Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1905.11054.
A citation records a reference. It does not transfer a finding from one paper to another.
Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-07T06:34:17.273281+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-06T00:42:33.594845Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-05-09T04:54:55.996041Z
0 of 0 outbound references displayed
External citation measurements
No source-named external measurement is stored.
No outbound reference observations are available for this paper version.
Observation 47357e81-0d1f-49e2-94e3-92ddbf5b28f6 · inbound
Inferring the properties of a population of compact binaries in presence of selection effects Constraining the fraction of binary black holes formed in isolation and young star clusters with gravitational-wave data
Reference 56
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.
Observation 8a37926f-2bcd-4a12-b178-7889b9249c7a · inbound
Accurate models for recoil velocity distribution in black hole mergers with comparable to extreme mass-ratios and their astrophysical implications Constraining the fraction of binary black holes formed in isolation and young star clusters with gravitational-wave data
Reference 55
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation fff17b27-84b9-4973-9dae-639dbcb0727f · inbound
Unified remnant models for aligned-spin, precessing, and eccentric binary black hole mergers Constraining the fraction of binary black holes formed in isolation and young star clusters with gravitational-wave data
Reference 49
Source-reported events for the cited work
Unavailable: canonical work link unavailable.