Paper Citation Record · LEDGER

The redshift dependence of black hole mass distribution: Is it reliable for standard sirens cosmology?

As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:2112.10256.

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

pith.paper-citation-record.v1
2112.10256 v3

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 2026-08-11T06:34:44.6726+00:00

measured 6 of 6 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T04:21:41.120800Z

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 8478dd42-35cc-4863-a149-66deb748e4b3 · inbound

Modeling Gravitational Wave Bias from 3D Power Spectra of Spectroscopic Surveys cites this paper.

Modeling Gravitational Wave Bias from 3D Power Spectra of Spectroscopic Surveys The redshift dependence of black hole mass distribution: Is it reliable for standard sirens cosmology?

Reference 138

Resolution: unresolved; no resolver link, observed 2026-08-07T04:21:41.120800Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 12fc7bc1-2bbf-4acd-90a1-f2f5e1844222 · inbound

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap cites this paper.

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap The redshift dependence of black hole mass distribution: Is it reliable for standard sirens cosmology?

Reference 56

Resolution: unresolved; no resolver link, observed 2026-08-04T19:47:52.003346Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b859cdb4-1245-44dc-badc-f8e243998974 · inbound

On the use of the Derivative Approximation for Likelihoods for Gravitational Wave Inference cites this paper.

On the use of the Derivative Approximation for Likelihoods for Gravitational Wave Inference The redshift dependence of black hole mass distribution: Is it reliable for standard sirens cosmology?

Reference 49

Resolution: metadata mismatch; arxiv_id, observed 2026-05-18T06:35:59.796669Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation 8fc316ae-29c4-49e2-afeb-91b4201a5997 · inbound

Emergent structure in the binary black hole mass distribution and implications for population-based cosmology cites this paper.

Emergent structure in the binary black hole mass distribution and implications for population-based cosmology The redshift dependence of black hole mass distribution: Is it reliable for standard sirens cosmology?

Reference 97

Resolution: metadata mismatch; arxiv_id, observed 2026-05-11T11:51:01.647582Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation 7a206e50-2e91-416c-a5a1-2ccec496e7dd · inbound

Gravitational-wave constraints on $H_0$ are robust to (putative) redshift evolution in the binary black hole mass spectrum at current sensitivity cites this paper.

Gravitational-wave constraints on $H_0$ are robust to (putative) redshift evolution in the binary black hole mass spectrum at current sensitivity The redshift dependence of black hole mass distribution: Is it reliable for standard sirens cosmology?

Reference 29

Resolution: verified exact; arxiv_id, observed 2026-05-20T03:48:02.765595Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation ea96e0de-5131-4d0d-8c42-762d17e12985 · 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 The redshift dependence of black hole mass distribution: Is it reliable for standard sirens cosmology?

Reference 266

Resolution: metadata mismatch; arxiv_id, observed 2026-06-29T02:43:03.290235Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.