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20142024
most citedWeighing the Giants IV: Cosmology and Neutrino Mass

306 citations · 1.2k across the 16 of their papers we have counts for

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16 papers · 1 filter

astro-ph.CO2024★ 17 cited

The SRG-eROSITA All-Sky Survey : Constraints on f(R) Gravity from Cluster Abundance

E. Artis, V. Ghirardini, E. Bulbul +28

The evolution of the cluster mass function traces the growth of the linear density perturbations and can be utilized for constraining the parameters of cosmological and alternative…

astro-ph.CO2022

On the road to percent accuracy: The Reaction Way

Matteo Cataneo

Taking advantage of the unprecedented statistical power of upcoming cosmic shear surveys will require exquisite knowledge of the matter power spectrum over a wide range of scales.…

astro-ph.CO2021★ 19 cited

The matter density PDF for modified gravity and dark energy with Large Deviations Theory

Matteo Cataneo, Cora Uhlemann, Christian Arnold +3

We present an analytical description of the probability distribution function (PDF) of the smoothed three-dimensional matter density field for modified gravity and dark energy. Our…

astro-ph.CO2021★ 43 cited

On the road to percent accuracy V: the non-linear power spectrum beyond CDM with massive neutrinos and baryonic feedback

Benjamin Bose, Bill S. Wright, Matteo Cataneo +7

In the context of forthcoming galaxy surveys, to ensure unbiased constraints on cosmology and gravity when using non-linear structure information, percent-level accuracy is require…

astro-ph.CO2020★ 134 cited

KiDS-1000 Cosmology: constraints beyond flat CDM

Tilman Tröster, Marika Asgari, Chris Blake +26

We present constraints on extensions to the flat CDM cosmological model by varying the spatial curvature , the sum of the neutrino masses , the dark energy equati…

astro-ph.CO2020★ 75 cited

On the road to percent accuracy IV: ReACT -- computing the non-linear power spectrum beyond CDM

Benjamin Bose, Matteo Cataneo, Tilman Tröster +3

To effectively exploit large-scale structure surveys, we depend on accurate and reliable predictions of non-linear cosmological structure formation. Tools for efficient and compreh…

astro-ph.CO2019

Hybrid : general, unified, non-linear matter power spectrum in redshift space

Benjamin Bose, Hans A. Winther, Alkistis Pourtsidou +4

Constraints on gravity and cosmology will greatly benefit from performing joint clustering and weak lensing analyses on large-scale structure data sets. Utilising non-linear inform…

astro-ph.CO2019★ 34 cited

On the road to percent accuracy III: non-linear reaction of the matter power spectrum to massive neutrinos

Matteo Cataneo, J. D. Emberson, Derek Inman +2

We analytically model the non-linear effects induced by massive neutrinos on the total matter power spectrum using the halo model reaction framework of Cataneo et al. 2019. In this…

astro-ph.CO2019★ 55 cited

On the road to percent accuracy II: calibration of the non-linear matter power spectrum for arbitrary cosmologies

Benjamin Giblin, Matteo Cataneo, Ben Moews +1

We introduce an emulator approach to predict the non-linear matter power spectrum for broad classes of beyond-CDM cosmologies, using only a suite of CDM -body simulations.…

astro-ph.CO2019★ 28 cited

Tests of Gravity with Galaxy Clusters

Matteo Cataneo, David Rapetti

Changes in the law of gravity have far-reaching implications for the formation and evolution of galaxy clusters, and appear as peculiar signatures in their mass-observable relation…

astro-ph.CO2018★ 122 cited

On the road to percent accuracy: nonlinear reaction of the matter power spectrum to dark energy and modified gravity

Matteo Cataneo, Lucas Lombriser, Catherine Heymans +4

We present a general method to compute the nonlinear matter power spectrum for dark energy and modified gravity scenarios with percent-level accuracy. By adopting the halo model an…

astro-ph.CO2017★ 19 cited

Cold dark energy constraints from the abundance of galaxy clusters

Caroline Heneka, David Rapetti, Matteo Cataneo +3

We constrain cold dark energy of negligible sound speed using galaxy cluster abundance observations. In contrast to standard quasi-homogeneous dark energy, negligible sound speed i…

astro-ph.CO2016★ 56 cited

Cluster abundance in chameleon gravity I: toward an accurate halo mass function prediction

Matteo Cataneo, David Rapetti, Lucas Lombriser +1

We refine the mass and environment dependent spherical collapse model of chameleon gravity by calibrating a phenomenological correction inspired by the parameterized post-Fr…

astro-ph.CO2016★ 40 cited

Efficient exploration of cosmology dependence in the EFT of LSS

Matteo Cataneo, Simon Foreman, Leonardo Senatore

The most effective use of data from current and upcoming large scale structure~(LSS) and CMB observations requires the ability to predict the clustering of LSS with very high preci…

astro-ph.CO2014★ 143 cited

New constraints on gravity from clusters of galaxies

Matteo Cataneo, David Rapetti, Fabian Schmidt +6

The abundance of massive galaxy clusters is a powerful probe of departures from General Relativity (GR) on cosmic scales. Despite current stringent constraints placed by stellar an…

astro-ph.CO2014★ 306 cited

Weighing the Giants IV: Cosmology and Neutrino Mass

Adam B. Mantz, Anja von der Linden, Steven W. Allen +14

We employ robust weak gravitational lensing measurements to improve cosmological constraints from measurements of the galaxy cluster mass function and its evolution, using X-ray se…