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Paper Citation Record · LEDGER

Accurate abundance analysis of late-type stars: advances in atomic physics

As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1604.07659.

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

pith.paper-citation-record.v1
1604.07659 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 2026-08-15T06:32:42.880941+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-05T10:57:04.566563Z

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

  • 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 17cae767-d1bf-407b-8504-1b10b0b3f04e · inbound

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations cites this paper.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations Accurate abundance analysis of late-type stars: advances in atomic physics

Reference 18

Resolution
unresolved
no resolver link, observed 2026-08-05T10:57:04.566563Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-05T10:57:04.566563Z digest=sha256:fe971796f5ff449ce8e072583abe55b60bfce2dcb69e17484309aafca9f621db

Observation ff5b8839-9ef1-4e29-99be-23a6689484ba · inbound

3D Non-LTE radiation transfer: theory and applications to stars, exoplanets, and kilonovae cites this paper.

3D Non-LTE radiation transfer: theory and applications to stars, exoplanets, and kilonovae Accurate abundance analysis of late-type stars: advances in atomic physics

Reference 45

Resolution
unresolved
no resolver link, observed 2026-08-03T23:48:49.780124Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-03T23:48:49.780124Z digest=sha256:e8290f86df0c0e0efb69fc755a0692ead34909fab9463f46c6265e64869d521b