Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Not just winds: why models find binary black hole formation is metallicity dependent, while binary neutron star formation is not
As of 20 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2411.02484.
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 2026-08-19T06:32:44.657259+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-12T14:12:24.268512Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-11T00:16:15.729268Z
Reference resolution
0 of 0 outbound references displayed
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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 b867b52a-788a-4253-8194-1358dbf60ed9 · inbound
Triple Evolution Pathways to Black Hole Low-Mass X-ray Binaries: Insights from V404 Cygni cites this paper.
Triple Evolution Pathways to Black Hole Low-Mass X-ray Binaries: Insights from V404 Cygni Not just winds: why models find binary black hole formation is metallicity dependent, while binary neutron star formation is not
Reference 165
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T14:12:24.268512Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation fba076fe-c653-4d53-8a4f-65e35cd27791 · inbound
Impact of accretion-induced chemically homogeneous evolution on stellar and compact binary populations cites this paper.
Impact of accretion-induced chemically homogeneous evolution on stellar and compact binary populations Not just winds: why models find binary black hole formation is metallicity dependent, while binary neutron star formation is not
Reference 122
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T21:32:15.960676Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation a30da17c-d75d-499c-aba4-05d74f67a017 · inbound
No evidence that the binary black hole mass distribution evolves with redshift cites this paper.
No evidence that the binary black hole mass distribution evolves with redshift Not just winds: why models find binary black hole formation is metallicity dependent, while binary neutron star formation is not
Reference 79
- Resolution
- verified exact
- local_arxiv, observed 2026-08-10T19:21:41.453851Z
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 6eac8458-e727-463d-80df-64c287d1d0bb · inbound
Implications of modern mass-loss rates for massive stars cites this paper.
Implications of modern mass-loss rates for massive stars Not just winds: why models find binary black hole formation is metallicity dependent, while binary neutron star formation is not
Reference 117
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T15:03:32.802594Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.