Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Tomography of cool giant and supergiant star atmospheres. I. Validation of the method
As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1711.08327.
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 2026-08-17T06:30:58.91139+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-14T15:00:24.072330Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-05-11T06:10:58.685828Z
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 cba4eb1b-afbc-4757-9bf5-a4c392e30513 · inbound
Numerical Simulations of Cosmic-Ray Acceleration at Core-Collapse Supernovae cites this paper.
Numerical Simulations of Cosmic-Ray Acceleration at Core-Collapse Supernovae Tomography of cool giant and supergiant star atmospheres. I. Validation of the method
Reference 10
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T15:00:24.072330Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 3028b762-078b-463c-ac22-057727b60d19 · inbound
3D Non-LTE radiation transfer: theory and applications to stars, exoplanets, and kilonovae cites this paper.
3D Non-LTE radiation transfer: theory and applications to stars, exoplanets, and kilonovae Tomography of cool giant and supergiant star atmospheres. I. Validation of the method
Reference 274
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T23:49:13.884871Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation bb426b3a-5515-40c7-966a-4673937cc236 · inbound
Tracing the s-Process: Spectroscopic Insights into Chemical Abundances in O- and C-rich Evolved Stars cites this paper.
Tracing the s-Process: Spectroscopic Insights into Chemical Abundances in O- and C-rich Evolved Stars Tomography of cool giant and supergiant star atmospheres. I. Validation of the method
Reference 40
- Resolution
- malformed identifier
- arxiv_id, observed 2026-07-04T22:33:49.965779Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.