We report 1.1 mm number counts revealed with the Atacama Large Millimeter/submillimeter Array (ALMA) in the Subaru/XMM-Newton Deep Survey Field (SXDF). The advent of ALMA enables us to reveal millimeter-wavelength number counts down to the faint end without source confusion. However, previous studies are based on the ensemble of serendipitously-detected sources in fields originally targeting different sources and could be biased due to the clustering of sources around the targets. We derive number counts in the flux range of 0.2-2 mJy by using 23 (>=4sigma) sources detected in a continuous 2.0 arcmin2 area of the SXDF. The number counts are consistent with previous results within errors, suggesting that the counts derived from serendipitously-detected sources are not significantly biased, although there could be field-to-field variation due to the small survey area. By using the best-fit function of the number counts, we find that ~40% of the extragalactic background light at 1.1 mm is resolved at S(1.1mm) > 0.2 mJy.
@article{arxiv.1602.08167,
title = {SXDF-ALMA 2 arcmin$^2$ Deep Survey: 1.1-mm Number Counts},
author = {Bunyo Hatsukade and Kotaro Kohno and Hideki Umehata and Itziar Aretxaga and Karina I. Caputi and James S. Dunlop and Soh Ikarashi and Daisuke Iono and Rob J. Ivison and Minju Lee and Ryu Makiya and Yuichi Matsuda and Kentaro Motohara and Kouichiro Nakanishi and Kouji Ohta and Ken-ich Tadaki and Yoichi Tamura and Wei-Hao Wang and Grant W. Wilson and Yuki Yamaguchi and Min S. Yun},
journal= {arXiv preprint arXiv:1602.08167},
year = {2016}
}
Comments
8 pages, 7 figures, Accepted for publication in PASJ