Paper Citation Record · LEDGER

Three-dimensional simulations of near-surface convection in main-sequence stars. III. The structure of small-scale magnetic flux concentrations

As of 13 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:1505.04739.

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

pith.paper-citation-record.v1
1505.04739 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 2026-08-13T06:32:02.005865+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T00:15:44.517612Z

measured 1 of 1 external citation measurements

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

Source: pith, observed 2026-08-05T02:28:24.338817Z

Reference resolution

0 of 0 outbound references displayed

verified exact0
verified fuzzy0
unresolved0
parse uncertain0
malformed identifier0
metadata mismatch0

External citation measurements

63
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation d33947dc-99de-4228-aece-1949bfe67826 · 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 Three-dimensional simulations of near-surface convection in main-sequence stars. III. The structure of small-scale magnetic flux concentrations

Reference 25

Resolution: metadata mismatch; local_arxiv, observed 2026-05-20T00:47:54.663995Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

Observation 3ea36eb1-89b5-4f9e-ac2c-c05f8902848f · inbound

Decoding the Radial Velocity Signatures of Solar Faculae with 3D MHD Simulations cites this paper.

Decoding the Radial Velocity Signatures of Solar Faculae with 3D MHD Simulations Three-dimensional simulations of near-surface convection in main-sequence stars. III. The structure of small-scale magnetic flux concentrations

Reference 51

Resolution: verified exact; local_arxiv, observed 2026-05-22T03:34:33.817810Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

Observation 6c9e31ff-56e3-4f46-9872-bd3f09d6e58c · inbound

Spectral Ratio Analysis: probing of a new suite of stellar activity indicators as a tool for astrophysical noise mitigation cites this paper.

Spectral Ratio Analysis: probing of a new suite of stellar activity indicators as a tool for astrophysical noise mitigation Three-dimensional simulations of near-surface convection in main-sequence stars. III. The structure of small-scale magnetic flux concentrations

Reference 41

Resolution: verified exact; local_arxiv, observed 2026-07-08T09:54:50.863182Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

Observation 63c85556-098e-4670-9390-b1030bb25747 · 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 Three-dimensional simulations of near-surface convection in main-sequence stars. III. The structure of small-scale magnetic flux concentrations

Reference 169

Resolution: unresolved; no resolver link, observed 2026-08-07T00:15:44.517612Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.