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We collected the parameters (position, absorption, spin, orbital period,etc..), when known, of all Galactic sources detected by INTEGRAL during itsfour first years of activity. We use these parameters to test theoreticalpredictions. For example, it is clear that HMXBs tend to be found mostly in thetangential direction of the Galactic arms, while LMXBs tend to be clustered inthe Galactic bulge. We then focus on HMXBs and present two possible new tools,in addition to the well-known ``Corbet-diagram'', to distinguish betweenBe-HMXBs and Sg-HMXBs

The Galactic population of HMXBs as seen with INTEGRAL during its four first years of activity