Paper Citation Record · LEDGER

Physical Models for the Astrophysical Population of Black Holes: Application to the Bump in the Mass Distribution of Gravitational Wave Sources

As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:2312.03973.

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

pith.paper-citation-record.v1
2312.03973 v3

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 6 of 6 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-11T06:34:44.6726+00:00

measured 6 of 6 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T18:29:55.165447Z

measured 1 of 1 external citation measurements

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

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External citation measurements

0
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 9160a0ad-8788-401c-9bbf-1e66b457d099 · inbound

Improving gravitational wave search sensitivity with TIER: Trigger Inference using Extended strain Representation cites this paper.

Improving gravitational wave search sensitivity with TIER: Trigger Inference using Extended strain Representation Physical Models for the Astrophysical Population of Black Holes: Application to the Bump in the Mass Distribution of Gravitational Wave Sources

Reference 36

Resolution: unresolved; no resolver link, observed 2026-08-06T18:29:55.165447Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d55a59b4-8298-4138-ad55-750eb8f60c5e · inbound

Gravitational-wave constraints on the pair-instability mass gap and nuclear burning in massive stars cites this paper.

Gravitational-wave constraints on the pair-instability mass gap and nuclear burning in massive stars Physical Models for the Astrophysical Population of Black Holes: Application to the Bump in the Mass Distribution of Gravitational Wave Sources

Reference 53

Resolution: verified exact; arxiv_id, observed 2026-05-09T02:16:34.248837Z

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 97323604-ff98-4a80-bd99-16f009ed9daa · inbound

Population of Binary Black Holes Inferred from One Hundred and Fifty Gravitational Wave Signals cites this paper.

Population of Binary Black Holes Inferred from One Hundred and Fifty Gravitational Wave Signals Physical Models for the Astrophysical Population of Black Holes: Application to the Bump in the Mass Distribution of Gravitational Wave Sources

Reference 56

Resolution: unresolved; no resolver link, observed 2026-08-04T07:34:41.898493Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ba220744-8f4f-4c23-ba03-521d1879438d · 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 Physical Models for the Astrophysical Population of Black Holes: Application to the Bump in the Mass Distribution of Gravitational Wave Sources

Reference 43

Resolution: verified exact; arxiv_id, observed 2026-05-16T05:37:23.644277Z

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 5aa194cb-d86d-4b04-aebf-23ea64fd5994 · 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 Physical Models for the Astrophysical Population of Black Holes: Application to the Bump in the Mass Distribution of Gravitational Wave Sources

Reference 30

Resolution: metadata mismatch; arxiv_id, observed 2026-05-11T11:51:01.635039Z

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 6c2564ac-7d01-4603-a45d-c502d37bc47f · inbound

The Chirp-Mass Ladder: A New Rung Emerges cites this paper.

The Chirp-Mass Ladder: A New Rung Emerges Physical Models for the Astrophysical Population of Black Holes: Application to the Bump in the Mass Distribution of Gravitational Wave Sources

Reference 197

Resolution: metadata mismatch; arxiv_id, observed 2026-06-26T23:10:13.946098Z

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.