Terrestrial and sub-Neptune exoplanets are expected to form in the inner regions of protoplanetary disks around their parent stars. Water plays a key role in their formation, although it is yet unclear whether water molecules are formed in situ or transported from the outer disk. The planetary system PDS 70 is a benchmark target to search for water in a disk hosting an 8-billion-km planet-carved gap separating an inner and outer disk. Using the data...
