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

IF 1.1 4区物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS

Journal of the Korean Astronomical Society Pub Date : 2016-10-31 DOI:10.5303/JKAS.2016.49.5.225

W. Jeong, Kyeongyeon Ko, Minjin Kim, J. Ko, Sam Kim, J. Pyo, S. Kim, Tae Hyun Kim, H. Seo, W. Park, Sung-Joon Park, Min Gyu Kim, Dong-Jin Kim, S. Cha, Y. Lee, Chung-Uk Lee, Seung-Lee Kim, S. Matsuura, C. Pearson, H. Matsuhara

{"title":"OPTICAL SURVEY WITH KMTNET FOR DUSTY STAR-FORMING GALAXIES IN THE AKARI DEEP FIELD SOUTH","authors":"W. Jeong, Kyeongyeon Ko, Minjin Kim, J. Ko, Sam Kim, J. Pyo, S. Kim, Tae Hyun Kim, H. Seo, W. Park, Sung-Joon Park, Min Gyu Kim, Dong-Jin Kim, S. Cha, Y. Lee, Chung-Uk Lee, Seung-Lee Kim, S. Matsuura, C. Pearson, H. Matsuhara","doi":"10.5303/JKAS.2016.49.5.225","DOIUrl":null,"url":null,"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.","PeriodicalId":49994,"journal":{"name":"Journal of the Korean Astronomical Society","volume":"49 1","pages":"225-232"},"PeriodicalIF":1.1000,"publicationDate":"2016-10-31","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"1","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Journal of the Korean Astronomical Society","FirstCategoryId":"101","ListUrlMain":"https://doi.org/10.5303/JKAS.2016.49.5.225","RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q3","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}

引用次数: 1

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.

查看原文本刊更多论文

用kmtnet对akari深场南部尘埃恒星形成星系的光学调查

我们使用韩国微透镜望远镜网络(KMTNet)对AKARI深场南部(ADF-S)进行了光学成像调查，以寻找尘埃恒星形成星系的光学对偶。ADF-S是一个深远红外成像调查区域，AKARI覆盖约12°²，其中深光学成像数据尚未获得。利用KMTNet望远镜(~4°²)的宽视场能力，我们获得了三个区域的B、R和I波段的光学图像。B, R和I波段图像的目标深度为~24等(AB)，在5σ，这使我们能够探测到AKARI在ADF-S中发现的大多数尘埃恒星形成星系。这些光学数据集将有助于限制光谱能量分布，以及识别罕见类型的尘埃恒星形成星系，如尘埃遮挡星系，高红移亚毫米星系。

本文章由计算机程序翻译，如有差异，请以英文原文为准。

求助全文

约1分钟内获得全文求助全文

来源期刊

Journal of the Korean Astronomical Society 地学天文-天文与天体物理

CiteScore

1.30

自引率

10.00%

发文量

审稿时长

>12 weeks

期刊介绍： JKAS is an international scientific journal publishing papers in all fields of astronomy and astrophysics. All manuscripts are subject to the scrutiny of referees. Manuscripts submitted to JKAS must comply with the ethics policy of JKAS. Six regular issues are published each year on February 28, April 30, June 30, August 31, October 31, and December 31. One year''s issues compose one volume.