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We present the results from the 1.2 mm continuum image obtained as part of the Atacama Large Millimeter/ submillimeter Array Spectroscopic Survey in the Hubble Ultra Deep Field. The 1.2 mm continuum image has a size of 2.9 (4.2) arcmin 2 within a primary beam response of 50% (10%) and an rms value of m -9 1 2 * ), and star formation rate ( = --M SFR 1 1000 yr 1 ). In an accompanying paper we show that the number counts are crucial to constrain galaxy evolution models and the understanding of star-forming galaxies at high redshift.doi:10.3847/1538-4357/ab765b fatcat:hutijijzi5g4tazxlvxqkn35nu