Determining Dust Properties in Protoplanetary Disks: SED-derived Masses and Settling With ALMA

Anneliese Rilinger, Catherine Espaillat, Zihua Xin +3

We present spectral energy distribution (SED) modeling of 338 disks around T Tauri stars from eleven star-forming regions, ranging from $\sim$0.5 to 10 Myr old. The disk masses we…