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Paper Citation Record · LEDGER

The distribution of heavy-elements in giant protoplanetary atmospheres: the importance of planetesimal-envelope interactions

As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1811.10904.

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

pith.paper-citation-record.v1
1811.10904 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 2026-08-17T06:30:58.91139+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T14:45:38.580261Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-14T10:40:32.914053Z

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 94dd2e9a-2c98-4966-bce2-00c6fe3e0288 · inbound

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes cites this paper.

How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes The distribution of heavy-elements in giant protoplanetary atmospheres: the importance of planetesimal-envelope interactions

Reference 104

Resolution
unresolved
no resolver link, observed 2026-08-14T14:45:38.580261Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T14:45:38.580261Z digest=sha256:a1b56d49185473f0a346e69f9475f66cea85d9197e85c5638d2f100e47eca914

Observation 2160fbe1-610a-498e-a9e9-27326d6e192e · inbound

Explaining the low luminosity of Uranus: A self-consistent thermal and structural evolution cites this paper.

Explaining the low luminosity of Uranus: A self-consistent thermal and structural evolution The distribution of heavy-elements in giant protoplanetary atmospheres: the importance of planetesimal-envelope interactions

Reference 56

Resolution
verified exact
local_arxiv, observed 2026-08-14T10:40:32.920208Z

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=2026-08-14T10:40:32.849857Z digest=sha256:553602b89425e358f2adfdc6480a4000ad936b09d7f38a27d9761ba1362c208d