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Conference Paper

Making h(t) for LIGO

MPS-Authors
/persons/resource/persons40518

Allen,  Bruce
Observational Relativity and Cosmology, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society;

/persons/resource/persons40525

Hewitson,  Martin
Observational Relativity and Cosmology, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society;

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0405070.pdf
(Preprint), 346KB

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Citation

Siemens, X., Allen, B., Creighton, J. D. E., Hewitson, M., & Landry, M. (2004). Making h(t) for LIGO. Classical and Quantum Gravity, 21(20 Sp. Iss.), S1723-S1735.


Cite as: https://hdl.handle.net/11858/00-001M-0000-0013-5186-B
Abstract
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).