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Paper Citation Record · LEDGER

Protoplanetary Disk Turbulence Driven by the Streaming Instability: Linear Evolution and Numerical Methods

As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:astro-ph/0702625.

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

pith.paper-citation-record.v1
astro-ph/0702625 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 3 of 3 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 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-12T17:35:54.155875Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-06-27T11:40:53.559718Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
  • unresolved0
  • parse uncertain0
  • malformed identifier0
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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 6b75a790-6cb1-412a-a217-623f5378b504 · 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 Protoplanetary Disk Turbulence Driven by the Streaming Instability: Linear Evolution and Numerical Methods

Reference 87

Resolution
unresolved
no resolver link, observed 2026-08-12T17:35:54.155875Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T17:35:54.155875Z digest=sha256:0b4d5f30f1a111e7b7ad0819e0bb0ffb2151251d73e18c66321b69ab2d1c4160

Observation fdfbd6c8-25bb-4134-b31b-35360242920c · inbound

Planet formation at the inner edge of the dead zone II. Outbursts, rings, vortices, and suppression of planetesimal formation cites this paper.

Planet formation at the inner edge of the dead zone II. Outbursts, rings, vortices, and suppression of planetesimal formation Protoplanetary Disk Turbulence Driven by the Streaming Instability: Linear Evolution and Numerical Methods

Reference 286

Resolution
verified exact
local_arxiv, observed 2026-06-27T11:40:53.561161Z

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=2026-07-11T11:50:26.030339Z digest=sha256:9ed930f00da4f6fc57419d720d8de8afb219fc6cf59324fa5916e8d106b0b400

Observation 91828262-8a20-4257-9360-c68f4d9ad17d · inbound

A JWST, ALMA and VLA survey of the Ophiuchus-A star-forming region: Unveiling hidden dust mass and connecting infrared outflows to their radio origins cites this paper.

A JWST, ALMA and VLA survey of the Ophiuchus-A star-forming region: Unveiling hidden dust mass and connecting infrared outflows to their radio origins Protoplanetary Disk Turbulence Driven by the Streaming Instability: Linear Evolution and Numerical Methods

Reference 214

Resolution
unresolved
no resolver link, observed 2026-08-01T23:21:02.883579Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T23:21:02.883579Z digest=sha256:9fc2471f479b879f16ed896b55491028a54a6e2ef546618f1ce359ac9eeb6815