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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 2026Show all

5 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.GA2026

The CAMELS-CROCODILE Simulation Suite: A New Cosmology--Astrophysics Playground for Machine Learning

Kentaro Nagamine, Yuri Oku, Atsushi J. Nishizawa +4

We present CAMELS-CROCODILE, a suite of cosmological hydrodynamic simulations that extends the CAMELS framework with the \gadget{} smoothed particle hydrodynamics code and the Osak…

hep-ph2026

Future of Artificial Intelligence for Science in Japan 2024 Community Report

Yoshitaka Itow, Jia Liu, Hirokazu Maesaka +16

This white paper summarizes scientific challenges and AI/ML research opportunities identified through the FAIRS Japan 2024 unconference process. The discussion focuses on three maj…

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…