Additional figures: Ten Aligned Orbits: Planet Migration in the Era of JWST and Ariel

We add supporting figures to Zak et al; Aligned Orbits in Ten Systems: Planet Migration in the Era of JWST and Ariel

w35N.pdf: MCMC results of WASP-35b. Three independent MCMC simulations are shown with different colors.

w44N.pdf: MCMC results of WASP-44b. Three independent MCMC simulations are shown with different colors.

w45N.pdf: MCMC results of WASP-45 Ab. Three independent MCMC simulations are shown with different colors.

w54N.pdf: MCMC results of WASP-54 Ab. Three independent MCMC simulations are shown with different colors.

w91N.pdf: MCMC results of WASP-91b. Three independent MCMC simulations are shown with different colors.

w99N.pdf: MCMC results of WASP-99b. Three independent MCMC simulations are shown with different colors.

w129N.pdf: MCMC results of WASP-129 Ab. Three independent MCMC simulations are shown with different colors.

w162N.pdf: MCMC results of WASP-162b. Three independent MCMC simulations are shown with different colors.

q7N.pdf: MCMC results of Qatar-7b. Three independent MCMC simulations are shown with different colors.

epicN.pdf: MCMC results of EPIC-219388192b. Three independent MCMC simulations are shown with different colors.

EPICLC.pdf: Phased $g$-band ASAS-SN data of EPIC-219388192 A with the detected stellar rotation period of $P_{\rm{Rot}}$ =12.29 $\pm$ 0.20 d.