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Paper Citation Record · LEDGER

Observational constraints on the origin of the elements. I. 3D NLTE formation of Mn lines in late-type stars

As of 22 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1905.05200.

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

pith.paper-citation-record.v1
1905.05200 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 3 of 3 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-22T06:32:14.747728+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T14:47:02.668281Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-14T14:47:02.879067Z

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 1a81775b-7ce5-4ca3-97e1-c2ebe223bcbb · inbound

Influence of inelastic collisions with hydrogen atoms on the non-LTE line formation for Fe I and Fe II in the 1D model atmospheres of late-type stars cites this paper.

Influence of inelastic collisions with hydrogen atoms on the non-LTE line formation for Fe I and Fe II in the 1D model atmospheres of late-type stars Observational constraints on the origin of the elements. I. 3D NLTE formation of Mn lines in late-type stars

Reference 13

Resolution
metadata mismatch
local_arxiv, observed 2026-08-14T14:47:02.886147Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

source=pdf_text observed=2026-08-14T14:47:02.668281Z digest=sha256:a8be78b337d08b9e137f51293fbe471a0bef7ed32a20aa2dfeb57cc0666654c4

Observation 0d8d677c-f592-48d4-a70f-c57463a14528 · 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 Observational constraints on the origin of the elements. I. 3D NLTE formation of Mn lines in late-type stars

Reference 24

Resolution
unresolved
no resolver link, observed 2026-08-05T10:57:04.584266Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-05T10:57:04.584266Z digest=sha256:91a06ac9fe2634f2d467a19b778fb930018a586f0bc56d9c3d02fdda5b41b3ee

Observation f55651ba-c6f2-448b-9aca-a18dfc47d543 · 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 Observational constraints on the origin of the elements. I. 3D NLTE formation of Mn lines in late-type stars

Reference 81

Resolution
unresolved
no resolver link, observed 2026-08-03T23:48:53.074650Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-03T23:48:53.074650Z digest=sha256:174e3018b0e5a1dc0ddd76736f088b92299cfa34d4579ee9a3df2e11e58339c6