High-resolution SMA imaging of bright submillimetre sources from the SCUBA-2 Cosmology Legacy Survey

We have used the Submillimeter Array (SMA) at 860 mu m to observe the brightest sources in the Submillimeter Common User Bolometer Array-2 (SCUBA-2) Cosmology Legacy Survey (S2CLS). The goal of this survey is to exploit the large field of the S2CLS along with the resolution and sensitivity of the SMA to construct a large sample of these rare sources and to study their statistical properties. We have targeted 70 of the brightest single-dish SCUBA-2 850 mu m sources down to S-850 approximate to 8 mJy, achieving an average synthesized beam of 2.4 arcsec and an average rms of sigma(860) = 1.5mJy beam(-1) in our primary beam-corrected maps. We searched our SMA maps for 4 sigma peaks, corresponding to S-860 greater than or similar to 6mJy sources, and detected 62, galaxies, including three pairs. We include in our study 35 archival observations, bringing our sample size to 105 bright single-dish submillimetre sources with interferometric followup. We compute the cumulative and differential number counts, finding them to overlap with previous single-dish survey number counts within the uncertainties, although our cumulative number count is systematically lower than the parent S2CLS cumulative number count by 14 +/- 6 per cent between 11 and 15 mJy. We estimate the probability that a greater than or similar to 10 mJy single-dish submillimetre source resolves into two or more galaxies with similar flux densities to be less than 15 per cent. Assuming the remaining 85 per cent of the targets are ultraluminous starburst galaxies between z = 2 and 3, we find a likely volume density of greater than or similar to 400 M-circle dot yr(-1) sources to be similar to 3(-0.6)(+0.7) x 10(-7) Mpc(-3). We show that the descendants of these galaxies could be greater than or similar to 4 x 10(11)M(circle dot) local quiescent galaxies, and that about 10 per cent of their total stellar mass would have formed during these short bursts of star formation.