activity
20182020
collaborators

8 papers

astro-ph.GA2020

Power Spectrum of Intrinsic Alignments of Galaxies in IllustrisTNG

Jingjing Shi, Toshiki Kurita, Masahiro Takada +3

We present the 3-{\it dimensional} intrinsic alignment power spectra between the projected 2d galaxy shape/spin and the 3d tidal field across using cosmo…

astro-ph.CO2020

Validating a minimal galaxy bias method for cosmological parameter inference using HSC-SDSS mock catalogs

Sunao Sugiyama, Masahiro Takada, Yosuke Kobayashi +4

We assess the performance of a perturbation theory inspired method for inferring cosmological parameters from the joint measurements of galaxy-galaxy weak lensing () and the pr…

astro-ph.CO2020

Accurate emulator for the redshift-space power spectrum of dark matter halos and its application to galaxy power spectrum

Yosuke Kobayashi, Takahiro Nishimichi, Masahiro Takada +2

An accurate theoretical template of the redshift-space galaxy power spectrum, if applicable out to nonlinear scales, enables us to extract more stringent and robust constraints on…

astro-ph.CO2020

Power spectrum of halo intrinsic alignments in simulations

Toshiki Kurita, Masahiro Takada, Takahiro Nishimichi +3

We use a suite of -body simulations to study intrinsic alignments (IA) of halo shapes with the surrounding large-scale structure in the CDM model. For this purpose, we develo…

astro-ph.CO2020

The impact of projection effects on cluster observables: stacked lensing and projected clustering

Tomomi Sunayama, Youngsoo Park, Masahiro Takada +6

An optical cluster finder inevitably suffers from projection effects, where it misidentifies a superposition of galaxies in multiple halos along the line-of-sight as a single clust…

astro-ph.CO2019

Fitting the nonlinear matter bispectrum by the Halofit approach

Ryuichi Takahashi, Takahiro Nishimichi, Toshiya Namikawa +5

We provide a new fitting formula of the matter bispectrum in the nonlinear regime calibrated by high-resolution cosmological -body simulations of cold dark matter (CDM,…