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Paper Citation Record · LEDGER

Supernova Simulations

As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 7 inbound Pith citation observations for arXiv:2403.18952.

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

pith.paper-citation-record.v1
2403.18952 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 7 of 7 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-09T06:31:02.800959+00:00

measured 7 of 7 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-08T12:47:49.504586Z

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

6
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 ad07e263-ce7c-4b15-bb7f-e8f661357082 · inbound

Impact of the nuclear equation of state on the explodability of massive stars cites this paper.

Impact of the nuclear equation of state on the explodability of massive stars Supernova Simulations

Reference 41

Resolution
unresolved
no resolver link, observed 2026-08-04T08:35:59.082496Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T08:35:59.082496Z digest=sha256:4339f6a686207cacd0b66866fbcacf6437db23946232741b08f9463ff230d4eb

Observation 60cc7e52-665d-4fbf-8766-3dd5460d3583 · 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 Supernova Simulations

Reference 96

Resolution
verified exact
arxiv_id, observed 2026-05-13T03:32:11.754180Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

source=arxiv_source observed=2026-05-13T03:30:02.910872Z digest=sha256:bf6774311c9366b806682c4a5d591b578710902613ad0e97fcb098be904c7927

Observation c15b87c7-5f29-4c78-918b-da111e1c6b32 · inbound

The first 3D MHD core-collapse progenitors I: General properties, convection and nuclear burning cites this paper.

The first 3D MHD core-collapse progenitors I: General properties, convection and nuclear burning Supernova Simulations

Reference 68

Resolution
verified exact
arxiv_id, observed 2026-05-25T05:50:23.279735Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

source=arxiv_source observed=2026-05-25T05:47:12.889439Z digest=sha256:861bf3f31d061bc4e47f6e62b38141928874642a81eab9de084e175ebb749470

Observation d18672a9-197d-4a26-ab81-adc9f16d7148 · inbound

The first 3D MHD core-collapse progenitors II: Rotation, magnetic-field amplification, and magnetic topology cites this paper.

The first 3D MHD core-collapse progenitors II: Rotation, magnetic-field amplification, and magnetic topology Supernova Simulations

Reference 78

Resolution
verified exact
arxiv_id, observed 2026-05-25T05:40:22.862948Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

source=arxiv_source observed=2026-05-25T05:39:27.922929Z digest=sha256:e051a80ac07d8aedaf1405391953838b51cf0f50c7527f7b50ce23401d2d3c4e

Observation be5a8401-71bd-4bd5-b44c-8b2cbde840e0 · inbound

Building three-dimensional giant stellar models for common envelope simulations cites this paper.

Building three-dimensional giant stellar models for common envelope simulations Supernova Simulations

Reference 91

Resolution
verified exact
arxiv_id, observed 2026-06-27T08:30:45.550026Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

source=arxiv_source observed=2026-06-27T08:27:59.759564Z digest=sha256:264120e4f25658a6dd20394a8800ddd4b8ff3e4aebc208f33b55dca520f1e55f

Observation e9f4cc8b-e5a7-4fff-bdb8-26f965804ffc · 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 Supernova Simulations

Reference 95

Resolution
verified exact
arxiv_id, observed 2026-06-26T03:38:58.940305Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

source=arxiv_source observed=2026-06-26T03:22:16.434196Z digest=sha256:5a5085e0823459f6b77ee65812d31164f2a40df62329d4353f8e7c3c2a228968

Observation f0082a66-62e1-417d-9f88-a43da8cb3a89 · inbound

Reconstructing Core-Collapse Supernova Gravitational-Wave Signals with Transdimensional Bayesian Inference cites this paper.

Reconstructing Core-Collapse Supernova Gravitational-Wave Signals with Transdimensional Bayesian Inference Supernova Simulations

Reference 13

Resolution
unresolved
no resolver link, observed 2026-08-08T12:47:49.504586Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-08T12:47:49.504586Z digest=sha256:8254e256aaa08f4375e16c10464a5535fa2554a2bc8c52caf085df91b0dfef3f