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Paper Citation Record · LEDGER

Further Evidence of Modified Spin-down in Sun-like Stars: Pileups in the Temperature-Period Distribution

As of 21 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2203.08920.

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

pith.paper-citation-record.v1
2203.08920 v2

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 2026-08-21T06:32:19.484+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-07-11T04:19:29.170180Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-15T15:06:10.025330Z

Reference resolution

0 of 0 outbound references displayed

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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 5b9b6724-9dbf-4d6d-a912-9ed66d075f2b · inbound

The TESS All-Sky Rotation Survey: Periods for 1,046,317 Stars Within 500 pc cites this paper.

The TESS All-Sky Rotation Survey: Periods for 1,046,317 Stars Within 500 pc Further Evidence of Modified Spin-down in Sun-like Stars: Pileups in the Temperature-Period Distribution

Reference 23

Resolution
verified exact
arxiv_id, observed 2026-05-15T15:06:10.028200Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

source=pdf_text observed=2026-05-15T15:03:38.581735Z digest=sha256:d2632685a72426d0b8304442bb88b878a31ef809a95122ce49a1097b0f27302a

Observation 2f780f8f-3f8a-43b0-a1fe-018b7ec3c9b3 · inbound

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet cites this paper.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca ii infrared triplet Further Evidence of Modified Spin-down in Sun-like Stars: Pileups in the Temperature-Period Distribution

Reference 50

Resolution
unresolved
no resolver link, observed 2026-07-11T04:19:29.170180Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-11T04:19:29.170180Z digest=sha256:c7bc07ee716fddb447df396cfc449a756dfec6d0a31ca4fe73ea285ebb8658b0