Making h(t) for LIGO

被引：15

作者：

Siemens, X

Allen, B

Creighton, J

Hewitson, M

Landry, M

机构：

[1] Univ Wisconsin, Dept Phys, Ctr Gravitat & Cosmol, Milwaukee, WI 53201 USA

[2] Max Planck Inst Gravitat Phys, Albert Einstein Inst, D-30167 Hannover, Germany

[3] Leibniz Univ Hannover, Aussenstelle Hannover, D-30167 Hannover, Germany

[4] LIGO Hanford Observ, Richland, WA 99352 USA

来源：

CLASSICAL AND QUANTUM GRAVITY | 2004年 / 21卷 / 20期

关键词：

D O I：

10.1088/0264-9381/21/20/015

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The conversion of the read-out from the anti-symmetric port of the LIGO interferometers into gravitational strain has thus far been performed in the frequency domain. Here we describe a conversion in the time domain which is based on the method developed by GEO. We illustrate the method using the Hanford 4 km interferometer during the second LIGO science run (S2).

引用

页码：S1723 / S1735

页数：13

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