Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
High-mass Star Formation through Filamentary Collapse and Clump-fed Accretion in G22
As of 16 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1711.08951.
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 2026-08-16T06:30:59.297886+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-15T15:23:50.162272Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-05-21T03:59:32.212291Z
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 9d7734d7-26f3-46d3-b4e9-f710a943e659 · inbound
Global and Local Infall in the ASHES Sample (GLASHES). II. Asymmetric Line Profiles around Dense Cores in 70 $\mu$m Dark Massive Clumps cites this paper.
Global and Local Infall in the ASHES Sample (GLASHES). II. Asymmetric Line Profiles around Dense Cores in 70 $\mu$m Dark Massive Clumps High-mass Star Formation through Filamentary Collapse and Clump-fed Accretion in G22
Reference 242
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-05-14T20:57:58.186988Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 23a1c5b1-7956-4c89-b549-b92daf24917a · 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 High-mass Star Formation through Filamentary Collapse and Clump-fed Accretion in G22
Reference 123
- Resolution
- verified exact
- local_arxiv, observed 2026-05-21T03:59:32.213887Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation f8353f51-fd4d-48ab-a283-47528a7606c5 · inbound
Hub-filament systems and the growth of massive stars: episodic accretion, clustered environments, and projection effects cites this paper.
Hub-filament systems and the growth of massive stars: episodic accretion, clustered environments, and projection effects High-mass Star Formation through Filamentary Collapse and Clump-fed Accretion in G22
Reference 70
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T15:23:50.162272Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.