Paper Citation Record · LEDGER

Full-shape analysis with simulation-based priors: cosmological parameters and the structure growth anomaly

As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 31 inbound Pith citation observations for arXiv:2409.10609.

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pith.paper-citation-record.v1
2409.10609 v2

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Pith citing papers itemized under the disclosed page cap.

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Pith citing papers

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Atomic Dark Matter, Interacting Dark Radiation, and the Hubble Tension cites this paper.

Atomic Dark Matter, Interacting Dark Radiation, and the Hubble Tension Full-shape analysis with simulation-based priors: cosmological parameters and the structure growth anomaly

Reference 117

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The constraining power of the Marked Power Spectrum: an analytical study cites this paper.

The constraining power of the Marked Power Spectrum: an analytical study Full-shape analysis with simulation-based priors: cosmological parameters and the structure growth anomaly

Reference 79

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The Millennium and Astrid galaxies in effective field theory: comparison with galaxy-halo connection models at the field level cites this paper.

The Millennium and Astrid galaxies in effective field theory: comparison with galaxy-halo connection models at the field level Full-shape analysis with simulation-based priors: cosmological parameters and the structure growth anomaly

Reference 50

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Reducing nuisance prior sensitivity via non-linear reparameterization, with application to EFT analyses of large-scale structure cites this paper.

Reducing nuisance prior sensitivity via non-linear reparameterization, with application to EFT analyses of large-scale structure Full-shape analysis with simulation-based priors: cosmological parameters and the structure growth anomaly

Reference 33

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The ACCEL2 Project: Precision Measurements of EFT Parameters and BAO Peak Shifts for the Lyman-$\alpha$ Forest cites this paper.

The ACCEL2 Project: Precision Measurements of EFT Parameters and BAO Peak Shifts for the Lyman-$\alpha$ Forest Full-shape analysis with simulation-based priors: cosmological parameters and the structure growth anomaly

Reference 120

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Observation 32289116-1928-449f-8368-46dbfc9a574d · inbound

Lyman Alpha Forest - Halo Cross-Correlations in Effective Field Theory cites this paper.

Lyman Alpha Forest - Halo Cross-Correlations in Effective Field Theory Full-shape analysis with simulation-based priors: cosmological parameters and the structure growth anomaly

Reference 80

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Bounds on Velocity-Dependent Dark Matter-Baryon Scattering from Large-Scale Structure cites this paper.

Bounds on Velocity-Dependent Dark Matter-Baryon Scattering from Large-Scale Structure Full-shape analysis with simulation-based priors: cosmological parameters and the structure growth anomaly

Reference 69

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Challenging $\Lambda$CDM: 5$\sigma$ Evidence for a Dynamical Dark Energy Late-Time Transition cites this paper.

Challenging $\Lambda$CDM: 5$\sigma$ Evidence for a Dynamical Dark Energy Late-Time Transition Full-shape analysis with simulation-based priors: cosmological parameters and the structure growth anomaly

Reference 34

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High-redshift Millennium and Astrid galaxies in effective field theory at the field level cites this paper.

High-redshift Millennium and Astrid galaxies in effective field theory at the field level Full-shape analysis with simulation-based priors: cosmological parameters and the structure growth anomaly

Reference 103

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Observation e272b412-0da9-4f2f-9f1a-3f75578240cc · inbound

Modeling Galaxy Surveys with Hybrid SBI cites this paper.

Modeling Galaxy Surveys with Hybrid SBI Full-shape analysis with simulation-based priors: cosmological parameters and the structure growth anomaly

Reference 26

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Observation 7e63e80b-c6b4-4250-8c8b-6d7561b66e1d · inbound

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors cites this paper.

Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors Full-shape analysis with simulation-based priors: cosmological parameters and the structure growth anomaly

Reference 39

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Modeling the Cosmological Lyman-$\alpha$ Forest at the Field Level cites this paper.

Modeling the Cosmological Lyman-$\alpha$ Forest at the Field Level Full-shape analysis with simulation-based priors: cosmological parameters and the structure growth anomaly

Reference 95

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Equivalence of the field-level inference and conventional analyses on large scales cites this paper.

Equivalence of the field-level inference and conventional analyses on large scales Full-shape analysis with simulation-based priors: cosmological parameters and the structure growth anomaly

Reference 97

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One-Loop Galaxy Bispectrum: Consistent Theory, Efficient Analysis with COBRA, and Implications for Cosmological Parameters cites this paper.

One-Loop Galaxy Bispectrum: Consistent Theory, Efficient Analysis with COBRA, and Implications for Cosmological Parameters Full-shape analysis with simulation-based priors: cosmological parameters and the structure growth anomaly

Reference 74

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Observation 3cba21a2-04ac-40e6-9ca5-9b6bd1411ff6 · inbound

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 Full-shape analysis with simulation-based priors: cosmological parameters and the structure growth anomaly

Reference 139

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Reanalyzing DESI DR1: 4. Percent-Level Cosmological Constraints from Combined Probes and Robust Evidence for the Normal Neutrino Mass Hierarchy cites this paper.

Reanalyzing DESI DR1: 4. Percent-Level Cosmological Constraints from Combined Probes and Robust Evidence for the Normal Neutrino Mass Hierarchy Full-shape analysis with simulation-based priors: cosmological parameters and the structure growth anomaly

Reference 124

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Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors cites this paper.

Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors Full-shape analysis with simulation-based priors: cosmological parameters and the structure growth anomaly

Reference 45

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Observation 0f7db2bb-f916-41a0-abb2-b4c0647c80ad · inbound

Floquet Dissipative Phase Transitions cites this paper.

Floquet Dissipative Phase Transitions Full-shape analysis with simulation-based priors: cosmological parameters and the structure growth anomaly

Reference 77

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Informative Priors on Primordial Non-Gaussianity Bias $b_{\phi}$ From Galaxy Formation cites this paper.

Informative Priors on Primordial Non-Gaussianity Bias $b_{\phi}$ From Galaxy Formation Full-shape analysis with simulation-based priors: cosmological parameters and the structure growth anomaly

Reference 47

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Multi-tracers, multi-surveys: a joint Fisher analysis of DESI+PFS cites this paper.

Multi-tracers, multi-surveys: a joint Fisher analysis of DESI+PFS Full-shape analysis with simulation-based priors: cosmological parameters and the structure growth anomaly

Reference 28

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Observation fbb3fb49-8370-41ae-83b6-c01a6552e14c · inbound

Multi-tracers, multi-surveys: a joint Fisher analysis of DESI+PFS cites this paper.

Multi-tracers, multi-surveys: a joint Fisher analysis of DESI+PFS Full-shape analysis with simulation-based priors: cosmological parameters and the structure growth anomaly

Reference 28

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Testing Scale-Dependent Modified Gravity with DESI DR1 cites this paper.

Testing Scale-Dependent Modified Gravity with DESI DR1 Full-shape analysis with simulation-based priors: cosmological parameters and the structure growth anomaly

Reference 104

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Observation 378ee85f-d853-4955-9887-2363ea308dd7 · inbound

Lyman-Alpha Forest and its Cross-Correlation with High-Redshift Galaxies in Effective Field Theory at the Field Level cites this paper.

Lyman-Alpha Forest and its Cross-Correlation with High-Redshift Galaxies in Effective Field Theory at the Field Level Full-shape analysis with simulation-based priors: cosmological parameters and the structure growth anomaly

Reference 126

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Observation 9049dd36-a016-4e71-b859-a59f051afeae · inbound

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 Full-shape analysis with simulation-based priors: cosmological parameters and the structure growth anomaly

Reference 90

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Modeling survey-window and integral-constraint effects on PNG in the galaxy power spectrum with light-cone mocks cites this paper.

Modeling survey-window and integral-constraint effects on PNG in the galaxy power spectrum with light-cone mocks Full-shape analysis with simulation-based priors: cosmological parameters and the structure growth anomaly

Reference 52

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Galaxy Power Spectrum at Two-Loop Order: Implications for Weak Lensing Surveys and New Physics cites this paper.

Galaxy Power Spectrum at Two-Loop Order: Implications for Weak Lensing Surveys and New Physics Full-shape analysis with simulation-based priors: cosmological parameters and the structure growth anomaly

Reference 87

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Alleviating prior dependencies for DESI DR1 clustering fits through reparameterization cites this paper.

Alleviating prior dependencies for DESI DR1 clustering fits through reparameterization Full-shape analysis with simulation-based priors: cosmological parameters and the structure growth anomaly

Reference 90

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Alleviating prior dependencies for DESI DR1 clustering fits through reparameterization cites this paper.

Alleviating prior dependencies for DESI DR1 clustering fits through reparameterization Full-shape analysis with simulation-based priors: cosmological parameters and the structure growth anomaly

Reference 90

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Simulation-Based Priors for HI Bias from Halo Occupation Physics cites this paper.

Simulation-Based Priors for HI Bias from Halo Occupation Physics Full-shape analysis with simulation-based priors: cosmological parameters and the structure growth anomaly

Reference 27

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Searching for Folded Primordial Non-Gaussianity with Galaxy Surveys cites this paper.

Searching for Folded Primordial Non-Gaussianity with Galaxy Surveys Full-shape analysis with simulation-based priors: cosmological parameters and the structure growth anomaly

Reference 105

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GGI Lectures on Large-Scale Structure Perturbation Theory (Effective Field Theory) cites this paper.

GGI Lectures on Large-Scale Structure Perturbation Theory (Effective Field Theory) Full-shape analysis with simulation-based priors: cosmological parameters and the structure growth anomaly

Reference 58

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