activity
20172026
most citedLuminous Quasars Do Not Live in the Most Overdense Regions of Galaxies at z~4

68 citations · 87 across the 20 of their papers we have counts for

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Showing astro-ph.COShow all

16 papers · 1 filter

astro-ph.CO2026

Limited Impact of CMB B-mode Polarization on Constraints on Cosmic Topology

Ryota Himeno, Atsushi J. Nishizawa, Kiyotomo Ichiki

The global spatial structure of the universe is a fundamental question in cosmology. Although the standard model usually assumes a trivial topology, a multiply connected universe c…

astro-ph.CO2026

Weak-lensing Shear-Selected Galaxy Clusters from the Hyper Suprime-Cam Subaru Strategic Program: III. A precision cosmological sample enabled by optical confirmation

I-Non Chiu, Kai-Feng Chen, Masamune Oguri +9

We develop fCAMIRA (forced-mode CAMIRA), a tool for optical cluster confirmation, and apply it to a sample of 129 weak-lensing (WL) shear-selected galaxy clusters identified in ape…

astro-ph.CO2026

Standard Reconstruction Shifts the Optimal Input Scale for CNN-Based Density-Field Reconstruction

Koichiro Nakashima, Kiyotomo Ichiki, Atsushi J. Nishizawa

We investigate convolutional neural network (CNN) methods for reconstructing the high-redshift density field from late-time large-scale structure, focusing on how the physical scal…

astro-ph.CO2025

Catalogs of optically-selected clusters and photometric luminous red galaxies from the Hyper Suprime-Cam Subaru Strategic Program final year dataset

Masamune Oguri, Yen-Ting Lin, Nobuhiro Okabe +9

We construct samples of optically-selected clusters and photometric luminous red galaxies (LRGs) from the Hyper Suprime-Cam Subaru Strategic Program final year dataset covering $\s…

astro-ph.CO2025★ 2 cited

Sensitivity toward dark matter annihilation imprints on 21-cm signal with SKA-Low: A convolutional neural network approach

Pravin Kumar Natwariya, Kenji Kadota, Atsushi J. Nishizawa

This study investigates the sensitivity of the radio interferometers to identify imprints of spatially inhomogeneous dark matter annihilation signatures in the 21-cm signal during…

astro-ph.CO2025

Cosmology and Source Redshift Constraints from Galaxy Clustering and Tomographic Weak Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model

Tianqing Zhang, Xiangchong Li, Sunao Sugiyama +13

The combination of galaxy clustering and weak lensing is a powerful probe of the cosmology model. We present a joint analysis of galaxy clustering and weak lensing cosmology using…

astro-ph.CO2025

Modelling Galaxy Clustering and Tomographic Galaxy-Galaxy Lensing with HSC Y3 and SDSS using the Point-Mass Correction Model and Redshift Self-Calibration

Tianqing Zhang, Sunao Sugiyama, Surhud More +13

The combination of galaxy-galaxy weak lensing and galaxy clustering is a powerful probe of the cosmological model, and exploration of how to best model and extract this information…

astro-ph.CO2025

Searching optimal scales for reconstructing cosmological initial conditions using convolutional neural networks

Koichiro Nakashima, Kiyotomo Ichiki, Atsushi J. Nishizawa +1

Reconstructing the initial density field of the Universe from the late-time matter distribution is a nontrivial task with implications for understanding structure formation in cosm…

astro-ph.CO2025

CMB lensing tomography with clustering estimation of lens redshift distributions

Shun Arai, John A. Peacock, Hironao Miyatake +1

We develop a clustering-based redshift estimation approach for CMB lensing tomography, focusing on the kernel function of the lensing galaxies. Within a linear galaxy bias framewor…

astro-ph.CO2024

Lyman- forest power spectrum and its cross-correlation with dark matter halos in different astrophysical models

Koichiro Nakashima, Atsushi J. Nishizawa, Kentaro Nagamine +2

The Ly forest, a series of HI absorption lines in the quasar spectra, is a powerful tool for probing the large-scale structure of the intergalactic medium. Its three-dimensional…

astro-ph.CO2024

Machine Learning Constraints on Dark Matter Annihilation during the Epoch of Reionization: A CNN Analysis of the 21-cm Signal

Atsushi J. Nishizawa, Pravin Kumar Natwariya, Kenji Kadota

We explore the impact of dark matter annihilation on the 21-cm signal during the cosmic dawn and epoch of reionization (EoR). Using modified 21cmFAST simulations and convolutional…

astro-ph.CO2024★ 4 cited

Exploring the baryonic effect signature in the Hyper Suprime-Cam Year 3 cosmic shear two-point correlations on small scales: the tension remains present

Ryo Terasawa, Xiangchong Li, Masahiro Takada +10

The baryonic feedback effect is considered as a possible solution to the so-called tension indicated in cosmic shear cosmology. The baryonic effect is more significant on sma…

astro-ph.CO2024★ 3 cited

Differentiating Warm Dark Matter Models through 21cm Line Intensity Mapping: A Convolutional Neural Network Approach

Koya Murakami, Kenji Kadota, Atsushi J. Nishizawa +2

We apply the convolutional neural networks (CNNs) to the mock 21cm maps from the post-reionization epoch to show that the cold dark matter and warm dark matter (WDM) model can…

astro-ph.CO2024

A Systematic Search of Distant Superclusters with the Subaru Hyper Suprime-Cam Survey

Tsung-Chi Chen, Yen-Ting Lin, Hsi-Yu Schive +13

Superclusters, encompassing environments across a wide range of overdensities, can be regarded as unique laboratories for studying galaxy evolution. Although numerous supercluster…

astro-ph.CO2023★ 3 cited

Optical Cluster Cosmology with SDSS redMaPPer clusters and HSC-Y3 lensing measurements

Tomomi Sunayama, Hironao Miyatake, Sunao Sugiyama +9

We present cosmology results obtained from a blind joint analysis of the abundance, projected clustering, and weak lensing of galaxy clusters measured from the Sloan Digital Sky Su…

astro-ph.CO2021★ 6 cited

Cosmological inference from the emulator based halo model II: Joint analysis of galaxy-galaxy weak lensing and galaxy clustering from HSC-Y1 and SDSS

Hironao Miyatake, Sunao Sugiyama, Masahiro Takada +25

We present high-fidelity cosmology results from a blinded joint analysis of galaxy-galaxy weak lensing () and projected galaxy clustering () measured from the Hype…