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Paper Citation Record · LEDGER

Magnetic support for neutrino-driven explosion of 3D non-rotating core-collapse supernova models

As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2202.07967.

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

pith.paper-citation-record.v1
2202.07967 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 2026-08-07T06:34:17.273281+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T13:05:39.890853Z

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 e90770db-46b3-4f42-93cd-28c1fd143de2 · inbound

Impact of rotation on the accretion of entropy perturbations in collapsing massive stars cites this paper.

Impact of rotation on the accretion of entropy perturbations in collapsing massive stars Magnetic support for neutrino-driven explosion of 3D non-rotating core-collapse supernova models

Reference 47

Resolution
malformed identifier
no resolver link, observed 2026-08-04T19:19:16.611362Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T19:19:16.611362Z digest=sha256:6a8eca583415b1ac9edc5dff7f34143c087a3aa464c2d3b0eddb632e85393b11

Observation f617fad6-dc28-4f0e-a220-47745428dfb1 · inbound

3D simulations of a complete convective silicon shell burning phase cites this paper.

3D simulations of a complete convective silicon shell burning phase Magnetic support for neutrino-driven explosion of 3D non-rotating core-collapse supernova models

Reference 241

Resolution
unresolved
no resolver link, observed 2026-08-06T13:05:39.890853Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-06T13:05:39.890853Z digest=sha256:2d605e8e110128080bacd84c9d57bd512cf2b343db779b04d98459d58dc810fa