Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Constraining stellar and orbital co-evolution through ensemble seismology of solar-like oscillators in binary systems -- A census of oscillating red-giants and main-sequence stars in Gaia DR3 binaries
As of 14 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2307.10812.
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 2026-08-14T06:32:32.682623+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-11T21:16:52.222770Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-07-11T04:27:48.838441Z
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 d937b99f-26af-4ea1-adf7-69e812a75f8a · inbound
Uniform characterisation of an ensemble of main-sequence benchmark stars: effect of Gaia-based data on grid search models cites this paper.
Uniform characterisation of an ensemble of main-sequence benchmark stars: effect of Gaia-based data on grid search models Constraining stellar and orbital co-evolution through ensemble seismology of solar-like oscillators in binary systems -- A census of oscillating red-giants and main-sequence stars in Gaia DR3 binaries
Reference 11
- Resolution
- unresolved
- no resolver link, observed 2026-08-11T21:16:52.222770Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 705ebb5a-e106-4af3-bae6-374114fb6c06 · 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 Constraining stellar and orbital co-evolution through ensemble seismology of solar-like oscillators in binary systems -- A census of oscillating red-giants and main-sequence stars in Gaia DR3 binaries
Reference 15
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-07-11T04:27:48.841669Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.