Paper Citation Record · LEDGER

The formation and retention of gas giant planets around stars with a range of metallicities

As of 20 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:astro-ph/0408019.

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

pith.paper-citation-record.v1
astro-ph/0408019 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 5 of 5 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-20T06:33:59.587034+00:00

measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T10:51:27.522977Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-10T18:17:33.030879Z

Reference resolution

0 of 0 outbound references displayed

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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 d98d8794-5253-4c9e-ae3c-ff48dac42340 · inbound

Correlation between planet formation rate and gas surface density: an analog of Kennicutt Schmidt law for planet formation cites this paper.

Correlation between planet formation rate and gas surface density: an analog of Kennicutt Schmidt law for planet formation The formation and retention of gas giant planets around stars with a range of metallicities

Reference 40

Resolution: unresolved; no resolver link, observed 2026-08-11T10:51:27.522977Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b380078c-05d3-4c56-a8c8-b9083e29aeb1 · inbound

TOI-3664 b, TOI-4034 b & TOI-6564 b: Three new hot Jupiters around stars approaching the terminal age main sequence cites this paper.

TOI-3664 b, TOI-4034 b & TOI-6564 b: Three new hot Jupiters around stars approaching the terminal age main sequence The formation and retention of gas giant planets around stars with a range of metallicities

Reference 94

Resolution: verified exact; local_arxiv, observed 2026-06-28T03:41:34.907797Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation cdc694aa-26ee-481b-895c-556743eb5989 · 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 The formation and retention of gas giant planets around stars with a range of metallicities

Reference 232

Resolution: unresolved; no resolver link, observed 2026-07-12T06:44:30.209178Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a8a12013-d016-43da-91ba-c9fc9e38e25c · inbound

Probing the origins. III. Exoplanet demographics across Galactic birth radii cites this paper.

Probing the origins. III. Exoplanet demographics across Galactic birth radii The formation and retention of gas giant planets around stars with a range of metallicities

Reference 90

Resolution: verified exact; local_arxiv, observed 2026-07-10T18:17:33.032140Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

Observation a0902072-065d-42a5-ac8e-3928335a5aeb · inbound

PANTERA. I. Hunting for the Most Metal-Rich Stars in the Solar Neighborhood with High-Resolution Spectroscopy cites this paper.

PANTERA. I. Hunting for the Most Metal-Rich Stars in the Solar Neighborhood with High-Resolution Spectroscopy The formation and retention of gas giant planets around stars with a range of metallicities

Reference 32

Resolution: unresolved; no resolver link, observed 2026-08-01T09:29:18.733340Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.