to each source found, and calculates both the area ($A=\pi ab$, where a and b are the semi-major and semi-minor axes, respectively) and the aspect ratio of the ellipse ($\epsilon = a/b$). The Barycenter position is derived by extracting sources at the 2$\sigma$ contours. The flux densities and peak flux are derived as described in §\[cal\], and the peak position is located by determining the position of the peak pixel. The flux density uncertainties include components from both the measurement uncertainty and a 15% calibration uncertainty, added in quadrature. The uncertainty in peak flux also includes a 15% calibration uncertainty. The last column of Table \[properties1\] lists whether or not each submillimeter source is associated with a *Spitzer* source (see §\[embedded\]). The peak fluxes (as well as the RMS noise of each map listed in Table \[info\]) are given in units of Jy beam$^{-1}$. To obtain these quantities in MJy sr$^{-1}$, a unit that can be used to compare between different instruments with different beams, the relevant conversions are: 1 Jy beam$^{-1}$ = 519.7 MJy sr$^{-1}$ at 350 $\mu$m; and 1 Jy beam$^{-1}$ = 310.3 MJy sr$^{-1}$ at 450 $\mu$m.

As stated in §\[subobs\], the DSOS corrected all of the 