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OPTICAL SURVEY WITH KMTNET FOR DUSTY STAR-FORMING GALAXIES IN THE AKARI DEEP FIELD SOUTH
정웅섭,Kyeongyeon Ko,김민진,고종완,Sam Kim,Jeonghyun Pyo,김성진,김태현,Hyun Jong Seo,Won-Kee Park,Sung-Joon Park,Min Gyu Kim,Dong Jin Kim,Sang-Mok Cha,Yongseok Lee,CHUNG-UK LEE,Seung-Lee Kim,Shuji Matsuura,Chris Pea 한국천문학회 2016 Journal of The Korean Astronomical Society Vol.49 No.5
We present an optical imaging survey of \textit{AKARI} Deep Field South (ADF-S) using the Korea Microlensing Telescope Network (KMTNet), to find optical counterparts of dusty star-forming galaxies. The ADF-S is a deep far-infrared imaging survey region with \textit{AKARI} covering around 12 deg$^2$, where the deep optical imaging data are not yet available. By utilizing the wide-field capability of the KMTNet telescopes ($\sim$4 deg$^2$), we obtain optical images in \textit{B}, \textit{R} and \textit{I} bands for three regions. The target depth of images in \textit{B}, \textit{R} and \textit{I} bands is $\sim$24 mag (AB) at 5$\sigma$, which enables us to detect most dusty star-forming galaxies discovered by \textit{AKARI} in the ADF-S. Those optical datasets will be helpful to constrain optical spectral energy distributions as well as to identify rare types of dusty star-forming galaxies such as dust-obscured galaxy, sub-millimeter galaxy at high redshift.