Paper Citation Record · LEDGER

Model-independent reconstruction of the Interacting Dark Energy Kernel: Binned and Gaussian process

As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 15 inbound Pith citation observations for arXiv:2305.16290.

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pith.paper-citation-record.v1
2305.16290 v2

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measured 0 of 0 reference resolution

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measured 15 of 15 standing notices

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Source: scholarly_work_events, retraction_status_cache, observed 2026-08-10T06:31:04.303077+00:00

measured 15 of 15 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-10T01:13:35.488687Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-03T07:47:45.341882Z

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Outbound references

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Pith citing papers

Observation e6b3e9a8-e25c-4519-a981-a6204ea08ee3 · 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-independent reconstruction of the Interacting Dark Energy Kernel: Binned and Gaussian process

Reference 139

Resolution: verified exact; arxiv_id, observed 2026-07-15T00:21:09.934933Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation d60c28ab-482b-4e9e-999d-eb478049b403 · inbound

Mapping the $\Lambda_{\rm s}$CDM scenario to $f(T)$ modified gravity: Effects on structure growth rate cites this paper.

Mapping the $\Lambda_{\rm s}$CDM scenario to $f(T)$ modified gravity: Effects on structure growth rate Model-independent reconstruction of the Interacting Dark Energy Kernel: Binned and Gaussian process

Reference 61

Resolution: unresolved; no resolver link, observed 2026-08-10T01:13:35.488687Z

Source-reported events for the cited work

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Observation 4f9885f5-1ee0-4798-ac0a-7fe5443befb2 · inbound

Is $\omega_0 \omega_a$CDM a good model for the clumpy Universe? cites this paper.

Is $\omega_0 \omega_a$CDM a good model for the clumpy Universe? Model-independent reconstruction of the Interacting Dark Energy Kernel: Binned and Gaussian process

Reference 26

Resolution: unresolved; no resolver link, observed 2026-08-06T21:15:08.998244Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f055fe54-65ea-42b9-9cfb-3aa5ca6080ac · inbound

How Holographic is the Dark Energy? A Spline Nodal reconstruction approach cites this paper.

How Holographic is the Dark Energy? A Spline Nodal reconstruction approach Model-independent reconstruction of the Interacting Dark Energy Kernel: Binned and Gaussian process

Reference 75

Resolution: unresolved; no resolver link, observed 2026-08-06T12:01:08.794353Z

Source-reported events for the cited work

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Observation 43769348-b821-4a3e-aded-9f6a779c848e · 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-independent reconstruction of the Interacting Dark Energy Kernel: Binned and Gaussian process

Reference 92

Resolution: verified exact; arxiv_id, observed 2026-07-15T00:21:09.934933Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation 1849e046-9818-43d4-ac2f-601d13bad90b · inbound

Robust Preference for Dark Sector Interactions cites this paper.

Robust Preference for Dark Sector Interactions Model-independent reconstruction of the Interacting Dark Energy Kernel: Binned and Gaussian process

Reference 82

Resolution: unresolved; no resolver link, observed 2026-08-03T11:11:48.832078Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation da54bdca-3577-42ce-b665-a4b3137b591e · inbound

Revisiting the Matter Creation Process: Observational Constraints on Gravitationally Induced Dark Energy and the Hubble Tension cites this paper.

Revisiting the Matter Creation Process: Observational Constraints on Gravitationally Induced Dark Energy and the Hubble Tension Model-independent reconstruction of the Interacting Dark Energy Kernel: Binned and Gaussian process

Reference 101

Resolution: verified exact; arxiv_id, observed 2026-07-15T00:21:09.934933Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation 53ec53bb-1c36-443f-a403-af846616004e · 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-independent reconstruction of the Interacting Dark Energy Kernel: Binned and Gaussian process

Reference 65

Resolution: verified exact; arxiv_id, observed 2026-07-15T00:21:09.934933Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation 195eca1e-13ab-44c2-8021-c1c6b5956814 · 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-independent reconstruction of the Interacting Dark Energy Kernel: Binned and Gaussian process

Reference 74

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 aea36a7a-af22-4ef5-9a05-d994440b71c7 · 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-independent reconstruction of the Interacting Dark Energy Kernel: Binned and Gaussian process

Reference 77

Resolution: verified exact; arxiv_id, observed 2026-07-15T00:21:09.934933Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation 453644de-8733-4547-a60d-3850db6415b6 · inbound

Latent-Space Gaussian Processes for Dark-Energy Reconstruction from Observational $H(z)$ Data cites this paper.

Latent-Space Gaussian Processes for Dark-Energy Reconstruction from Observational $H(z)$ Data Model-independent reconstruction of the Interacting Dark Energy Kernel: Binned and Gaussian process

Reference 19

Resolution: verified exact; arxiv_id, observed 2026-07-15T00:21:09.934933Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation 6cac990a-61d3-4dd6-bc56-aea5df58d440 · inbound

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

Negative neutrino mass or negative dark energy? Model-independent reconstruction of the Interacting Dark Energy Kernel: Binned and Gaussian process

Reference 58

Resolution: verified exact; arxiv_id, observed 2026-07-15T00:21:09.934933Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation 0fe65364-1570-4a8f-88d0-7e3827b28c68 · inbound

Non-linear Structure Formation in Planck+DESI Favoured Interacting Dark Energy Cosmologies cites this paper.

Non-linear Structure Formation in Planck+DESI Favoured Interacting Dark Energy Cosmologies Model-independent reconstruction of the Interacting Dark Energy Kernel: Binned and Gaussian process

Reference 62

Resolution: verified exact; arxiv_id, observed 2026-07-15T00:21:09.934933Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation 8c9c6fc7-3a60-499c-859c-581b6e1fa164 · 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-independent reconstruction of the Interacting Dark Energy Kernel: Binned and Gaussian process

Reference 161

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

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 13af9fc1-9c2d-4e8c-a445-296ca11fcfbf · inbound

Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide cites this paper.

Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide Model-independent reconstruction of the Interacting Dark Energy Kernel: Binned and Gaussian process

Reference 50

Resolution: unresolved; no resolver link, observed 2026-08-01T16:30:00.085425Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.