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Paper Citation Record · LEDGER

Convergence of the critical cooling rate for protoplanetary disk fragmentation achieved; the key role of numerical dissipation of angular momentum

As of 5 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1706.00417.

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

pith.paper-citation-record.v1
1706.00417 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 2026-08-05T06:32:48.257954+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-04T19:31:00.890372Z

measured 0 of 1 external citation measurements

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 95e71546-ebd6-4f24-aded-44be798b4db9 · inbound

Dust growth and planet formation by disc fragmentation cites this paper.

Dust growth and planet formation by disc fragmentation Convergence of the critical cooling rate for protoplanetary disk fragmentation achieved; the key role of numerical dissipation of angular momentum

Reference 18

Resolution
unresolved
no resolver link, observed 2026-08-04T19:31:00.890372Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-04T19:31:00.890372Z digest=sha256:b2daba6bd5da0cd475fffd2d394f1bde3c4e69aa75188603991305f812af8966

Observation 2e969633-6fb6-4bca-9832-cf97a216e3c6 · inbound

SPH methods in the modelling of compact objects cites this paper.

SPH methods in the modelling of compact objects Convergence of the critical cooling rate for protoplanetary disk fragmentation achieved; the key role of numerical dissipation of angular momentum

Reference 134

Resolution
unresolved
no resolver link, observed 2026-08-02T01:02:18.453993Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T01:02:18.453993Z digest=sha256:4c50f6869382532e0ef7f173a34096f206517e0bafd9312418ea26992e8c4155