Paper Citation Record · LEDGER

Extremely Metal-Poor Stars. VIII. High-Resolution, High-Signal-To-Noise Analysis of Five Stars with [Fe/H] < -3.5

As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:astro-ph/0107304.

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

pith.paper-citation-record.v1
astro-ph/0107304 v1

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measured 0 of 0 reference resolution

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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 2026-08-10T06:31:04.303077+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-04T10:56:50.777934Z

measured 0 of 1 external citation measurements

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

Source: cited_works

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Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation f9e895be-ff69-4597-b2d6-28110730af98 · inbound

The complex stellar system M 22: confirming abundance variations with high precision differential measurements cites this paper.

The complex stellar system M 22: confirming abundance variations with high precision differential measurements Extremely Metal-Poor Stars. VIII. High-Resolution, High-Signal-To-Noise Analysis of Five Stars with [Fe/H] < -3.5

Reference 228

Resolution: unresolved; no resolver link, observed 2026-08-02T02:58:16.341051Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 68cf93d9-6d73-4222-8ce5-0354511d631b · inbound

The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios cites this paper.

The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios Extremely Metal-Poor Stars. VIII. High-Resolution, High-Signal-To-Noise Analysis of Five Stars with [Fe/H] < -3.5

Reference 230

Resolution: unresolved; no resolver link, observed 2026-08-02T02:59:31.649513Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a2621d2d-7ea0-42eb-be87-4d300744902d · inbound

Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum cites this paper.

Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum Extremely Metal-Poor Stars. VIII. High-Resolution, High-Signal-To-Noise Analysis of Five Stars with [Fe/H] < -3.5

Reference 86

Resolution: unresolved; no resolver link, observed 2026-08-04T10:56:50.777934Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.