Naoki Yoshida

Professor

University of Tokyo

Japan

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About

Naoki Yoshida is a Professor at the University of Tokyo, Japan. His research focuses on cosmology and astrophysics, particularly examining the behavior of dark matter, stellar evolution, and the formation of galaxies in the early universe. Recent articles authored by Professor Yoshida explore topics such as dark matter clumping, quantum algorithms for simulations, and protoplanetary disk dynamics.

Articles (20)

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2025

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2022

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2022

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2021

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2021

Collaborators (15)

Richard Ellis

Professor of Astrophysics

University College London

UNITED KINGDOM

Naoki Yoshida

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Articles (20)

JWST, ALMA, and Keck Spectroscopic Constraints on the UV Luminosity Functions at z ∼ 7–14: Clumpiness and Compactness of the Brightest Galaxies in the Early Universe

An analytic model of gravitational collapse induced by radiative cooling: instability scale, density profile, and mass infall rate

ΛCDM Star Clusters at Cosmic Dawn: Stellar Densities, Environment, and Equilibrium

The Stellar Initial Mass Function of Early Dark Matter–free Gas Objects

The signature of subgalactic dark matter clumping in the global 21-cm signal of hydrogen

Toward a realistic description of dark matter overdensities around black holes

Quantum algorithm for collisionless Boltzmann simulation of self-gravitating systems

The Effect of Stellar Evolution on Dispersal of Protoplanetary Disks: Disk Fraction in Star-forming Regions

A Merger-driven Scenario for Clumpy Galaxy Formation in the Epoch of Reionization: Physical Properties of Clumps in the FirstLight Simulation

The Supersonic Project: Early Star Formation with the Streaming Velocity

Machine learning for observational cosmology

Reionization and the ISM/Stellar Origins with JWST and ALMA (RIOJA): The Core of the Highest-redshift Galaxy Overdensity at z = 7.88 Confirmed by NIRSpec/JWST

Simulations of High-redshift [O iii] Emitters: Chemical Evolution and Multiline Diagnostics

The Supersonic Project: The Eccentricity and Rotational Support of SIGOs and DM GHOSts

The Supersonic Project: The Early Evolutionary Path of Supersonically Induced Gas Objects

Euclid detectability of pair instability supernovae in binary population synthesis models consistent with merging binary black holes

Detecting Preheating in Protoclusters with Lyα Forest Tomography

H2 Cooling and Gravitational Collapse of Supersonically Induced Gas Objects

Deep-learning Reconstruction of Three-dimensional Galaxy Distributions with Intensity Mapping Observations

Deep Learning for Line Intensity Mapping Observations: Information Extraction from Noisy Maps

Collaborators (15)

Richard Ellis

Y Fudamoto

Nozomu Tominaga

Takuya Hashimoto

Ataru Tanikawa

Hiroshi Matsuo

Mark Vogelsberger

Kana Moriwaki

Michael Grudić

Koichi Miyamoto

Donghui Jeong

Shingo Hirano

Takashi Hosokawa

Federico Marinacci

Khee-Gan Lee

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