JWST如何测量初期光照、重 ionized 及星系组装
天体物理学
2009-11-11 v2
摘要
我们总结了将于 2011 年发射至 L2 轨道的詹姆斯·韦伯太空望远镜的设计与性能，以及它如何在 particular 地设计来研究 First Light、Reionization 和 Galaxy Assembly 的时代。
关键词
引用
@article{arxiv.astro-ph/0506253,
title = {How JWST can measure First Light, Reionization and Galaxy Assembly},
author = {R. A. Windhorst and S. H. Cohen and R. A. Jansen and C. Conselice and H. Yan},
journal= {arXiv preprint arXiv:astro-ph/0506253},
year = {2009}
}
备注
12 pages, Latex2e requires 'elsart' (included), 7 Postscript figures. To appear in the Proceedings of the UC Irvine Workshop on "First Light and Reionization: Theoretical Study and Experimental Detection of the First Luminous Sources", eds. A. Cooray & E. Barton (New Astron. Rev., 2005). A full-resolution PDF version is available at www.asu.edu/clas/hst/www/jwst/ . Revision includes minor corrections and legible labels in Fig. 6