Detection and characterization are the two main paths for the exoplanets research. Detection experiments are driven by the need of exploring and filling-in those parts of the mass vs. orbit dimension plane that are poorly populated when not empty. This is of paramount interest in understanding formation and evolution of planetary systems. On the same time, we need information enabling us to understand the internal structure of known planets and have hints on the presence and composition of their atmosphere. While the two paths are being explored in parallel, it is trivial that detection is the basic step for the further characterization. I will give an overview on some recent results, e.g., those obtained by GAPS, a long term Italian led project with HARPS-N at TNG, and with LBT. Moreover, I'll present projects under study in the contest of the ESA Cosmic Vision, e.g., CHEOPS, PLATO 2.0, and EChO, emphasizing the Italian contribution to their implementation.