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Paper Citation Record · LEDGER

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

As of 8 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 2026-08-08T06:32:00.761636+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
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  • 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 2026-08-08T06:32:00.761636+00:00.

source=arxiv_source observed=2026-05-13T03:30:02.910872Z digest=sha256:6528e7c9102206ff5460f65c2703774ea3478183f9b1d59cac5f70646fdbae72

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 2026-08-08T06:32:00.761636+00:00.

source=arxiv_source observed=2026-06-26T03:22:16.434196Z digest=sha256:6101397526ed0ed9f2c66fc7225e2a19041c9af34ae0d123c2acc43d3d0301d4

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=sha256:228e05c85dc8028d1209e6c28405d3ce3e347c9678ad0fd7b85feef9ed76786f