Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Pulsational pair-instability supernovae in very close binaries
As of 6 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:1810.13412.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-06T06:34:29.942622+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-07-08T17:53:06.845093Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-07-08T17:55:20.615491Z
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 6fae74da-f42f-408f-8db1-8a9e29ad758f · inbound
GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs cites this paper.
GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs Pulsational pair-instability supernovae in very close binaries
Reference 215
- Resolution
- verified exact
- arxiv_id, observed 2026-05-12T14:08:36.650425Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.
Observation 09d1e5bc-2163-49aa-b251-345a6c7162af · inbound
The Black Hole Mass Gap as a New Probe of Millicharged Particles cites this paper.
The Black Hole Mass Gap as a New Probe of Millicharged Particles Pulsational pair-instability supernovae in very close binaries
Reference 87
- Resolution
- verified exact
- arxiv_id, observed 2026-05-13T21:03:19.808427Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.
Observation 8ba067f6-e85a-4bcd-8c8d-a8802c9f4d37 · inbound
Constraints on the Primordial Black Hole Abundance using Pulsar Parameter Drifts cites this paper.
Constraints on the Primordial Black Hole Abundance using Pulsar Parameter Drifts Pulsational pair-instability supernovae in very close binaries
Reference 11
- Resolution
- metadata mismatch
- arxiv_id, observed 2026-05-11T20:06:17.670349Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.
Observation 5d9fa28a-4cc3-4423-9408-a6b37730f599 · inbound
Temperature-resolved sensitivities of $^{56}{\rm Ni}$ production to helium-burning reactions in pair-instability supernovae cites this paper.
Temperature-resolved sensitivities of $^{56}{\rm Ni}$ production to helium-burning reactions in pair-instability supernovae Pulsational pair-instability supernovae in very close binaries
Reference 40
- Resolution
- verified exact
- arxiv_id, observed 2026-07-01T16:25:49.717054Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.
Observation e3c3ae03-c703-4bad-a0e0-2f9a19d221ba · inbound
Targeting black holes from metal-poor progenitors with next-generation gravitational-wave detectors cites this paper.
Targeting black holes from metal-poor progenitors with next-generation gravitational-wave detectors Pulsational pair-instability supernovae in very close binaries
Reference 69
- Resolution
- verified exact
- arxiv_id, observed 2026-07-02T04:26:35.891110Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.
Observation 0f8f632d-d6fa-4195-9994-c9d4860c2ad2 · inbound
A Possible Triple Formation Scenario of Binary Black Hole Merge With One In Pair-instability Supernova Mass Gap cites this paper.
A Possible Triple Formation Scenario of Binary Black Hole Merge With One In Pair-instability Supernova Mass Gap Pulsational pair-instability supernovae in very close binaries
Reference 47
- Resolution
- verified exact
- local_arxiv, observed 2026-07-08T17:55:20.616854Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.