df3aeae158881ff31f1549384980ce808340859dfa8a7