Astronomical calibration and analysis of data obtained with phased-array feed radio telescopes

被引：0

作者：

Oosterloo, Tom ^{[1
]}

机构：

[1] Netherlands Inst Radio Astron, NL-7990 AA Dwingeloo, Netherlands

来源：

2012 INTERNATIONAL CONFERENCE ON ELECTROMAGNETICS IN ADVANCED APPLICATIONS (ICEAA) | 2012年

关键词：

D O I：

暂无

中图分类号：

TM [电工技术]; TN [电子技术、通信技术];

学科分类号：

0808 ; 0809 ;

摘要：

In the next few years, a number of new radio telescopes will become operational that will be equipped with phased-array feeds (PAFs). The large field-of-view offered by the PAFs will make it possible to survey the sky more than ten times faster than with current radio telescopes. This will have a large impact on astronomy. However, the the different nature of the instrument and the large data rates of these instruments imply that new techniques and algorithms have to be developed in order to be able to handle the data and the data stream. I briefly discuss two of the main issues.

引用

页码：190 / 193

页数：4