Diving Beneath the Sea of Stellar Activity: Chromatic Radial Velocities of the Young AU Mic Planetary System

We present updated radial-velocity (RV) analyses of the AU Mic system. AU Mic is a young (22 Myr) early M dwarf known to host two transiting planets - P_{b}\sim8.46 days, R_{b}=4.38_{-0.18}^{+0.18}\ R_{\oplus}, P_{c}\sim18.86 days, R_{c}=3.51_{-0.16}^{+0.16}\ R_{\oplus}. With visible RVs from CARMENES-VIS, CHIRON, HARPS, HIRES, {\sc {\textsc{Minerva}}}-Australis, and TRES, as well... Show more