  Three new obscured Milky Way clusters were detected as surface density peaks
in the 2MASS point source catalog during our on-going search for hidden
globular clusters and massive Arches-like star clusters. One more cluster was
discovered serendipitously during a visual inspection of the candidates.
  The first deep J, H, and Ks imaging of the cluster [IBP2002] CC01 is
presented. We estimated a cluster age of ~1-3 Myr, distance modulus of
(m-M)0=12.56+-0.08 mag (D=3.5 Kpc), and extinction of AV~7.7 mag. We also
derived the initial mass function slope for the cluster: Gamma=-2.23+-0.16. The
integration over the initial mass function yielded a total cluster mass
M_{total}<=1800+-200Msol. CC01 appears to be a regular, not very massive star
cluster, whose formation has probably been induced by the shock front from the
nearby HII region Sh2-228.
