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We present multi-waveband optical imaging data obtained from observations ofthe Subaru/XMM-Newton Deep Survey (SXDS). The survey field, centered atR.A.=02:18:00, decl.=-05:00:00, has been the focus of a wide range ofmulti-wavelength observing programs spanning from X-ray to radio wavelengths. Alarge part of the optical imaging observations are carried out with Suprime-Camon Subaru Telescope at Mauna Kea in the course of Subaru Telescope ObservatoryProjects. This paper describes our optical observations, data reduction andanalysis procedures employed, and the characteristics of the data products. Atotal area of 1.22 sqdeg is covered in five contiguous sub-fields, each ofwhich corresponds to a single Suprime-Cam field of view (34'x27'), in fivebroad-band filters B, V, Rc, i', z' to the depths of B=28.4, V=27.8, Rc=27.7,i'=27.7 and z'=26.6 (AB, 3-sigma, 2-arcsec aperture). The data are reduced andcompiled into five multi-waveband photometric catalogs, separately for eachSuprime-Cam pointing. The i'-band catalogs contain about 900,000 objects,making the SXDS catalogs one of the largest multi-waveband catalogs incorresponding depth and area coverage. The SXDS catalogs can be used for anextensive range of astronomical applications such as the number density of theGalactic halo stars to the large scale structures at the distant universe. Thenumber counts of galaxies are derived and compared with those of existing deepextragalactic surveys. The optical data, the source catalogs, and configurationfiles used to create the catalogs are publicly available via the SXDS web page(http://www.naoj.org/Science/SubaruProject/SXDS/index.html)

The Subaru/XMM-Newton Deep Survey (SXDS) - II. Optical Imaging and Photometric Catalogs