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Radio astrometric campaigns using VLBI have provided distances and propermotions for masers associated with young massive stars (BeSSeL survey). Theongoing BAaDE project plans to obtain astrometric information of SiO maserstars located in the inner Galaxy. These stars are associated with evolved,mass-losing stars. By overlapping optical (Gaia), infrared (2MASS, MSX andWISE) and radio (BAaDE) sources, we expect to obtain important clues on theintrinsic properties and population distribution of late-type stars. Moreover,a comparison of the Galactic parameters obtained with Gaia and VLBI can be doneusing radio observations on different targets: young massive stars (BeSSeL) andevolved stars (BAaDE).

Maser, infrared and optical emission for late-type stars in the Galactic plane