We report INTEGRAL /IBIS results on temporal and spectral behaviour of the Low Mass X-ray Binary XB 1832–330 located in the globular cluster NGC 6652 .
During the 2003-2005 monitoring of the Galactic Centre , the source shows a weak flux variability and an everage flux in the 20–150 keV of about 2 \times 10 ^ { -10 } erg s ^ { -1 } cm ^ { -2 } .
The overall energy spectrum extends up to 150 keV and is well described by a Comptonization model with an electrons temperature of \sim 22 keV and a plasma optical depth of 1.8 .
We thus confirm the persistent nature of this burtser .