Paper Citation Record · LEDGER

Understanding the high-mass binary black hole population from stable mass transfer and super-Eddington accretion in BPASS

As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:2206.13842.

A citation records a reference. It does not transfer a finding from one paper to another.

pith.paper-citation-record.v1
2206.13842 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 6 of 6 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 6 of 6 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T22:52:12.141662Z

measured 1 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-08-05T02:28:24.338817Z

Reference resolution

0 of 0 outbound references displayed

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External citation measurements

1
arxiv_reference, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 4e22ab87-bf94-4582-b5c7-d4274eabaa15 · inbound

Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop cites this paper.

Nowhere left to hide: revealing realistic gravitational-wave populations in high dimensions and high resolution with PixelPop Understanding the high-mass binary black hole population from stable mass transfer and super-Eddington accretion in BPASS

Reference 20

Resolution: unresolved; no resolver link, observed 2026-08-06T22:52:12.141662Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a9c450f9-7867-4a40-98cf-d8a493baa74c · inbound

Exploring the astrophysical origins of binary black holes using normalising flows cites this paper.

Exploring the astrophysical origins of binary black holes using normalising flows Understanding the high-mass binary black hole population from stable mass transfer and super-Eddington accretion in BPASS

Reference 41

Resolution: unresolved; no resolver link, observed 2026-08-05T15:53:36.958259Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 15b2d893-fcb7-4f33-a26d-a755cfa97bd9 · inbound

Stable mass transfer in massive binaries leading to merging black holes cites this paper.

Stable mass transfer in massive binaries leading to merging black holes Understanding the high-mass binary black hole population from stable mass transfer and super-Eddington accretion in BPASS

Reference 46

Resolution: unresolved; no resolver link, observed 2026-08-03T14:34:25.695961Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8fdd37bf-6fa6-4610-be27-50d6dd7825d7 · inbound

Second-Generation Mass Peak in the Gravitational-Wave Population as a Probe of Globular Clusters cites this paper.

Second-Generation Mass Peak in the Gravitational-Wave Population as a Probe of Globular Clusters Understanding the high-mass binary black hole population from stable mass transfer and super-Eddington accretion in BPASS

Reference 9

Resolution: verified exact; arxiv_id, observed 2026-05-11T06:11:02.803179Z

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 ed5a334a-d880-411f-8d91-26ff1180f743 · inbound

The impact of stellar binaries and star cluster dynamics on pair-instability supernovae cites this paper.

The impact of stellar binaries and star cluster dynamics on pair-instability supernovae Understanding the high-mass binary black hole population from stable mass transfer and super-Eddington accretion in BPASS

Reference 234

Resolution: verified exact; arxiv_id, observed 2026-06-29T02:43:03.469613Z

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 d6d38459-59b2-4421-9037-2caf78d1d939 · inbound

A Four-dimensional Model-agnostic Probe into the Astrophysical Origins of Binary Black Hole Subpopulations cites this paper.

A Four-dimensional Model-agnostic Probe into the Astrophysical Origins of Binary Black Hole Subpopulations Understanding the high-mass binary black hole population from stable mass transfer and super-Eddington accretion in BPASS

Reference 119

Resolution: unresolved; no resolver link, observed 2026-07-31T01:54:12.464052Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.