Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Modeling Asteroseismic Yields for the Roman Galactic Bulge Time-Domain Survey
As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2503.04999.
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 2026-08-17T06:30:58.91139+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-06T21:32:04.316462Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, 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
0
arxiv_reference, observed 2026-08-05T02:28:24.338817Z
Outbound references
No outbound reference observations are available for this paper version.
Pith citing papers
Observation ab269a84-e391-47c5-ac49-b0ff471694e8 · inbound
Anchoring Stellar Age Indicators: A Cross-Calibration of [C/N] and Gyrochronology Ages via the Age-Velocity-Dispersion Relation cites this paper.
Anchoring Stellar Age Indicators: A Cross-Calibration of [C/N] and Gyrochronology Ages via the Age-Velocity-Dispersion Relation Modeling Asteroseismic Yields for the Roman Galactic Bulge Time-Domain Survey
Reference 108
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T21:32:04.316462Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 4e99506e-267f-4264-84ab-6801dd88095f · inbound
Evaluating the Sensitivity of the Age Inferences of Red Giant Stars to Machine Learning Methodology cites this paper.
Evaluating the Sensitivity of the Age Inferences of Red Giant Stars to Machine Learning Methodology Modeling Asteroseismic Yields for the Roman Galactic Bulge Time-Domain Survey
Reference 129
- Resolution
- verified exact
- arxiv_id, observed 2026-06-25T22:48:38.628841Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.
Observation 57f41376-7cd4-44e6-bc0d-0cf5f5a6f87c · inbound
Detecting Solar-Like Oscillations in the Highest Mass TESS Giants cites this paper.
Detecting Solar-Like Oscillations in the Highest Mass TESS Giants Modeling Asteroseismic Yields for the Roman Galactic Bulge Time-Domain Survey
Reference 67
- Resolution
- unresolved
- no resolver link, observed 2026-07-31T16:17:45.563384Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.