前景辐射与33GHz以下实验
天体物理学
2007-05-23 v1
摘要
In this paper I report on the recent results obtained from the Tenerife switched beam (10 GHz to 33 GHz) experiment and Jodrell Bank 5 GHz interferometer and their predictions for foreground levels. The full data analysis and results will be presented elsewhere. It is found that free-free emission dominates above 10 GHz, whereas synchrotron emission dominates below 5 GHz.
引用
@article{arxiv.astro-ph/9905087,
title = {Foregrounds and experiments below 33GHz},
author = {A. W. Jones},
journal= {arXiv preprint arXiv:astro-ph/9905087},
year = {2007}
}
备注
7 pages, 5 figures, invited review in "Microwave Foregrounds", eds. A de Oliveira-Costa & M. Tegmark (ASP: San Francisco)