Paper Citation Record · LEDGER

Observed Gravitational-Wave Populations

As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 18 inbound Pith citation observations for arXiv:2410.19145.

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

pith.paper-citation-record.v1
2410.19145 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 18 of 18 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-18T06:34:40.430872+00:00

measured 18 of 18 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T12:29:10.365372Z

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

verified exact0
verified fuzzy0
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External citation measurements

1
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 f34f62c3-1c05-47f8-978b-64edb276a9f6 · inbound

Blinded Mock Data Challenge for Gravitational-Wave Cosmology-I: Assessing the Robustness of Methods Using Binary Black Holes Mass Spectrum cites this paper.

Blinded Mock Data Challenge for Gravitational-Wave Cosmology-I: Assessing the Robustness of Methods Using Binary Black Holes Mass Spectrum Observed Gravitational-Wave Populations

Reference 2024

Resolution: unresolved; no resolver link, observed 2026-08-11T12:29:10.365372Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation fcbe203c-477f-4ed4-82ff-75f6944bc751 · inbound

Revealing the $\chi_{\rm eff}$-$q$ Correlation among Coalescing Binary Black Holes and Tentative Evidence for AGN-driven Hierarchical Mergers cites this paper.

Revealing the $\chi_{\rm eff}$-$q$ Correlation among Coalescing Binary Black Holes and Tentative Evidence for AGN-driven Hierarchical Mergers Observed Gravitational-Wave Populations

Reference 13

Resolution: unresolved; no resolver link, observed 2026-08-10T20:03:24.797359Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1b3eb696-f287-4d4a-ae53-324d5a6783a5 · inbound

No evidence that the binary black hole mass distribution evolves with redshift cites this paper.

No evidence that the binary black hole mass distribution evolves with redshift Observed Gravitational-Wave Populations

Reference 26

Resolution: unresolved; no resolver link, observed 2026-08-10T19:21:40.658133Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d188d831-3aae-45b1-922b-4968f02e7a45 · inbound

A Possible Mass Ratio and Spin-Orbit Misalignment Correlation for Mergers of Binary Black Holes in Nuclear Star Clusters cites this paper.

A Possible Mass Ratio and Spin-Orbit Misalignment Correlation for Mergers of Binary Black Holes in Nuclear Star Clusters Observed Gravitational-Wave Populations

Reference 28

Resolution: unresolved; no resolver link, observed 2026-08-10T13:41:03.181313Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 73daa7e3-e30a-41ab-903a-91cfeb625b97 · inbound

Gravitational Wave Cosmology cites this paper.

Gravitational Wave Cosmology Observed Gravitational-Wave Populations

Reference 10

Resolution: unresolved; no resolver link, observed 2026-08-09T19:46:36.190746Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 125948f2-ae95-45c2-865a-5c94b2071426 · 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 Observed Gravitational-Wave Populations

Reference 14

Resolution: unresolved; no resolver link, observed 2026-08-07T15:36:20.627509Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0ee1bc48-2fa4-4200-80f2-429e889d37d8 · 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 Observed Gravitational-Wave Populations

Reference 7

Resolution: unresolved; no resolver link, observed 2026-08-06T22:52:12.105793Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation cd8b6aed-516e-4ef0-bc26-f2aa7f195f27 · 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 Observed Gravitational-Wave Populations

Reference 5

Resolution: verified exact; arxiv_id, observed 2026-05-19T04:37:03.688508Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation b4a7e795-e870-45f3-97b6-7aa88da1e845 · inbound

Exploring the astrophysical origins of binary black holes using normalising flows cites this paper.

Exploring the astrophysical origins of binary black holes using normalising flows Observed Gravitational-Wave Populations

Reference 13

Resolution: unresolved; no resolver link, observed 2026-08-05T15:53:33.139708Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c59fa560-6b06-4a1b-842d-19f8af684d64 · 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 Observed Gravitational-Wave Populations

Reference 2

Resolution: verified exact; arxiv_id, observed 2026-05-11T11:51:01.738511Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation 98c4c464-b001-41a7-a978-27a974a75f7c · inbound

Gravitational-wave astronomy requires population-informed parameter estimation cites this paper.

Gravitational-wave astronomy requires population-informed parameter estimation Observed Gravitational-Wave Populations

Reference 60

Resolution: verified exact; arxiv_id, observed 2026-05-10T08:22:37.204216Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation 64c40703-f9d8-4a15-a7eb-abc782a9dc55 · inbound

Gravitational-wave astronomy requires population-informed parameter estimation cites this paper.

Gravitational-wave astronomy requires population-informed parameter estimation Observed Gravitational-Wave Populations

Reference 60

Resolution: unresolved; no resolver link, observed 2026-08-02T16:12:03.755135Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ba310707-c40f-4610-a769-68bdcb573b61 · inbound

Agnostically decoding gravitational wave model deficiencies in GWTC-3 cites this paper.

Agnostically decoding gravitational wave model deficiencies in GWTC-3 Observed Gravitational-Wave Populations

Reference 5

Resolution: verified exact; arxiv_id, observed 2026-05-12T09:31:26.703426Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation 093848a4-ed20-438a-977a-e6d1310ce84b · inbound

How do the LIGO-Virgo-KAGRA's Heavy Black Holes Form? No evidence for core-collapse Intermediate-mass black holes in GWTC-4 cites this paper.

How do the LIGO-Virgo-KAGRA's Heavy Black Holes Form? No evidence for core-collapse Intermediate-mass black holes in GWTC-4 Observed Gravitational-Wave Populations

Reference 107

Resolution: metadata mismatch; arxiv_id, observed 2026-05-08T23:14:23.721811Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation 05d44235-1081-473d-a452-00791ca724cd · inbound

Secondary-Mass Features improve Spectral-Siren $H_0$ Constraints cites this paper.

Secondary-Mass Features improve Spectral-Siren $H_0$ Constraints Observed Gravitational-Wave Populations

Reference 17

Resolution: verified exact; arxiv_id, observed 2026-05-13T02:07:06.807750Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation 05b0b38c-ef5d-4cbe-b1ac-df894525451b · inbound

The geometry of lunar gravitational wave detection cites this paper.

The geometry of lunar gravitational wave detection Observed Gravitational-Wave Populations

Reference 18

Resolution: verified exact; arxiv_id, observed 2026-07-02T09:46:50.042805Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation e7131555-e297-42c9-9116-b3148adf89e1 · inbound

Fortifying gravitational-wave population inference with normalizing flows cites this paper.

Fortifying gravitational-wave population inference with normalizing flows Observed Gravitational-Wave Populations

Reference 17

Resolution: unresolved; no resolver link, observed 2026-08-02T11:35:57.638699Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0ff8fcf5-57fb-488e-aeea-7ca7a592db9f · 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 Observed Gravitational-Wave Populations

Reference 9

Resolution: verified exact; arxiv_id, observed 2026-07-04T06:59:37.963986Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.