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Paper Citation Record · LEDGER

Chemical abundance patterns in the inner Galaxy: the Scutum Red Supergiant Clusters

As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:0902.2378.

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

pith.paper-citation-record.v1
0902.2378 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 2026-08-08T06:32:00.761636+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T15:25:34.596528Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-02T18:47:16.652152Z

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 4441981e-a947-4032-b3cb-3a21cf69b58c · inbound

Stellar evolution through the Red Supergiant phase cites this paper.

Stellar evolution through the Red Supergiant phase Chemical abundance patterns in the inner Galaxy: the Scutum Red Supergiant Clusters

Reference 40

Resolution
unresolved
no resolver link, observed 2026-08-06T15:25:34.596528Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T15:25:34.596528Z digest=sha256:7e00e405189fbe0cd2309ea1a2740c1acbc336e380c8ea2d4210f81e7c2d205d

Observation 9de7d658-ab32-4ff0-a07e-60b7897365ed · inbound

Hot or Cold? Radial Redistribution of Stars in FIRE Simulations of Milky Way-Mass Galaxies and the Asymmetry of Inward versus Outward Migrators cites this paper.

Hot or Cold? Radial Redistribution of Stars in FIRE Simulations of Milky Way-Mass Galaxies and the Asymmetry of Inward versus Outward Migrators Chemical abundance patterns in the inner Galaxy: the Scutum Red Supergiant Clusters

Reference 257

Resolution
verified exact
local_arxiv, observed 2026-07-02T18:47:16.653416Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:9bdf9c9d42e168755087d33de0777a77daf5dff79da07a9ac9406b0d1e2169ab