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Masami Ouchi

National Astronomical Observatory of Japan
H指数:76
被引数:2.1万

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Lyα Intensity Mapping in HETDEX: Galaxy-Lyα Intensity Cross-power Spectrum

HETDEX中的Lyα强度映射:星系-Lyα强度的交叉功率谱

2026-03-030
OA
VENUS: A Strongly Lensed Clumpy Galaxy at z ∼ 11–12 Behind the Galaxy Cluster MACS J0257.1-2325

VENUS:位于星系团MACS J0257.1-2325后方的一个强引力透镜致密星系(红移z ∼ 11–12)

2026-01-010
OA
Comprehensive JWST+ALMA Study on the Extended Lyα Emitters; Himiko; and CR7 at z ∼ 7: Blue Major Merger Systems in Stark Contrast to Submillimeter Galaxies

基于JWST和ALMA的扩展莱曼阿尔法发射体、Himiko和CR7在红移z≈7的综合研究:与亚毫米波星系形成鲜明对比的蓝色主要合并系统

2025-12-120
OA
Primordial rotating disk composed of at least 15 dense star-forming clumps at cosmic dawn
2025-08-070
PRE
ALMA Lensing Cluster Survey: Physical Characterization of Near-infrared-dark Intrinsically Faint ALMA Sources at z = 2–4

ALMA透镜星系巡天:z = 2–4处近红外暗且固有光度较弱的ALMA源物理特性研究

2025-08-070
PRE
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
ALMA Lensing Cluster Survey: Deep 1.2 mm Number Counts and Infrared Luminosity Functions at z ≃ 1-8

ALMA透镜集群调查: z ≈ 1-8处的深1.2毫米数计数和红外光度函数

2024-11-271
OA
The MUSE eXtremely Deep Field: Detections of circumgalactic Si II* emission at z ≳ 2☆
2024-11-190
PRE
MAMMOTH-Subaru. II. Diverse Populations of Circumgalactic Lyα Nebulae at Cosmic Noon
2024-11-150
OA