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B

B. Magnelli

university of miami
H指数:61
被引数:1.5万

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Resolved SED Modeling with JWST and ALMA: The Role of Stellar Mass Surface Density in Regulating Star Formation in Cosmic Noon Galaxies

詹姆斯·韦伯太空望远镜(JWST)和阿塔卡马大型毫米/亚毫米波阵列(ALMA)的解析SED建模:恒星质量表面密度在宇宙正午星系中调控恒星形成的作用

2026-09-110
OAAI
PANORAMIC: Discovery of an ultra-massive grand-design spiral galaxy at z ∼ 5.2

PANORAMIC:在红移z∼5.2处发现一个超巨质量规整旋涡星系

2025-04-160
PRE
Behind the dust veil: A panchromatic view of an optically dark galaxy at z=4.82
2025-01-290
OA
Accelerated formation of ultra-massive galaxies in the first billion years
Nature
IF48.5
2024-11-130
PRE
A photo-z cautionary tale: Redshift confirmation of COSBO-7 at z=2.625

一个phote-z警示故事: 在z = 2.625时COSBO-7的红移确认

2024-10-216
OA
NOEMA formIng Cluster survEy (NICE): Characterizing eight massive galaxy groups at 1.5 < z < 4 in the COSMOS field
2024-09-273
OA
JWST/CEERS sheds light on dusty star-forming galaxies: Forming bulges, lopsidedness, and outside-in quenching at cosmic noon
2024-08-029
OA
CEERS: 7.7 μm PAH Star Formation Rate Calibration with JWST MIRI
2024-07-175
OA
Noema formIng Cluster survEy (NICE): Discovery of a starbursting galaxy group with a radio-luminous core at z=3.95

Noema形成星系团调查 (NICE): 在z = 3.95处发现了一个具有无线电发光核心的星爆星系群

2024-04-249
OA
CEERS: MIRI deciphers the spatial distribution of dust-obscured star formation in galaxies at 0.1 < z < 2.5
2023-10-1014
OA