Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Filament formation due to diffusive instabilities in dusty protoplanetary disks
As of 21 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 1 inbound Pith citation observation for arXiv:2311.17996.
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 2026-08-01T10:42:14.552369Z
A source-named dated measurement, never combined with another source.
Source: cited_works
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 1494241f-5030-4972-83c5-65b5b2192e4e · inbound
Dust and Gas Transport in Substructured Nonideal MHD Wind-Launching Disks with Embedded Planets cites this paper.
Dust and Gas Transport in Substructured Nonideal MHD Wind-Launching Disks with Embedded Planets Filament formation due to diffusive instabilities in dusty protoplanetary disks
Reference 142
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T10:42:14.552369Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.