no code implementations • 1 Sep 2020 • Jingjing Shi, Toshiki Kurita, Masahiro Takada, Ken Osato, Yosuke Kobayashi, Takahiro Nishimichi
The shape of massive disk- and spheroid-galaxies tend to align with the tidal field.
Astrophysics of Galaxies Cosmology and Nongalactic Astrophysics
no code implementations • 17 Jul 2020 • Shogo Masaki, Takahiro Nishimichi, Masahiro Takada
To generate initial conditions for cosmological $N$-body simulations, one needs to prepare a uniform distribution of simulation particles, so-called the pre-initial condition (pre-IC).
Cosmology and Nongalactic Astrophysics
1 code implementation • 18 Mar 2020 • Takahiro Nishimichi, Guido D'Amico, Mikhail M. Ivanov, Leonardo Senatore, Marko Simonović, Masahiro Takada, Matias Zaldarriaga, Pierre Zhang
An accurate theoretical template for the galaxy power spectrum is a key for the success of ongoing and future spectroscopic surveys.
Cosmology and Nongalactic Astrophysics
no code implementations • 28 Nov 2019 • Masato Shirasaki, Kana Moriwaki, Taira Oogi, Naoki Yoshida, Shiro Ikeda, Takahiro Nishimichi
We study the non-Gaussian information in denoised maps using one-point probability distribution functions (PDFs) and also perform matching analysis for positive peaks and massive clusters.
1 code implementation • 23 Oct 2018 • Ken Osato, Takahiro Nishimichi, Francis Bernardeau, Atsushi Taruya
We study the accuracy with which cosmological parameters can be determined from real space power spectrum of matter density contrast at weakly nonlinear scales using analytical approaches.
Cosmology and Nongalactic Astrophysics
2 code implementations • 5 Jun 2017 • Ryuichi Takahashi, Takashi Hamana, Masato Shirasaki, Toshiya Namikawa, Takahiro Nishimichi, Ken Osato, Kosei Shiroyama
The data sets include full-sky convergence and shear maps from redshifts $z=0. 05$ to $5. 3$ at intervals of $150 \, h^{-1}{\rm Mpc}$ comoving radial distance (corresponding to a redshift interval of $\Delta z \simeq 0. 05$ at the nearby universe), enabling the construction of a mock shear catalog for an arbitrary source distribution up to $z=5. 3$.
Cosmology and Nongalactic Astrophysics General Relativity and Quantum Cosmology
1 code implementation • 13 Aug 2012 • Ryuichi Takahashi, Masanori Sato, Takahiro Nishimichi, Atsushi Taruya, Masamune Oguri
The simulation results are used to re-calibrate the fitting parameters of the halofit model so as to reproduce small-scale power spectra of the $N$-body simulations, while keeping the precision at large scales.
Cosmology and Nongalactic Astrophysics General Relativity and Quantum Cosmology
1 code implementation • 6 Aug 2012 • Atsushi Taruya, Francis Bernardeau, Takahiro Nishimichi, Sandrine Codis
The fortran program with which direct and fast calculations of power spectra can be done, RegPT, is publicly released as part of this paper.
Cosmology and Nongalactic Astrophysics General Relativity and Quantum Cosmology