Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Dynamical Accretion Flows -- ALMAGAL: Flows along filamentary structures in high-mass star-forming clusters
As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2408.08299.
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 2026-08-10T06:31:04.303077+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-10T10:07:44.448643Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-10T10:07:44.564170Z
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 b2f936e6-1f0c-4f8d-aa4b-187a96a582dd · inbound
Star formation from low to high mass: A comparative view cites this paper.
Star formation from low to high mass: A comparative view Dynamical Accretion Flows -- ALMAGAL: Flows along filamentary structures in high-mass star-forming clusters
Reference 49
- Resolution
- verified exact
- local_arxiv, observed 2026-08-10T10:07:44.571843Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation 669db09b-8f23-49c3-a44a-e8011454aa58 · 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 Dynamical Accretion Flows -- ALMAGAL: Flows along filamentary structures in high-mass star-forming clusters
Reference 50
- Resolution
- unresolved
- no resolver link, observed 2026-07-14T15:02:03.459139Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 8cb1439a-4264-4468-96bd-e3c824f1d538 · 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 Dynamical Accretion Flows -- ALMAGAL: Flows along filamentary structures in high-mass star-forming clusters
Reference 50
- Resolution
- unresolved
- no resolver link, observed 2026-08-02T07:32:02.801844Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.