Paper Citation Record · LEDGER

Evolution of the Convective Core Mass during the Main Sequence

As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2409.00460.

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

pith.paper-citation-record.v1
2409.00460 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 2026-08-07T06:34:17.273281+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T15:03:31.825800Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-04T12:09:49.332180Z

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 a81abf18-737a-4fc7-9117-2aea0f9f5fb5 · inbound

Implications of modern mass-loss rates for massive stars cites this paper.

Implications of modern mass-loss rates for massive stars Evolution of the Convective Core Mass during the Main Sequence

Reference 109

Resolution: unresolved; no resolver link, observed 2026-08-06T15:03:31.825800Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a5f4b1c7-4422-481c-917f-15c71284a9b2 · inbound

Stable mass transfer in massive binaries leading to merging black holes cites this paper.

Stable mass transfer in massive binaries leading to merging black holes Evolution of the Convective Core Mass during the Main Sequence

Reference 169

Resolution: unresolved; no resolver link, observed 2026-08-03T14:34:39.902925Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c359bc47-b3da-474f-ac45-1bfef79ed42b · inbound

Modern tidal interaction models for rapid binary population synthesis: II. Binary black hole formation, mergers, and spins cites this paper.

Modern tidal interaction models for rapid binary population synthesis: II. Binary black hole formation, mergers, and spins Evolution of the Convective Core Mass during the Main Sequence

Reference 53

Resolution: verified exact; arxiv_id, observed 2026-07-04T12:09:49.334034Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation b61d463c-df92-40a6-b5e5-4b91d8e21056 · 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 Evolution of the Convective Core Mass during the Main Sequence

Reference 97

Resolution: unresolved; no resolver link, observed 2026-08-01T00:42:27.058159Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.