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We present both the observations and the data reduction procedures of theSubaru COSMOS 20 project that is an optical imaging survey of the HST COSMOSfield, carried out by using Suprime-Cam on the Subaru Telescope with thefollowing 20 optical filters: 6 broad-band (B, g', V, r', i', and z'), 2narrow-band (NB711 and NB816), and 12 intermediate-band filters (IA427, IA464,IA484, IA505, IA527, IA574, IA624, IA679, IA709, IA738, IA767, and IA827). Apart of this project is described in Taniguchi et al. (2007) and Capak et al.(2007) for the six broad-band and one narrow-band (NB816) filter data. In thispaper, we present details of the observations and data reduction for remaining13 filters (the 12 IA filters and NB711). In particular, we describe theaccuracy of both photometry and astrometry in all the filter bands. We alsopresent optical properties of the Suprime-Cam IA filter system in Appendix.

The Subaru COSMOS 20: Subaru Optical Imaging of the HST COSMOS Field with 20 Filters