arrow
K

Kristen B. W. McQuinn

Rutgers the State University of New Jersey
H指数:28
被引数:2,525

个人简介

暂无内容

教育背景

暂无内容

工作经历

暂无内容

荣誉奖项

暂无内容

Growth of aromatic hydrocarbon dust particles in the extremely metal-poor galaxy Sextans A

极端贫金属星系 Sextans A 中芳香烃尘埃粒子的生长

2026-09-290
OA
CLASSY. XIV. The Nitrogen Exception—Multiphase Enrichment and Feedback in High-z Analogs*

CLASSY. XIV. 氮异常—高红移模拟中的多相富集与反馈

2026-04-270
OAAI
A GLIMPSE into the UV Continuum Slopes of the Faintest Galaxies in the Epoch of Reionization

再电离时期最暗星系的紫外连续谱斜率初探

2026-04-200
OAAI
The first GLIMPSE of the faint galaxy population at Cosmic Dawn with JWST: The evolution of the ultraviolet luminosity function across z ∼ 9-15
2026-02-016
PRE
Scylla. V. Constraints on the Spatial and Temporal Distribution of Bursts and the Interaction History of the Magellanic Clouds from Their Resolved Stellar Populations

Scylla. V. 亮爆发现象的空间和时间分布约束以及麦哲伦星系的相互作用历史,均来自其可分辨的恒星群体

2026-01-120
OAAI
The Star Formation History and Evolution of the Ultra-Diffuse M81 Satellite F8D1

星系M81卫星系F8D1的恒星形成历史与演化

2026-01-010
OA
GLOW. II. A Census of Oxygen in Low-mass Galaxies*

GLOW. II. 低质量星系中氧元素的普查*

2026-01-010
OA
GLOW. I. Comprehensive Measurements of Gas-rich, Star-forming, Low-mass Galaxies in the Nearby Universe*

GLOW. I. 对附近宇宙中富气体、恒星形成、低质量星系的全面测量*

2026-01-010
OA
Scylla: Observational Evidence for an Order of Magnitude in Dust-mass Opacity Evolution with Interstellar Medium Density in the Large Magellanic Cloud

斯库拉:大麦哲伦云中星际介质密度对尘埃质量消光系数演化一个数量级变化的观测证据

2026-01-010
OA
Wide Binaries in an Ultra-faint Dwarf Galaxy: Discovery; Population Modeling; and A Nail in the Coffin of Primordial black hole Dark Matter

超暗矮星系中的宽 binaries:发现;族群建模;以及原始黑洞暗物质棺材中的最后一颗钉子

2025-10-270
OA
Discovery of SiC and Iron Dust around AGB Stars in the Very Metal-poor Sextans a Dwarf Galaxy with JWST: Implications for Dust Production at High Redshift

利用JWST在金属量极低的 Sextans a 矮星系中发现AGB恒星周围的SiC和铁粉尘:对高红移处粉尘产生的启示

2025-09-120
OAAI
The first billion years according to JWST

根据JWST的第一个十亿年

2025-08-080
PRE
GLIMPSE: An Ultrafaint ≃105 M⊙ Pop III Galaxy Candidate and First Constraints on the Pop III UV Luminosity Function at z ≃  6–7

GLIMPSE:一个质量约为10^5 M⊙的极暗弱 Population III 星系候选体,以及对 z ≃ 6–7 处 Population III 紫外光度函数的首个约束

2025-08-040
PRE