Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
The impact of non-dipolar magnetic fields in core-collapse supernovae
As of 14 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1909.02824.
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 2026-08-14T06:32:32.682623+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-14T05:32:55.543674Z
A source-named dated measurement, never combined with another source.
Source: cited_works
Reference resolution
0 of 0 outbound references displayed
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- malformed identifier0
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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 5ead686f-83a0-4c11-819c-26009671173c · inbound
Magnetorotational core collapse of possible GRB progenitors. I. Explosion mechanisms cites this paper.
Magnetorotational core collapse of possible GRB progenitors. I. Explosion mechanisms The impact of non-dipolar magnetic fields in core-collapse supernovae
Reference 6
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T05:32:55.543674Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 25cab818-a06b-4e34-b20f-64464f9f29e0 · inbound
Transport Properties of the MRI in Differentially Rotating Neutron Stars cites this paper.
Transport Properties of the MRI in Differentially Rotating Neutron Stars The impact of non-dipolar magnetic fields in core-collapse supernovae
Reference 31
- Resolution
- unresolved
- no resolver link, observed 2026-07-31T14:28:12.669867Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 1ce18b38-2614-4eba-8d98-951cfb84e0c0 · 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 impact of non-dipolar magnetic fields in core-collapse supernovae
Reference 110
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T13:05:39.576191Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.