Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Stellar rotation rates in Kepler eccentric (heartbeat) binaries obtained from r-mode signatures
As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2201.02458.
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 2026-08-18T06:34:40.430872+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-15T14:18:44.452350Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-12T12:11:58.180000Z
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 c14a6896-1ac7-49fd-bc6d-7a8487a28a55 · inbound
Gravity modes and potential evidence for Rossby Waves in late O-type supergiants cites this paper.
Gravity modes and potential evidence for Rossby Waves in late O-type supergiants Stellar rotation rates in Kepler eccentric (heartbeat) binaries obtained from r-mode signatures
Reference 31
- Resolution
- verified exact
- local_arxiv, observed 2026-08-12T12:11:58.192188Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation 0e1b9e83-6075-4e15-9b33-2b32b28982a8 · inbound
Gravity modes and potential evidence for Rossby Waves in late O-type supergiants cites this paper.
Gravity modes and potential evidence for Rossby Waves in late O-type supergiants Stellar rotation rates in Kepler eccentric (heartbeat) binaries obtained from r-mode signatures
Reference 31
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T14:18:44.452350Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.