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Paper Citation Record · LEDGER

The Mass and Size Distribution of Planetesimals Formed by the Streaming Instability. II. The Effect of the Radial Gas Pressure Gradient

As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1810.10018.

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

pith.paper-citation-record.v1
1810.10018 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 2026-08-15T06:32:42.880941+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T13:53:19.139688Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-25T14:55:57.295782Z

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 f4cf69c7-23bb-4b4d-9b75-aa20f724430e · inbound

Trans-Neptunian Binaries as Evidence for Planetesimal Formation by the Streaming Instability cites this paper.

Trans-Neptunian Binaries as Evidence for Planetesimal Formation by the Streaming Instability The Mass and Size Distribution of Planetesimals Formed by the Streaming Instability. II. The Effect of the Radial Gas Pressure Gradient

Reference 12

Resolution
verified exact
arxiv_id, observed 2026-05-25T14:55:57.298744Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-05-25T14:51:41.872962Z digest=sha256:f89a4ba956a8e69317d18bbf11e7e5dcd872d95ac95ad7ce6f9030ea170fb746

Observation 13bde04d-d9d7-4204-8eec-d9a9d394ff91 · inbound

Pebbles versus Planetesimals: The case of Trappist-1 cites this paper.

Pebbles versus Planetesimals: The case of Trappist-1 The Mass and Size Distribution of Planetesimals Formed by the Streaming Instability. II. The Effect of the Radial Gas Pressure Gradient

Reference 1

Resolution
unresolved
no resolver link, observed 2026-08-14T13:53:19.139688Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T13:53:19.139688Z digest=sha256:5bc28c6873306737ff1bec9156f5faedc4e51027f8c81699c04674fef715429c