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Paper Citation Record · LEDGER

How to make giant planets via pebble accretion

As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2309.03807.

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

pith.paper-citation-record.v1
2309.03807 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 2026-08-12T21:58:36.791773Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-12T21:58:37.172831Z

Reference resolution

0 of 0 outbound references displayed

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  • verified fuzzy0
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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 567aaa9f-bf8a-4a7c-9468-49ed52ea1eec · inbound

Searching for GEMS: Two Super-Jupiters around M-dwarfs -- Signatures of Instability or Accretion? cites this paper.

Searching for GEMS: Two Super-Jupiters around M-dwarfs -- Signatures of Instability or Accretion? How to make giant planets via pebble accretion

Reference 111

Resolution
verified exact
local_arxiv, observed 2026-08-12T21:58:37.284213Z

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=pdf_text observed=2026-08-12T21:58:36.791773Z digest=sha256:b1645a777b1d3009c9a4b1b668f96b1faa12e129c457ab8d98875baadf65b4d3

Observation 8bed84b3-a15d-4218-b938-188778c5f7fb · inbound

The majority of hot Jupiters formed beyond the water ice line cites this paper.

The majority of hot Jupiters formed beyond the water ice line How to make giant planets via pebble accretion

Reference 25

Resolution
unresolved
no resolver link, observed 2026-08-02T00:06:49.462135Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T00:06:49.462135Z digest=sha256:130453bd7894ff13ae0582edcf5893ef3ce78a8ac185ad4b9a18eaeb99370ac7