  In the course of a mid-infrared imaging campaign of close-by active galaxies,
we discovered the mid-infrared counterparts of bright compact radio sources in
the central star-forming region of NGC1808. We aim at confirming that these
sources are deeply embedded, young star clusters and at deriving some of their
intrinsic properties. To complement the mid-infrared data, we have collected a
set of near-infrared data with ISAAC at the VLT: J, Ks, and L' images, as well
as low-resolution, long-slit spectra for three of the sources. Surprisingly,
the new images unveil a near-infrared counterpart for only one of the
mid-infrared/radio sources, namely M8 in the L' band. All the other sources are
so deeply embedded that their emission does not pop out above an extended
diffuse near-infrared emission. The near-infrared spectra of the sources look
alike, with intense, ionised hydrogen lines. This supports the interpretation
of these sources in terms of embedded young clusters. We derive extinctions and
ionising photon production rates for two of the clusters.
