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http://dx.doi.org/10.5303/JKAS.2016.49.5.225

OPTICAL SURVEY WITH KMTNET FOR DUSTY STAR-FORMING GALAXIES IN THE AKARI DEEP FIELD SOUTH  

JEONG, WOONG-SEOB (Korea Astronomy and Space Science Institute)
KO, KYEONGYEON (Korea Astronomy and Space Science Institute)
KIM, MINJIN (Korea Astronomy and Space Science Institute)
KO, JONGWAN (Korea Astronomy and Space Science Institute)
KIM, SAM (Pontificia Universidad Catolica de Chile)
PYO, JEONGHYUN (Korea Astronomy and Space Science Institute)
KIM, SEONG JIN (Korea Astronomy and Space Science Institute)
KIM, TAEHYUN (Korea Astronomy and Space Science Institute)
SEO, HYUN JONG (Korea Astronomy and Space Science Institute)
PARK, WON-KEE (Korea Astronomy and Space Science Institute)
PARK, SUNG-JOON (Korea Astronomy and Space Science Institute)
KIM, MIN GYU (Korea Astronomy and Space Science Institute)
KIM, DONG JIN (Korea Astronomy and Space Science Institute)
CHA, SANG-MOK (Korea Astronomy and Space Science Institute)
LEE, YONGSEOK (Korea Astronomy and Space Science Institute)
LEE, CHUNG-UK (Korea Astronomy and Space Science Institute)
KIM, SEUNG-LEE (Korea Astronomy and Space Science Institute)
MATSUURA, SHUJI (Kwansei Gakuin University)
PEARSON, CHRIS (Rutherford Appleton Laboratory)
MATSUHARA, HIDEO (Institute of Space and Astronautical Science, JAXA)
Publication Information
Journal of The Korean Astronomical Society / v.49, no.5, 2016 , pp. 225-232 More about this Journal
Abstract
We present an optical imaging survey of 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 AKARI covering around 12 deg2, where the deep optical imaging data are not yet available. By utilizing the wide-field capability of the KMTNet telescopes (~4 deg2), we obtain optical images in B, R and I bands for three regions. The target depth of images in B, R and I bands is ~24 mag (AB) at 5σ, which enables us to detect most dusty star-forming galaxies discovered by 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.
Keywords
infrared; galaxies — galaxies; high-redshift — cosmology; observations;
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