Paper Citation Record · LEDGER

Model selection applied to reconstructions of the Dark Energy

As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 8 inbound Pith citation observations for arXiv:2111.10457.

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

pith.paper-citation-record.v1
2111.10457 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 8 of 8 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-15T06:32:42.880941+00:00

measured 8 of 8 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-12T04:57:06.721713Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-24T03:53:54.611781Z

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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 bdc00f85-3dc9-464c-a363-2f24e45dcb96 · 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 Model selection applied to reconstructions of the Dark Energy

Reference 110

Resolution: verified exact; arxiv_id, observed 2026-05-24T03:53:54.618402Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation e8f2b35f-1cae-41a3-ae87-5f3149e8ce37 · inbound

Exploring cosmological imprints of phantom crossing with dynamical dark energy in Horndeski gravity cites this paper.

Exploring cosmological imprints of phantom crossing with dynamical dark energy in Horndeski gravity Model selection applied to reconstructions of the Dark Energy

Reference 22

Resolution: unresolved; no resolver link, observed 2026-08-12T04:57:06.721713Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a06f799c-8c07-4813-84dc-776de9194ee1 · 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 Model selection applied to reconstructions of the Dark Energy

Reference 169

Resolution: verified exact; arxiv_id, observed 2026-05-18T04:50:55.218038Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation 60620c7d-0f81-414c-9fa6-6edc5e7fe57f · inbound

Probing dynamical dark energy with late-time data: Evidence, tensions, and the limits of the $w_0w_a$CDM framework cites this paper.

Probing dynamical dark energy with late-time data: Evidence, tensions, and the limits of the $w_0w_a$CDM framework Model selection applied to reconstructions of the Dark Energy

Reference 121

Resolution: verified exact; arxiv_id, observed 2026-05-21T13:30:11.921589Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation dbdac468-fa3b-474f-8fbe-f537e39d29d6 · inbound

Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families cites this paper.

Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families Model selection applied to reconstructions of the Dark Energy

Reference 132

Resolution: unresolved; no resolver link, observed 2026-07-15T12:01:04.317365Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7c498a10-7a05-480b-abf6-6634fba74996 · inbound

Do equation of state parametrizations of dark energy faithfully capture the dynamics of the late universe? cites this paper.

Do equation of state parametrizations of dark energy faithfully capture the dynamics of the late universe? Model selection applied to reconstructions of the Dark Energy

Reference 75

Resolution: verified exact; arxiv_id, observed 2026-05-10T14:20:31.184213Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation 57552f48-d95e-4b67-8375-2bdcfabea017 · inbound

Negative neutrino mass or negative dark energy? cites this paper.

Negative neutrino mass or negative dark energy? Model selection applied to reconstructions of the Dark Energy

Reference 57

Resolution: verified exact; arxiv_id, observed 2026-05-21T03:03:55.613360Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation 58c487d3-690f-42f5-8408-84a6e1e91c4d · inbound

Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus cites this paper.

Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus Model selection applied to reconstructions of the Dark Energy

Reference 110

Resolution: unresolved; no resolver link, observed 2026-07-11T09:40:49.196932Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.