  We present first results of our NAOS-CONICA search for close substellar
companions around young nearby stars. This program was started only a few
months ago. We have obtained 1st epoch images of several targets which are
unpublished young stars (age<100 Myrs), hence ideal targets to look for
planetary companions. For one target star we could even take a 2nd epoch image.
By comparing both images we could look for co-moving companions of the target
star. Those data show clearly that the detection of planetary companions m <13
Mjup inward a saturn-like orbit (r<10 AU) is feasible with NAOS-CONICA and in
addition that the astrometric confirmation of those companions is doable with
only a few weeks of epoch difference.
