Paper Citation Record · LEDGER

Relativistic simulations of rotational core collapse. I. Methods, initial models, and code tests

As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:astro-ph/0204288.

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

pith.paper-citation-record.v1
astro-ph/0204288 v1

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 2026-08-15T06:32:42.880941+00:00

measured 6 of 6 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T04:16:46.982147Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-06-29T05:53:09.185444Z

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 6c97e464-870b-4e50-942c-ddfb82084349 · inbound

Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves cites this paper.

Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves Relativistic simulations of rotational core collapse. I. Methods, initial models, and code tests

Reference 83

Resolution: unresolved; no resolver link, observed 2026-07-13T16:48:58.103396Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9c9b64ea-97cd-4a29-a04d-5da3cdd83735 · inbound

Toward More Realistic Machine-Learning Inference of the Dense-Matter Equation of State from Supernova Gravitational Waves cites this paper.

Reference 83

Resolution: unresolved; no resolver link, observed 2026-08-04T05:43:31.303572Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation dfb07fe7-686a-45d5-b5b9-a276bbf7d522 · inbound

Parameter Estimation Horizon of Core-Collapse Supernovae with Current and Next-Generation Gravitational-Wave Detectors cites this paper.

Parameter Estimation Horizon of Core-Collapse Supernovae with Current and Next-Generation Gravitational-Wave Detectors Relativistic simulations of rotational core collapse. I. Methods, initial models, and code tests

Reference 102

Resolution: verified exact; arxiv_id, observed 2026-05-11T18:26:11.410747Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation d4ed14be-5cd9-4ce1-8370-be43a335a6b0 · inbound

Exact Mass Conservation in Binary Neutron Star Merger Simulations cites this paper.

Exact Mass Conservation in Binary Neutron Star Merger Simulations Relativistic simulations of rotational core collapse. I. Methods, initial models, and code tests

Reference 2

Resolution: verified exact; local_arxiv, observed 2026-06-29T05:53:09.186721Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation 1eb2236a-3881-4cc0-b385-47e945fbb3e6 · inbound

Parameter Estimation Horizon of Core-Collapse Supernovae with a Network of Gravitational-Wave Detectors cites this paper.

Parameter Estimation Horizon of Core-Collapse Supernovae with a Network of Gravitational-Wave Detectors Relativistic simulations of rotational core collapse. I. Methods, initial models, and code tests

Reference 95

Resolution: unresolved; no resolver link, observed 2026-08-04T23:55:23.457923Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c6530713-42ca-4ce1-8e94-cb3377792570 · inbound

On the nature of oscillating modes of proto-neutron stars cites this paper.

On the nature of oscillating modes of proto-neutron stars Relativistic simulations of rotational core collapse. I. Methods, initial models, and code tests

Reference 63

Resolution: unresolved; no resolver link, observed 2026-08-14T04:16:46.982147Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.