Paper Citation Record · LEDGER

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

As of 22 August 2026, this Paper Citation Record lists 17 of 17 outbound references and 4 inbound Pith citation observations for arXiv:2412.14244.

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

pith.paper-citation-record.v1
2412.14244 v2

Coverage vector

measured 17 of 17 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-08-11T12:29:10.408861Z

measured 21 of 21 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-22T06:32:14.747728+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-09T19:46:36.160374Z

measured 0 of 1 external citation measurements

A source-named dated measurement, never combined with another source.

Source: arxiv_reference, observed 2026-05-20T03:48:02.829632Z

Reference resolution

17 of 17 outbound references displayed

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External citation measurements

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Outbound references

Observation 0a388b2b-3e41-4b32-8c84-2d3f28c05198 · outbound

This paper cites 2015, Class.

Blinded Mock Data Challenge for Gravitational-Wave Cosmology-I: Assessing the Robustness of Methods Using Binary Black Holes Mass Spectrum 2015, Class

Reference 1

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Source-reported events for the cited work

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Observation f04a8f33-7c92-4466-b008-c3d3f4176df7 · outbound

This paper cites The Gravitational Wave Bias Parameter from Angular Power Spectra: Bridging Between Galaxies and Binary Black Holes.

Blinded Mock Data Challenge for Gravitational-Wave Cosmology-I: Assessing the Robustness of Methods Using Binary Black Holes Mass Spectrum The Gravitational Wave Bias Parameter from Angular Power Spectra: Bridging Between Galaxies and Binary Black Holes

Reference 4

Resolution: unresolved; no resolver link, observed 2026-08-11T12:29:10.368247Z

Source-reported events for the cited work

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Observation 9ac6fd9c-17b9-41fd-b4b2-6b33684f894c · outbound

This paper cites No need to know: astrophysics-free gravitational-wave cosmology.

Blinded Mock Data Challenge for Gravitational-Wave Cosmology-I: Assessing the Robustness of Methods Using Binary Black Holes Mass Spectrum No need to know: astrophysics-free gravitational-wave cosmology

Reference 7

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Observation 79356b50-a6da-44e5-9368-50a877882024 · outbound

This paper cites A robust cosmic standard ruler from the cross-correlations of galaxies and dark sirens.

Blinded Mock Data Challenge for Gravitational-Wave Cosmology-I: Assessing the Robustness of Methods Using Binary Black Holes Mass Spectrum A robust cosmic standard ruler from the cross-correlations of galaxies and dark sirens

Reference 8

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Observation 3af83c0b-d1e9-41b2-8fb0-44e0be68c0df · outbound

This paper cites Gravitational-wave dark siren cosmology systematics from galaxy weighting.

Blinded Mock Data Challenge for Gravitational-Wave Cosmology-I: Assessing the Robustness of Methods Using Binary Black Holes Mass Spectrum Gravitational-wave dark siren cosmology systematics from galaxy weighting

Reference 9

Resolution: unresolved; no resolver link, observed 2026-08-11T12:29:10.385412Z

Source-reported events for the cited work

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Observation 45fef9c7-accd-4c40-8d50-d8e7fb154b61 · outbound

This paper cites Current and future constraints on cosmology and modified gravitational wave friction from binary black holes.

Blinded Mock Data Challenge for Gravitational-Wave Cosmology-I: Assessing the Robustness of Methods Using Binary Black Holes Mass Spectrum Current and future constraints on cosmology and modified gravitational wave friction from binary black holes

Reference 10

Resolution: unresolved; no resolver link, observed 2026-08-11T12:29:10.388103Z

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Observation cabe7e40-64f9-47f8-8414-b36941ec3f94 · outbound

This paper cites Beyond Gaps and Bumps: Spectral Siren Cosmology with Non-Parametric Population Models.

Blinded Mock Data Challenge for Gravitational-Wave Cosmology-I: Assessing the Robustness of Methods Using Binary Black Holes Mass Spectrum Beyond Gaps and Bumps: Spectral Siren Cosmology with Non-Parametric Population Models

Reference 11

Resolution: unresolved; no resolver link, observed 2026-08-11T12:29:10.391569Z

Source-reported events for the cited work

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Observation df2bb9e7-16aa-49c1-99e6-55ea40dcf449 · outbound

This paper cites an unresolved cited work.

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

Reference 12

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Source-reported events for the cited work

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Observation 2d20fa49-2dff-49eb-8d43-5a55a0f5afc9 · outbound

This paper cites Be careful in multi-messenger inference of the Hubble constant: A path forward for robust inference.

Blinded Mock Data Challenge for Gravitational-Wave Cosmology-I: Assessing the Robustness of Methods Using Binary Black Holes Mass Spectrum Be careful in multi-messenger inference of the Hubble constant: A path forward for robust inference

Reference 14

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Observation 75764933-3b2e-4b61-ba2c-e7506764e8e7 · outbound

This paper cites A standard siren measurement of the Hubble constant using gravitational wave events from the first three LIGO/Virgo observing runs and the DESI Legacy Survey.

Blinded Mock Data Challenge for Gravitational-Wave Cosmology-I: Assessing the Robustness of Methods Using Binary Black Holes Mass Spectrum A standard siren measurement of the Hubble constant using gravitational wave events from the first three LIGO/Virgo observing runs and the DESI Legacy Survey

Reference 15

Resolution: unresolved; no resolver link, observed 2026-08-11T12:29:10.403466Z

Source-reported events for the cited work

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Observation a1574141-dc6b-4433-994f-1b0b13866f76 · outbound

This paper cites Fiducial-Cosmology-dependent systematics for the DESI 2024 BAO Analysis.

Blinded Mock Data Challenge for Gravitational-Wave Cosmology-I: Assessing the Robustness of Methods Using Binary Black Holes Mass Spectrum Fiducial-Cosmology-dependent systematics for the DESI 2024 BAO Analysis

Reference 16

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Source-reported events for the cited work

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Observation 142950c5-44d5-4e66-83ab-3c71460685f8 · outbound

This paper cites Investigating the impact of galaxies' compact binary hosting probability for gravitational-wave cosmology.

Blinded Mock Data Challenge for Gravitational-Wave Cosmology-I: Assessing the Robustness of Methods Using Binary Black Holes Mass Spectrum Investigating the impact of galaxies' compact binary hosting probability for gravitational-wave cosmology

Reference 17

Resolution: unresolved; no resolver link, observed 2026-08-11T12:29:10.408861Z

Source-reported events for the cited work

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Observation 5a7d65de-eef4-4d42-aad3-4b27718ee9da · outbound

This paper cites The DESI Experiment Part I: Science,Targeting, and Survey Design.

Blinded Mock Data Challenge for Gravitational-Wave Cosmology-I: Assessing the Robustness of Methods Using Binary Black Holes Mass Spectrum The DESI Experiment Part I: Science,Targeting, and Survey Design

Reference 2016

Resolution: unresolved; no resolver link, observed 2026-08-11T12:29:10.361384Z

Source-reported events for the cited work

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Observation b95d428a-0d12-4f27-9dc5-8a711d4e2bc1 · outbound

This paper cites Time Delay Lens Modeling Challenge: I. Experimental Design.

Blinded Mock Data Challenge for Gravitational-Wave Cosmology-I: Assessing the Robustness of Methods Using Binary Black Holes Mass Spectrum Time Delay Lens Modeling Challenge: I. Experimental Design

Reference 2018

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Source-reported events for the cited work

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Observation 0e78af8c-ae5f-4bda-bd19-830f910fad47 · outbound

This paper cites The redshift dependence of black hole mass distribution: Is it reliable for standard sirens cosmology?.

Blinded Mock Data Challenge for Gravitational-Wave Cosmology-I: Assessing the Robustness of Methods Using Binary Black Holes Mass Spectrum The redshift dependence of black hole mass distribution: Is it reliable for standard sirens cosmology?

Reference 2021

Resolution: unresolved; no resolver link, observed 2026-08-11T12:29:10.397305Z

Source-reported events for the cited work

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Observation 3584635f-1e06-4311-b426-0d30f9735712 · outbound

This paper cites Spectral sirens: cosmology from the full mass distribution of compact binaries.

Blinded Mock Data Challenge for Gravitational-Wave Cosmology-I: Assessing the Robustness of Methods Using Binary Black Holes Mass Spectrum Spectral sirens: cosmology from the full mass distribution of compact binaries

Reference 2022

Resolution: unresolved; no resolver link, observed 2026-08-11T12:29:10.375868Z

Source-reported events for the cited work

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Observation f34f62c3-1c05-47f8-978b-64edb276a9f6 · outbound

This paper cites Observed Gravitational-Wave Populations.

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

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Pith citing papers

Observation 4fa13ce0-e9fa-440f-8e0e-624d13969523 · inbound

Gravitational Wave Cosmology cites this paper.

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

Reference 5

Resolution: unresolved; no resolver link, observed 2026-08-09T19:46:36.160374Z

Source-reported events for the cited work

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Observation 3ecc3fee-ad79-4185-a242-0753a7313bde · inbound

Spectral siren cosmology from gravitational-wave observations in GWTC-4.0 cites this paper.

Spectral siren cosmology from gravitational-wave observations in GWTC-4.0 Blinded Mock Data Challenge for Gravitational-Wave Cosmology-I: Assessing the Robustness of Methods Using Binary Black Holes Mass Spectrum

Reference 13

Resolution: unresolved; no resolver link, observed 2026-08-05T10:56:35.187217Z

Source-reported events for the cited work

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Observation f9933e44-714a-436b-ac84-2b40ce4bfaaf · 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 Blinded Mock Data Challenge for Gravitational-Wave Cosmology-I: Assessing the Robustness of Methods Using Binary Black Holes Mass Spectrum

Reference 99

Resolution: metadata mismatch; arxiv_id, observed 2026-05-11T11:51:01.353125Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

Observation 93fb4fd2-bbc3-4c8a-acc4-6e876948375a · 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 Blinded Mock Data Challenge for Gravitational-Wave Cosmology-I: Assessing the Robustness of Methods Using Binary Black Holes Mass Spectrum

Reference 35

Resolution: verified exact; arxiv_id, observed 2026-05-20T03:48:02.832935Z

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No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.