Paper Citation Record · LEDGER

The rate of WD-WD head-on collisions may be as high as the SNe Ia rate

As of 13 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:1211.4584.

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

pith.paper-citation-record.v1
1211.4584 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 5 of 5 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-12T06:34:41.77262+00:00

measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-12T20:25:19.773552Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-06T22:10:26.440612Z

Reference resolution

0 of 0 outbound references displayed

verified exact0
verified fuzzy0
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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 b9a343bf-bf20-40c0-b3cc-a3d5c690af6e · inbound

Type Ia supernovae cites this paper.

Type Ia supernovae The rate of WD-WD head-on collisions may be as high as the SNe Ia rate

Reference 51

Resolution: unresolved; no resolver link, observed 2026-08-12T20:25:19.773552Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation bbe80f31-962e-4c1c-80e8-7db4124644fc · inbound

Hierarchical Three-Body Problem at High Eccentricities = Simple Pendulum III: Precessing Quadrupole cites this paper.

Hierarchical Three-Body Problem at High Eccentricities = Simple Pendulum III: Precessing Quadrupole The rate of WD-WD head-on collisions may be as high as the SNe Ia rate

Reference 19

Resolution: unresolved; no resolver link, observed 2026-08-11T19:25:51.840717Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ae21de60-5f05-49be-929a-3bb570e32b8b · inbound

Cataclysmic Variables in Triples: Formation Models and New Discoveries cites this paper.

Cataclysmic Variables in Triples: Formation Models and New Discoveries The rate of WD-WD head-on collisions may be as high as the SNe Ia rate

Reference 63

Resolution: unresolved; no resolver link, observed 2026-08-10T15:31:36.455729Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 62dc9909-5cec-48d4-be84-a6f564b0909d · inbound

Double Compact Binary Merger Rate Density in Open Star Clusters: Black Holes, Neutron Stars, and White Dwarfs cites this paper.

Double Compact Binary Merger Rate Density in Open Star Clusters: Black Holes, Neutron Stars, and White Dwarfs The rate of WD-WD head-on collisions may be as high as the SNe Ia rate

Reference 27

Resolution: metadata mismatch; local_arxiv, observed 2026-08-06T22:10:26.593984Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation 7befbb02-4290-4471-9ea7-ac6108323b7e · inbound

Recoiling Black Holes I. Burst of Observables cites this paper.

Recoiling Black Holes I. Burst of Observables The rate of WD-WD head-on collisions may be as high as the SNe Ia rate

Reference 56

Resolution: unresolved; no resolver link, observed 2026-08-11T13:18:05.478766Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.