Paper Citation Record · LEDGER

The Magnetorotational Instability in Core Collapse Supernova Explosions

As of 14 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:astro-ph/0208128.

A citation records a reference. It does not transfer a finding from one paper to another.

pith.paper-citation-record.v1
astro-ph/0208128 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 2 of 2 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-14T06:32:32.682623+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T13:05:39.705441Z

measured 0 of 1 external citation measurements

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 75c31498-89ba-45a7-9649-84f4aca909cb · 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 Magnetorotational Instability in Core Collapse Supernova Explosions

Reference 23

Resolution: unresolved; no resolver link, observed 2026-07-31T14:28:12.620447Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6dc39ecb-9b37-44bf-95c1-3f5c0954234e · 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 Magnetorotational Instability in Core Collapse Supernova Explosions

Reference 161

Resolution: unresolved; no resolver link, observed 2026-08-06T13:05:39.705441Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.