Paper Citation Record · LEDGER

The redshift evolution of the binary black hole merger rate: a weighty matter

As of 14 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 10 inbound Pith citation observations for arXiv:2110.01634.

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

pith.paper-citation-record.v1
2110.01634 v2

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measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 10 of 10 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-14T06:32:32.682623+00:00

measured 10 of 10 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T00:25:50.678826Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-08T17:55:20.516727Z

Reference resolution

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External citation measurements

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Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 64123621-24c4-46e3-8a38-fbfea0c1a1cf · inbound

Evidence for eccentricity in the population of binary black holes observed by LIGO-Virgo-KAGRA cites this paper.

Evidence for eccentricity in the population of binary black holes observed by LIGO-Virgo-KAGRA The redshift evolution of the binary black hole merger rate: a weighty matter

Reference 251

Resolution: verified exact; arxiv_id, observed 2026-05-24T01:35:55.264474Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 5b409725-e085-4096-b8a4-c9537dd4ae0d · inbound

Progress toward the detection of the gravitational-wave background from stellar-mass binary black holes: a mock data challenge cites this paper.

Progress toward the detection of the gravitational-wave background from stellar-mass binary black holes: a mock data challenge The redshift evolution of the binary black hole merger rate: a weighty matter

Reference 13

Resolution: unresolved; no resolver link, observed 2026-08-07T00:25:50.678826Z

Source-reported events for the cited work

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Observation f8e776bb-510d-4d3a-a66d-92d74f01c0bd · 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 The redshift evolution of the binary black hole merger rate: a weighty matter

Reference 101

Resolution: unresolved; no resolver link, observed 2026-08-06T22:52:12.357635Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e15e50d6-e297-4022-b3f5-81adc740e26a · inbound

Comparing the Spatial Correlation of Binary Black Hole Mergers to Large-Scale Structure through the Illustris Simulation cites this paper.

Comparing the Spatial Correlation of Binary Black Hole Mergers to Large-Scale Structure through the Illustris Simulation The redshift evolution of the binary black hole merger rate: a weighty matter

Reference 68

Resolution: unresolved; no resolver link, observed 2026-08-06T17:06:55.725845Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 658d1ff8-1faf-4b1e-8c5e-348a59ff0e28 · 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 The redshift evolution of the binary black hole merger rate: a weighty matter

Reference 40

Resolution: unresolved; no resolver link, observed 2026-08-05T15:53:36.839431Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0f514777-5e07-4b5f-8624-b1b63c7260a5 · inbound

High Power Accretion in Massive Binary Systems and the Impact of Metallicity cites this paper.

High Power Accretion in Massive Binary Systems and the Impact of Metallicity The redshift evolution of the binary black hole merger rate: a weighty matter

Reference 76

Resolution: unresolved; no resolver link, observed 2026-08-04T18:26:36.572940Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 680bcff3-aa8f-4d1f-a3f3-f792af43558c · inbound

Scalar fields around black hole binaries in LIGO-Virgo-KAGRA cites this paper.

Scalar fields around black hole binaries in LIGO-Virgo-KAGRA The redshift evolution of the binary black hole merger rate: a weighty matter

Reference 125

Resolution: verified exact; arxiv_id, observed 2026-05-18T05:50:57.011929Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation f820ea6d-0711-4bdf-ad9d-179f36dc28c6 · inbound

Not too close! Evaluating the impact of the baseline on the localization of binary black holes by next-generation gravitational-wave detectors cites this paper.

Not too close! Evaluating the impact of the baseline on the localization of binary black holes by next-generation gravitational-wave detectors The redshift evolution of the binary black hole merger rate: a weighty matter

Reference 33

Resolution: verified exact; arxiv_id, observed 2026-05-11T10:31:02.460816Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 86f7e1db-3d1d-4fe7-b40d-8fe47f67bea8 · inbound

No Evidence for Superradiant Axions in LIGO-Virgo-KAGRA GWTC-5 Binary Black Hole Spins cites this paper.

No Evidence for Superradiant Axions in LIGO-Virgo-KAGRA GWTC-5 Binary Black Hole Spins The redshift evolution of the binary black hole merger rate: a weighty matter

Reference 84

Resolution: verified exact; arxiv_id, observed 2026-07-03T19:58:53.821672Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 2ccb51d0-d1b0-4d4e-ad60-be5d338541b3 · inbound

A Possible Triple Formation Scenario of Binary Black Hole Merge With One In Pair-instability Supernova Mass Gap cites this paper.

A Possible Triple Formation Scenario of Binary Black Hole Merge With One In Pair-instability Supernova Mass Gap The redshift evolution of the binary black hole merger rate: a weighty matter

Reference 101

Resolution: verified exact; local_arxiv, observed 2026-07-08T17:55:20.518333Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.