SXDF-UDS-CANDELS-ALMA 1.5 arcmin2 deep survey

We have conducted 1.1 mm ALMA observations of a contiguous 105'' × 50'' or 1.5 arcmin² window in the SXDF-UDS-CANDELS. We achieved a 5σ sensitivity of 0.28 mJy, giving a flat sensus of dusty star-forming galaxies with L _IR ~6×10¹¹ L _⊙ (if T _dust=40K) up to z ~ 10 thanks to the negative K-correction at this wavelength. We detected 5 brightest sources (S/N>6) and 18 low-significant sources (5>S/N>4 they may contain spurious detections, though). One of the 5 brightest ALMA sources (S _1.1mm = 0.84 +/- 0.09 mJy) is extremely faint in the WFC3 and VLT/HAWK-I images, demonstrating that a contiguous ALMA imaging survey uncovers a faint dust-obscured population invisible in the deep optical/near-infrared surveys. We find a possible [CII]-line emitter at z=5.955 or a low-z CO emitting galaxy within the field, allowing us to constrain the [CII] and/or CO luminosity functions across the history of the universe.