高红移离子化背景的演化
天体物理学
2015-06-24 v1
摘要
我们采用最大似然分析方法,以约束 2 < z < 4.5 区间内离子化背景的数值及其演化,并考虑可能的系统误差。(本文拥有更详尽的摘要)
引用
@article{arxiv.astro-ph/9609100,
title = {Evolution of the Ionizing Background at High Redshifts},
author = {Andrew Cooke and Brian Espey and Bob Carswell},
journal= {arXiv preprint arXiv:astro-ph/9609100},
year = {2015}
}
备注
12 figures (9 of those double plots), 17 pages. Accepted by MNRAS