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Paper Citation Record · LEDGER

Dust mass in protoplanetary disks with porous dust opacities

As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2411.00277.

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

pith.paper-citation-record.v1
2411.00277 v1

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 2026-08-19T06:32:44.657259+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-16T12:17:45.907107Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-11T19:34:25.364332Z

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 327c972d-908f-4733-8e2b-1b54840547cb · inbound

On the formation of super-Jupiters: Core Accretion or Gravitational Instability? cites this paper.

On the formation of super-Jupiters: Core Accretion or Gravitational Instability? Dust mass in protoplanetary disks with porous dust opacities

Reference 21

Resolution
metadata mismatch
local_arxiv, observed 2026-08-11T19:34:25.371782Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

source=arxiv_source observed=2026-08-11T19:34:24.186354Z digest=sha256:1500496751a4a9b02243a894540053e1f3e1176692bd4e1a8a846ccfb04a5814

Observation b549c2a8-5771-4354-a3e9-60a1e27a610e · inbound

Turbulence Inhibits Planetesimal Formation in Class 0/I Disks Subject to Infall cites this paper.

Turbulence Inhibits Planetesimal Formation in Class 0/I Disks Subject to Infall Dust mass in protoplanetary disks with porous dust opacities

Reference 42

Resolution
unresolved
no resolver link, observed 2026-08-16T12:17:45.907107Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T12:17:45.907107Z digest=sha256:a9d67684fc69910ee012351651f59a900b60b6bc1b39b139e1fd0f9d3e42a36a