  Recent studies have shown that the area around the massive, obscured cluster
RSGC3 may harbour several clusters of red supergiants. In this paper, we
analyse a clump of photometrically selected red supergiant candidates 20' south
of RSGC3 in order to confirm the existence of another of these clusters. Using
medium-resolution infrared spectroscopy around 2.27 microns, we derived
spectral types and velocities along the line of sight for the selected
candidates, confirming their nature and possible association. We find a compact
clump of eight red supergiants and four other candidates at some distance, all
of them spectroscopically confirmed red supergiants. The majority of these
objects must form an open cluster, which we name Alicante 10. Because of the
high reddening and strong field contamination, the cluster sequence is not
clearly seen in 2MASS or GPS-UKIDSS. From the observed sources, we derive
E(J-Ks)=2.6 and d~6 kpc. Although the cluster is smaller than RSGC3, it has an
initial mass in excess of 10000 solar masses, and it seems to be part of the
RSGC3 complex. With the new members this association already has 35
spectroscopically confirmed red supergiants, confirming its place as one of the
most active sites of recent stellar formation in the Galaxy.
