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Paper Citation Record · LEDGER

How mergers magnetise massive stars

As of 23 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:1910.14058.

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

pith.paper-citation-record.v1
1910.14058 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 2026-08-22T06:32:14.747728+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-15T15:19:17.055569Z

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 fb869c3d-80bf-45b3-871a-96243ff543cf · 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 How mergers magnetise massive stars

Reference 139

Resolution
unresolved
no resolver link, observed 2026-08-03T14:34:36.606613Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-03T14:34:36.606613Z digest=sha256:eeebf5771e5093d335c8892817b4cb67f8fd7ddcad336881308ca42b1ae9e9f3

Observation 201e98a5-d103-4c70-a2f6-0d7057ffa189 · inbound

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir cites this paper.

First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir How mergers magnetise massive stars

Reference 179

Resolution
unresolved
no resolver link, observed 2026-08-15T15:19:17.055569Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T15:19:17.055569Z digest=sha256:fffbb269ef1c3411acd750f4ef24c95d35b051147f216b8a04e2ffde61fa4845

Observation 97f19bde-8afe-4a16-ae1c-41d4eb6e8cc4 · inbound

Something new under the Sun: A magnetically driven CH/CN anti-correlation cites this paper.

Something new under the Sun: A magnetically driven CH/CN anti-correlation How mergers magnetise massive stars

Reference 21

Resolution
unresolved
no resolver link, observed 2026-08-07T00:15:38.697134Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T00:15:38.697134Z digest=sha256:05802c897a0162644c655a516c37bc88b9759ded4558f1b344dba1de1a5a9db2

Observation 42594510-66c5-46c3-95a1-3c5f2f38086d · inbound

The symphony of pulsations and binarity among massive stars using HERMES spectroscopy and TESS photometry cites this paper.

The symphony of pulsations and binarity among massive stars using HERMES spectroscopy and TESS photometry How mergers magnetise massive stars

Reference 31

Resolution
unresolved
no resolver link, observed 2026-08-05T20:04:19.650172Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-05T20:04:19.650172Z digest=sha256:fb5a6cc7119545f9252b1f3cad6e6e1bb881d4d9898b01c4924ce9d1e13cdb24