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Paper Citation Record · LEDGER

Near-infrared chemical abundances of stars in the Sculptor dwarf galaxy

As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2210.06731.

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

pith.paper-citation-record.v1
2210.06731 v2

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 2026-08-17T06:30:58.91139+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-16T00:12:18.906131Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-15T14:56:16.055603Z

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 77753e29-c5c5-4104-b348-dadb24b81874 · inbound

Chemical Abundances and Globular Clusters of Milky Way Dwarf Galaxies cites this paper.

Chemical Abundances and Globular Clusters of Milky Way Dwarf Galaxies Near-infrared chemical abundances of stars in the Sculptor dwarf galaxy

Reference 100

Resolution
verified exact
local_arxiv, observed 2026-08-15T14:56:16.060569Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

source=arxiv_source observed=2026-08-15T14:56:15.973684Z digest=sha256:666e45cba5ab222d4d6383affeedde1a24a97f16f324c33e197e68bc4b1c8844

Observation 961310c9-f977-40d8-a12c-1604f08e20e9 · inbound

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics cites this paper.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics Near-infrared chemical abundances of stars in the Sculptor dwarf galaxy

Reference 289

Resolution
unresolved
no resolver link, observed 2026-08-16T00:12:18.906131Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:18.906131Z digest=sha256:ad39b3438c54939eec5c600aa9da36b4766e74f14c57a739a992dbe0b165db15