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Paper Citation Record · LEDGER

Properties of Galactic early-type O-supergiants: A combined FUV-UV and optical analysis

As of 16 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:1205.3075.

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

pith.paper-citation-record.v1
1205.3075 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 2026-08-16T06:30:59.297886+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-15T14:18:45.951184Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-06-26T18:09:41.201052Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
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  • 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 d6cf7ff7-e864-45f2-8194-b58395c8299e · inbound

Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI cites this paper.

Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI Properties of Galactic early-type O-supergiants: A combined FUV-UV and optical analysis

Reference 187

Resolution
verified exact
local_arxiv, observed 2026-06-26T18:09:41.202752Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:814956d597c5a9f2c5267df15f9a7233b15d04426911364341efcd92b4d99300

Observation 35555ff1-81f0-46f4-9982-c0257e6d10f0 · inbound

An Halpha survey of infrared bow-shocks around OB-type stars cites this paper.

An Halpha survey of infrared bow-shocks around OB-type stars Properties of Galactic early-type O-supergiants: A combined FUV-UV and optical analysis

Reference 95

Resolution
unresolved
no resolver link, observed 2026-07-31T12:04:43.494700Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-31T12:04:43.494700Z digest=sha256:1f0d279da77c536e3ddb5254f6f6352133afecb07847c5e670d92e4b6d9ab66f

Observation 6549883d-cd82-42b7-b738-ee47eabe290f · inbound

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants cites this paper.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants Properties of Galactic early-type O-supergiants: A combined FUV-UV and optical analysis

Reference 54

Resolution
unresolved
no resolver link, observed 2026-08-12T12:11:54.127162Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T12:11:54.127162Z digest=sha256:5d4849f091f6049ac1117769fcc9a78ff256fc0cb0f52f7acab84bff8e1a5913

Observation 443ed8da-065d-4179-a7eb-4884e3e458c8 · inbound

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants cites this paper.

Gravity modes and potential evidence for Rossby Waves in late O-type supergiants Properties of Galactic early-type O-supergiants: A combined FUV-UV and optical analysis

Reference 54

Resolution
unresolved
no resolver link, observed 2026-08-15T14:18:45.951184Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T14:18:45.951184Z digest=sha256:2256f168ccbeecc6209217f42d10160803cd536bf8677047cbf7007d92e45c8d