It adopts the advanced “CCD-style” bolometer array with 12 $\times$ 32 pixels, resulting in a 259 $\times$ 097 field of view. SHARC-II features relatively high angular resolution: it has a beam size of 85 at 350 $\mu$m and $\sim$11$\arcsec$ at 450 $\mu$m with good focus and pointing. Since the atmospheric transmission is very sensitive to the weather at the higher frequencies at which SHARC-II operates, it only works well in very dry weather. Under optimal weather conditions ($\tau_{225\ GHz} < 0.05$), SHARC-II can reach an RMS noise of 25 mJy beam$^{-1}$ in one hour of integration at 350 $\mu$m.

Because SHARC-II achieves optimum performance at 350 $\mu$m, a wavelength at which high-quality data is often difficult to obtain, and because the peak of a 15 K blackbody occurs closer to 350 $\mu$m than 450 $\mu$m, we mapped our sources at 350 $\mu$m. We also present three sources that were mapped at 450 $\mu$m. In this paper, we present the basic data of this survey, including images and source properties, in a manner that is consistent with other papers presenting submillimeter and millimeter continuum data on the c2d cores and clouds. We leave a detailed analysis combining all available data on 