Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
High-mass star formation across the Large Magellanic Cloud I. Chemical properties and hot molecular cores observed with ALMA at 1.2 mm
As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2405.01710.
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 2026-08-08T06:32:00.761636+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-07T05:12:18.354299Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-07T06:16:28.064256Z
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 c695c4db-47cb-4c19-a67c-f972fc0e0022 · inbound
The detection of spatially resolved protosteller outflows and episodic jets in the outer Galaxy cites this paper.
The detection of spatially resolved protosteller outflows and episodic jets in the outer Galaxy High-mass star formation across the Large Magellanic Cloud I. Chemical properties and hot molecular cores observed with ALMA at 1.2 mm
Reference 23
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-08-07T05:12:19.445310Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.
Observation 2de67041-d372-4773-90d8-83df777a844c · inbound
Chemistry of Dark Molecular Clouds cites this paper.
Chemistry of Dark Molecular Clouds High-mass star formation across the Large Magellanic Cloud I. Chemical properties and hot molecular cores observed with ALMA at 1.2 mm
Reference 290
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T02:17:12.210280Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.