Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Masses and Luminosities of O and B - type stars and red super giants
As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1003.2335.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-10T06:31:04.303077+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-07T20:40:57.478179Z
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 1e8ed8e0-a7ef-4186-a7f5-79e4f71e31ed · 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 Masses and Luminosities of O and B - type stars and red super giants
Reference 89
- Resolution
- unresolved
- no resolver link, observed 2026-07-31T12:04:43.460032Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 2a297db0-5be6-4687-93a5-e7c2979a7977 · inbound
A multi-epoch spectral and photometric study to understand the nature of the interesting Be star candidate HD 249179 cites this paper.
A multi-epoch spectral and photometric study to understand the nature of the interesting Be star candidate HD 249179 Masses and Luminosities of O and B - type stars and red super giants
Reference 71
- Resolution
- unresolved
- no resolver link, observed 2026-08-04T17:48:13.898926Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 1822470e-7418-429b-b692-68a417d75650 · inbound
Why do massive stars form bow shocks? Bulk ISM motion as the main driver of bow shock formation and geometry cites this paper.
Why do massive stars form bow shocks? Bulk ISM motion as the main driver of bow shock formation and geometry Masses and Luminosities of O and B - type stars and red super giants
Reference 175
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T20:40:57.478179Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.