Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
No evidence that the binary black hole mass distribution evolves with redshift
As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 7 inbound Pith citation observations for arXiv:2501.10295.
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 2026-08-06T06:34:29.942622+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-06T17:20:17.660823Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-07-02T04:26:36.019049Z
Reference resolution
0 of 0 outbound references displayed
- verified exact0
- verified fuzzy0
- unresolved0
- parse uncertain0
- malformed identifier0
- metadata mismatch0
External citation measurements
No source-named external measurement is stored.
Outbound references
No outbound reference observations are available for this paper version.
Pith citing papers
Observation 0b811e0b-223f-469a-a061-22ee205a3a37 · inbound
The fault in our sirens: Hierarchical diagnosis of waveform systematics in Hubble-Lema\^itre constant measurements cites this paper.
The fault in our sirens: Hierarchical diagnosis of waveform systematics in Hubble-Lema\^itre constant measurements No evidence that the binary black hole mass distribution evolves with redshift
Reference 43
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T17:20:17.660823Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation b5069002-145a-43fc-b7c7-4165e8540a1b · inbound
Upper Limits on the Isotropic Gravitational-Wave Background from the first part of LIGO, Virgo, and KAGRA's fourth Observing Run cites this paper.
Upper Limits on the Isotropic Gravitational-Wave Background from the first part of LIGO, Virgo, and KAGRA's fourth Observing Run No evidence that the binary black hole mass distribution evolves with redshift
Reference 78
- Resolution
- unresolved
- no resolver link, observed 2026-08-05T14:59:58.068831Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation a1471320-01f8-4d6b-9f93-52138a5890fd · 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 No evidence that the binary black hole mass distribution evolves with redshift
Reference 105
- Resolution
- metadata mismatch
- arxiv_id, observed 2026-05-11T11:51:01.699744Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.
Observation e5a343d6-8721-4915-8abb-e4490829587b · inbound
Radio sirens: inferring $H_0$ with binary black holes and neutral hydrogen in the era of the Einstein Telescope and the SKA Observatory cites this paper.
Radio sirens: inferring $H_0$ with binary black holes and neutral hydrogen in the era of the Einstein Telescope and the SKA Observatory No evidence that the binary black hole mass distribution evolves with redshift
Reference 83
- Resolution
- metadata mismatch
- arxiv_id, observed 2026-05-14T20:39:27.942908Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.
Observation 4dbe65e8-1aaf-4179-a037-e59459b36cf3 · 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 No evidence that the binary black hole mass distribution evolves with redshift
Reference 32
- Resolution
- verified exact
- arxiv_id, observed 2026-05-20T03:48:02.741076Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.
Observation d70c87e2-eafb-454d-8b2f-cdea11c0a596 · inbound
GWTC-5.0: Constraints on the Cosmic Expansion Rate and Modified Gravitational-wave Propagation cites this paper.
GWTC-5.0: Constraints on the Cosmic Expansion Rate and Modified Gravitational-wave Propagation No evidence that the binary black hole mass distribution evolves with redshift
Reference 14
- Resolution
- verified exact
- arxiv_id, observed 2026-06-29T16:33:39.734596Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.
Observation c00c865a-d359-4235-bcc8-3952b7f11111 · inbound
Targeting black holes from metal-poor progenitors with next-generation gravitational-wave detectors cites this paper.
Targeting black holes from metal-poor progenitors with next-generation gravitational-wave detectors No evidence that the binary black hole mass distribution evolves with redshift
Reference 54
- Resolution
- verified exact
- arxiv_id, observed 2026-07-02T04:26:36.020536Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.