Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
The Physical Properties of Red Supergiants
As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:0911.4720.
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 2026-08-18T06:34:40.430872+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-16T11:56:28.410502Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-16T12:16:17.039197Z
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 7269246e-8662-4950-b6a7-361438936da8 · inbound
Machine Learning Classification of Young Stellar Objects and Evolved Stars in the Magellanic Clouds Using the Probabilistic Random Forest Classifier cites this paper.
Machine Learning Classification of Young Stellar Objects and Evolved Stars in the Magellanic Clouds Using the Probabilistic Random Forest Classifier The Physical Properties of Red Supergiants
Reference 26
- Resolution
- unresolved
- no resolver link, observed 2026-08-16T11:56:28.410502Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 8b7800e0-1e99-4e7d-bdf3-d59f2bc5867e · inbound
Dusty stellar sources classification by implementing machine learning methods based on spectroscopic observations in the Magellanic Clouds cites this paper.
Dusty stellar sources classification by implementing machine learning methods based on spectroscopic observations in the Magellanic Clouds The Physical Properties of Red Supergiants
Reference 55
- Resolution
- verified exact
- local_arxiv, observed 2026-08-16T11:56:16.716221Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.