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Ben Forrest

university of california
H指数:18
被引数:1,285

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A massive and evolved slow-rotating galaxy in the early Universe

早期宇宙中一个庞大且演化的慢旋转星系

2026-05-040
PRE
Metal-poor Gas Accretion Drives Giant Clump Formation at 0.6 < z < 2.6

金属贫气体吸积驱动0.6 < z < 2.6期间的巨团块形成

2026-01-010
OAAI
CANUCS/Technicolor Data Release 1: Imaging; Photometry; Slit Spectroscopy; and Stellar Population Parameters*

CANUCS/Technicolor 数据发布1:成像;光度测量;狭缝光谱学;以及恒星种群参数*

2025-12-160
OA
The HST-Hyperion Survey: Grism Observations of a z ∼ 2.5 Protosupercluster

HST-超新星巡天:对z∼2.5原超星系团的透射光栅观测

2025-05-140
OA
Insights into environmental quenching at z ∼ 1: an enhancement of faint, low-mass passive galaxies in clusters

z ∼ 1 时环境熄灭的见解:星系团中暗淡、低质量被动星系的增强

2025-04-170
OA
MAGAZ3NE: Evidence for Galactic Conformity in z ≳ 3 Protoclusters
2024-12-200
OA
MAGAZ3NE: Massive, Extremely Dusty Galaxies at z ∼ 2 Lead to Photometric Overestimation of Number Densities of the Most Massive Galaxies at 3 < z < 4
2024-12-020
OA
Protoclusters as drivers of stellar mass growth in the early Universe, a case study: Taralay - a massive protocluster at z ∼ 4.57
2024-01-316
OA
The stellar mass function of quiescent galaxies in 2 < z < 2.5 protoclusters
2023-12-062
OA
Elentari:a massive proto-supercluster at z ∼ 3.3 in the cosmos field
2023-08-250
PRE