Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Magnetic and tidal migration of close-in planets. Influence of secular evolution on their population
As of 13 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2104.01004.
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 2026-08-13T06:32:02.005865+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-03T12:59:16.698699Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-05T02:28:24.338817Z
Reference resolution
0 of 0 outbound references displayed
- verified exact0
- verified fuzzy0
- unresolved0
- parse uncertain0
- malformed identifier0
- metadata mismatch0
External citation measurements
35
pith, observed 2026-08-05T02:28:24.338817Z
Outbound references
No outbound reference observations are available for this paper version.
Pith citing papers
Observation 52213aa9-79e2-4313-9786-1324bff86980 · 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 Magnetic and tidal migration of close-in planets. Influence of secular evolution on their population
Reference 2
- Resolution
- verified exact
- local_arxiv, observed 2026-07-11T04:27:48.695286Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.
Observation b5abeb2e-c68a-4857-8a77-888570f7a42a · inbound
Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations cites this paper.
Tidal dissipation in magnetised, rotating stars and planets: linear calculations exploring various magnetic field configurations Magnetic and tidal migration of close-in planets. Influence of secular evolution on their population
Reference 15
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T12:59:16.698699Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.