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Paper Citation Record · LEDGER

HMcode-2020: Improved modelling of non-linear cosmological power spectra with baryonic feedback

As of 23 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 28 inbound Pith citation observations for arXiv:2009.01858.

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pith.paper-citation-record.v1
2009.01858 v2

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Pith citing papers itemized under the disclosed page cap.

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Pith citing papers

Observation 408ac96a-79fc-472b-ac0c-b2e40cfa9841 · inbound

Emulating Recombination with Neural Networks using Universal Differential Equations cites this paper.

Emulating Recombination with Neural Networks using Universal Differential Equations HMcode-2020: Improved modelling of non-linear cosmological power spectra with baryonic feedback

Reference 39

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Observation d7edc3d9-1eab-4811-a110-eeddfe4c516a · inbound

De-baryonifying halos via optimal transport cites this paper.

De-baryonifying halos via optimal transport HMcode-2020: Improved modelling of non-linear cosmological power spectra with baryonic feedback

Reference 21

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Observation 1ff2dd83-c497-48d1-8a01-7809323c7e54 · inbound

Pixelization effects in cosmic shear angular power spectra cites this paper.

Pixelization effects in cosmic shear angular power spectra HMcode-2020: Improved modelling of non-linear cosmological power spectra with baryonic feedback

Reference 40

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Observation 79e82145-9b2e-406d-943d-3583bb2f8d86 · inbound

Tuning the cosmic instrument: robust cosmology through combined probes cites this paper.

Tuning the cosmic instrument: robust cosmology through combined probes HMcode-2020: Improved modelling of non-linear cosmological power spectra with baryonic feedback

Reference 105

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Observation ac3ab785-1a4d-438b-b5f0-d88933990cc8 · inbound

Reconstructing the shape of the non-linear matter power spectrum using CMB lensing and cosmic shear cites this paper.

Reconstructing the shape of the non-linear matter power spectrum using CMB lensing and cosmic shear HMcode-2020: Improved modelling of non-linear cosmological power spectra with baryonic feedback

Reference 41

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Observation 9678466c-b8eb-4356-9a58-d466dee7f9bc · inbound

Weighing neutrinos with 21cm Intensity Mapping at the SKAO cites this paper.

Weighing neutrinos with 21cm Intensity Mapping at the SKAO HMcode-2020: Improved modelling of non-linear cosmological power spectra with baryonic feedback

Reference 55

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Observation 6367b2b0-6753-4069-99de-f4148bc51b8b · inbound

Late-time suppression of structure growth as a solution for the $S_8$ tension cites this paper.

Late-time suppression of structure growth as a solution for the $S_8$ tension HMcode-2020: Improved modelling of non-linear cosmological power spectra with baryonic feedback

Reference 31

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Observation 0e6061d8-b114-424b-8753-6d3f31f86a93 · inbound

A frequentist view on the two-body decaying dark matter model cites this paper.

A frequentist view on the two-body decaying dark matter model HMcode-2020: Improved modelling of non-linear cosmological power spectra with baryonic feedback

Reference 67

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Measurement of the Dispersion$\unicode{x2013}$Galaxy Cross-Power Spectrum with the Second CHIME/FRB Catalog cites this paper.

Measurement of the Dispersion$\unicode{x2013}$Galaxy Cross-Power Spectrum with the Second CHIME/FRB Catalog HMcode-2020: Improved modelling of non-linear cosmological power spectra with baryonic feedback

Reference 49

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Observation 89fbfd75-1dae-41f5-ba0e-ff8f9c1c41e5 · inbound

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

Bayesian and frequentist perspectives agree on dynamical dark energy HMcode-2020: Improved modelling of non-linear cosmological power spectra with baryonic feedback

Reference 43

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Observation 169e54b7-8fbd-46f6-a22f-35bad5fb3c51 · inbound

Cosmology from a joint analysis of second and third order shear statistics with Subaru Hyper Suprime-Cam Year 3 data cites this paper.

Cosmology from a joint analysis of second and third order shear statistics with Subaru Hyper Suprime-Cam Year 3 data HMcode-2020: Improved modelling of non-linear cosmological power spectra with baryonic feedback

Reference 63

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Observation 01ec59a3-f3f1-43b0-8a50-677cabb6431b · inbound

The simple way to measure evolving dark energy without prior-volume effects cites this paper.

The simple way to measure evolving dark energy without prior-volume effects HMcode-2020: Improved modelling of non-linear cosmological power spectra with baryonic feedback

Reference 60

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Observation 07f8cad5-e4a5-42fc-8173-026cdd89b087 · inbound

Non-linear infusion of intrinsic alignment and source clustering: impact on non-Gaussian cosmic shear statistics cites this paper.

Non-linear infusion of intrinsic alignment and source clustering: impact on non-Gaussian cosmic shear statistics HMcode-2020: Improved modelling of non-linear cosmological power spectra with baryonic feedback

Reference 102

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Unbiased analysis of primordial non-Gaussianity: the multipoles of the full relativistic power spectrum cites this paper.

Unbiased analysis of primordial non-Gaussianity: the multipoles of the full relativistic power spectrum HMcode-2020: Improved modelling of non-linear cosmological power spectra with baryonic feedback

Reference 82

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Observation 4f04fa9d-210b-4597-a0c9-5d395e8feb2b · inbound

Cosmological tensions in Proca-Nuevo theory cites this paper.

Cosmological tensions in Proca-Nuevo theory HMcode-2020: Improved modelling of non-linear cosmological power spectra with baryonic feedback

Reference 95

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Observation dbe17caa-0538-41f1-b0c2-061815c5c0c3 · inbound

Floquet Dissipative Phase Transitions cites this paper.

Floquet Dissipative Phase Transitions HMcode-2020: Improved modelling of non-linear cosmological power spectra with baryonic feedback

Reference 17

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Ultra-light axion constraints from Planck and ACT: the role of nonlinear modelling cites this paper.

Ultra-light axion constraints from Planck and ACT: the role of nonlinear modelling HMcode-2020: Improved modelling of non-linear cosmological power spectra with baryonic feedback

Reference 19

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(The) Wiggles going non-linear HMcode-2020: Improved modelling of non-linear cosmological power spectra with baryonic feedback

Reference 32

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(The) Wiggles going non-linear HMcode-2020: Improved modelling of non-linear cosmological power spectra with baryonic feedback

Reference 32

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The sound of dynamical dark energy and modified gravity cites this paper.

The sound of dynamical dark energy and modified gravity HMcode-2020: Improved modelling of non-linear cosmological power spectra with baryonic feedback

Reference 99

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CMB Constraints on Pre-Inflationary Axion Dark Matter Isocurvature cites this paper.

CMB Constraints on Pre-Inflationary Axion Dark Matter Isocurvature HMcode-2020: Improved modelling of non-linear cosmological power spectra with baryonic feedback

Reference 43

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Dark Matter with a Drag at Low Redshift cites this paper.

Dark Matter with a Drag at Low Redshift HMcode-2020: Improved modelling of non-linear cosmological power spectra with baryonic feedback

Reference 74

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The $H_0$ world cup. II. A comprehensive competition between proposed Hubble tension solutions cites this paper.

The $H_0$ world cup. II. A comprehensive competition between proposed Hubble tension solutions HMcode-2020: Improved modelling of non-linear cosmological power spectra with baryonic feedback

Reference 248

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CAMB v2: cosmological power spectra for high-precision surveys cites this paper.

CAMB v2: cosmological power spectra for high-precision surveys HMcode-2020: Improved modelling of non-linear cosmological power spectra with baryonic feedback

Reference 74

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Early- and late-time constraints on Wald-Gauss-Bonnet topological dark energy and implications for the $H_0$ and $S_8$ tensions cites this paper.

Early- and late-time constraints on Wald-Gauss-Bonnet topological dark energy and implications for the $H_0$ and $S_8$ tensions HMcode-2020: Improved modelling of non-linear cosmological power spectra with baryonic feedback

Reference 104

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Observation 8b9bc5e7-6760-4d58-bf9a-44f896b87dbe · inbound

Shear-kSZ: A New Estimator for the Matter-Electron Power Spectrum from kSZ Tomography and Weak Lensing cites this paper.

Shear-kSZ: A New Estimator for the Matter-Electron Power Spectrum from kSZ Tomography and Weak Lensing HMcode-2020: Improved modelling of non-linear cosmological power spectra with baryonic feedback

Reference 64

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Direct shear $\times$ kSZ correlation: controlling baryons without modeling galaxies cites this paper.

Direct shear $\times$ kSZ correlation: controlling baryons without modeling galaxies HMcode-2020: Improved modelling of non-linear cosmological power spectra with baryonic feedback

Reference 5

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KiDS-1000: Improved constraints on cosmology, intrinsic alignments and baryonic feedback from clipped cosmic shear cites this paper.

KiDS-1000: Improved constraints on cosmology, intrinsic alignments and baryonic feedback from clipped cosmic shear HMcode-2020: Improved modelling of non-linear cosmological power spectra with baryonic feedback

Reference 264

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