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Paper Citation Record · LEDGER

When the black holes align: a subpopulation of aligned massive binary black holes observed via gravitational waves

As of 7 August 2026, this Paper Citation Record lists 2 of 2 outbound references and 3 inbound Pith citation observations for arXiv:2606.23305.

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

pith.paper-citation-record.v1
2606.23305 v2

Coverage vector

measured 2 of 2 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-08-04T04:42:05.544638Z

measured 5 of 5 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 2026-07-31T22:07:32.670990Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-02T07:56:46.865743Z

Reference resolution

2 of 2 outbound references displayed

  • verified exact0
  • verified fuzzy0
  • unresolved2
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

External citation measurements

No source-named external measurement is stored.

Outbound references

Observation aff9433c-261a-4c0b-acf1-9994d644f6ba · outbound

This paper cites GWTC-4.0: Population Properties of Merging Compact Binaries.

When the black holes align: a subpopulation of aligned massive binary black holes observed via gravitational waves GWTC-4.0: Population Properties of Merging Compact Binaries

Reference 1

Resolution
unresolved
no resolver link, observed 2026-08-04T04:42:05.475577Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T04:42:05.475577Z digest=sha256:ce401dd3f560c7f0c4445853a8dccbad7f9c16ceff69ffe54364d2d56770c3fb

Observation db0f9f73-452a-4242-9e0d-b7c72d67b20e · outbound

This paper cites The model follows stellar-mass BHs from their capture into the AGN disk to BBH formation and merger.

When the black holes align: a subpopulation of aligned massive binary black holes observed via gravitational waves The model follows stellar-mass BHs from their capture into the AGN disk to BBH formation and merger

Reference 2023

Resolution
unresolved
no resolver link, observed 2026-08-04T04:42:05.544638Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T04:42:05.544638Z digest=sha256:2aba38d8fff3194cbfb7e0470db8502d34ef5c61c2be4cfad1e860f947e806d1

Pith citing papers

Observation 15011904-50fd-49d1-850d-48947700166d · inbound

Distinct spin properties and astrophysical origin of low mass binary black holes in gravitational wave data cites this paper.

Distinct spin properties and astrophysical origin of low mass binary black holes in gravitational wave data When the black holes align: a subpopulation of aligned massive binary black holes observed via gravitational waves

Reference 80

Resolution
verified exact
local_arxiv, observed 2026-07-02T07:56:46.867055Z

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=arxiv_source observed=2026-07-02T07:55:37.395171Z digest=sha256:7de423992a5fedc4b555c490a1ea5981fb8836fd33c1d45d0db7cb346b7446b9

Observation 03e8062a-dff4-480f-9077-ec2d44059d30 · inbound

High-mass binary black hole mergers from detailed binary evolution models cites this paper.

High-mass binary black hole mergers from detailed binary evolution models When the black holes align: a subpopulation of aligned massive binary black holes observed via gravitational waves

Reference 133

Resolution
unresolved
no resolver link, observed 2026-07-31T22:07:32.670990Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-31T22:07:32.670990Z digest=sha256:26f6a72b10ee9c7b16399de0c1c79eaeb8c4f423905c1a196f8993d96b5c9118

Observation eafc10be-e0f5-4da5-815e-bf279b22705f · 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 When the black holes align: a subpopulation of aligned massive binary black holes observed via gravitational waves

Reference 47

Resolution
unresolved
no resolver link, observed 2026-07-31T01:54:12.255367Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-31T01:54:12.255367Z digest=sha256:d06e873fab35ff8274a134411765861136fea1d585b861cb7a76628d63a65c49