Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Planetesimal Accretion in Binary Systems: Could Planets Form Around Alpha Centauri B ?
As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 1 inbound Pith citation observation for arXiv:1001.2614.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-11T06:34:44.6726+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-10T21:20:40.994013Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-10T21:20:41.685557Z
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 c1bbb7bd-820a-40e4-b06a-b3987ebf9733 · 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 Planetesimal Accretion in Binary Systems: Could Planets Form Around Alpha Centauri B ?
Reference 34
- Resolution
- verified exact
- local_arxiv, observed 2026-08-10T21:20:41.690953Z
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.