The Subaru/XMM-Newton Deep Survey (SXDS) is a new deep Optical/X-ray survey which aim to take full advantage of the capabilities
of the Subaru Telescope and the XMM-Newton. The SXDS is part of an ambitious project to obtain extensive multi-wavelength
data across a ∼ 1.3 deg2 region of sky. Other wavelength data (infrared, submillimeter, and radio) are being pursued through various facilities. Combined
with suitably deep images at other wavelengths the SXDS would provide an accurate census of the contents of the Universe without
suffering from the biasing effects of large-scale structures. This paper describes the location, size and depth of this survey.
Keywords surveys - large-scale structure - optical imaging - X-rays:galaxies - active galaxies