We report Submillimeter Array ( SMA ) observations of the 880 \mu m dust continuum emission for four dust-obscured galaxies ( DOGs ) in the local universe .
Two DOGs are clearly detected with S _ { \nu } ( 880 \mu m ) = 10 - 13 mJy and S / N > 5 , but the other two are not detected with 3 \sigma upper limits of S _ { \nu } ( 880 \mu m ) = 5 - 9 mJy .
Including an additional two local DOGs with submillimeter data from the literature , we determine the dust masses and temperatures for six local DOGs .
The infrared luminosities and dust masses for these DOGs are in the range 1.2 - 4.9 \times 10 ^ { 11 } ( L _ { \odot } ) and 4 - 14 \times 10 ^ { 7 } ( M _ { \odot } ) , respectively .
The dust temperatures derived from a two-component modified blackbody function are 23 - 26 K and 60 - 124 K for the cold and warm dust components , respectively .
Comparison of local DOGs with other infrared luminous galaxies with submillimeter detections shows that the dust temperatures and masses do not differ significantly among these objects .
Thus , as argued previously , local DOGs are not a distinctive population among dusty galaxies , but simply represent the high-end tail of the dust obscuration distribution .