Quijote-PNG: the information content of the halo power spectrum and bispectrum

WR Coulton, F Villaescusa-Navarro… - The Astrophysical …, 2023‏ - iopscience.iop.org
We investigate how much can be learnt about four types of primordial non-Gaussianity
(PNG) from small-scale measurements of the halo field. Using the quijote-png simulations …

Fisher for complements: extracting cosmology and neutrino mass from the counts-in-cells PDF

C Uhlemann, O Friedrich… - Monthly Notices of …, 2020‏ - academic.oup.com
We comprehensively analyse the cosmology dependence of counts-in-cells statistics. We
focus on the shape of the one-point probability distribution function (PDF) of the matter …

Galaxy power spectrum multipoles covariance in perturbation theory

D Wadekar, R Scoccimarro - Physical Review D, 2020‏ - APS
We compute the covariance of the galaxy power spectrum multipoles in perturbation theory,
including the effects of nonlinear evolution, nonlinear and nonlocal bias, radial redshift …

On the impact of galaxy bias uncertainties on primordial non-Gaussianity constraints

A Barreira - Journal of Cosmology and Astroparticle Physics, 2020‏ - iopscience.iop.org
We study the impact that uncertainties on assumed relations between galaxy bias
parameters have on constraints of the local PNG f NL parameter. We focus on the relation …

Comparing approximate methods for mock catalogues and covariance matrices–III: bispectrum

M Colavincenzo, E Sefusatti, P Monaco… - Monthly Notices of …, 2019‏ - academic.oup.com
We compare the measurements of the bispectrum and the estimate of its covariance
obtained from a set of different methods for the efficient generation of approximate dark …

Fitting the nonlinear matter bispectrum by the Halofit approach

R Takahashi, T Nishimichi, T Namikawa… - The Astrophysical …, 2020‏ - iopscience.iop.org
We provide a new fitting formula of the matter bispectrum in the nonlinear regime calibrated
by high-resolution cosmological N-body simulations of 41 cold dark matter (wCDM, w …

Perturbation theory approach to predict the covariance matrices of the galaxy power spectrum and bispectrum in redshift space

NS Sugiyama, S Saito, F Beutler… - Monthly Notices of the …, 2020‏ - academic.oup.com
In this paper, we predict the covariance matrices of both the power spectrum and the
bispectrum, including full non-Gaussian contributions, redshift space distortions, linear bias …

Stochastic gravitational wave background anisotropies in the mHz band: astrophysical dependencies

G Cusin, I Dvorkin, C Pitrou… - Monthly Notices of the …, 2020‏ - academic.oup.com
We show that the anisotropies of the astrophysical stochastic gravitational wave background
in the mHz band have a strong dependence on the modelling of galactic and sub-galactic …

Bispectrum non-Gaussian covariance in redshift space

J Salvalaggio, L Castiblanco, J Noreña… - … of Cosmology and …, 2024‏ - iopscience.iop.org
We provide an analytical description of the galaxy bispectrum covariance and the power
spectrum-bispectrum cross-covariance in redshift space that captures the dominant non …

The covariance of squeezed bispectrum configurations

M Biagetti, L Castiblanco, J Noreña… - Journal of Cosmology …, 2022‏ - iopscience.iop.org
We measure the halo bispectrum covariance in a large set of N-body simulations and
compare it with theoretical expectations. We find a large correlation among (even mildly) …