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Paper Citation Record · LEDGER

Effects of close binary evolution on the main-sequence morphology of young star clusters

As of 23 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.

pith.paper-citation-record.v1
1912.07294 v2

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 2026-08-22T06:32:14.747728+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-03T14:34:30.500956Z

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 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.

source=pdf_text observed=2026-08-03T14:34:30.500956Z digest=sha256:df4dd68bc385db885cf825d84ac0ae56f391f7870d0fcef6e0ef38d308579537

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.

source=arxiv_source observed=2026-08-01T14:44:02.103433Z digest=sha256:c54c7ed9a47569dee4237eda29e67509ce2886d76aa380aa5c2fb7923baa358c