2008MNRAS.387..707Y

We present high-resolution interferometric imaging of LH850.02, the brightest 850- and 1200-µm submillimetre (submm) galaxy in the Lockman Hole. Our observations were made at 890µm with the Submillimetre Array (SMA). Our high-resolution submm imaging detects LH850.02 at ≳6σ as a single compact (size ≲1arcsec or ≲8kpc) point source and yields its absolute position to ∼0.2-arcsec accuracy. LH850.02 has two alternative radio counterparts within the Submillimetre Common User Bolometer Array (SCUBA) beam (LH850.02N and LH850.02S), both of which are statistically very unlikely to be so close to the SCUBA source position by chance. However, the precise astrometry from the SMA shows that the submm emission arises entirely from LH850.02N, and is not associated with LH850.02S (by far the brighter of the two alternative identifications at 24µm). Fits to the optical-infrared (IR) multicolour photometry of LH850.02N and LH850.02S indicate that both lie at z ~ 3.3, and are therefore likely to be physically associated. At these redshifts, the 24-µm-to-submm flux density ratios suggest that LH850.02N has an Arp220-type starburst-dominated far-IR spectral energy distribution (SED), while LH850.02S is more similar to Mrk231, with less dust enshrouded star formation activity, but a significant contribution at 24µm (rest frame 5-6µm) from an active nucleus. This complex mix of star formation and active galactic nucleus (AGN) activity in multicomponent sources may be common in the high-redshift ultraluminous galaxy population, and highlights the need for precise astrometry from high-resolution interferometric imaging for a more complete understanding.