The AEGIS-X survey of the Extended Groth Strip region is a 1.6Ms Chandra survey covering 0.67 square degrees to a depth of 2x10^-16 erg/s/cm^2 (0.5-10 keV). With excellent supporting ground and space-based panchromatic data, from the UV to radio, and ~20 000 spectroscopic redshifts from the DEEP2 and DEEP3 surveys, this X-ray survey has been designed for studying the co-evolution of black holes and their host galaxies. The second phase of AEGIS-X was completed last month and comprises of an additional 1.8Ms in the region of the strip, where the supporting data is strongest.  I will present details of the X-ray data and the point source catalogue, including initial results from the new data, and key results from the survey, including the environment, stellar mass function, morphology, host galaxy and optical spectral properties of the X-ray sources.