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Paper Citation Record · LEDGER

Are Coronae of Magnetically Active Stars Heated by Flares? II. EUV and X-Ray Flare Statistics and the Differential Emission Measure Distribution

As of 16 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:astro-ph/0209075.

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

pith.paper-citation-record.v1
astro-ph/0209075 v2

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 2026-08-16T06:30:59.297886+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-04T01:30:02.966307Z

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

  • verified exact0
  • verified fuzzy0
  • unresolved0
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

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 eaf731bd-6bc4-4804-b4a0-1d068ac3232f · 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? II. EUV and X-Ray Flare Statistics and the Differential Emission Measure Distribution

Reference 9

Resolution
unresolved
no resolver link, observed 2026-08-01T06:15:37.618848Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T06:15:37.618848Z digest=sha256:9671709bf997d210c393d60ff16b0cb9dc5019130706250447da24d9fbc6b0d9

Observation 6a8b568f-e567-4484-a063-25a80208f7ef · 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? II. EUV and X-Ray Flare Statistics and the Differential Emission Measure Distribution

Reference 9

Resolution
unresolved
no resolver link, observed 2026-08-04T01:30:02.966307Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-04T01:30:02.966307Z digest=sha256:0f7460e1aa13d504ce0cd71fdaace1c3658948da31801ff42e8b5ea5309909d6