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Paper Citation Record · LEDGER

Supernova Simulations

As of 10 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 2026-08-10T06:31:04.303077+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 2026-08-10T06:31:04.303077+00:00.

source=arxiv_source observed=2026-05-13T03:30:02.910872Z digest=sha256:34f3079a166e3367cf50d51ac72a24c9fbe48d8dc7f2531afdbc4ef14285824e

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 2026-08-10T06:31:04.303077+00:00.

source=arxiv_source observed=2026-05-25T05:47:12.889439Z digest=sha256:a58a79a6c3c930414cab55345a410ac8f5c2d8c86aa3229daab4650235218f22

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 2026-08-10T06:31:04.303077+00:00.

source=arxiv_source observed=2026-05-25T05:39:27.922929Z digest=sha256:41f87318a603e4c32e52b40964d0dba26e79c8c24f44169e8985bc7f5a198808

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 2026-08-10T06:31:04.303077+00:00.

source=arxiv_source observed=2026-06-27T08:27:59.759564Z digest=sha256:15d0cc517d2aabccabe6c429871ebf2f286920f3bfba2df95bb68dabfe3a0ff5

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 2026-08-10T06:31:04.303077+00:00.

source=arxiv_source observed=2026-06-26T03:22:16.434196Z digest=sha256:a54c71a7c7bdf11986181960ea82bb5b28c283e9a8058ad9ec39624aa74e7e8b

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=sha256:9c0e6de22b0d7401cca5aa09a3b860b30b34e57190b3785e8b0afd1b51d66ecb