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Paper Citation Record · LEDGER

The lowest detected stellar Fe abundance: The halo star SMSS J160540.18-144323.1

As of 20 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1904.07471.

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

pith.paper-citation-record.v1
1904.07471 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 2026-08-20T06:33:59.587034+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-02T02:59:18.499475Z

measured 0 of 1 external citation measurements

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

Source: cited_works

Reference resolution

0 of 0 outbound references displayed

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  • verified fuzzy0
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  • 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 c3075317-2e3d-462b-bdbd-215e348c44db · 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 The lowest detected stellar Fe abundance: The halo star SMSS J160540.18-144323.1

Reference 119

Resolution
unresolved
no resolver link, observed 2026-08-02T02:58:16.078682Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T02:58:16.078682Z digest=sha256:4ca5e823bb020715c180bca416a86747ca2b136bcfece6818906a34ef1bda690

Observation f9709fb0-4ad1-4aed-a88c-e3ca42b7e999 · 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 The lowest detected stellar Fe abundance: The halo star SMSS J160540.18-144323.1

Reference 121

Resolution
unresolved
no resolver link, observed 2026-08-02T02:59:18.499475Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T02:59:18.499475Z digest=sha256:ca0c57f1954e13ff34648e05a906f8a29b157751e9bca46c4a6b524b451335c1