Optics for LISA

被引:16
作者
Robertson, DI
McNamara, P
Ward, H
Hough, J
机构
[1] Department of Physics and Astronomy, Glasgow University
关键词
D O I
10.1088/0264-9381/14/6/029
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present one of the potentially significant limits to the sensitivity of the LISA interferometer-that of beam pointing noise-and describe one possible sensor whose fundamental sensitivity is significantly better than that required.
引用
收藏
页码:1575 / 1577
页数:3
相关论文
共 4 条
[1]  
Danzmann K, 1997, CLASSICAL QUANT GRAV, V14, P1399, DOI 10.1088/0264-9381/14/6/002
[2]  
Danzmann K., 1996, LISA PREPHASE REPORT
[3]  
MORRISON E, 1994, APPL OPTICS, V33, P22
[4]   Interferometry for LISA [J].
Robertson, D ;
Hough, J .
CLASSICAL AND QUANTUM GRAVITY, 1996, 13 (11A) :A271-A277