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Paper Citation Record · LEDGER

A 3D Simulation of a Type II-P Supernova: from Core Bounce to Beyond Shock Breakout

As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:2411.03434.

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

pith.paper-citation-record.v1
2411.03434 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 6 of 6 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-17T06:30:58.91139+00:00

measured 6 of 6 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-16T05:43:51.604578Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-02T14:37:04.088680Z

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 41bda2ed-db07-48ae-b0dd-2b1be7b4cf37 · inbound

The two alternative explosion mechanisms of core-collapse supernovae: 2024 status report cites this paper.

The two alternative explosion mechanisms of core-collapse supernovae: 2024 status report A 3D Simulation of a Type II-P Supernova: from Core Bounce to Beyond Shock Breakout

Reference 63

Resolution
unresolved
no resolver link, observed 2026-08-12T21:35:45.759973Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-12T21:35:45.759973Z digest=sha256:f43c2202a14f13c310a8208f644ca4146e48d9733ff2926a8dcb306fc818a818

Observation c5b59f4a-f0b2-4673-a992-90dc4e30efe9 · inbound

Channels of Stellar-mass Black Hole Formation cites this paper.

Channels of Stellar-mass Black Hole Formation A 3D Simulation of a Type II-P Supernova: from Core Bounce to Beyond Shock Breakout

Reference 105

Resolution
unresolved
no resolver link, observed 2026-08-11T18:34:33.764022Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-11T18:34:33.764022Z digest=sha256:e7ebf0d50a9a0fcdbe534bfca544237abe63279b8e27ae2f3faac9ef89bb0367

Observation 4c08a3ff-19b4-4858-b887-e03e1ecadee1 · inbound

Expanding Ejecta Method: I. Mapping Supernova Morphology with Intensity Interferometry cites this paper.

Expanding Ejecta Method: I. Mapping Supernova Morphology with Intensity Interferometry A 3D Simulation of a Type II-P Supernova: from Core Bounce to Beyond Shock Breakout

Reference 121

Resolution
unresolved
no resolver link, observed 2026-08-16T05:43:51.604578Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T05:43:51.604578Z digest=sha256:e38c208d595f645b0ffe008bbae5d26f2057798b6fac044d071f03093bd674fe

Observation da6b7d8b-7b39-40da-b560-768ca78cd1f6 · inbound

SEDONA-GesaRaT: an AI-Accelerated Radiative Transfer Program for 3-D Supernova Simulations cites this paper.

SEDONA-GesaRaT: an AI-Accelerated Radiative Transfer Program for 3-D Supernova Simulations A 3D Simulation of a Type II-P Supernova: from Core Bounce to Beyond Shock Breakout

Reference 35

Resolution
unresolved
no resolver link, observed 2026-08-06T17:07:29.053190Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-06T17:07:29.053190Z digest=sha256:29b1e7cbcd3513d21a4214a4154229c1fb12214013df31b05e2049eeed206b5b

Observation b7deb3ed-e7fe-4e0a-a83e-2fc72a69d1d6 · inbound

Potassium abundances in extremely metal poor stars: Implications for nucleosynthesis in the final stages of massive star evolution cites this paper.

Potassium abundances in extremely metal poor stars: Implications for nucleosynthesis in the final stages of massive star evolution A 3D Simulation of a Type II-P Supernova: from Core Bounce to Beyond Shock Breakout

Reference 65

Resolution
unresolved
no resolver link, observed 2026-08-05T15:11:07.994496Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-05T15:11:07.994496Z digest=sha256:0dd409c95af55434875af26dc71c4028a8963e4aed71d4fc4cbb8fd310c1d0b7

Observation 820dca3e-8e80-4ade-a40c-aed884d514c2 · inbound

Neutrino mass ordering from the next Galactic supernova at DUNE, HK, and JUNO cites this paper.

Neutrino mass ordering from the next Galactic supernova at DUNE, HK, and JUNO A 3D Simulation of a Type II-P Supernova: from Core Bounce to Beyond Shock Breakout

Reference 33

Resolution
verified exact
arxiv_id, observed 2026-07-02T14:37:04.089912Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

source=pdf_text observed=2026-06-28T00:17:31.776169Z digest=sha256:98bd3204731fc3cbd1bc0ab96a16effffa65b0d7450ddb854491e002f81d8bf5