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Laura C. Keating

University of Cambridge
H指数:30
被引数:2,942

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The thesan-zoom project: mystery N/O more - uncovering the origin of peculiar chemical abundances and a not-so-fundamental metallicity relation at 3 < z < 12
2026-05-012
PRE
Metallicity Gradients in Modern Cosmological Simulations. II. The Role of Bursty versus Smooth Feedback at High Redshift

金属丰度梯度在现代宇宙学模拟中的作用。II. 高红移下爆发式与平滑反馈的作用

2026-04-160
OAAI
A dense web of neutral gas in a galaxy proto-cluster post-reionization

再电离后星系原星系团中的中性气体密集网络

2026-01-020
PRE
Updated dark pixel fraction constraints on reionization's end from the Lyman-series forests of XQR-30

来自XQR-30莱曼系列森林的更新暗像素分数约束,关于再电离结束的评估

2026-01-010
PRE
Overmassive black holes in the early Universe can be explained by gas-rich, dark matter-dominated galaxies

早期宇宙中的超重黑洞可以通过富气体、暗物质主导的星系来解释。

2026-01-010
OAAI
The thesan-zoom project: star formation efficiency from giant molecular clouds to galactic scale in high-redshift starbursts

The thesan-zoom project: 高红移星暴星系中从巨分子云到星系尺度的恒星形成效率

2025-12-011
PRE
The thesan-zoom project: burst, quench, repeat - unveiling the evolution of high-redshift galaxies along the star-forming main sequence

The thesan-zoom project: burst, quench, repeat - 揭示高红移星系在恒星形成主序列上的演化

2025-11-015
OAAI
Percent-level timing of reionisation: Self-consistent, implicit-likelihood inference from XQR-30+Lyα forest data

百分之一精度的再电离时序:基于XQR-30+Lyα森林数据的自洽隐式似然推断

2025-04-140
PRE
The JWST-PRIMAL archival survey: A JWST/NIRSpec reference sample for the physical properties and Lyman-α absorption and emission of ∼600 galaxies at z=5.0-13.4
2025-01-0610
PRE
Evidence of Pop III stars' chemical signature in neutral gas at z ∼ 6 A study based on the E-XQR-30 spectroscopic sample

Pop III星在z ∼ 6中性气体中化学特征的证据 -- 基于E-XQR-30光谱样品的研究

2024-07-315
OA