Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Fits for the convective envelope mass in massive stars
As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2402.13180.
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 2026-08-17T06:30:58.91139+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-03T01:21:04.206546Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-07-04T12:09:49.327227Z
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 07859e4e-4f6b-4946-8b9b-8bdba06f9292 · inbound
Modern tidal interaction models for rapid binary population synthesis: I. Methods cites this paper.
Modern tidal interaction models for rapid binary population synthesis: I. Methods Fits for the convective envelope mass in massive stars
Reference 58
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T01:21:04.206546Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation e90169c2-ce45-4d12-a737-1d33aa21cc38 · inbound
Modern tidal interaction models for rapid binary population synthesis: II. Binary black hole formation, mergers, and spins cites this paper.
Modern tidal interaction models for rapid binary population synthesis: II. Binary black hole formation, mergers, and spins Fits for the convective envelope mass in massive stars
Reference 30
- Resolution
- verified exact
- arxiv_id, observed 2026-07-04T12:09:49.328576Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.