Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Which black hole formed first? Mass-ratio reversal in massive binary stars from gravitational-wave data
As of 21 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 1 inbound Pith citation observation for arXiv:2205.12329.
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 2026-08-21T06:32:19.484+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-05-19T02:22:28.762392Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-05-19T02:22:56.256556Z
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 057d519e-a6e6-4c38-8ce9-63fedd3f1743 · inbound
Disentangling spinning and nonspinning binary black hole populations with spin sorting cites this paper.
Disentangling spinning and nonspinning binary black hole populations with spin sorting Which black hole formed first? Mass-ratio reversal in massive binary stars from gravitational-wave data
Reference 36
- Resolution
- verified exact
- arxiv_id, observed 2026-05-19T02:22:56.261267Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.