Oral title: Protoplanet mass estimates via ALMA kinematics 

Oral abstract: How can we confirm and calculate the mass of protoplanets detected with high-contrast AO imaging? I will show that 
embedded companions can distort velocity maps on small and large scales through their circumplanetary disks and corotating 
zones, respectively, providing dynamical masses. ALMA data on MWC758 already reveals kinematical distortions which can be 
explained by an unseen 10MJup companion.