Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
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 7 inbound Pith citation observations for arXiv:2112.10256.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-11T06:34:44.6726+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-11T12:29:10.397305Z
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
- verified exact0
- verified fuzzy0
- unresolved0
- parse uncertain0
- malformed identifier0
- metadata mismatch0
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 0e78af8c-ae5f-4bda-bd19-830f910fad47 · inbound
Blinded Mock Data Challenge for Gravitational-Wave Cosmology-I: Assessing the Robustness of Methods Using Binary Black Holes Mass Spectrum cites this paper.
Blinded Mock Data Challenge for Gravitational-Wave Cosmology-I: Assessing the Robustness of Methods Using Binary Black Holes Mass Spectrum The redshift dependence of black hole mass distribution: Is it reliable for standard sirens cosmology?
Reference 2021
- Resolution
- unresolved
- no resolver link, observed 2026-08-11T12:29:10.397305Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
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.