Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Luminosities and mass-loss rates of SMC and LMC AGB stars and Red Supergiants
As of 13 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:0908.3087.
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 2026-08-13T06:32:02.005865+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-12T14:37:35.117636Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-12T14:37:36.816705Z
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 df787abd-8467-43d9-9e06-f93593458c84 · inbound
JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822 cites this paper.
JWST NIRCam and MIRI Reveal the Dust-Producing AGB Population of NGC 6822 Luminosities and mass-loss rates of SMC and LMC AGB stars and Red Supergiants
Reference 58
- Resolution
- unresolved
- no resolver link, observed 2026-07-14T03:55:10.305506Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation ce4bef51-53e1-40a6-bb35-a785742d6660 · inbound
Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems cites this paper.
Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems Luminosities and mass-loss rates of SMC and LMC AGB stars and Red Supergiants
Reference 67
- Resolution
- verified exact
- local_arxiv, observed 2026-08-12T14:37:36.821378Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.