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Paper Citation Record · LEDGER

Evidence of an Upper Bound on the Masses of Planets and its Implications for Giant Planet Formation

As of 13 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1801.06185.

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

pith.paper-citation-record.v1
1801.06185 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 2026-08-12T06:34:41.77262+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T19:34:24.317433Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-12T06:48:34.545711Z

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 0d8c2426-bf20-4351-9beb-3f20cb3f11a4 · 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? Evidence of an Upper Bound on the Masses of Planets and its Implications for Giant Planet Formation

Reference 37

Resolution
unresolved
no resolver link, observed 2026-08-11T19:34:24.317433Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-11T19:34:24.317433Z digest=sha256:b8b1686924fcf866e3a7666586a1f3fcf3e1038b2808d61e13c22305a81c1fd7

Observation 483e99c8-0a58-42ca-9230-1af663713c00 · inbound

Uniform Metallicity Measurements of M Dwarf Planet Hosts Support Metallicity-Dependent Sub-Neptune Formation cites this paper.

Uniform Metallicity Measurements of M Dwarf Planet Hosts Support Metallicity-Dependent Sub-Neptune Formation Evidence of an Upper Bound on the Masses of Planets and its Implications for Giant Planet Formation

Reference 231

Resolution
verified exact
local_arxiv, observed 2026-07-12T06:48:34.547585Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

source=arxiv_source observed=2026-07-12T06:44:30.209178Z digest=sha256:802f600068310ca1f93f5645a0e12e605fc565fe8901b05a46d949b4cca12ff8