Paper Citation Record · LEDGER

Using The Baryonic Tully-Fisher Relation to Measure $H_o$

As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 10 inbound Pith citation observations for arXiv:2006.08615.

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

pith.paper-citation-record.v1
2006.08615 v2

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measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 10 of 10 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 10 of 10 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-16T10:37:59.496331Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-02T06:16:43.242069Z

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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 1917b64f-6d9d-44bf-a70d-851fa4bfe821 · inbound

$\Lambda_{\rm s}$CDM cosmology from a type-II minimally modified gravity cites this paper.

$\Lambda_{\rm s}$CDM cosmology from a type-II minimally modified gravity Using The Baryonic Tully-Fisher Relation to Measure $H_o$

Reference 33

Resolution: verified exact; arxiv_id, observed 2026-05-24T03:53:54.649914Z

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 2c51cdcb-1143-4e60-a9e3-8e7e06c0891f · inbound

Updated Constraints on Omnipotent Dark Energy: A Comprehensive Analysis with CMB and BAO Data cites this paper.

Updated Constraints on Omnipotent Dark Energy: A Comprehensive Analysis with CMB and BAO Data Using The Baryonic Tully-Fisher Relation to Measure $H_o$

Reference 33

Resolution: unresolved; no resolver link, observed 2026-08-16T10:37:59.496331Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9dd01e8a-c54f-4391-9d64-58ecdabb24ba · inbound

Dark Energy Crosses the Line: Quantifying and Testing the Evidence for Phantom Crossing cites this paper.

Dark Energy Crosses the Line: Quantifying and Testing the Evidence for Phantom Crossing Using The Baryonic Tully-Fisher Relation to Measure $H_o$

Reference 34

Resolution: unresolved; no resolver link, observed 2026-08-15T18:44:18.808184Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2431457b-da0a-434b-9db5-c075a4e20a8f · inbound

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

Two Dynamical Scenarios for Binned Master Sample Interpretation Using The Baryonic Tully-Fisher Relation to Measure $H_o$

Reference 30

Resolution: unresolved; no resolver link, observed 2026-08-06T16:16:23.256220Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 764c6fd1-b59d-408b-a2be-9dfaafd437f0 · inbound

Nonlinear Matter Power Spectrum from relativistic $N$-body Simulations: $\Lambda_{\rm s}$CDM versus $\Lambda$CDM cites this paper.

Nonlinear Matter Power Spectrum from relativistic $N$-body Simulations: $\Lambda_{\rm s}$CDM versus $\Lambda$CDM Using The Baryonic Tully-Fisher Relation to Measure $H_o$

Reference 32

Resolution: verified exact; arxiv_id, observed 2026-05-18T04:50:55.098596Z

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 33ca81e2-e407-49bd-aef7-92d98f1d1463 · inbound

Redshift Duality with Pantheon+SH0ES in a Planck-anchored Flat $\Lambda$CDM Framework: Implications for Hubble Tension and Observational Inference cites this paper.

Redshift Duality with Pantheon+SH0ES in a Planck-anchored Flat $\Lambda$CDM Framework: Implications for Hubble Tension and Observational Inference Using The Baryonic Tully-Fisher Relation to Measure $H_o$

Reference 86

Resolution: verified exact; arxiv_id, observed 2026-07-02T00:46:23.819571Z

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 0fd9ebe1-c9d9-4fa8-949d-810dcad96f9e · inbound

Cosmological Viability of Exponential Infrared $f(T)$ Gravity cites this paper.

Cosmological Viability of Exponential Infrared $f(T)$ Gravity Using The Baryonic Tully-Fisher Relation to Measure $H_o$

Reference 34

Resolution: verified exact; arxiv_id, observed 2026-07-01T11:15:42.642380Z

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 e543525a-b86e-4a1e-abcd-c1fd981eb7d2 · inbound

Intertwined Constraints in Extended Cosmologies: Dark Energy, Curvature, Neutrinos, and Inflation cites this paper.

Intertwined Constraints in Extended Cosmologies: Dark Energy, Curvature, Neutrinos, and Inflation Using The Baryonic Tully-Fisher Relation to Measure $H_o$

Reference 74

Resolution: verified exact; arxiv_id, observed 2026-07-02T06:16:43.243440Z

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 b3ff48c4-02e1-4cd1-80d6-e51d5d3164c1 · inbound

FAST Ultra-Deep Survey: the baryonic Tully-Fisher relation in FUDS0 field cites this paper.

FAST Ultra-Deep Survey: the baryonic Tully-Fisher relation in FUDS0 field Using The Baryonic Tully-Fisher Relation to Measure $H_o$

Reference 78

Resolution: unresolved; no resolver link, observed 2026-08-08T18:54:00.176399Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 02fda2dd-5b39-4203-b396-64218f6103b1 · inbound

Parameter-free prediction of the asymptotic acceleration scale confirmed by weak lensing cites this paper.

Parameter-free prediction of the asymptotic acceleration scale confirmed by weak lensing Using The Baryonic Tully-Fisher Relation to Measure $H_o$

Reference 25

Resolution: unresolved; no resolver link, observed 2026-08-10T14:51:04.158308Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.