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Paper Citation Record · LEDGER

The Most Metal-Poor Stars. II. Chemical Abundances of 190 Metal-Poor Stars Including 10 New Stars With [Fe/H] < -3.5

As of 21 July 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1208.3003.

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

pith.paper-citation-record.v1
1208.3003 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

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-07-01T05:11:37.277965Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-01T05:15:24.741369Z

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 2fdd12fc-3e02-4b9d-b24b-08c6aed2fa32 · inbound

Three Extremely Metal-Poor stars: discovery of a new CEMP-no star cites this paper.

Three Extremely Metal-Poor stars: discovery of a new CEMP-no star The Most Metal-Poor Stars. II. Chemical Abundances of 190 Metal-Poor Stars Including 10 New Stars With [Fe/H] < -3.5

Reference 240

Resolution
verified exact
local_arxiv, observed 2026-06-28T06:41:43.670873Z

Source-reported events for the cited work

Unavailable: named source frontier unavailable.

source=arxiv_source observed=2026-06-28T04:03:22.700387Z digest=sha256:cf02f6b8d9fa402db5c87099a7f34bd885b7c3864dfb516e413137a34e187ee9

Observation 2b280680-44b4-4188-8d45-a498813b5cba · inbound

The Sc, Ti, and V Abundance Discrepancy: Testing High-Mass IMF Variation and Massive-Star Rotation cites this paper.

The Sc, Ti, and V Abundance Discrepancy: Testing High-Mass IMF Variation and Massive-Star Rotation The Most Metal-Poor Stars. II. Chemical Abundances of 190 Metal-Poor Stars Including 10 New Stars With [Fe/H] < -3.5

Reference 66

Resolution
verified exact
local_arxiv, observed 2026-07-01T05:15:24.744116Z

Source-reported events for the cited work

Unavailable: named source frontier unavailable.

source=arxiv_source observed=2026-07-01T05:11:37.277965Z digest=sha256:054faee64250925b04008dbaba4b61dff18f1c9b2a287f7b9a9d3aaee94845a2