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R. A. Meyer

max-planck-institut für astronomie
H指数:37
被引数:5,117

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JWST+ALMA Reveal the Buildup of Stellar Mass in the Cores of Dusty Star-forming Galaxies at Cosmic Noon

詹姆斯·韦伯太空望远镜+阿塔卡马大型毫米/亚毫米波阵列揭示宇宙正午时期尘埃星系形成星系核心的恒星质量积累

2026-04-200
OA
JWST Spectroscopic Insights Into the Diversity of Galaxies in the First 500 Myr: Short-Lived Snapshots Along a Common Evolutionary Pathway

JWST光谱学洞见:前500百万年星系多样性研究——共同演化路径上的短暂快照

2026-04-140
OA
A JWST Paα Calibration of the Radio Luminosity–Star Formation Rate Relation at z ∼ 1.3

基于JWST的Paα校准,研究z ∼ 1.3处射电光度—恒星形成率关系

2026-02-180
OAAI
ALMA and JWST Identification of Faint Dusty Star-forming Galaxies up to z ∼ 8 and Their Connection with Other Galaxy Populations

ALMA与JWST对红移z∼8的暗淡尘埃星系形成星系的识别及其与其他星系群体的联系

2026-02-110
OAAI
Resolving the Dusty Star-forming Galaxy GN20 at z = 4.055 with NOEMA and JWST: A Similar Distribution of Stars; Gas; and Dust Despite Distinct Apparent Profiles

使用NOEMA和JWST解析z = 4.055处的尘埃星形成星系GN20:尽管表观轮廓不同,但恒星、气体和尘埃分布相似

2025-12-230
OAAI
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
Insight into the starburst nature of Galaxy GN-z11 with JWST MIRI spectroscopy

利用JWST MIRI光谱学研究GN-z11星系的星爆性质

2025-02-140
PRE
An Hα view of galaxy buildup in the first 2 Gyr: Luminosity functions at z ∼ 4-6.5 from NIRCam/grism spectroscopy

前2个Gyr中星系堆积的h α 视图: NIRCam/grism光谱在z ∼ 4-6.5处的光度函数

2025-02-120
PRE
Mapping dusty galaxy growth at z > 5 with FRESCO: detection of Hα in submm galaxy HDF850.1 and the surrounding overdense structures
2025-01-094
OA
A SPectroscopic Survey of Biased Halos In the Reionization Era (ASPIRE): JWST Supports Earlier Reionization around [O III] Emitters
2024-11-140
OA
JWST FRESCO: a comprehensive census of H β plus [O III] emitters at 6.8 < z < 9.0 in the GOODS fields
2024-10-142
OA
A SPectroscopic Survey of Biased Halos In the Reionization Era (ASPIRE): Broad-line AGN at z=4-5 Revealed by JWST/NIRCam WFSS
2024-10-091
OA
A first look at spatially resolved star formation at 4.8 < z < 6.5 with JWST FRESCO NIRCam slitless spectroscopy
2024-09-276
OA