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Paper Citation Record · LEDGER

Analyzing the Large-Scale Bulk Flow using CosmicFlows4: Increasing Tension with the Standard Cosmological Model

As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 18 inbound Pith citation observations for arXiv:2302.02028.

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pith.paper-citation-record.v1
2302.02028 v1

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measured 0 of 0 reference resolution

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Source: paper_references, paper_reference_links

measured 18 of 18 standing notices

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Source: scholarly_work_events, retraction_status_cache, observed 2026-08-17T06:30:58.91139+00:00

measured 18 of 18 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-16T12:17:22.726305Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-10T17:27:26.884896Z

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External citation measurements

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Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 363435d7-a161-4fbb-a08b-c137ce5c0016 · inbound

Dispersion in the Hubble-Lema\^{i}tre constant measurements from gravitational clustering cites this paper.

Dispersion in the Hubble-Lema\^{i}tre constant measurements from gravitational clustering Analyzing the Large-Scale Bulk Flow using CosmicFlows4: Increasing Tension with the Standard Cosmological Model

Reference 21

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arxiv_id, observed 2026-05-23T22:55:51.407186Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

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Observation bd50ed94-87e6-4961-bf62-4d1eb71ae289 · inbound

Anisotropy in Pantheon+ supernovae cites this paper.

Anisotropy in Pantheon+ supernovae Analyzing the Large-Scale Bulk Flow using CosmicFlows4: Increasing Tension with the Standard Cosmological Model

Reference 12

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Observation e067ba9c-df5d-46fd-ae75-074c93212ec5 · inbound

Horndeski in motion cites this paper.

Horndeski in motion Analyzing the Large-Scale Bulk Flow using CosmicFlows4: Increasing Tension with the Standard Cosmological Model

Reference 71

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Observation 6e76feca-b7cb-4df0-8d20-fcac7f6d95df · inbound

Redshift tomography of the kinematic matter dipole cites this paper.

Redshift tomography of the kinematic matter dipole Analyzing the Large-Scale Bulk Flow using CosmicFlows4: Increasing Tension with the Standard Cosmological Model

Reference 68

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Observation d3624890-ebd7-4cdd-977d-c04057904034 · inbound

Alleviating the Hubble Tension with a Local Void and Transitions of the Absolute Magnitude cites this paper.

Alleviating the Hubble Tension with a Local Void and Transitions of the Absolute Magnitude Analyzing the Large-Scale Bulk Flow using CosmicFlows4: Increasing Tension with the Standard Cosmological Model

Reference 57

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Observation 1a2bc4bc-c2bc-4951-9667-47e335ad8040 · inbound

Two Dynamical Scenarios for Binned Master Sample Interpretation cites this paper.

Two Dynamical Scenarios for Binned Master Sample Interpretation Analyzing the Large-Scale Bulk Flow using CosmicFlows4: Increasing Tension with the Standard Cosmological Model

Reference 42

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Observation 4023da6e-9c49-45a5-824a-05ff8b8583bf · inbound

Encyclopedia of Astrophysics: The Expanding Universe cites this paper.

Encyclopedia of Astrophysics: The Expanding Universe Analyzing the Large-Scale Bulk Flow using CosmicFlows4: Increasing Tension with the Standard Cosmological Model

Reference 30

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no resolver link, observed 2026-08-04T18:34:02.751178Z

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Observation 8c9c499e-3593-4fff-83ce-6dae3d360214 · inbound

Updates on dipolar anisotropy in local measurements of the Hubble constant from Cosmicflows-4 cites this paper.

Updates on dipolar anisotropy in local measurements of the Hubble constant from Cosmicflows-4 Analyzing the Large-Scale Bulk Flow using CosmicFlows4: Increasing Tension with the Standard Cosmological Model

Reference 88

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verified exact
arxiv_id, observed 2026-05-17T02:51:27.870196Z

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Observation dd7a2a3a-c062-4cd1-b90f-a196ce6d6de3 · inbound

New constraints on cosmic anisotropy from galaxy clusters using an improved dipole fitting method cites this paper.

New constraints on cosmic anisotropy from galaxy clusters using an improved dipole fitting method Analyzing the Large-Scale Bulk Flow using CosmicFlows4: Increasing Tension with the Standard Cosmological Model

Reference 190

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verified exact
arxiv_id, observed 2026-05-16T02:27:10.797580Z

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No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

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Observation 1cd6f5be-a00e-4729-81ac-466ea6595254 · inbound

Probing cosmic anisotropy with galaxy clusters and supernovae cites this paper.

Probing cosmic anisotropy with galaxy clusters and supernovae Analyzing the Large-Scale Bulk Flow using CosmicFlows4: Increasing Tension with the Standard Cosmological Model

Reference 15

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verified exact
arxiv_id, observed 2026-05-10T22:00:49.691936Z

Source-reported events for the cited work

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Observation a9d0a753-718f-4b7a-b187-45a07f4a2827 · inbound

A First Observational Assessment of Cosmic Backreaction Over an Extended Redshift Range cites this paper.

A First Observational Assessment of Cosmic Backreaction Over an Extended Redshift Range Analyzing the Large-Scale Bulk Flow using CosmicFlows4: Increasing Tension with the Standard Cosmological Model

Reference 40

Resolution
unresolved
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Observation 1f369d15-fdf4-4e64-aa11-5d1c58c7ba16 · inbound

Expected redshift drift for tilted observers cites this paper.

Expected redshift drift for tilted observers Analyzing the Large-Scale Bulk Flow using CosmicFlows4: Increasing Tension with the Standard Cosmological Model

Reference 28

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verified exact
arxiv_id, observed 2026-05-20T20:49:00.971514Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

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Observation 27925008-a2eb-46dd-8790-8e57f2dc0488 · inbound

Expected redshift drift for tilted observers cites this paper.

Expected redshift drift for tilted observers Analyzing the Large-Scale Bulk Flow using CosmicFlows4: Increasing Tension with the Standard Cosmological Model

Reference 28

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unresolved
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Observation c9676063-3fe8-4cb4-958f-07d3212c202c · inbound

Multipolar structure of the local expansion rate from incomplete sky data cites this paper.

Multipolar structure of the local expansion rate from incomplete sky data Analyzing the Large-Scale Bulk Flow using CosmicFlows4: Increasing Tension with the Standard Cosmological Model

Reference 103

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Observation 86c40d14-1e5e-4e38-9a5b-7fcb487b42a4 · inbound

A low value of $H_0$ in tension with the distance ladder from Megamasers using peculiar velocity reconstruction cites this paper.

A low value of $H_0$ in tension with the distance ladder from Megamasers using peculiar velocity reconstruction Analyzing the Large-Scale Bulk Flow using CosmicFlows4: Increasing Tension with the Standard Cosmological Model

Reference 34

Resolution
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Observation d5e98d50-b208-42b0-8a20-5c9ede729ea5 · inbound

A low value of $H_0$ in tension with the distance ladder from Megamasers using peculiar velocity reconstruction cites this paper.

A low value of $H_0$ in tension with the distance ladder from Megamasers using peculiar velocity reconstruction Analyzing the Large-Scale Bulk Flow using CosmicFlows4: Increasing Tension with the Standard Cosmological Model

Reference 34

Resolution
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Observation 8cd21c38-1791-4b1d-b891-a0e06083d48d · inbound

A low value of $H_0$ in tension with the distance ladder from Megamasers using peculiar velocity reconstruction cites this paper.

A low value of $H_0$ in tension with the distance ladder from Megamasers using peculiar velocity reconstruction Analyzing the Large-Scale Bulk Flow using CosmicFlows4: Increasing Tension with the Standard Cosmological Model

Reference 34

Resolution
unresolved
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Observation f00aab1d-3a2d-4901-80dd-7dd0804d0c24 · inbound

Redshift Dependence of $H_0$ Dipole in Pantheon+ Supernovae cites this paper.

Redshift Dependence of $H_0$ Dipole in Pantheon+ Supernovae Analyzing the Large-Scale Bulk Flow using CosmicFlows4: Increasing Tension with the Standard Cosmological Model

Reference 47

Resolution
unresolved
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