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Gillian Wilson

University of California System
H指数:47
被引数:8,520

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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
Traversing the Star-forming Main Sequence with Molecular Gas Stacks of z ∼ 1.6 Cluster Galaxies

在z∼1.6星系团星系中通过分子气体堆栈横穿恒星形成主序列

2025-05-230
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
LoVoCCS. II. Weak Lensing Mass Distributions, Red-sequence Galaxy Distributions, and Their Alignment with the Brightest Cluster Galaxy in 58 Nearby X-Ray-luminous Galaxy Clusters
2024-10-040
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
GOGREEN: A critical assessment of environmental trends in cosmological hydrodynamical simulations at z ≈ 1
2022-11-248
OA