The Very Small Array - status report
天体物理学
2007-05-23 v1
摘要
We are contructing an interferometric telescope, the Very Small Array, to study the cosmic microwave background on angular scales 0.2--4.5 degrees. The physical layout and electronic design of the telescope are optimised to give maximum protection from systematic effects, while still providing sufficient sensitivity to make high signal-to-noise images. A prototype single baseline is currently being tested, with scientific results expected during 2000.
关键词
引用
@article{arxiv.astro-ph/9804175,
title = {The Very Small Array - status report},
author = {Michael E. Jones and P. F. Scott},
journal= {arXiv preprint arXiv:astro-ph/9804175},
year = {2007}
}
备注
4 pages, 3 figures. To be published in proceedings of the 33rd Rencontres de Moriond, Fundamental Parameters in Cosmology