Paper Citation Record · LEDGER

The final core collapse of pulsational pair instability supernovae

As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2101.06889.

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

pith.paper-citation-record.v1
2101.06889 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 4 of 4 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 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-08T12:47:49.847233Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-06-29T13:23:28.778579Z

Reference resolution

0 of 0 outbound references displayed

verified exact0
verified fuzzy0
unresolved0
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malformed identifier0
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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 2ed61e8f-1584-4e15-af6b-45062f3e5580 · 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 The final core collapse of pulsational pair instability supernovae

Reference 46

Resolution: malformed identifier; arxiv_id, observed 2026-06-29T13:23:28.780101Z

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.

Observation a1351632-47c5-4aaf-8424-6d473cbacb1b · 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 The final core collapse of pulsational pair instability supernovae

Reference 3

Resolution: unresolved; no resolver link, observed 2026-08-01T04:13:58.442968Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b0f220b6-b348-458e-9356-ee820155516b · inbound

3D simulations of a complete convective silicon shell burning phase cites this paper.

3D simulations of a complete convective silicon shell burning phase The final core collapse of pulsational pair instability supernovae

Reference 287

Resolution: unresolved; no resolver link, observed 2026-08-06T13:05:40.008998Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a7e8581f-bb6f-48f0-8029-8e332c704064 · 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 The final core collapse of pulsational pair instability supernovae

Reference 47

Resolution: unresolved; no resolver link, observed 2026-08-08T12:47:49.847233Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.