  In this paper the results of matching the RAdial Velocity Experiment (RAVE),
a spectroscopic Southern hemisphere survey (9 $ < I_{DENIS} <$ 12), and
XMM-Newton Serendipitous Source Catalogue (3XMM) are presented. The latest data
releases of RAVE and XMM were matched and a X-ray RAVE catalogue of 1071 stars
was obtained. Then the catalogue was checked for possible Gould Belt (GB)
members. We obtained a subsample of 10 stars that meet the GB membership
criteria. This subsample and GB member candidates were tested photometrically
and kinematically. Among the members there are two BY Dra type variables, an
NGC2451 open cluster member, a high proper motion star. The rest are regular
main sequence stars. The members have very low velocity dispersions which lead
us to think that the members belong in a single structure. We also found out
that a kinematical GB membership test might be possible to derive given a large
enough GB member sample as they fit in a narrow interval in space velocity
diagrams.
