Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Revisiting the statistical equilibrium of H$^-$ in stellar atmospheres
As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2407.19833.
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 2026-08-11T06:34:44.6726+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-07T00:23:02.199365Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-10T05:30:23.456663Z
Reference resolution
0 of 0 outbound references displayed
- verified exact0
- verified fuzzy0
- unresolved0
- parse uncertain0
- malformed identifier0
- metadata mismatch0
External citation measurements
0
pith, observed 2026-08-10T05:30:23.456663Z
Outbound references
No outbound reference observations are available for this paper version.
Pith citing papers
Observation 60e36e9b-41e0-4602-8364-925ae45a3e56 · inbound
The Future of Solar modelling: requirements for a new generation of solar models cites this paper.
The Future of Solar modelling: requirements for a new generation of solar models Revisiting the statistical equilibrium of H$^-$ in stellar atmospheres
Reference 20
- Resolution
- verified exact
- local_arxiv, observed 2026-08-07T00:23:41.071628Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 6103ef9f-4678-4c19-ad32-9d629d24df77 · 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 Revisiting the statistical equilibrium of H$^-$ in stellar atmospheres
Reference 47
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T23:48:49.860710Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.