Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
New rotation period measurements for M dwarfs in the southern hemisphere: an abundance of slowly rotating, fully convective stars
As of 16 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1807.09365.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-15T06:32:42.880941+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-07-11T11:50:26.030339Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-06-26T16:39:36.011779Z
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 0cd12a28-dd4a-43c6-ae91-ec415d7f0c42 · inbound
The high-energy radiation environment of the habitable-zone super-Earth LHS 1140b cites this paper.
The high-energy radiation environment of the habitable-zone super-Earth LHS 1140b New rotation period measurements for M dwarfs in the southern hemisphere: an abundance of slowly rotating, fully convective stars
Reference 32
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-05-25T19:06:09.130805Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.
Observation 3a1cbf57-bac7-44e1-a36a-6a8f829bdaf7 · inbound
Star-planet interaction in the Proxima system cites this paper.
Star-planet interaction in the Proxima system New rotation period measurements for M dwarfs in the southern hemisphere: an abundance of slowly rotating, fully convective stars
Reference 122
- Resolution
- verified exact
- local_arxiv, observed 2026-05-25T02:10:13.026587Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.
Observation 68586d06-d02c-4019-8958-41df4b3791b5 · inbound
Upper Limits on Planet-Induced GHz Radio Emission from Inactive M Dwarfs cites this paper.
Upper Limits on Planet-Induced GHz Radio Emission from Inactive M Dwarfs New rotation period measurements for M dwarfs in the southern hemisphere: an abundance of slowly rotating, fully convective stars
Reference 123
- Resolution
- verified exact
- local_arxiv, observed 2026-06-26T16:39:36.013066Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.