Paper Citation Record · LEDGER

The NextGen Model Atmosphere grid: II. Spherically symmetric model atmospheres for giant stars with effective temperatures between 3000 and 6800~K

As of 13 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:astro-ph/9907194.

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

pith.paper-citation-record.v1
astro-ph/9907194 v1

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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 2026-08-13T06:32:02.005865+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-12T14:37:34.934862Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-06-27T22:51:22.636934Z

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Outbound references

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Pith citing papers

Observation f94d4a39-e140-4718-a15a-c40225c03550 · 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 The NextGen Model Atmosphere grid: II. Spherically symmetric model atmospheres for giant stars with effective temperatures between 3000 and 6800~K

Reference 214

Resolution: unresolved; no resolver link, observed 2026-08-03T23:49:08.713813Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0b368130-bdf9-43a6-ac5a-8b94cd7d9019 · inbound

Study of photometric and spectral variability of the roAp star HD~210684 cites this paper.

Study of photometric and spectral variability of the roAp star HD~210684 The NextGen Model Atmosphere grid: II. Spherically symmetric model atmospheres for giant stars with effective temperatures between 3000 and 6800~K

Reference 51

Resolution: verified exact; local_arxiv, observed 2026-06-27T22:51:22.638533Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

Observation 1d1feecd-a9d0-4b86-8a9e-d0d31b3df985 · inbound

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems cites this paper.

Pulsation periods reveal tension between theoretical and empirical radii for classical Cepheids in eclipsing binary systems The NextGen Model Atmosphere grid: II. Spherically symmetric model atmospheres for giant stars with effective temperatures between 3000 and 6800~K

Reference 27

Resolution: unresolved; no resolver link, observed 2026-08-12T14:37:34.934862Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.