Calibrating non-parametric morphological indicators from {it JWST} images for galaxies over $0.5
Abstract: The measurements of morphological indicators of galaxies are often influenced by a series of observational effects. In this study, we utilize a sample of over 800 TNG50 simulated galaxies with log($M_*$/M$_odot$)$>9$ at $0.5
2024-04-26