Paper Citation Record · LEDGER

Grids of stellar models with rotation IV. Models from 1.7 to 120 Msun at a metallicity Z = 0.0004

As of 4 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:1904.04009.

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

pith.paper-citation-record.v1
1904.04009 v1

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measured 0 of 0 reference resolution

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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 2026-08-03T06:30:56.289259+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-03T02:40:46.373740Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-06-26T18:09:41.433143Z

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Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation e7b9a30a-b8e2-4e7e-9917-819f14894517 · 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 Grids of stellar models with rotation IV. Models from 1.7 to 120 Msun at a metallicity Z = 0.0004

Reference 299

Resolution: verified exact; local_arxiv, observed 2026-06-26T18:09:41.434807Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-03T06:30:56.289259+00:00.

Observation b81450f4-c527-4ee0-b654-a2caa7a30760 · 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 Grids of stellar models with rotation IV. Models from 1.7 to 120 Msun at a metallicity Z = 0.0004

Reference 226

Resolution: unresolved; no resolver link, observed 2026-08-01T00:42:40.811854Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d3184f21-96ed-48b8-8b0f-4199bd9e3aa4 · inbound

HCO$^+$ and the Effect of Mixing in SN 1987A cites this paper.

HCO$^+$ and the Effect of Mixing in SN 1987A Grids of stellar models with rotation IV. Models from 1.7 to 120 Msun at a metallicity Z = 0.0004

Reference 184

Resolution: unresolved; no resolver link, observed 2026-08-01T00:40:48.659678Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f824fb38-6fb8-484a-84fd-695b7fa6d672 · 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 Grids of stellar models with rotation IV. Models from 1.7 to 120 Msun at a metallicity Z = 0.0004

Reference 126

Resolution: unresolved; no resolver link, observed 2026-08-03T02:40:46.373740Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.