Making h(t) for LIGO

Details Making h(t) for LIGO Making h(t) for LIGO

2004-05-13

arxiv.org/abs/gr-qc/0405070v1

Class.Quant.Grav. 21 (2004) S1723-S1736

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

14 pages, 8 figures

Scientific paper

10.1088/0264-9381/21/20/015

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 4km interferometer during the second LIGO science run (S2).

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