Making h( t) for LIGO. Siemens, X., Allen, B., Creighton, J. D E, Hewitson, M., & Landry, M. Classical and Quantum Gravity, 21(20):S1723--S1735, September, 2004. Paper doi abstract bibtex 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).
@article{siemens_making_2004,
title = {Making h( t) for {LIGO}},
volume = {21},
url = {http://stacks.iop.org/0264-9381/21/i=20/a=015?key=crossref.b06734d42199c5cabb19120b3346b352},
doi = {10.1088/0264-9381/21/20/015},
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 4 km interferometer during the second LIGO science run (S2).},
number = {20},
journal = {Classical and Quantum Gravity},
author = {Siemens, Xavier and Allen, Bruce and Creighton, Jolien D E and Hewitson, Martin and Landry, Michael},
month = sep,
year = {2004},
pages = {S1723--S1735}
}
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