Revealing the gas properties of the most typical planet-forming disks

Planets are formed from the gas and dust in disks around young stars, both of which will benefit from the Wideband Sensitivity Upgrade. However, the largest limitation to analyzing the emission from these disks will continue to be the limited angular resolution and image reconstruction methods. In this talk, I will present how visibility-based techniques can efficiently recover the gas morphology and brightness temperature in compact and faint disks, where image-based techniques are unable to operate. These techniques will be crucial to optimize the recovery of information of the improved spectral scan capabilities. These results are part of Kurtovic \& Pinilla