Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Extragalactic chemical abundances: do HII regions and young stars tell the same story? The case of the spiral galaxy NGC 300
As of 13 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 1 inbound Pith citation observation for arXiv:0905.2791.
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 2026-08-12T14:30:37.283825Z
A source-named dated measurement, never combined with another source.
Source: cited_works
Reference resolution
0 of 0 outbound references displayed
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- 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 00584c82-8875-428f-9ecb-3e23fd89fc10 · inbound
Analysis of the Internal Radial Gradient of Chemical Abundances in Spiral Galaxies from CALIFA cites this paper.
Analysis of the Internal Radial Gradient of Chemical Abundances in Spiral Galaxies from CALIFA Extragalactic chemical abundances: do HII regions and young stars tell the same story? The case of the spiral galaxy NGC 300
Reference 3
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T14:30:37.283825Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.