Paper Citation Record · LEDGER

Procoli: Profiles of cosmological likelihoods

As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 16 inbound Pith citation observations for arXiv:2401.14225.

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pith.paper-citation-record.v1
2401.14225 v1

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Pith citing papers itemized under the disclosed page cap.

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Pith citing papers

Observation 6f7262a2-ed37-4607-8efe-3941e7883924 · inbound

Constraints on Lorentz Invariance Violation from Gamma-ray Burst rest-frame spectral lags using Profile Likelihood cites this paper.

Constraints on Lorentz Invariance Violation from Gamma-ray Burst rest-frame spectral lags using Profile Likelihood Procoli: Profiles of cosmological likelihoods

Reference 10

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Primordial Sharp Features through the Nonlinear Regime of Structure Formation cites this paper.

Primordial Sharp Features through the Nonlinear Regime of Structure Formation Procoli: Profiles of cosmological likelihoods

Reference 188

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Bayesian and frequentist perspectives agree on dynamical dark energy cites this paper.

Bayesian and frequentist perspectives agree on dynamical dark energy Procoli: Profiles of cosmological likelihoods

Reference 22

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Debiasing inference in large-scale structure with non-flat volume measures cites this paper.

Debiasing inference in large-scale structure with non-flat volume measures Procoli: Profiles of cosmological likelihoods

Reference 71

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Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses cites this paper.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses Procoli: Profiles of cosmological likelihoods

Reference 148

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Observation 480fffe9-7aa2-4f15-ae11-11e8e198fa37 · inbound

Probing the sound speed and clustering of dark energy cites this paper.

Probing the sound speed and clustering of dark energy Procoli: Profiles of cosmological likelihoods

Reference 2024

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Neutrino mass limits and decaying dark matter: background evolution versus perturbations cites this paper.

Neutrino mass limits and decaying dark matter: background evolution versus perturbations Procoli: Profiles of cosmological likelihoods

Reference 64

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Observation 5772fda9-a36b-4ada-90f1-4bfb9f3681ec · inbound

Disentangling cosmic distance tensions with early and late dark energy cites this paper.

Disentangling cosmic distance tensions with early and late dark energy Procoli: Profiles of cosmological likelihoods

Reference 112

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Double the axions, half the tension: multi-field early dark energy eases the Hubble tension cites this paper.

Double the axions, half the tension: multi-field early dark energy eases the Hubble tension Procoli: Profiles of cosmological likelihoods

Reference 175

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Reionization History and Neutrino Mass cites this paper.

Reionization History and Neutrino Mass Procoli: Profiles of cosmological likelihoods

Reference 25

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Recoupled Dark Radiation reconciling CMB and DESI BAO measurements cites this paper.

Recoupled Dark Radiation reconciling CMB and DESI BAO measurements Procoli: Profiles of cosmological likelihoods

Reference 69

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First full-shape joint analysis of the two- and three-point correlation functions on real data: $\Lambda$CDM cosmological constraints from BOSS DR12 cites this paper.

First full-shape joint analysis of the two- and three-point correlation functions on real data: $\Lambda$CDM cosmological constraints from BOSS DR12 Procoli: Profiles of cosmological likelihoods

Reference 252

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Dark energy perturbations and the robustness of cosmological neutrino-mass constraints cites this paper.

Dark energy perturbations and the robustness of cosmological neutrino-mass constraints Procoli: Profiles of cosmological likelihoods

Reference 52

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Dark energy perturbations and the robustness of cosmological neutrino-mass constraints cites this paper.

Dark energy perturbations and the robustness of cosmological neutrino-mass constraints Procoli: Profiles of cosmological likelihoods

Reference 52

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Observation 7275efe7-9997-41fa-895c-5597b3b83407 · inbound

Determination of neutron star radius from pulse profile modeling using profile likelihood cites this paper.

Determination of neutron star radius from pulse profile modeling using profile likelihood Procoli: Profiles of cosmological likelihoods

Reference 20

Resolution: unresolved; no resolver link, observed 2026-07-14T06:38:48.754265Z

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The $H_0$ World Cup. I. Summary of the baseline group stage results cites this paper.

The $H_0$ World Cup. I. Summary of the baseline group stage results Procoli: Profiles of cosmological likelihoods

Reference 139

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