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Sarah E. I. Bosman

max-planck-institut für astronomie
H指数:33
被引数:3,414

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First-star imprints in a metal-poor galaxy overdensity near the end of reionization

在再电离结束附近贫金属星系过密区的第一代恒星印记

2026-09-290
PRE
BEES: Quasar Lifetime Measurements from Extended Rest-optical Emission Line Nebulae at z ∼ 6

BEES: 来自红移 z ∼ 6 处扩展静止光学发射线星云的类星体寿命测量

2026-05-200
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
Bridging Quasars and Little Red Dots: Insights into Broad-line Active Galactic Nuclei at z = 5–8 from the First JWST COSMOS-3D Dataset

连接类星体与小红点:来自首批JWST COSMOS-3D数据集关于z = 5–8宽线类星体的见解

2025-12-310
OAAI
SHELLQs–JWST Perspective on the Intrinsic Mass Relation between Supermassive Black Holes and Their Host Galaxies at z > 6

SHELLQs–JWST视角下z > 6时超大质量黑洞与其宿主星系的本征质量关系

2025-12-170
OAAI
Discovery of a Little Red Dot Candidate at z ≳ 10 in COSMOS-web Based on MIRI-NIRCam Selection

基于MIRI-NIRCam选择的COSMOS-web中红移z ≳ 10的小红点候选体的发现

2025-12-020
OAAI
SHELLQs-JWST Unveils the Host Galaxies of 12 Quasars at z > 6

SHELLQs-JWST 揭示了 z > 6 处12个类星体的宿主星系

2025-10-280
OA
A 13 Billion Year View of Galaxy Growth: Metallicity Gradient Evolution from the Local Universe to z = 9 with JWST and Archival Surveys

130亿年视角下的星系增长:从局部宇宙到z=9的金属丰度梯度演化(使用JWST和档案调查)

2025-09-260
OAAI
MIDIS: MIRI Uncovers Virgil; the First Little Red Dot with Clear Detection of Its Host Galaxy at z ≃ 6.6

MIDIS:MIRI揭示维吉尔;首个在z ≃ 6.6处清晰探测到宿主星系的小红点。

2025-08-120
OA
A post-starburst pathway for the formation of massive galaxies and black holes at z > 6

星爆后演化路径:z>6时巨质量星系与黑洞的形成

2025-08-110
PRE
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
MIRI Deep Imaging Survey (MIDIS) of the Hubble Ultra Deep Field: Survey description and early results for the galaxy population detected at 5.6 μm☆

MIRI深度成像巡天(MIDIS)对哈勃超深空场的观测:巡天描述及在5.6 μm探测到的星系群体的早期结果☆

2025-04-040
PRE
A Quasar-anchored Protocluster at z=6.6 in the ASPIRE Survey. I. Properties of [O iii] Emitters in a 10 Mpc Overdensity Structure

ASPIRE 调查中 z=6.6 处的一个类星体锚定原星系团。I. 一个 10 Mpc 过密结构中 [O iii] 发射体的性质

2025-03-041
OA
A SPectroscopic Survey of Biased Halos In the Reionization Era (ASPIRE): JWST Supports Earlier Reionization around [O III] Emitters
2024-11-140
OA