Pith. sign in

Paper Citation Record · LEDGER

The Stagger-grid: A grid of 3D stellar atmosphere models - V. Fe line shapes, shifts and asymmetries

As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1403.6245.

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

pith.paper-citation-record.v1
1403.6245 v1

Coverage vector

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 2026-08-10T06:31:04.303077+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-10T19:16:43.933676Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-03T23:29:02.437024Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
  • unresolved0
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

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 16727e32-41ba-4f1f-9bf5-ce071ee265e1 · inbound

MAGIS (Measuring Abundances of red super Giants with Infrared Spectroscopy) project I. Establishment of an abundance analysis procedure for red supergiants and its evaluation with nearby stars cites this paper.

MAGIS (Measuring Abundances of red super Giants with Infrared Spectroscopy) project I. Establishment of an abundance analysis procedure for red supergiants and its evaluation with nearby stars The Stagger-grid: A grid of 3D stellar atmosphere models - V. Fe line shapes, shifts and asymmetries

Reference 87

Resolution
unresolved
no resolver link, observed 2026-08-10T19:16:43.933676Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T19:16:43.933676Z digest=sha256:2a1aec43e230a94ed529dfccab07e8a8943fa19a0830936ecce8eb5d14dfd24e

Observation 2e58264a-434e-45b3-b396-7f95644df2db · inbound

Modeling Doppler Shifts in Radial-Velocity Data with Deep Learning toward Earth-mass Exoplanet Detection cites this paper.

Modeling Doppler Shifts in Radial-Velocity Data with Deep Learning toward Earth-mass Exoplanet Detection The Stagger-grid: A grid of 3D stellar atmosphere models - V. Fe line shapes, shifts and asymmetries

Reference 255

Resolution
verified exact
local_arxiv, observed 2026-07-03T23:29:02.438449Z

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=2026-06-26T22:17:04.261961Z digest=sha256:490ae38247825fa9047a05d16c945bbb794d79f1615610b754d2a0cd9e4585f5

Observation 52cd1fcc-5414-4bb1-8359-adb181707040 · 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 The Stagger-grid: A grid of 3D stellar atmosphere models - V. Fe line shapes, shifts and asymmetries

Reference 67

Resolution
unresolved
no resolver link, observed 2026-08-04T10:56:50.660956Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-04T10:56:50.660956Z digest=sha256:097fc0814cf3fedb1ff1efa32c0f4476dcd2e4a30e41573da30419db325ca41b