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Fig. 14.

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Morphology measurement for representative galaxy group including model NoBHL, BHs3hl6v2L, and BHs3hl6v10L. The first model is a galaxy without a BH and the latter two are the same galaxy with the same BH seeding initial mass and time but different AGN wind velocities. The face-on images from the raw stellar density (top) and synthetic luminosity (bottom) are illustrated separately. The surface luminosity images have been obtained by post-processing the stellar light with a 3D radiation transfer, then redshifted, pixelized, and convolved with the JWST PSF. The dust absorption has been implemented as well. The JWST filter F200W have been used. Morphological measurements and fittings are also calculated by STATMORPH, including the Gini/M20, CAS and single Sersic profile. The galaxy center, major axis and half-light radius of the asymmetry and fitting Sersic model are colored with blue and red separately.

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