activity
20062026
most citedRevising the Halofit Model for the Nonlinear Matter Power Spectrum

1.1k citations · 7k across the 146 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

8 papers · 1 filter

astro-ph.GA2023

Multi-stream radial structure of cold dark matter haloes from particle trajectories: deep inside splashback radius

Yohsuke Enomoto, Takahiro Nishimichi, Atsushi Taruya

By tracking trajectories of dark matter (DM) particles accreting onto haloes in cosmological -body simulations, we investigate the radial phase-space distribution of cold dark m…

astro-ph.GA2021★ 2 cited

Mock catalogues of emission line galaxies based on the local mass density in dark-matter only simulations

Ken Osato, Takahiro Nishimichi, Masahiro Takada

The high-precision measurement of spatial clustering of emission line galaxies (ELGs) is a primary objective for upcoming cosmological spectroscopic surveys. The source of strong e…

astro-ph.GA2020★ 28 cited

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.GA2019★ 15 cited

Semi-analytic modelling of AGNs: auto-correlation function and halo occupation

Taira Oogi, Hikari Shirakata, Masahiro Nagashima +5

The spatial clustering of active galactic nuclei (AGNs) is considered to be one of the important diagnostics for the understanding of the underlying processes behind their activiti…

astro-ph.GA2019★ 8 cited

New constraints on red-spiral galaxies from their kinematics in clusters of galaxies

Akinari Hamabata, Taira Oogi, Masamune Oguri +2

The distributions of the pairwise line-of-sight velocity between galaxies and their host clusters are segregated according to the galaxy's colour and morphology. We investigate the…

astro-ph.GA2018★ 12 cited

Constraining cluster masses from the stacked phase space distribution at large radii

Akinari Hamabata, Masamune Oguri, Takahiro Nishimichi

Velocity dispersions have been employed as a method to measure masses of clusters. To complement this conventional method, we explore the possibility of constraining cluster masses…