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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Príomhchruthaitheoirí:	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
Formáid:	Artigo
Teanga:	Inglês
Foilsithe / Cruthaithe:	IOP Publishing 2025-01-01
Sraith:	The Astrophysical Journal
Ábhair:	Galaxy evolution High-redshift galaxies Galaxies Galaxy quenching Quenched galaxies
Rochtain ar líne:	https://doi.org/10.3847/1538-4357/ae03ad
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