Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Is there an excess of black holes around $20 M_{\odot}$? Optimising the complexity of population models with the use of reversible jump MCMC
As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 7 inbound Pith citation observations for arXiv:2305.08909.
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 2026-08-07T15:36:22.608029Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-07-03T12:58:07.877509Z
Reference resolution
0 of 0 outbound references displayed
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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 68db4e06-bee1-4517-9ea8-e02d9f2f8037 · inbound
The Long Road to Alignment: Measuring Black Hole Spin Orientation with Expanding Gravitational-Wave Datasets cites this paper.
The Long Road to Alignment: Measuring Black Hole Spin Orientation with Expanding Gravitational-Wave Datasets Is there an excess of black holes around $20 M_{\odot}$? Optimising the complexity of population models with the use of reversible jump MCMC
Reference 32
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T15:36:22.608029Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 50c171cc-765f-4935-a35b-2bebfba95aed · 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 Is there an excess of black holes around $20 M_{\odot}$? Optimising the complexity of population models with the use of reversible jump MCMC
Reference 91
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T22:52:12.331057Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation fa2ead9a-fa54-4f22-b974-0d824506126c · 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 Is there an excess of black holes around $20 M_{\odot}$? Optimising the complexity of population models with the use of reversible jump MCMC
Reference 37
- Resolution
- verified exact
- arxiv_id, observed 2026-05-19T04:37:03.724194Z
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 86e57a02-9beb-452d-8307-9fa0a9e58ef0 · inbound
Measurement prospects for the pair-instability mass cutoff with gravitational waves cites this paper.
Measurement prospects for the pair-instability mass cutoff with gravitational waves Is there an excess of black holes around $20 M_{\odot}$? Optimising the complexity of population models with the use of reversible jump MCMC
Reference 73
- Resolution
- verified exact
- arxiv_id, observed 2026-05-16T05:37:23.827561Z
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 ad1b0f9d-9f99-49d3-9c3c-7b19666ef6af · 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 Is there an excess of black holes around $20 M_{\odot}$? Optimising the complexity of population models with the use of reversible jump MCMC
Reference 73
- Resolution
- metadata mismatch
- arxiv_id, observed 2026-05-11T11:51:01.269341Z
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 b6ae5db6-ee24-475c-b478-adfe1fac09c2 · inbound
Evidence for additional structure in the effective spin distribution hints at multiple formation pathways in GWTC-5.0 cites this paper.
Evidence for additional structure in the effective spin distribution hints at multiple formation pathways in GWTC-5.0 Is there an excess of black holes around $20 M_{\odot}$? Optimising the complexity of population models with the use of reversible jump MCMC
Reference 89
- Resolution
- verified exact
- arxiv_id, observed 2026-07-03T12:58:07.878918Z
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 6c2eba80-fb20-4c1f-afdd-b9598ad25a50 · inbound
Joint population and strong-lensing inference for resolved gravitational-wave events probes the black-hole merger rate beyond the peak of star formation cites this paper.
Joint population and strong-lensing inference for resolved gravitational-wave events probes the black-hole merger rate beyond the peak of star formation Is there an excess of black holes around $20 M_{\odot}$? Optimising the complexity of population models with the use of reversible jump MCMC
Reference 85
- Resolution
- verified exact
- arxiv_id, observed 2026-06-30T14:34:46.200730Z
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.