We present early results from the first IR imaging of the weak X-ray sources
discovered in a recent Chandra survey towards the Galactic Centre. From our VLT
observations we will identify likely counterparts to a sample of the hardest
sources in order to place constraints on the nature of this previously unknown
population.Comment: To appear in RevMexAA(SC) Conference Series, Proc. of IAU Colloquium
194, Compact Binaries in the Galaxy and Beyond, La Paz, Mexico, 17-21 Nov.,
200