Paper Citation Record · LEDGER

Core Collapse Supernova Gravitational Wave Emission for Progenitors of 9.6, 15, and 25 Solar Masses

As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 8 inbound Pith citation observations for arXiv:2208.10643.

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

pith.paper-citation-record.v1
2208.10643 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 8 of 8 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-19T06:32:44.657259+00:00

measured 8 of 8 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T04:16:47.242320Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-06-29T13:23:28.775728Z

Reference resolution

0 of 0 outbound references displayed

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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 bcc35092-cf4f-4b57-9460-b2a53bf759e0 · inbound

The Gravitational-Wave Power Gap in Core-Collapse Supernovae: Insights from 60 Axisymmetric Simulations cites this paper.

The Gravitational-Wave Power Gap in Core-Collapse Supernovae: Insights from 60 Axisymmetric Simulations Core Collapse Supernova Gravitational Wave Emission for Progenitors of 9.6, 15, and 25 Solar Masses

Reference 37

Resolution: unresolved; no resolver link, observed 2026-08-04T05:44:58.743551Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 31d4ca14-2732-4e3c-9336-7e55c2336831 · 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 Core Collapse Supernova Gravitational Wave Emission for Progenitors of 9.6, 15, and 25 Solar Masses

Reference 46

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 8c7bfd43-6a85-466f-993d-512acc68ce79 · inbound

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

Reference 46

Resolution: unresolved; no resolver link, observed 2026-08-04T05:43:27.232217Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation fa1fab1b-62a6-4a70-9f88-dba60d445749 · 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 Core Collapse Supernova Gravitational Wave Emission for Progenitors of 9.6, 15, and 25 Solar Masses

Reference 28

Resolution: verified exact; arxiv_id, observed 2026-05-11T18:26:11.121362Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 31646c1f-a5c4-4c7f-8865-c5b584592988 · inbound

Contrastive self-supervised convolutional autoencoder for core-collapse supernova gravitational-wave detection cites this paper.

Contrastive self-supervised convolutional autoencoder for core-collapse supernova gravitational-wave detection Core Collapse Supernova Gravitational Wave Emission for Progenitors of 9.6, 15, and 25 Solar Masses

Reference 160

Resolution: verified exact; arxiv_id, observed 2026-05-21T03:33:56.001326Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 5a241a72-4f16-4b3c-9860-c9fb53d3f9f6 · inbound

Impact of the equation of state on core collapse supernovae I: the low-$T/|W|$ instability cites this paper.

Impact of the equation of state on core collapse supernovae I: the low-$T/|W|$ instability Core Collapse Supernova Gravitational Wave Emission for Progenitors of 9.6, 15, and 25 Solar Masses

Reference 64

Resolution: malformed identifier; arxiv_id, observed 2026-06-29T13:23:28.777525Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation c678f8ea-21c1-4eb3-ada6-ae8873b9d81e · inbound

Universal relations applied to proto-neutron star generated gravitational waves from three-dimensional core collapse supernova simulations cites this paper.

Universal relations applied to proto-neutron star generated gravitational waves from three-dimensional core collapse supernova simulations Core Collapse Supernova Gravitational Wave Emission for Progenitors of 9.6, 15, and 25 Solar Masses

Reference 4

Resolution: unresolved; no resolver link, observed 2026-08-01T04:13:58.534039Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation df84d928-ef03-46be-8b8f-219a483fb7b2 · inbound

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

On the nature of oscillating modes of proto-neutron stars Core Collapse Supernova Gravitational Wave Emission for Progenitors of 9.6, 15, and 25 Solar Masses

Reference 106

Resolution: unresolved; no resolver link, observed 2026-08-14T04:16:47.242320Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.