arrow
H

Hiroya Umeda

the university of tokyo
H指数:18
被引数:2,215

个人简介

暂无内容

教育背景

暂无内容

工作经历

暂无内容

荣誉奖项

暂无内容

Discovery of a Little Red Dot Candidate at z ≳ 10 in COSMOS-web Based on MIRI-NIRCam Selection

基于MIRI-NIRCam选择的COSMOS-web中红移z ≳ 10的小红点候选体的发现

2025-12-020
OAAI
SILVERRUSH. XIV. Lyα Luminosity Functions and Angular Correlation Functions from 20,000 Lyα Emitters at z ∼ 2.2-7.3 from up to 24 deg2 HSC-SSP and CHORUS Surveys: Linking the Postreionization Epoch to the Heart of Reionization

SILVERRUSH. XIV. 来自HSC-SSP和CHORUS巡天中多达24平方度、红移z ∼ 2.2-7.3的20,000个Lyα发射体的Lyα光度函数和角相关函数:连接再电离后时期与再电离核心阶段

2025-03-182
OA
The Physical Origin of Extreme Emission Line Galaxies at High Redshifts: Strong [O iii] Emission Lines Produced by Obscured Active Galactic Nuclei

高红移极端发射线星系的物理起源:由被遮蔽的活跃星系核产生的强[O iii]发射线

2025-03-120
OA
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

JWST、ALMA和Keck光谱观测对z∼7-14处紫外光度函数的约束:早期宇宙中最亮星系的成团性与致密性

2025-02-079
OA
EMPRESS. XIV. Strong High-ionization Lines of Young Galaxies at z=0-8: Ionizing Spectra Consistent with the Intermediate-mass Black Holes with MBH ∼ 103-106 M ⊙

十四皇后.z = 0-8处年轻星系的强高电离线: 电离光谱与MBH ∼ 103-106 M ⊙ 的中等质量黑洞一致

2024-05-033
OA
EMPRESS. XII. Statistics on the Dynamics and Gas Mass Fraction of Extremely Metal-poor Galaxies
2024-01-124
OA