Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Can we believe the strong-line abundances in giant HII regions and emission-line galaxies?
As of 13 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 1 inbound Pith citation observation for arXiv:1906.04520.
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 2026-08-10T21:17:48.393928Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-10T21:17:48.773000Z
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 4065eba8-a70e-4afd-aa92-0579f48636a3 · inbound
Nebular emission from composite star-forming galaxies -- I. A novel modelling approach cites this paper.
Nebular emission from composite star-forming galaxies -- I. A novel modelling approach Can we believe the strong-line abundances in giant HII regions and emission-line galaxies?
Reference 89
- Resolution
- verified exact
- local_arxiv, observed 2026-08-10T21:17:48.779437Z
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.