Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
The Dynamics of Neutrino-Driven Supernova Explosions after Shock Revival in 2D and 3D
As of 23 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1506.05139.
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 2026-08-22T06:32:14.747728+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-06T13:05:39.956535Z
A source-named dated measurement, never combined with another source.
Source: cited_works
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 de23e2f9-a280-437a-969b-7de62cd47693 · 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 The Dynamics of Neutrino-Driven Supernova Explosions after Shock Revival in 2D and 3D
Reference 97
- 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 905a6b12-d3a3-42a5-b034-8b140d58d628 · 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 The Dynamics of Neutrino-Driven Supernova Explosions after Shock Revival in 2D and 3D
Reference 97
- Resolution
- unresolved
- no resolver link, observed 2026-08-04T05:43:32.940636Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation d5b430d5-10ba-4d24-9c23-fb5e42800946 · inbound
3D simulations of a complete convective silicon shell burning phase cites this paper.
3D simulations of a complete convective silicon shell burning phase The Dynamics of Neutrino-Driven Supernova Explosions after Shock Revival in 2D and 3D
Reference 267
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T13:05:39.956535Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.