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Paper Citation Record · LEDGER

Activity time series of old stars from late F to early K. IV. Limits of the correction of radial velocities using chromospheric emission

As of 23 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1911.05319.

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

pith.paper-citation-record.v1
1911.05319 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 2 of 2 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-22T06:32:14.747728+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-16T00:33:17.312979Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-08T09:54:50.824572Z

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 abe02e43-de15-4ac1-88b0-12445d9823bd · inbound

Spectral Ratio Analysis: probing of a new suite of stellar activity indicators as a tool for astrophysical noise mitigation cites this paper.

Spectral Ratio Analysis: probing of a new suite of stellar activity indicators as a tool for astrophysical noise mitigation Activity time series of old stars from late F to early K. IV. Limits of the correction of radial velocities using chromospheric emission

Reference 16

Resolution
verified exact
local_arxiv, observed 2026-07-08T09:54:50.826848Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:4b8f760f05bd61b9e1467bbe523c94f2e20de3d5439fa81267dc02c223402843

Observation 6af40e0f-d2da-4bee-921c-a565862a3cdd · inbound

Three new exoplanet systems from the Dispersed Matter Planet Project cites this paper.

Three new exoplanet systems from the Dispersed Matter Planet Project Activity time series of old stars from late F to early K. IV. Limits of the correction of radial velocities using chromospheric emission

Reference 148

Resolution
unresolved
no resolver link, observed 2026-08-16T00:33:17.312979Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:33:17.312979Z digest=sha256:3d8041e1cd1d4662bc9304f0350a14a211bdc9d6238689249abf1e57c224dea6