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Paper: Dusty Starbursts within a z=3 Large Scale Structure
Volume: 499, Revolution in Astronomy with ALMA: The Third Year
Page: 29
Authors: Umehata, H.; Kohno, K.; Iono, Y. T. D.; Nakanishi, K.; Hatsukade, B.; Ikarashi, S.; Izumi, T.; Matsuda, Y.; Ivison, R.; Yun, M.; Wilson, G.; Hughes, D.
Abstract: We present the results of an ALMA survey of submillimeter galaxies (SMGs) in the SSA22 field. Totally 45 sources discovered by the AzTEC/ASTE survey were observed at 1.1mm to find 64 ALMA-identified SMGs with S/N≥4.5. This is the largest SMG survey in Band 6 in ALMA Cycle1. Previous panoramic Lyman-alpha emitter (LAE) surveys have unveiled that SSA22 is not a general field but a highly biased field at z=3.1. We find large excess in the number counts and surface number density compared to the ALESS survey in ECDFS, which suggests SMGs are preferentially formed in the dense environment at z∼3.
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