Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Neutrino-Driven Convection in Core-Collapse Supernovae: High-Resolution Simulations
As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:1510.05022.
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 2026-08-19T06:32:44.657259+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-06T13:05:40.019204Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-05-11T18:26:10.911013Z
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 29c82737-f92d-4a0a-add0-9348bb7ca68d · inbound
The Gravitational-Wave Power Gap in Core-Collapse Supernovae: Insights from 60 Axisymmetric Simulations cites this paper.
The Gravitational-Wave Power Gap in Core-Collapse Supernovae: Insights from 60 Axisymmetric Simulations Neutrino-Driven Convection in Core-Collapse Supernovae: High-Resolution Simulations
Reference 89
- Resolution
- unresolved
- no resolver link, observed 2026-08-04T05:44:58.866373Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation c1e8891e-8fbc-4252-b35e-3703799b6c4f · inbound
Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves cites this paper.
Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves Neutrino-Driven Convection in Core-Collapse Supernovae: High-Resolution Simulations
Reference 99
- Resolution
- unresolved
- no resolver link, observed 2026-07-13T16:48:58.103396Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 803c2638-55cf-4a24-b20d-d4bcbfe7441c · inbound
Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves cites this paper.
Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves Neutrino-Driven Convection in Core-Collapse Supernovae: High-Resolution Simulations
Reference 99
- Resolution
- unresolved
- no resolver link, observed 2026-08-04T05:43:33.330844Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation d089fdef-09a5-4c4d-a56c-fb5c6e940621 · 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 Neutrino-Driven Convection in Core-Collapse Supernovae: High-Resolution Simulations
Reference 23
- Resolution
- verified exact
- arxiv_id, observed 2026-07-04T20:56:35.705496Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.
Observation d703dbc9-fdb3-4fa3-8f57-b33e4d7f443c · inbound
3D simulations of a complete convective silicon shell burning phase cites this paper.
3D simulations of a complete convective silicon shell burning phase Neutrino-Driven Convection in Core-Collapse Supernovae: High-Resolution Simulations
Reference 291
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T13:05:40.019204Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.