Pith. sign in

Paper Citation Record · LEDGER

Giant planet formation at the pressure maxima of protoplanetary disks

As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1610.01232.

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

pith.paper-citation-record.v1
1610.01232 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 2026-08-12T06:34:41.77262+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T23:13:10.581370Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-06-26T15:29:33.752123Z

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 99fa604d-134b-4988-a671-4fcb1caebe0f · inbound

Accretion of Uranus and Neptune: confronting different giant impact scenarios cites this paper.

Accretion of Uranus and Neptune: confronting different giant impact scenarios Giant planet formation at the pressure maxima of protoplanetary disks

Reference 2017

Resolution
unresolved
no resolver link, observed 2026-08-11T23:13:10.581370Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-11T23:13:10.581370Z digest=sha256:b98da86e3ba310cde7ae3fd24421490e39151bdd90ddef1efbf9299cd8f708e3

Observation 7f2f3079-9693-4d14-b7ef-dbaca36410c9 · inbound

Planet-Planet Secular Migration Predicts a Stellar Obliquity-Period Anti-Correlation cites this paper.

Planet-Planet Secular Migration Predicts a Stellar Obliquity-Period Anti-Correlation Giant planet formation at the pressure maxima of protoplanetary disks

Reference 118

Resolution
verified exact
local_arxiv, observed 2026-06-26T15:29:33.753295Z

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=2026-07-11T11:50:26.030339Z digest=sha256:f52fbe0c1400c75ff2530ddb2ca407fa9faca46fbdc5af63f7bde587d7d64f04