Paper Citation Record · LEDGER

Late-transition vs smooth $H(z)$ deformation models for the resolution of the Hubble crisis

As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 7 inbound Pith citation observations for arXiv:2110.04336.

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

pith.paper-citation-record.v1
2110.04336 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 7 of 7 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-08T06:32:00.761636+00:00

measured 7 of 7 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T18:51:43.952813Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-02T15:37:06.228173Z

Reference resolution

0 of 0 outbound references displayed

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External citation measurements

No source-named external measurement is stored.

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 521633a2-b006-474c-b98d-3e21ed476805 · inbound

Model-independent calibration of Gamma-Ray Bursts with neural networks cites this paper.

Model-independent calibration of Gamma-Ray Bursts with neural networks Late-transition vs smooth $H(z)$ deformation models for the resolution of the Hubble crisis

Reference 84

Resolution: verified exact; arxiv_id, observed 2026-05-23T17:55:44.535257Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation f9c3d969-e200-48f0-82ec-a49c961d4366 · inbound

An overview of what current data can (and cannot yet) say about evolving dark energy cites this paper.

An overview of what current data can (and cannot yet) say about evolving dark energy Late-transition vs smooth $H(z)$ deformation models for the resolution of the Hubble crisis

Reference 184

Resolution: unresolved; no resolver link, observed 2026-08-07T18:51:43.952813Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4e49b160-230e-42a2-9866-e7658c740c44 · inbound

Exploring the interplay of late-time dynamical dark energy and new physics before recombination cites this paper.

Exploring the interplay of late-time dynamical dark energy and new physics before recombination Late-transition vs smooth $H(z)$ deformation models for the resolution of the Hubble crisis

Reference 106

Resolution: verified exact; arxiv_id, observed 2026-05-14T23:13:15.261267Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation ad7d7bcd-4165-4f8f-b19a-5f36950cdf5d · inbound

Impact of the SNe Ia Magnitude Transition at 20 Mpc on Cosmological Parameter Estimation cites this paper.

Impact of the SNe Ia Magnitude Transition at 20 Mpc on Cosmological Parameter Estimation Late-transition vs smooth $H(z)$ deformation models for the resolution of the Hubble crisis

Reference 58

Resolution: metadata mismatch; arxiv_id, observed 2026-05-10T14:40:32.811542Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation 836bfdf6-952b-460a-a882-5bf56584291b · inbound

What it takes to solve the Hubble tension through Modifications of Cosmological Recombination II: in light of ACT DR6 and DESI DR2 cites this paper.

What it takes to solve the Hubble tension through Modifications of Cosmological Recombination II: in light of ACT DR6 and DESI DR2 Late-transition vs smooth $H(z)$ deformation models for the resolution of the Hubble crisis

Reference 49

Resolution: verified exact; arxiv_id, observed 2026-07-02T15:37:06.229837Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation 64b3ef4f-2914-41bd-a15a-b46216a59865 · inbound

Hubble tension: a short review of theoretical explanations cites this paper.

Hubble tension: a short review of theoretical explanations Late-transition vs smooth $H(z)$ deformation models for the resolution of the Hubble crisis

Reference 221

Resolution: unresolved; no resolver link, observed 2026-08-01T07:20:08.206032Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3d411708-e19a-4a63-8dfb-25a8820a0efd · inbound

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? cites this paper.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Late-transition vs smooth $H(z)$ deformation models for the resolution of the Hubble crisis

Reference 95

Resolution: unresolved; no resolver link, observed 2026-08-06T00:32:11.878877Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.