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 May. 25, 2023

To detect the 21 cm global spectrum from the Cosmic Dawn: single antenna and interferometer


Speaker: Bin Yue  (NAOC)

Venue: SWIFAR Building 2111

Time: 15:00 PM, Thursday, May. 25, 2023

Abstract:

The 21 cm global spectrum (monopole) from the Cosmic Dawn is a powerful tool to detect the thermal history of the Universe and Pop III stars. Different from the power spectrum that needs large interferometer array to observe, monopole signal can be detected by a single small-aperture and wide-field antenna. Some of these experiments have been constructed on Earth, for example the EDGES, SARAS, and so on, but the measured results are still in debate, mainly because the systematics and the ionospheric effects are hard to perfectly migrated. In future, the space programs, e.g. Hongmeng (DSL), DAPPER, can do better measurements in the lunar-orbit sites. On the other hand, if the beam is anisotropic, AND/OR the sky is non-flat, the monopole also contributes to the interferometer visibility. So an interferometer also has the ability to measure the 21 cm global spectrum. This is kind of independent measurements based on different principle. In this talk, I will review the recent progress in single antenna 21 cm global spectrum observations, and introduce the algorithm of extracting monopole signal from the visibilities, and show some simulated results for some typical array configurations.


Report PPT:  SWIFAR_Bin Yue.pdf

附件【SWIFAR_Bin Yue.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