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Source: paper_references, paper_reference_links
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.
A citation records a reference. It does not transfer a finding from one paper to another.
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One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-09T06:31:02.800959+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-10T01:13:35.488687Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-07-03T07:47:45.341882Z
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0 of 0 outbound references displayed
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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 2026-08-09T06:31:02.800959+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
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Source-reported events for the cited work
Unavailable: canonical work link unavailable.
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
Unavailable: canonical work link unavailable.
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 2026-08-09T06:31:02.800959+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 2026-08-09T06:31:02.800959+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 2026-08-09T06:31:02.800959+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
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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 2026-08-09T06:31:02.800959+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 2026-08-09T06:31:02.800959+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 2026-08-09T06:31:02.800959+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 2026-08-09T06:31:02.800959+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.