activity
20072023
most citedThe Subaru FMOS galaxy redshift survey (FastSound). IV. New constraint on gravity theory from redshift space distortions at

249 citations · 2k across the 59 of their papers we have counts for

collaborators

60 papers

astro-ph.CO2023★ 8 cited

Nonlinear redshift space distortion in halo ellipticity correlations: Analytical model and N-body simulations

Teppei Okumura, Atsushi Taruya, Toshiki Kurita +1

We present an analytic model of nonlinear correlators of galaxy/halo ellipticities in redshift space. The three-dimensional ellipticity field is not affected by the redshift-space…

astro-ph.CO2023

Mock Observatory: two thousand lightcone mock catalogues of luminous red galaxies from the Hyper Suprime-Cam Survey for the cosmological large-scale analysis

Shogo Ishikawa, Teppei Okumura, Takahiro Nishimichi

Estimating a reliable covariance matrix for correlation functions of galaxies is a crucial task to obtain accurate cosmological constraints from galaxy surveys. We generate 2,000 i…

astro-ph.GA2023

Galaxy-dark matter connection of photometric galaxies from the HSC-SSP Survey: Galaxy-galaxy lensing and the halo model

Navin Chaurasiya, Surhud More, Shogo Ishikawa +3

We infer the connection between the stellar mass of galaxies from the Subaru Hyper Suprime-Cam (HSC) survey, and their dark matter halo masses and its evolution in two bins of reds…

astro-ph.CO2023★ 20 cited

Quadratic shape biases in three-dimensional halo intrinsic alignments

Kazuyuki Akitsu, Yin Li, Teppei Okumura

Understanding the nonlinear relation between the shapes of halos or galaxies and the surrounding matter distribution is essential in accurate modeling of their intrinsic alignments…

astro-ph.CO2023★ 12 cited

Statistical anisotropy in galaxy ellipticity correlations

Maresuke Shiraishi, Teppei Okumura, Kazuyuki Akitsu

As well as the galaxy number density and peculiar velocity, the galaxy intrinsic alignment can be used to test the cosmic isotropy. We study distinctive impacts of the isotropy bre…

astro-ph.CO2023★ 29 cited

First Constraints on Growth Rate from Redshift-Space Ellipticity Correlations of SDSS Galaxies at

Teppei Okumura, Atsushi Taruya

We report the first constraints on the growth rate of the universe, , with intrinsic alignments (IAs) of galaxies. We measure the galaxy density-intrinsic ellipticity c…

astro-ph.CO2022★ 2 cited

Cosmological gravity probes: connecting recent theoretical developments to forthcoming observations

Shun Arai, Katsuki Aoki, Yuji Chinone +20

Since the discovery of the accelerated expansion of the present Universe, significant theoretical developments have been made in the area of modified gravity. In the meantime, cosm…

astro-ph.CO2022★ 21 cited

Gravitational wave fossils in nonlinear regime: halo tidal bias and intrinsic alignments from gravitational wave separate universe simulations

Kazuyuki Akitsu, Yin Li, Teppei Okumura

We investigate impacts of long-wavelength gravitational waves (GWs) on nonlinear structure formation by utilizing the tidal separate universe simulations. Based on the equivalence…

astro-ph.CO2022★ 9 cited

Relativistic distortions in galaxy density-ellipticity correlations: gravitational redshift and peculiar velocity effects

Shohei Saga, Teppei Okumura, Atsushi Taruya +1

We study relativistic effects, arising from the light propagation in an inhomogeneous universe. We particularly investigate the effects imprinted in a cross-correlation function be…

astro-ph.GA2022★ 7 cited

Clustering of emission line galaxies with IllustrisTNG I.: fundamental properties and halo occupation distribution

Ken Osato, Teppei Okumura

Upcoming spectroscopic redshift surveys use emission line galaxies (ELGs) to trace the three-dimensional matter distributions with wider area coverage in the deeper Universe. Since…

astro-ph.CO2021★ 15 cited

Distinguishing between CDM and gravity models using halo ellipticity correlations in simulations

Yao-Tsung Chuang, Teppei Okumura, Masato Shirasaki

There is a growing interest in utilizing intrinsic alignment (IA) of galaxy shapes as a geometric and dynamical probe of cosmology. In this paper we present the first measurements…

astro-ph.CO2021★ 34 cited

Tightening geometric and dynamical constraints on dark energy and gravity: galaxy clustering, intrinsic alignment and kinetic Sunyaev-Zel'dovich effect

Teppei Okumura, Atsushi Taruya

Conventionally, in galaxy surveys, cosmological constraints on the growth and expansion history of the universe have been obtained from the measurements of redshift-space distortio…

astro-ph.CO2021★ 19 cited

First Evidence of Intrinsic Alignments of Red Galaxies at : Cross-correlation between CFHTLenS and FastSound Samples

Motonari Tonegawa, Teppei Okumura

We report the first evidence for intrinsic alignment (IA) of red galaxies at . We measure the gravitational shear-intrinsic ellipticity (GI) cross-correlation function at $z\s…

astro-ph.GA2021★ 17 cited

Halo-model analysis of the clustering of photometric luminous red galaxies at from the Subaru Hyper Suprime-Cam Survey

Shogo Ishikawa, Teppei Okumura, Masamune Oguri +1

We present the clustering analysis of photometric luminous red galaxies (LRGs) at a redshift range of using photometric LRGs selected from the Hyper…

astro-ph.CO2021★ 6 cited

Alcock-Paczynski effects on wide-angle galaxy statistics

Maresuke Shiraishi, Kazuyuki Akitsu, Teppei Okumura

The Alcock-Paczynski (AP) effect is a geometrical distortion in three-dimensional observed galaxy statistics. In anticipation of precision cosmology based on ongoing and upcoming a…

astro-ph.CO2020★ 12 cited

Wide-angle effects on galaxy ellipticity correlations

Maresuke Shiraishi, Atsushi Taruya, Teppei Okumura +1

We show an efficient way to compute wide-angle or all-sky statistics of galaxy intrinsic alignment in three-dimensional configuration space. For this purpose, we expand the two-poi…

astro-ph.GA2020★ 16 cited

Angular clustering and host halo properties of [OII] emitters at in the Subaru HSC survey

Teppei Okumura, Masao Hayashi, I-Non Chiu +4

We study the angular correlation function of star-forming galaxies and properties of their host dark matter halos at z>1 using the Hyper-Suprime Cam (HSC) SSP survey. We use [OII]…

astro-ph.CO2020★ 32 cited

Cosmological simulation in tides: power spectra and halo shape responses, and shape assembly bias

Kazuyuki Akitsu, Yin Li, Teppei Okumura

The well-developed separate universe technique enables accurate calibration of the response of any observable to an isotropic long-wavelength density fluctuation. The large-scale e…

astro-ph.CO2020★ 6 cited

Minimum variance estimation of statistical anisotropy via galaxy survey

Maresuke Shiraishi, Teppei Okumura, Kazuyuki Akitsu

We consider the benefits of measuring cosmic statistical anisotropy from redshift-space correlators of the galaxy number density fluctuation and the peculiar velocity field without…

astro-ph.CO2020★ 1 cited

Standard candles and sirens rescue

Aniket Agrawal, Teppei Okumura, Toshifumi Futamase

We show that future observations of binary neutron star systems with electromagnetic counterparts together with the traditional probes of low- and high-redshift Type Ia supernovae…

astro-ph.CO2020★ 4 cited

New measures to test modified gravity cosmologies

Jiro Matsumoto, Teppei Okumura, Misao Sasaki

The observed accelerated expansion of the Universe may be explained by dark energy or the breakdown of general relativity (GR) on cosmological scales. When the latter case, a modif…

astro-ph.CO2020★ 21 cited

A clustering-based self-calibration of the richness-to-mass relation of CAMIRA galaxy clusters out to in the Hyper Suprime-Cam survey

I-Non Chiu, Teppei Okumura, Masamune Oguri +3

We perform a self-calibration of the richness-to-mass (-) relation of CAMIRA galaxy clusters with richness at redshift by modeling redshift-space tw…

astro-ph.CO2020★ 8 cited

Minimum variance estimation of galaxy power spectrum in redshift space

Maresuke Shiraishi, Teppei Okumura, Naonori S. Sugiyama +1

We study an efficient way to enhance the measurability of the galaxy density and/or velocity power spectrum in redshift space. It is based on the angular decomposition with the Tri…

astro-ph.CO2020★ 29 cited

Testing tidal alignment models for anisotropic correlations of halo ellipticities with N-body simulations

Teppei Okumura, Atsushi Taruya, Takahiro Nishimichi

There is a growing interest of using the intrinsic alignment (IA) of galaxy images as a tool to extract cosmological information complimentary to galaxy clustering analysis. Recent…