Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Searching for additional structure and redshift evolution in the observed binary black hole population with a parametric time-dependent mass distribution
As of 5 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2502.20445.
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 2026-08-04T06:34:03.388597+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-06-26T13:59:14.326070Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-07-04T06:59:38.051748Z
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 ca8d583f-716b-4789-944f-96e85b09fbc0 · inbound
Comparing astrophysical models to gravitational-wave data in the observable space cites this paper.
Comparing astrophysical models to gravitational-wave data in the observable space Searching for additional structure and redshift evolution in the observed binary black hole population with a parametric time-dependent mass distribution
Reference 28
- Resolution
- verified exact
- arxiv_id, observed 2026-05-19T04:37:03.865170Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.
Observation 78c21c51-732e-4d91-91b0-242bc015744a · 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 Searching for additional structure and redshift evolution in the observed binary black hole population with a parametric time-dependent mass distribution
Reference 13
- Resolution
- metadata mismatch
- arxiv_id, observed 2026-05-11T11:51:01.828462Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.
Observation 0112db0a-5355-42e2-9897-c6de4c284002 · 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 Searching for additional structure and redshift evolution in the observed binary black hole population with a parametric time-dependent mass distribution
Reference 143
- Resolution
- metadata mismatch
- arxiv_id, observed 2026-05-14T20:39:27.998911Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.
Observation 8ab51c1e-2765-4ad6-958c-246ec09e68e2 · 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 Searching for additional structure and redshift evolution in the observed binary black hole population with a parametric time-dependent mass distribution
Reference 22
- Resolution
- verified exact
- arxiv_id, observed 2026-05-20T03:48:02.735177Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.
Observation b9a04789-6753-4765-960a-8f0df69b1627 · inbound
Population-level correlations in Bayesian statistics: an illustrative model for gravitational-wave astronomy cites this paper.
Population-level correlations in Bayesian statistics: an illustrative model for gravitational-wave astronomy Searching for additional structure and redshift evolution in the observed binary black hole population with a parametric time-dependent mass distribution
Reference 18
- Resolution
- verified exact
- arxiv_id, observed 2026-07-04T06:59:38.052986Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.