Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
ALMA-IMF. XXI.: N$_2$H$^+$ kinematics in the G012.80 protocluster: Evidence for filament rotation and evolution
As of 23 July 2026, this Paper Citation Record lists 0 of 0 outbound references and 1 inbound Pith citation observation for arXiv:2510.03447.
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 2026-07-23T06:31:01.910684+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-07-14T15:02:03.459139Z
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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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 06e87d6f-9a8e-4f7d-8ba2-1634d9f03c5a · inbound
How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching cites this paper.
How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching ALMA-IMF. XXI.: N$_2$H$^+$ kinematics in the G012.80 protocluster: Evidence for filament rotation and evolution
Reference 46
- Resolution
- unresolved
- no resolver link, observed 2026-07-14T15:02:03.459139Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.