Paper Citation Record · LEDGER

The metal-rich nature of stars with planets

As of 13 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:astro-ph/0105216.

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

pith.paper-citation-record.v1
astro-ph/0105216 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 4 of 4 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 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T19:34:24.277203Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-01T06:05:29.795547Z

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 eb7c25f8-9f56-4b32-b5d0-d187f1e7f8ee · inbound

On the formation of super-Jupiters: Core Accretion or Gravitational Instability? cites this paper.

On the formation of super-Jupiters: Core Accretion or Gravitational Instability? The metal-rich nature of stars with planets

Reference 33

Resolution: unresolved; no resolver link, observed 2026-08-11T19:34:24.277203Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e5ffcd47-ccc5-4c40-b250-ea622bc7efb2 · inbound

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations cites this paper.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations The metal-rich nature of stars with planets

Reference 150

Resolution: unresolved; no resolver link, observed 2026-08-05T10:57:04.971783Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a367ea3b-d13d-47c6-a955-878543754a57 · inbound

The 35-Myr old infant planet TOI-837 b has a mildly misaligned orbit cites this paper.

The 35-Myr old infant planet TOI-837 b has a mildly misaligned orbit The metal-rich nature of stars with planets

Reference 287

Resolution: verified exact; local_arxiv, observed 2026-06-28T07:11:45.627690Z

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.

Observation 528d3521-afd2-457f-a58e-0c8c469ad9a1 · inbound

The GAPS programme at TNG: LXXVI. TOI-1533: a compact system hosting a super-Neptune-mass pair with disparate radii cites this paper.

The GAPS programme at TNG: LXXVI. TOI-1533: a compact system hosting a super-Neptune-mass pair with disparate radii The metal-rich nature of stars with planets

Reference 288

Resolution: verified exact; local_arxiv, observed 2026-07-01T06:05:29.797063Z

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.