A Multi-Wavelength Investigation of Dust and Stellar Mass Distributions in Galaxies: Insights from High-Resolution JWST Imaging

2023/05/18 by Liu, Zhaoran, Morishita, Takahiro, Kodama, Tadayuki
#Astrophysics of Galaxies (astro-ph.GA) #FOS: Physical sciences

paper · doi:10.48550/arxiv.2305.10944

Abstract

We study the morphological properties of mid-infrared selected galaxies at 1.0

Related

• JWST UNCOVERs the Optical Size - Stellar Mass Relation at 4
• JWST+ALMA reveal the build up of stellar mass in the cores of dusty star-forming galaxies at Cosmic Noon
• UNCOVER: The rest ultraviolet to near infrared multiwavelength structures and dust distributions of sub-millimeter-detected galaxies in Abell 2744
• Stellar Morphology of Optically Dark or Faint Galaxies at z>3 with JWST
• JWST’s PEARLS: Resolved study of the stellar and dust components in starburst galaxies at cosmic noon