Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Revealing the Chemical Structure of the Magellanic Clouds with APOGEE. II. Abundance Gradients of the Large Magellanic Cloud
As of 21 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 1 inbound Pith citation observation for arXiv:2309.12503.
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 2026-08-21T06:32:19.484+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-07T04:26:36.478163Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-07T04:26:36.748867Z
Reference resolution
0 of 0 outbound references displayed
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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 720ca80d-0cfa-4bc8-8dcb-1b8647c66dbb · inbound
Str\"omgren photometric metallicity map of the Magellanic Cloud stars using Gaia DR3--XP spectra cites this paper.
Str\"omgren photometric metallicity map of the Magellanic Cloud stars using Gaia DR3--XP spectra Revealing the Chemical Structure of the Magellanic Clouds with APOGEE. II. Abundance Gradients of the Large Magellanic Cloud
Reference 55
- Resolution
- verified exact
- local_arxiv, observed 2026-08-07T04:26:36.753455Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.