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Paper Citation Record · LEDGER

Chemical Abundance Analysis of Tucana III, the Second $r$-process Enhanced Ultra-Faint 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:1812.01022.

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

pith.paper-citation-record.v1
1812.01022 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 2026-08-14T13:13:29.922278Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-25T14:55:57.284681Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • 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 b5242ba6-e313-43a7-b0b3-614608825106 · inbound

Contribution of type Ia supernovae to the chemical enrichment of the ultra-faint dwarf galaxy Bootes I cites this paper.

Contribution of type Ia supernovae to the chemical enrichment of the ultra-faint dwarf galaxy Bootes I Chemical Abundance Analysis of Tucana III, the Second $r$-process Enhanced Ultra-Faint Dwarf Galaxy

Reference 24

Resolution
verified exact
arxiv_id, observed 2026-05-25T14:55:57.287648Z

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=2026-05-25T14:52:26.098245Z digest=sha256:6580d596515182d3e4792606f84749aab2ba531547e9ce53f242147c2fc61a3d

Observation b3348f1e-a26b-470d-b1eb-91f0acee2bc6 · inbound

Using failed supernovae to constrain the Galactic r-process element production cites this paper.

Using failed supernovae to constrain the Galactic r-process element production Chemical Abundance Analysis of Tucana III, the Second $r$-process Enhanced Ultra-Faint Dwarf Galaxy

Reference 86

Resolution
unresolved
no resolver link, observed 2026-08-14T13:13:29.922278Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T13:13:29.922278Z digest=sha256:7cb50a74ee15519bb24854fb04b1a5b2b4dfb73ed50de002128153569db42de2