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Paper Citation Record · LEDGER

Constraining the fraction of binary black holes formed in isolation and young star clusters with gravitational-wave data

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.

pith.paper-citation-record.v1
1905.11054 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 3 of 3 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-07T06:34:17.273281+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T00:42:33.594845Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-09T04:54:55.996041Z

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 47357e81-0d1f-49e2-94e3-92ddbf5b28f6 · inbound

Inferring the properties of a population of compact binaries in presence of selection effects cites this paper.

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

Resolution
verified exact
arxiv_id, observed 2026-05-09T04:54:56.000376Z

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.

source=pdf_text observed=2026-05-24T13:43:48.580253Z digest=sha256:86d28c50efec8f37a53cf23a783a1b28f61c07a02b4ba8f235845d5e99494d61

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 cites this paper.

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

Resolution
unresolved
no resolver link, observed 2026-08-03T22:13:51.289723Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-03T22:13:51.289723Z digest=sha256:66d2ac384e4ed9683096dcf58dae1329846e59dfc99f13660bf8ff062c67398e

Observation fff17b27-84b9-4973-9dae-639dbcb0727f · inbound

Unified remnant models for aligned-spin, precessing, and eccentric binary black hole mergers cites this paper.

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

Resolution
unresolved
no resolver link, observed 2026-08-06T00:42:33.594845Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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