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Paper Citation Record · LEDGER

Mass loss from late-type WN stars and its Z-dependence: very massive stars approaching the Eddington limit

As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:0803.0866.

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

pith.paper-citation-record.v1
0803.0866 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 4 of 4 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-12T06:34:41.77262+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T14:01:38.526881Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-06-28T13:02:10.909651Z

Reference resolution

0 of 0 outbound references displayed

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  • verified fuzzy0
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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 9db45750-a8eb-4c41-bde4-5b09c736c197 · inbound

Wolf-Rayet Colliding Wind Binaries cites this paper.

Wolf-Rayet Colliding Wind Binaries Mass loss from late-type WN stars and its Z-dependence: very massive stars approaching the Eddington limit

Reference 58

Resolution
unresolved
no resolver link, observed 2026-08-11T14:01:38.526881Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-11T14:01:38.526881Z digest=sha256:3d984595ba775f7c30edc09e0c6971684d8f204ce5c143f0e14899a33a7c2c16

Observation e98421bb-5947-4210-b71b-4737704c3620 · inbound

Can current models predict the local black hole merger rate? cites this paper.

Can current models predict the local black hole merger rate? Mass loss from late-type WN stars and its Z-dependence: very massive stars approaching the Eddington limit

Reference 103

Resolution
verified exact
local_arxiv, observed 2026-06-28T13:02:10.910902Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:326b5991df85c879ec051a1a7aeec4b7ed4ffba532a61afba6dd54ac1261ea4b

Observation 20d3911f-670a-4e98-8347-17bfed75eb0d · inbound

Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI cites this paper.

Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI Mass loss from late-type WN stars and its Z-dependence: very massive stars approaching the Eddington limit

Reference 181

Resolution
verified exact
local_arxiv, observed 2026-06-26T18:09:41.735466Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:1c755d194c3ace84f93b98cc163856299aa1162f39ee1f1d7d8bd145886cf643

Observation 63cbd4c1-846b-43de-9380-0f8329388ded · inbound

The Stellar Winds Atlas II: Black Hole Formation at Solar Metallicity cites this paper.

The Stellar Winds Atlas II: Black Hole Formation at Solar Metallicity Mass loss from late-type WN stars and its Z-dependence: very massive stars approaching the Eddington limit

Reference 236

Resolution
unresolved
no resolver link, observed 2026-08-01T00:42:41.607972Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T00:42:41.607972Z digest=sha256:4966ceef9604f8caaa198bcabcdda53dfb817537a052b02755bdfd854471b2bc