SCUBA-2 Ultra Deep Imaging EAO Survey (Studies). III. Multiwavelength Properties, Luminosity Functions, and Preliminary Source Catalog of 450 μm Selected Galaxies

@article{Lim2019SCUBA2UD,
  title={SCUBA-2 Ultra Deep Imaging EAO Survey (Studies). III. Multiwavelength Properties, Luminosity Functions, and Preliminary Source Catalog of 450 $\mu$m Selected Galaxies},
  author={Chen-Fatt Lim and Wei-Hao Wang and I. R. Smail and Douglas Scott and Chian-Chou Chen and Yu-Yen Chang and James M. Simpson and Yoshiki Toba and Xinwen Shu and David L. Clements and J Greenslade and Yiping Ao and Arif Babul and J. E. Birkin and Scott C. Chapman and T. Cheng and Brian S. Cho and Helmut Dannerbauer and Ugnė Dudzevi{\vc}iūtė and James S. Dunlop and Yu Gao and Tomotsugu Goto and Luis C. Ho and L. T. Hsu and Ho Seong Hwang and Woong-Seob Jeong and Maciej Koprowski and Chien-Hsiu Lee and Ming-yi Lin and Weipeng Lin and Michał Jerzy Michałowski and Harriet Parsons and Marcin Sawicki and Raphael Shirley and Hyunjin Shim and S Urquhart and Jianfa Wang and Tiejun Wang},
  journal={The Astrophysical Journal},
  year={2019},
  volume={889},
  pages={80}
}
We construct a SCUBA-2 450 μm map in the COSMOS field that covers an area of 300 arcmin2 and reaches a 1σ noise level of 0.65 mJy in the deepest region. We extract 256 sources detected at 450 μm with signal-to-noise ratios >4.0 and analyze the physical properties of their multiwavelength counterparts. We find that most of the sources are at z lesssim 3, with a median of $z={1.79}_{-0.15}^{+0.03} \% $. About ${35}_{-25}^{+32} \% $ of our sources are classified as starburst galaxies based on… Expand
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