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Paper Citation Record · LEDGER

Rotating Massive Main-Sequence Stars II: Simulating a Population of LMC early B-type Stars as a Test of Rotational Mixing

As of 16 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1102.0766.

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

pith.paper-citation-record.v1
1102.0766 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 2026-08-16T06:30:59.297886+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-10T23:05:22.299782Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-10T23:05:22.897815Z

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 67e2c26f-6f36-49f0-8cae-c2a96194e469 · inbound

Probing Heavy Axion-like Particles from Massive Stars with X-rays and Gamma Rays cites this paper.

Probing Heavy Axion-like Particles from Massive Stars with X-rays and Gamma Rays Rotating Massive Main-Sequence Stars II: Simulating a Population of LMC early B-type Stars as a Test of Rotational Mixing

Reference 86

Resolution
verified exact
local_arxiv, observed 2026-08-10T23:05:22.902814Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

source=pdf_text observed=2026-08-10T23:05:22.299782Z digest=sha256:a02f9eb6a9416d68b838b1494b96f71cb3cfc0449d95e3c2609dd2c39fdce9af

Observation a07eda96-5102-4eb3-9239-253bf47319c1 · 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 Rotating Massive Main-Sequence Stars II: Simulating a Population of LMC early B-type Stars as a Test of Rotational Mixing

Reference 38

Resolution
unresolved
no resolver link, observed 2026-08-03T02:40:39.377702Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-03T02:40:39.377702Z digest=sha256:7043470ad3c5a8e3fcb489961215e000a46a483fa8f9f025f8ffe0aec4be31e2