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Paper Citation Record · LEDGER

Spectroscopic and physical parameters of Galactic O-type stars. III. Mass discrepancy and rotational mixing

As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1803.03410.

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

pith.paper-citation-record.v1
1803.03410 v1

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 2026-08-08T06:32:00.761636+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-08T13:33:06.253240Z

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

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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 8c732458-ab5d-4088-97ec-e734a47d2db8 · inbound

The IACOB project XIX. Revisiting massive-star evolution with empirical TAMS constraints: updated models, overshoot calibration, and the population of blue supergiants cites this paper.

The IACOB project XIX. Revisiting massive-star evolution with empirical TAMS constraints: updated models, overshoot calibration, and the population of blue supergiants Spectroscopic and physical parameters of Galactic O-type stars. III. Mass discrepancy and rotational mixing

Reference 196

Resolution
unresolved
no resolver link, observed 2026-08-03T02:40:53.736725Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-03T02:40:53.736725Z digest=sha256:2ce86970416f2ac461a7da1a534dd1fb021c9063c80b99cad24bbefefa0839d3

Observation 84235dfd-7f08-4c22-9182-7a9b1cc16b07 · 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 Spectroscopic and physical parameters of Galactic O-type stars. III. Mass discrepancy and rotational mixing

Reference 5

Resolution
unresolved
no resolver link, observed 2026-08-08T13:33:06.253240Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-08T13:33:06.253240Z digest=sha256:e606801811eb440319c2bee5e2d4434270c16269b7ca39ae66b4d977d9dfc603