针对背景受限远紫外观测提出的新型无间隙COS G140L模式
天体物理仪器与方法
2016-09-21 v1
摘要
在此我们描述了哈勃空间望远镜（HST）上的宇宙起源光谱仪（COS）的一种新G140L观测模式的观测与定标流程。该模式CENWAV = 800旨在将远紫外波段完全移至A段探测器上，从而通过简化两个通道间的定标管理并减少该波长区域的像散，实现更高效的观测与分析。我们还描述了该新模式尤其适用的一些科学兴趣领域。
引用
@article{arxiv.1606.00402,
title = {New Gapless COS G140L Mode Proposed for Background-Limited Far-UV Observations},
author = {Keith Redwine and Stephan R. McCandliss and Brian Fleming and Kevin France and Wei Zheng and Steven Osterman and J. Christopher Howk and Scott F. Anderson and Boris T. Gaensicke},
journal= {arXiv preprint arXiv:1606.00402},
year = {2016}
}
备注
18 pages, 8 figures. This is an author-created, un-copyedited version of an article accepted for publication/published in Publications of the Astronomical Society of the Pacific. IOP Publishing Ltd is not responsible for any errors or omissions in this version of the manuscript or any version derived from it