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Paper Citation Record · LEDGER

3D non-LTE abundance analyses of late-type stars

As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2401.00697.

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

pith.paper-citation-record.v1
2401.00697 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 4 of 4 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 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T21:44:33.053948Z

measured 1 of 1 external citation measurements

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

Source: pith, observed 2026-08-10T05:30:23.456663Z

Reference resolution

0 of 0 outbound references displayed

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External citation measurements

3
pith, observed 2026-08-10T05:30:23.456663Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 11eed9c3-66cd-44ff-bf26-8f216f25795b · inbound

Performance of the Stellar Abundances and atmospheric Parameters Pipeline adapted for M dwarfs I. Atmospheric parameters from the spectroscopic module cites this paper.

Performance of the Stellar Abundances and atmospheric Parameters Pipeline adapted for M dwarfs I. Atmospheric parameters from the spectroscopic module 3D non-LTE abundance analyses of late-type stars

Reference 77

Resolution
unresolved
no resolver link, observed 2026-08-07T21:44:33.053948Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T21:44:33.053948Z digest=sha256:d3f9df98d8958d7ff147b4919c258f6174747ae8b519626b6fa01888feb9701d

Observation af31d3eb-b14e-45f3-ab9e-2998506bc2bf · inbound

Impact of <3D> NLTE on GCE of oxygen with the RAdial Velocity Experiment cites this paper.

Impact of <3D> NLTE on GCE of oxygen with the RAdial Velocity Experiment 3D non-LTE abundance analyses of late-type stars

Reference 45

Resolution
unresolved
no resolver link, observed 2026-08-07T14:09:07.766315Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T14:09:07.766315Z digest=sha256:cfbc2835f9112efaece60d2814b02ec758776bd5efe612247ca3c7f7b399114b

Observation edcf124d-d89b-40f4-995c-440d7b5146bf · inbound

The Future of Solar modelling: requirements for a new generation of solar models cites this paper.

The Future of Solar modelling: requirements for a new generation of solar models 3D non-LTE abundance analyses of late-type stars

Reference 140

Resolution
verified exact
local_arxiv, observed 2026-08-07T00:23:04.404285Z

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.

source=arxiv_source observed=2026-08-07T00:23:02.809607Z digest=sha256:54d076004600911d845b70a37da6093bf7c9f650d8e6c9940136e123d9b33e67

Observation 5219234d-cb4d-4e32-8d2e-b41df4150ee1 · 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 3D non-LTE abundance analyses of late-type stars

Reference 97

Resolution
unresolved
no resolver link, observed 2026-08-05T10:57:04.806913Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-05T10:57:04.806913Z digest=sha256:94d1f73035ceaf95430703e4f3153320148586a10cf2d00c826eb8e60af3a806