Paper Citation Record · LEDGER

Are Coronae of Magnetically Active Stars Heated by Flares? III. Analytical Distribution of Superimposed Flares

As of 14 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:astro-ph/0312405.

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

pith.paper-citation-record.v1
astro-ph/0312405 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 2 of 2 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-14T06:32:32.682623+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-04T01:30:03.091481Z

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 5caeb6cf-2b58-46e9-b23a-b55fc468caab · inbound

Stellar impact on exoplanetary atmospheric evolution and habitability cites this paper.

Stellar impact on exoplanetary atmospheric evolution and habitability Are Coronae of Magnetically Active Stars Heated by Flares? III. Analytical Distribution of Superimposed Flares

Reference 10

Resolution: unresolved; no resolver link, observed 2026-08-01T06:15:37.778689Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 69787ebc-1abe-4e24-b634-38c6cf2726c4 · inbound

Stellar impact on exoplanetary atmospheric evolution and habitability cites this paper.

Stellar impact on exoplanetary atmospheric evolution and habitability Are Coronae of Magnetically Active Stars Heated by Flares? III. Analytical Distribution of Superimposed Flares

Reference 10

Resolution: unresolved; no resolver link, observed 2026-08-04T01:30:03.091481Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.