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Paper Citation Record · LEDGER

Tomography of cool giant and supergiant star atmospheres. I. Validation of the method

As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1711.08327.

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

pith.paper-citation-record.v1
1711.08327 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 2026-08-07T06:34:17.273281+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-03T23:49:13.884871Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-11T06:10:58.685828Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
  • unresolved0
  • parse uncertain0
  • 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 3028b762-078b-463c-ac22-057727b60d19 · 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 Tomography of cool giant and supergiant star atmospheres. I. Validation of the method

Reference 274

Resolution
unresolved
no resolver link, observed 2026-08-03T23:49:13.884871Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-03T23:49:13.884871Z digest=sha256:9da20b7283d45b5f1859e5f46da1b50519ea581761399c799479c377d476a7cf

Observation bb426b3a-5515-40c7-966a-4673937cc236 · inbound

Tracing the s-Process: Spectroscopic Insights into Chemical Abundances in O- and C-rich Evolved Stars cites this paper.

Tracing the s-Process: Spectroscopic Insights into Chemical Abundances in O- and C-rich Evolved Stars Tomography of cool giant and supergiant star atmospheres. I. Validation of the method

Reference 40

Resolution
malformed identifier
arxiv_id, observed 2026-07-04T22:33:49.965779Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=pdf_text observed=2026-05-10T17:47:10.739575Z digest=sha256:436544a33e297b3e1fd84d2563b78b21badda14770a4bb63c5f1c6748030c974