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Stellar Mass Assembly History of Massive Quiescent Galaxies since z ∼ 4: Insights from Spatially Resolved Spectral Energy Distribution Fitting with JWST Data

Massive quiescent galaxies at high redshift show significantly more compact morphology than their local counterparts. To examine their internal structure across a wide redshift range and investigate potential redshift dependence, we performed spatially resolved spectral energy distribution fitting u...

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Asıl Yazarlar: Novan Saputra Haryana, Masayuki Akiyama, Abdurro’uf, Hesti Retno Tri Wulandari, Juan Pablo Alfonzo, Kianhong Lee, Naoki Matsumoto, Ryo Albert Sutanto, Muhammad Nur Ihsan Effendi, Itsna Khoirul Fitriana, Ibnu Nurul Huda, Anton Timur Jaelani, Sultan Hadi Kusuma, Lucky Puspitarini, Dian P. Triani
Materyal Türü: Artigo
Dil:Inglês
Baskı/Yayın Bilgisi: IOP Publishing 2025-01-01
Seri Bilgileri:The Astrophysical Journal
Konular:
Galaxy evolution
High-redshift galaxies
Galaxies
Galaxy quenching
Quenched galaxies
Online Erişim:https://doi.org/10.3847/1538-4357/ae03ad
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