摘要: We present the first James Webb Space Telescope/NIRCam-led determination of
$79.5$. Their star formation main sequence is
consistent with predictions from simulations. Lastly, we introduce an
analytical framework to constrain main-sequence evolution at $z>7$ based on
galaxy ages and basic assumptions, through which we find results consistent
with expectations from cosmological simulations. While this work only gives a
glimpse of the properties of typical galaxies that are thought to drive the
reionization of the universe, it clearly shows the potential of JWST to unveil
unprecedented details on galaxy formation in the first billion years.
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分类：
天文学
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天文学
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引用：
ChinaXiv:202303.05019
(或此版本
ChinaXiv:202303.05019V1)
DOI:10.12074/202303.05019V1
CSTR:32003.36.ChinaXiv.202303.05019.V1
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科创链TXID：
f955ae05-9e14-47ba-a5d4-634c59094707
- 推荐引用方式：
N. Leethochawalit,M. Trenti,P. Santini,L. Yang,E. Merlin,M. Castellano,A. Fontana,T. Treu,C. Mason,K. Glazebrook,T. Jones,B. Vulcani,T. Nanayakkara,D. Marchesini,S. Mascia,T. Morishita,G. Roberts-Borsani,A. Bonchi,D. Paris,K. Boyett,V. Strait,A. Calabro`,L. Pentericci,M. Bradac,X. Wang,C. Scarlata.Early results from GLASS-JWST. X: Rest-frame UV-optical properties of
galaxies at 7 < z < 9.中国科学院科技论文预发布平台.[ChinaXiv:202303.05019V1]
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