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Paper Citation Record · LEDGER

Activity time series of old stars from late F to early K. I. Simulating radial velocity, astrometry, photometry, and chromospheric emission

As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1904.01437.

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

pith.paper-citation-record.v1
1904.01437 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 2026-08-08T06:32:00.761636+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-08T00:10:26.086392Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-01T03:05:19.463147Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
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  • 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 6e6e56d1-17fa-4bcf-b70b-20a783321bf3 · inbound

Magnetic activity in cool stars: manifestations and relevance to exoplanets cites this paper.

Magnetic activity in cool stars: manifestations and relevance to exoplanets Activity time series of old stars from late F to early K. I. Simulating radial velocity, astrometry, photometry, and chromospheric emission

Reference 154

Resolution
verified exact
local_arxiv, observed 2026-07-01T03:05:19.464610Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:104f35c50b82cc130e4acbcd041c12d7ed910d2d216a67002e2aba63688fed6d

Observation f2221b7d-9a29-48ac-b32a-296e1d4026cd · inbound

Searching for Habitable Exoplanets with Relative Astrometry (SHERA). I. The Case for Searching for Planets in Binary Star Systems cites this paper.

Searching for Habitable Exoplanets with Relative Astrometry (SHERA). I. The Case for Searching for Planets in Binary Star Systems Activity time series of old stars from late F to early K. I. Simulating radial velocity, astrometry, photometry, and chromospheric emission

Reference 92

Resolution
unresolved
no resolver link, observed 2026-08-08T00:10:26.086392Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-08T00:10:26.086392Z digest=sha256:cdf889604b084e409c7ff7ab535e4301426b0d77873ab4aa353eda51691db1b6