Paper Citation Record · LEDGER

Line formation in solar granulation: I. Fe line shapes, shifts and asymmetries

As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:astro-ph/0005320.

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

pith.paper-citation-record.v1
astro-ph/0005320 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 5 of 5 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-10T06:31:04.303077+00:00

measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T19:11:30.011635Z

measured 1 of 1 external citation measurements

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

Source: pith, observed 2026-08-05T02:28:24.338817Z

Reference resolution

0 of 0 outbound references displayed

verified exact0
verified fuzzy0
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malformed identifier0
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External citation measurements

73
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation acb9e416-55d9-4aba-84ac-b0e6a3d330eb · inbound

Differentiable Stellar Atmospheres with Physics-Informed Neural Networks cites this paper.

Differentiable Stellar Atmospheres with Physics-Informed Neural Networks Line formation in solar granulation: I. Fe line shapes, shifts and asymmetries

Reference 4

Resolution: unresolved; no resolver link, observed 2026-08-06T19:11:30.011635Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ae72e243-0212-4e6d-8609-a5e81fd7fbb0 · inbound

Sensitivity of spectral lines to granulation: The Sun cites this paper.

Sensitivity of spectral lines to granulation: The Sun Line formation in solar granulation: I. Fe line shapes, shifts and asymmetries

Reference 2

Resolution: verified exact; local_arxiv, observed 2026-05-18T17:06:38.953561Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation 5477d581-d386-4404-823a-f306ab76c178 · 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 Line formation in solar granulation: I. Fe line shapes, shifts and asymmetries

Reference 30

Resolution: unresolved; no resolver link, observed 2026-08-03T23:48:48.809226Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 151c891c-5873-4697-839a-a158e55cba93 · inbound

Sensitivity of spectral lines to granulation: from the Sun to K-type stars cites this paper.

Sensitivity of spectral lines to granulation: from the Sun to K-type stars Line formation in solar granulation: I. Fe line shapes, shifts and asymmetries

Reference 4

Resolution: verified exact; local_arxiv, observed 2026-05-21T07:14:02.337885Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation acdf2de4-3c13-44c3-8da3-a29e328753e6 · inbound

Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum cites this paper.

Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum Line formation in solar granulation: I. Fe line shapes, shifts and asymmetries

Reference 59

Resolution: unresolved; no resolver link, observed 2026-08-04T10:56:50.620186Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.