Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
On the nature of star-forming filaments: II. Sub-filaments and velocities
As of 21 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1509.03321.
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 2026-08-21T06:32:19.484+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-07-11T11:50:26.030339Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-05-22T08:11:15.819218Z
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 7618f697-7172-48bf-ba37-9a22c5637a0a · 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 On the nature of star-forming filaments: II. Sub-filaments and velocities
Reference 216
- Resolution
- verified exact
- local_arxiv, observed 2026-05-21T03:59:32.335609Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.
Observation 4fba5aa2-81e1-4eab-a667-7a387fa23935 · inbound
Numerical simulations of shock-driven, supersonic turbulence in colliding three-temperature laboratory plasmas cites this paper.
Numerical simulations of shock-driven, supersonic turbulence in colliding three-temperature laboratory plasmas On the nature of star-forming filaments: II. Sub-filaments and velocities
Reference 181
- Resolution
- verified exact
- local_arxiv, observed 2026-05-22T08:11:15.822305Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.
Observation ffada8fd-bd9b-4f32-85c4-204c8d33470c · inbound
Emergence of high-mass stars in complex fiber networks (EMERGE) VI. Turbulence dissipation and the formation of dense fibers cites this paper.
Emergence of high-mass stars in complex fiber networks (EMERGE) VI. Turbulence dissipation and the formation of dense fibers On the nature of star-forming filaments: II. Sub-filaments and velocities
Reference 151
- Resolution
- unresolved
- no resolver link, observed 2026-07-11T07:55:39.166465Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.