Baryonic Tully-Fisher relation where galaxies from our sample are plotted based on the inclination used for kinematic modeling. For both UDGs (stars) and standard dwarfs (diamonds), rotational velocities obtained using H I inclinations are given in blue, while the ones obtained using optical inclinations are given in orange. We note that here we do not make a distinction between the optically reliable vs. unreliable and/or rotationally flagged vs. unflagged galaxies, as long as their PA_H I − PA_op < 45°.