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Paper Citation Record · LEDGER

Long-time 3D supernova simulations of non-rotating progenitors with magnetic fields

As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2412.01155.

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

pith.paper-citation-record.v1
2412.01155 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 3 of 3 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 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T00:15:14.190351Z

measured 1 of 1 external citation measurements

A source-named dated measurement, never combined with another source.

Source: arxiv_reference, observed 2026-08-05T02:28:24.338817Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
  • unresolved0
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

External citation measurements

0
arxiv_reference, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 3005f83e-fa3b-4224-a219-cc61488d2294 · inbound

Reproducing morphological features in the supernova remnant G11.2-0.3 by simulating jittering jets cites this paper.

Reproducing morphological features in the supernova remnant G11.2-0.3 by simulating jittering jets Long-time 3D supernova simulations of non-rotating progenitors with magnetic fields

Reference 163

Resolution
verified exact
arxiv_id, observed 2026-05-13T03:32:11.712722Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=arxiv_source observed=2026-05-13T03:30:02.910872Z digest=sha256:64376dd9b1d2c095bd5cbd639be8cb2feaef49b0956c3c1eec3f0f28ecc8dcda

Observation 0c0a40b2-9327-401d-9727-a1526a9e59e7 · inbound

Stellar black hole binaries from two common envelope evolution phases in triple stellar systems cites this paper.

Stellar black hole binaries from two common envelope evolution phases in triple stellar systems Long-time 3D supernova simulations of non-rotating progenitors with magnetic fields

Reference 167

Resolution
verified exact
arxiv_id, observed 2026-06-26T03:38:58.933945Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=arxiv_source observed=2026-06-26T03:22:16.434196Z digest=sha256:0b580509125ae02f1f45684664894e6a55af5e242147339890a6f1772012bf60

Observation 5f48032f-111d-4a0d-87df-75746cd9dd3f · inbound

A "Neutrino Fog" For Gravitational Waves: The Stochastic Gravitational Wave Background from Supernova Neutrino Memory cites this paper.

A "Neutrino Fog" For Gravitational Waves: The Stochastic Gravitational Wave Background from Supernova Neutrino Memory Long-time 3D supernova simulations of non-rotating progenitors with magnetic fields

Reference 68

Resolution
unresolved
no resolver link, observed 2026-08-07T00:15:14.190351Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T00:15:14.190351Z digest=sha256:987d8da19522295e62a742ade8f0751c701d59a0551870e7b5ee1467483ef041