Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
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.
Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-10T06:31:04.303077+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-07T21:44:33.053948Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-10T05:30:23.456663Z
0 of 0 outbound references displayed
External citation measurements
3
pith, observed 2026-08-10T05:30:23.456663Z
No outbound reference observations are available for this paper version.
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 3D non-LTE abundance analyses of late-type stars
Reference 77
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation af31d3eb-b14e-45f3-ab9e-2998506bc2bf · inbound
Impact of <3D> NLTE on GCE of oxygen with the RAdial Velocity Experiment 3D non-LTE abundance analyses of late-type stars
Reference 45
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation edcf124d-d89b-40f4-995c-440d7b5146bf · inbound
The Future of Solar modelling: requirements for a new generation of solar models 3D non-LTE abundance analyses of late-type stars
Reference 140
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 5219234d-cb4d-4e32-8d2e-b41df4150ee1 · inbound
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
Source-reported events for the cited work
Unavailable: canonical work link unavailable.