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Paper Citation Record · LEDGER

One size does not fit all: Evidence for a range of mixing efficiencies in stellar evolution calculations

As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2107.09075.

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

pith.paper-citation-record.v1
2107.09075 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 2026-08-09T06:31:02.800959+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-08T13:33:06.472365Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-14T09:00:22.706835Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
  • unresolved0
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  • 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 88330f54-e8f3-42a0-abb9-111c7093c9f7 · inbound

Asteroseismic forward modelling of 36 $\beta$ Cep pulsators and inferences on their internal differential rotation cites this paper.

Asteroseismic forward modelling of 36 $\beta$ Cep pulsators and inferences on their internal differential rotation One size does not fit all: Evidence for a range of mixing efficiencies in stellar evolution calculations

Reference 79

Resolution
verified exact
local_arxiv, observed 2026-07-14T09:00:22.708679Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

source=arxiv_source observed=2026-07-14T08:55:08.442634Z digest=sha256:9e62702080ce70cadb03e80480347052072cea248480d1e3ca631756ad15bb11

Observation 24ea7585-b0e7-4859-9508-caf4c4932012 · inbound

The IACOB project XVIII. Prevalence of short-period binaries among Galactic helium rich O-type stars cites this paper.

The IACOB project XVIII. Prevalence of short-period binaries among Galactic helium rich O-type stars One size does not fit all: Evidence for a range of mixing efficiencies in stellar evolution calculations

Reference 72

Resolution
unresolved
no resolver link, observed 2026-08-08T13:33:06.472365Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-08T13:33:06.472365Z digest=sha256:e1a307aaccf84e81c635483e941d5ad6c61b782c9d4a30c3761367bddeab67f5