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Paper Citation Record · LEDGER

Pebble-driven Planet Formation around Very Low-mass Stars and Brown Dwarfs

As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2004.07239.

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

pith.paper-citation-record.v1
2004.07239 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 3 of 3 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-07T06:34:17.273281+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-01T23:21:08.055495Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-12T07:48:36.579539Z

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 e5d6055e-84ea-4700-b887-be8c8318da87 · inbound

On the Eccentricity Distribution and Tidal Evolution of Transiting Brown Dwarfs cites this paper.

On the Eccentricity Distribution and Tidal Evolution of Transiting Brown Dwarfs Pebble-driven Planet Formation around Very Low-mass Stars and Brown Dwarfs

Reference 119

Resolution
verified exact
local_arxiv, observed 2026-07-12T07:48:36.581462Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=arxiv_source observed=2026-07-12T07:45:39.933353Z digest=sha256:70a798040f2b1fe54c759cc94d699803f59485f28cc9bd03b7f6aec06889eee4

Observation 40dcae50-21a4-46fe-84d3-1d80bbda4427 · inbound

Discovering and Characterising Exoplanets and Ultracool Dwarfs with the Square Kilometre Array cites this paper.

Discovering and Characterising Exoplanets and Ultracool Dwarfs with the Square Kilometre Array Pebble-driven Planet Formation around Very Low-mass Stars and Brown Dwarfs

Reference 180

Resolution
unresolved
no resolver link, observed 2026-07-14T05:08:13.679880Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-14T05:08:13.679880Z digest=sha256:05c4242c40f54480ab45ab92a8477b371bffafe5edf5784876fc922680b19b21

Observation d7b557f5-ebfb-4347-af6e-3d2e756527a5 · inbound

A JWST, ALMA and VLA survey of the Ophiuchus-A star-forming region: Unveiling hidden dust mass and connecting infrared outflows to their radio origins cites this paper.

A JWST, ALMA and VLA survey of the Ophiuchus-A star-forming region: Unveiling hidden dust mass and connecting infrared outflows to their radio origins Pebble-driven Planet Formation around Very Low-mass Stars and Brown Dwarfs

Reference 251

Resolution
unresolved
no resolver link, observed 2026-08-01T23:21:08.055495Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T23:21:08.055495Z digest=sha256:db5435cc041c6b797151edaaf476a35a9eb628e82c1ea07479542d8a2e2a41a9