Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Dynamic star formation in the massive DR21 filament
As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1003.4198.
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 2026-08-11T06:34:44.6726+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-11T04:45:22.819257Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-05-21T03:59:32.185979Z
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 aa331a6f-a973-41db-bcbb-087baa701b66 · inbound
Study of the physical and chemical properties of dense clumps at different evolutionary stages in several regions of massive star and stellar cluster formation cites this paper.
Study of the physical and chemical properties of dense clumps at different evolutionary stages in several regions of massive star and stellar cluster formation Dynamic star formation in the massive DR21 filament
Reference 34
- Resolution
- unresolved
- no resolver link, observed 2026-08-11T04:45:22.819257Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 751fef98-3487-4b83-a246-49109af34444 · inbound
Evolution of compressed clouds formed by filament coalescence. I. Oblique collisions cites this paper.
Evolution of compressed clouds formed by filament coalescence. I. Oblique collisions Dynamic star formation in the massive DR21 filament
Reference 139
- Resolution
- verified exact
- local_arxiv, observed 2026-05-21T03:59:32.187511Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 035c906b-35fa-4df1-afce-c05a8bd09cca · inbound
Challenges in probing turbulent and magnetic support in cores: the W43-MM1 protocluster case study cites this paper.
Challenges in probing turbulent and magnetic support in cores: the W43-MM1 protocluster case study Dynamic star formation in the massive DR21 filament
Reference 52
- Resolution
- unresolved
- no resolver link, observed 2026-07-14T00:54:38.663915Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.