Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Effects of close binary evolution on the main-sequence morphology of young star clusters
As of 4 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1912.07294.
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 2026-08-04T06:34:03.388597+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-03T14:34:30.500956Z
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 b1a502c0-5300-4794-aab3-c7101eb5ee8e · inbound
Stable mass transfer in massive binaries leading to merging black holes cites this paper.
Stable mass transfer in massive binaries leading to merging black holes Effects of close binary evolution on the main-sequence morphology of young star clusters
Reference 86
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T14:34:30.500956Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation b90054c5-a796-41c9-b788-155c703965d5 · inbound
Examining the stellar-merger origin of the blue main sequence in the open cluster NGC\,3532 with N-body simulations cites this paper.
Examining the stellar-merger origin of the blue main sequence in the open cluster NGC\,3532 with N-body simulations Effects of close binary evolution on the main-sequence morphology of young star clusters
Reference 13
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T14:44:02.103433Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.