云南大学中国西南天文研究所

 首页 Home | 研究所简介 SWIFAR | 人员 People | 科学研究 Science | 科研设备 Facilities | 学术活动 Activities | 人才培养 Education | 国际合作 Collaborations | 科学普及 Outreach | 诚聘英才 Recruitment | 访问指南 For Visitors 
 
 首页 Home 
 研究所简介 SWIFAR 
 人员 People 
 科学研究 Science 
 学术活动 Activities 
 人才培养 Education 
 科学普及 Outreach 
 诚聘英才 Recruitment 
 访问指南 For Visitors 
 内部链接 Internal 
 
  过往活动 Past Events
当前位置: 首页 Home>>过往活动 Past Events>>正文
 

Colloquium on Apr. 21, 2022

Deep Learning Application for Reconstruction of Large-Scale Structure of the Universe


Speaker: Kana Moriwaki (University of Tokyo)

Venue: Video Conference

Time: 16:00 PM, Thursday, Apr. 21, 2022

Abstract:

Line intensity mapping (LIM) is an observational technique that measures collective line intensity emissions from distant galaxies and intergalactic media. Observed large-scale structures provide information on cosmology and galaxy formation and evolution. A limitation with LIM is line confusion, where the contributions of different lines from different redshifts are all confused. In this study, we propose to use machine learning to solve it. We devise a generative adversarial network that extracts designated signals from LIM data. By training it on mock observational maps that simulate future observations, our network properly reconstructs the peak positions and statistics of intensity fluctuations. In this talk, I will introduce our new machine-learning architecture, show the results of the reconstruction, and discuss how it is done by the network.


Report PPT:  SWIFAR_Kana Moriwaki.pdf

附件【SWIFAR_Kana Moriwaki.pdf已下载
关闭窗口

版权所有:云南大学中国西南天文研究所 

South-Western Institute For Astronomy Research, YNU