A Submillimeter Continuum Survey of Local Dust-Obscured Galaxies
  We conduct a 350 micron dust continuum emission survey of 17 dust-obscured
galaxies (DOGs) at z = 0.05-0.08 with the Caltech Submillimeter Observatory
(CSO). We detect 14 DOGs with S_350 = 114-650 mJy and S/N > 3. By including two
additional DOGs with submillimeter data in the literature, we are able to study
dust contents for a sample of 16 local DOGs that consists of 12 bump and 4
power-law types. We determine their physical parameters with a two-component
modified blackbody function model. The derived dust temperatures are in the
range 57-122 K and 22-35 K for the warm and cold dust components, respectively.
The total dust mass and the mass fraction of warm dust component are
3-34$\times10^{7} M_\odot$ and 0.03-2.52%, respectively. We compare these
results with those of other submillimeter-detected infrared luminous galaxies.
The bump DOGs, the majority of the DOG sample, show similar distributions of
dust temperatures and total dust mass to the comparison sample. The power-law
DOGs show a hint of smaller dust masses than other samples, but need to be
tested with a larger sample. These findings support that the reason why DOGs
show heavy dust obscuration is not an overall amount of dust content, but
probably the spatial distribution of dust therein.
