Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Determining the Structure of Rotating Massive Stellar Cores with Gravitational Waves
As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2011.09000.
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 2026-08-11T06:34:44.6726+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-04T23:55:23.207112Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-05-11T18:26:11.625218Z
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 d71eda5b-04e5-4823-b393-ad5d74e55452 · inbound
Parameter Estimation Horizon of Core-Collapse Supernovae with Current and Next-Generation Gravitational-Wave Detectors cites this paper.
Parameter Estimation Horizon of Core-Collapse Supernovae with Current and Next-Generation Gravitational-Wave Detectors Determining the Structure of Rotating Massive Stellar Cores with Gravitational Waves
Reference 63
- Resolution
- verified exact
- arxiv_id, observed 2026-05-11T18:26:11.627628Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 1b2e2d04-1b15-43f3-9d1a-041f236e82e5 · inbound
Parameter Estimation Horizon of Core-Collapse Supernovae with a Network of Gravitational-Wave Detectors cites this paper.
Parameter Estimation Horizon of Core-Collapse Supernovae with a Network of Gravitational-Wave Detectors Determining the Structure of Rotating Massive Stellar Cores with Gravitational Waves
Reference 42
- Resolution
- unresolved
- no resolver link, observed 2026-08-04T23:55:23.207112Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.