Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Convective characteristics of Fe I lines across the solar disc
As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2310.15782.
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 2026-08-15T06:32:42.880941+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-04T10:56:50.667175Z
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 8b36751d-d56b-48f9-82e7-000a8b25b9cd · 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 Convective characteristics of Fe I lines across the solar disc
Reference 159
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T23:49:02.681935Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 3f2e77cf-f79e-4d4a-977c-555f807edd5d · inbound
Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum cites this paper.
Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum Convective characteristics of Fe I lines across the solar disc
Reference 68
- Resolution
- unresolved
- no resolver link, observed 2026-08-04T10:56:50.667175Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.