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Minami Nakane

the university of tokyo
H指数:9
被引数:265

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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
Spatially Resolved Physical Properties of Young Star Clusters and Star-forming Clumps in the Brightest z > 6 Galaxy, the Strongly Lensed Cosmic Spear at z = 6.2

在明亮 z > 6 星系(强引力透镜宇宙矛,z = 6.2)中年轻星团和恒星形成团块的空域分辨物理特性

2026-01-010
OA
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
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