Paper Citation Record · LEDGER

Explaining the coexistence of large-scale and small-scale magnetic fields in fully convective stars

As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:1510.05541.

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

pith.paper-citation-record.v1
1510.05541 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 2026-08-18T06:34:40.430872+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-07-14T03:58:35.317650Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-01T03:05:19.423261Z

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 bee596b0-d873-46fa-9538-eb8158f5df6a · inbound

Testing the reliability of magnetic field strength measurements for M dwarfs cites this paper.

Testing the reliability of magnetic field strength measurements for M dwarfs Explaining the coexistence of large-scale and small-scale magnetic fields in fully convective stars

Reference 31

Resolution: metadata mismatch; local_arxiv, observed 2026-05-20T00:47:54.649053Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation 6c59af74-cb4f-4ab6-b91b-17b688cad163 · inbound

Magnetic activity in cool stars: manifestations and relevance to exoplanets cites this paper.

Magnetic activity in cool stars: manifestations and relevance to exoplanets Explaining the coexistence of large-scale and small-scale magnetic fields in fully convective stars

Reference 173

Resolution: verified exact; local_arxiv, observed 2026-07-01T03:05:19.424462Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation ac4440d6-a623-4866-9537-9f11860bf380 · inbound

Magnetic activity in cool stars: manifestations and relevance to exoplanets cites this paper.

Magnetic activity in cool stars: manifestations and relevance to exoplanets Explaining the coexistence of large-scale and small-scale magnetic fields in fully convective stars

Reference 9

Resolution: unresolved; no resolver link, observed 2026-07-13T07:12:16.870340Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 06147d68-a53f-4b54-8883-2fae6a25323b · inbound

Unstable magnetospheric accretion on the T Tauri star TW Hya cites this paper.

Unstable magnetospheric accretion on the T Tauri star TW Hya Explaining the coexistence of large-scale and small-scale magnetic fields in fully convective stars

Reference 57

Resolution: unresolved; no resolver link, observed 2026-07-14T03:58:35.317650Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.