Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Estimates of (convective core) masses, radii, and relative ages for $\sim$14,000 Gaia-discovered gravity-mode pulsators monitored by TESS
As of 13 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2410.05367.
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 2026-08-12T11:00:24.871130Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-06T20:22:47.552018Z
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 143fa642-e8be-43c3-a75f-0cb35a09caab · inbound
KIC 4150611: A quadruply eclipsing heptuple star system with a g-mode period-spacing pattern Asteroseismic modelling of the g-mode period-spacing pattern cites this paper.
KIC 4150611: A quadruply eclipsing heptuple star system with a g-mode period-spacing pattern Asteroseismic modelling of the g-mode period-spacing pattern Estimates of (convective core) masses, radii, and relative ages for $\sim$14,000 Gaia-discovered gravity-mode pulsators monitored by TESS
Reference 36
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T11:00:24.871130Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation b8d668c8-ced3-4b89-9c8d-d8a0af8ffe18 · inbound
From stellar light to astrophysical insight: automating variable star research with machine learning cites this paper.
From stellar light to astrophysical insight: automating variable star research with machine learning Estimates of (convective core) masses, radii, and relative ages for $\sim$14,000 Gaia-discovered gravity-mode pulsators monitored by TESS
Reference 127
- Resolution
- verified exact
- local_arxiv, observed 2026-08-06T20:22:47.645425Z
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.