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Paper Citation Record · LEDGER

3-D gas-phase elemental abundances across the formation histories of Milky Way-mass galaxies in the FIRE simulations: initial conditions for chemical tagging

As of 16 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2102.06220.

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

pith.paper-citation-record.v1
2102.06220 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 2026-08-16T06:30:59.297886+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-02T02:59:12.299380Z

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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  • malformed identifier0
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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 127912b1-0ab8-49e8-8f1f-0b22760e2f30 · 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 3-D gas-phase elemental abundances across the formation histories of Milky Way-mass galaxies in the FIRE simulations: initial conditions for chemical tagging

Reference 36

Resolution
unresolved
no resolver link, observed 2026-08-02T02:58:15.890255Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T02:58:15.890255Z digest=sha256:6c3f5dcdf2f333f45e5b082b14c3a6f3085b686c6ed9d6e5b9d27d2ded80d4bf

Observation 48bd829b-06df-4326-81d7-0b59eb112b70 · 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 3-D gas-phase elemental abundances across the formation histories of Milky Way-mass galaxies in the FIRE simulations: initial conditions for chemical tagging

Reference 36

Resolution
unresolved
no resolver link, observed 2026-08-02T02:59:12.299380Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T02:59:12.299380Z digest=sha256:d8623dd520bdb9bf09d507524d83b18ddbe88766cd9c6019708b9eed62cf57b2