  We give an update on our long-term program of Galactic Cepheids started in
2012, whose goal is to measure the visual orbits of Cepheid companions. Using
the VLTI/PIONIER and CHARA/MIRC instruments, we have now detected several com-
panions, and we already have a good orbital coverage for several of them. By
combining interferometry and radial velocities, we can now derive all the
orbital elements of the systems, and we will be soon able to estimate the
Cepheid masses.
