宇宙起源摄谱仪：在轨仪器性能
天体物理仪器与方法
2015-05-20 v1
摘要
宇宙起源摄谱仪（COS）于2009年5月作为第4次维修任务的一部分安装于哈勃太空望远镜上，旨在提供远紫外和近紫外波段（FUV、NUV）的高灵敏度、中低分辨率光谱。COS是迄今为止已发射的最灵敏的FUV/NUV摄谱仪，其波长覆盖范围为900{\AA}至3200{\AA}，峰值有效面积接近3000 cm^2。本文描述了仪器设计、维修任务在轨验证（SMOV）的结果以及持续的性能监测计划。
引用
@article{arxiv.1012.5827,
title = {The Cosmic Origins Spectrograph: On-Orbit Instrument Performance},
author = {S. Osterman and J. Green and C. Froning and S. Béland and E. Burgh and K. France and S. Penton and T. Delker and D. Ebbets and D. Sahnow and J. Bacinski and R. Kimble and J. Andrews and E. Wilkinson and J. McPhate and O. Siegmund and T. Ake and A. Aloisi and C. Biagetti and R. Diaz and W. Dixon and S. Friedman and P. Ghavamian and P. Goudfrooij and G. Hartig and C. Keyes and D. Lennon and D. Massa and S. Niemi and C. Oliveira and R. Osten and C. Proffitt and T. Smith and D. Soderblom},
journal= {arXiv preprint arXiv:1012.5827},
year = {2015}
}
备注
9 pages, 7 figures, submitted to Astrophysics and Space Science