  A UV image in the direction of Ophiuchus, obtained with the FAUST instrument
is analysed. Suitable candidates as unrecognized subluminous stars are selected
comparing the observed UV flux to the predicted one. The uv-excess objects were
observed at the 1.0 m Wise telescope. This method yields to the detection of
eight broad Balmer lines objects. Six are classified as sds and two wds,
comparing the Hbeta line profile with that of stellar model atmospheres.
