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Paper Citation Record · LEDGER

Wavelike nature of the vertical shear instability in global protoplanetary disks

As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2206.03840.

A citation records a reference. It does not transfer a finding from one paper to another.

pith.paper-citation-record.v1
2206.03840 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 2 of 2 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-17T06:30:58.91139+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-12T17:35:54.118935Z

measured 0 of 1 external citation measurements

A source-named dated measurement, never combined with another source.

Source: pith, observed 2026-08-12T17:35:54.328108Z

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 28a6b178-0bb8-48a5-acb2-a6b62a84e398 · inbound

Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows cites this paper.

Developing a Non-Newtonian Fluid Model for Dust, for Application to Astrophysical Flows Wavelike nature of the vertical shear instability in global protoplanetary disks

Reference 78

Resolution
verified exact
local_arxiv, observed 2026-08-12T17:35:54.333242Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

source=arxiv_source observed=2026-08-12T17:35:54.118935Z digest=sha256:eaf1d77f81546acacd4ed1c8644061297434659811a5966a65a985f91ec6a611

Observation fbd8e20c-efe2-4bbd-8381-e1009df270fe · 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 Wavelike nature of the vertical shear instability in global protoplanetary disks

Reference 131

Resolution
unresolved
no resolver link, observed 2026-08-01T10:42:13.609394Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T10:42:13.609394Z digest=sha256:d06bb66748f1d977e8062e986be4faaf213c6a45a07eb5b1752d5eb806d4313b