Pith. sign in

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 16 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 8 inbound Pith citation observations for arXiv:2305.08909.

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

pith.paper-citation-record.v1
2305.08909 v3

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 8 of 8 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-16T06:30:59.297886+00:00

measured 8 of 8 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-16T10:19:04.246668Z

measured 0 of 1 external citation measurements

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

  • 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 1c1dddad-eb1c-4ca4-b9b1-6e948a3bc51d · inbound

Constraining Population III stellar demographics with next-generation gravitational-wave observatories cites this paper.

Constraining Population III stellar demographics with next-generation gravitational-wave observatories 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 75

Resolution
unresolved
no resolver link, observed 2026-08-16T10:19:04.246668Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T10:19:04.246668Z digest=sha256:c9853293b7744d56b916201528e581a1a3850634352e8f0773ee986af574127d

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.

source=pdf_text observed=2026-08-07T15:36:22.608029Z digest=sha256:fcef093826e8fd157047715816eb32da3e6dcfeffa0462fcc336c653589989a4

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.

source=pdf_text observed=2026-08-06T22:52:12.331057Z digest=sha256:64ae11e552c66c04ac1b26a7784d49123fbd3dd6ef013b7fc46bbac3818eae8f

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 2026-08-16T06:30:59.297886+00:00.

source=pdf_text observed=2026-05-19T04:36:12.661648Z digest=sha256:2825281ab6ea71184e754a96d2b22225f7fc1730654fe69f22da8975e1cc8a2a

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 2026-08-16T06:30:59.297886+00:00.

source=pdf_text observed=2026-05-16T05:35:56.364232Z digest=sha256:606c61bf67e7cf2db4c783d1fcb6febb163af2e6d1e40a67b52f897917099f5e

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 2026-08-16T06:30:59.297886+00:00.

source=pdf_text observed=2026-05-10T12:31:50.358428Z digest=sha256:7962b8a4252dbec58177bc633bcce25ba606bd8cf3f0cef4c0a35c6bcc7e5fb8

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 2026-08-16T06:30:59.297886+00:00.

source=pdf_text observed=2026-06-27T08:41:37.044992Z digest=sha256:eef876027b2393f03aa8022d26aeae63685f881711009703a4851996277ded9b

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 2026-08-16T06:30:59.297886+00:00.

source=pdf_text observed=2026-06-30T05:24:03.103599Z digest=sha256:758403e5f664908bb1aba38498f3b4852aba748ce0d0434cb1af7366d65ffa9c