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Paper Citation Record · LEDGER

Chemical analysis of 8 recently discovered extra-solar planet host stars

As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:astro-ph/0009182.

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

pith.paper-citation-record.v1
astro-ph/0009182 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 2026-08-19T06:32:44.657259+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-10T18:07:03.115455Z

measured 1 of 1 external citation measurements

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

Source: pith, observed 2026-08-05T02:28:24.338817Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
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  • malformed identifier0
  • metadata mismatch0

External citation measurements

1
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 291b8022-a317-466d-9c08-15b47adf10d9 · inbound

Where in the Milky Way Do Exoplanets Preferentially Form? cites this paper.

Where in the Milky Way Do Exoplanets Preferentially Form? Chemical analysis of 8 recently discovered extra-solar planet host stars

Reference 38

Resolution
unresolved
no resolver link, observed 2026-08-10T18:07:03.115455Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T18:07:03.115455Z digest=sha256:619b38d9173c2a2483ef265821a008ec5c7e2dbf41c586402b4e817c7d439369

Observation 933fb76d-5630-4bab-aee6-acaef40695db · inbound

Chemical Abundances of the Bioessential Elements C, O and S, and the Refractory Elements Fe and Ni, in Solar-type Exoplanet-hosting Stars from HARPS North and South cites this paper.

Chemical Abundances of the Bioessential Elements C, O and S, and the Refractory Elements Fe and Ni, in Solar-type Exoplanet-hosting Stars from HARPS North and South Chemical analysis of 8 recently discovered extra-solar planet host stars

Reference 86

Resolution
verified exact
local_arxiv, observed 2026-07-01T01:55:14.181682Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

source=arxiv_source observed=2026-07-01T01:51:43.577683Z digest=sha256:837e56bce99b32c5768a70ccad5cf3ddadb8b5b71d2eb415bb9ecf0c6b0df542